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c000000 | Aeolis Palus is a plain between the northern wall of Gale crater and the northern foothills of Aeolis Mons (Mount Sharp) on Mars. It is located at 4.47°S 137.42°E / -4.47; 137.42. The NASA Mars Science Laboratory mission landed the Curiosity rover on Aeolis Palus in August 2012. Curiosity spent two (Earth) years explo... | Aeolis Palus | https://en.wikipedia.org/wiki/Aeolis_Palus |
c000001 | On September 26, 2013, NASA scientists reported the Mars Curiosity rover detected "abundant, easily accessible" water (1.5 to 3 weight percent) in soil samples at the Rocknest region of Aeolis Palus in Gale Crater. In addition, NASA reported the rover found two principal soil types: a fine-grained mafic type and a loca... | Aeolis Palus | https://en.wikipedia.org/wiki/Aeolis_Palus |
c000002 | On December 16, 2014, NASA reported detecting, based on measurements by the Curiosity rover, an unusual increase, then decrease, in the amounts of methane in the atmosphere of the planet Mars; in addition, organic chemicals were detected in powder drilled from a rock by the Curiosity rover. Also, based on deuterium to ... | Aeolis Palus | https://en.wikipedia.org/wiki/Aeolis_Palus |
c000003 | Akshata Krishnamurthy (born 27 December 1990) is an Indian space systems engineer working as Principal Investigator and Science Phase Lead at the NASA Jet Propulsion Laboratory. She is currently working on Mars 2020. She was named to Fortune India's "Most Powerful Women" Krishnamurthy was born on 27 December 1990 in Be... | Akshata Krishnamurthy | https://en.wikipedia.org/wiki/Akshata_Krishnamurthy |
c000004 | At MIT, she was the President of the Graduate Association of Aeronautics and Astronautics (GA^3) student organization and Co-Chair of the MIT India Conference. Krishnamurthy interned at NASA's Jet Propulsion Laboratory as part of the ASTERIA mission while working on her PhD. In April 2021, she and her colleagues receiv... | Akshata Krishnamurthy | https://en.wikipedia.org/wiki/Akshata_Krishnamurthy |
c000005 | Luigi G. Napolitano Award from the International Astronautical Federation for contributions to aerospace science (2017) Dr. Robbin Chapman Excellence Through Adversity Award from the MIT Office of Graduate Education (2018) Amelia Earhart Fellowship by the Zonta International Foundation (July 2018) Emerging Space Leade... | Akshata Krishnamurthy | https://en.wikipedia.org/wiki/Akshata_Krishnamurthy |
c000006 | Allen "Al" Chen is an American aerospace engineer. He was the Entry, Descent, and Landing (EDL) Operations Lead on the Mars Science Laboratory mission and the EDL Lead for the Mars 2020 mission. Chen is from Newtown, Pennsylvania, and is a graduate of Lawrenceville School. He is a fan of the Philadelphia Eagles and Phi... | Allen Chen | https://en.wikipedia.org/wiki/Allen_Chen |
c000007 | Chen received a Fully Employed Master of Business Administration (FEMBA) from the UCLA Anderson School of Management in 2007. Allen Chen has worked at NASA's Jet Propulsion Laboratory in Pasadena, California for his entire career. He joined the Mars Science Laboratory EDL team in 2002. On August 5, 2012, Chen announced... | Allen Chen | https://en.wikipedia.org/wiki/Allen_Chen |
c000008 | Chen narrated the Mars 2020 landing procedures with Guidance and Controls Operations Lead Swati Mohan on February 18, 2021. Chen stated he's excited to be a part of bringing Martian samples back to Earth. He considers his Mars 2020 EDL team to be a second family to him. Nelessen, Adam; Sackier, Chloe; Clark, Ian; Bruga... | Allen Chen | https://en.wikipedia.org/wiki/Allen_Chen |
c000009 | APXS is also an abbreviation for APache eXtenSion tool, an extension for Apache web servers. An alpha particle X-ray spectrometer (APXS) is a spectrometer that analyses the chemical element composition of a sample from scattered alpha particles and fluorescent X-rays after a sample is irradiated with alpha particles an... | Alpha particle X-ray spectrometer | https://en.wikipedia.org/wiki/Alpha_particle_X-ray_spectrometer |
c000010 | APS/APXS devices will be included on several upcoming missions. Several forms of radiation are used in APXS. They include alpha particles, protons, and X-rays. Alpha particles, protons, and X-rays are emitted during the radioactive decay of unstable atoms. A common source of alpha particles is curium-244. It emits part... | Alpha particle X-ray spectrometer | https://en.wikipedia.org/wiki/Alpha_particle_X-ray_spectrometer |
c000011 | Some of the alpha particles are absorbed by the atomic nuclei. The [alpha,proton] process produces protons of a defined energy which are detected. Sodium, magnesium, silicon, aluminium and sulfur can be detected by this method. This method was only used in the Mars Pathfinder APXS. For the Mars Exploration Rovers the p... | Alpha particle X-ray spectrometer | https://en.wikipedia.org/wiki/Alpha_particle_X-ray_spectrometer |
c000012 | Alpha Proton X-Ray Spectrometer, for Mars Pathfinder by the Max Planck Institute and the University of Chicago. Alpha Particle X-ray Spectrometer, for Spirit (MER-A) and Opportunity (MER-B) Mars Exploration Rovers. Alpha Particle X-ray Spectrometer, for Curiosity (MSL). The principal investigator for Curiosity's APXS i... | Alpha particle X-ray spectrometer | https://en.wikipedia.org/wiki/Alpha_particle_X-ray_spectrometer |
c000013 | The Bagnold Dunes is a 35-kilometre-long (22 mi) group of dark grey dunes in the Gale Crater on Mars. They are named after Ralph Alger Bagnold, who crossed the Libyan Desert and was one of the first explorers to acquire a deep understanding of the physics behind sand dunes. The dunes migrate around 0.4 metres (1.3 ft) ... | Bagnold Dunes | https://en.wikipedia.org/wiki/Bagnold_Dunes |
c000014 | Bathurst Inlet is a rock on the surface of Aeolis Palus, between Peace Vallis and Aeolis Mons ("Mount Sharp"), in Gale crater on the planet Mars. The rock was encountered by the Curiosity rover on the way from Bradbury Landing to Glenelg Intrigue on September 30, 2012 and was named after Bathurst Inlet, a deep inlet l... | Bathurst Inlet (rock) | https://en.wikipedia.org/wiki/Bathurst_Inlet_%28rock%29 |
c000015 | J. "Bob" Balaram (born 28 June 1959) is an Indian-American scientist and engineer currently working for National Aeronautics and Space Administration. He is the chief engineer and designer of Ingenuity (project name: Mars 2020 helicopter), the first extraterrestrial aircraft, that was attached underside of car-sized Pe... | Bob Balaram | https://en.wikipedia.org/wiki/Bob_Balaram |
c000016 | In 2012 MiMi Aung was leading then JPL director Charles Elachi on a tour of the Autonomous Systems Division. Looking at the drones demonstrating onboard navigation algorithms in one of the labs, Elachi asked, “ Hey, why don't we do that on Mars?” Engineer Bob Balaram briefed Elachi about feasibility, and a week later E... | Bob Balaram | https://en.wikipedia.org/wiki/Bob_Balaram |
c000017 | J. (Bob) Balaram; Timothy Canham; Courtney Duncan; Matt Golombek; Håvard Fjær Grip; Wayne Johnson; Justin Maki; Amelia Quon; Ryan Stern; David Zhu (2018). "Mars Helicopter Technology Demonstrator" (PDF). SciTech Forum Conference 8–12 January 2018 Kissimmee, Florida. American Institute of Aeronautics and Astronautics (A... | Bob Balaram | https://en.wikipedia.org/wiki/Bob_Balaram |
c000018 | Bradbury Landing is the August 6, 2012, landing site within Gale crater on planet Mars of the Mars Science Laboratory (MSL) Curiosity rover. On August 22, 2012, on what would have been his 92nd birthday, NASA named the site for author Ray Bradbury, who had died on June 5, 2012. The coordinates of the landing site on Ma... | Bradbury Landing | https://en.wikipedia.org/wiki/Bradbury_Landing |
c000019 | The landing site contains material washed down from the wall of the crater, which will provide scientists with the opportunity to investigate the rocks that form the bedrock in this area. The landing ellipse also contains a rock type that is very dense, very brightly colored, and unlike any rock type previously investi... | Bradbury Landing | https://en.wikipedia.org/wiki/Bradbury_Landing |
c000020 | Two canyons were cut in the mound through the layers containing clay minerals and sulfate salts after deposition of the layers. These canyons expose layers of rock representing tens or hundreds of millions of years of environmental change. Curiosity may be able to investigate these layers in the canyon closest to the l... | Bradbury Landing | https://en.wikipedia.org/wiki/Bradbury_Landing |
c000021 | CheMin, short for Chemistry and Mineralogy, is an instrument located in the interior of the Curiosity rover that is exploring the surface of Gale crater on Mars. David Blake, from NASA Ames Research Center, is the Principal Investigator. CheMin identifies and quantifies the minerals present in rocks and soil delivered ... | CheMin | https://en.wikipedia.org/wiki/CheMin |
c000022 | In operation, the collimated X-ray source produces and directs a beam through a transmission sample cell containing powdered material. A CCD (charge-coupled device) imager is positioned on the opposite side of the sample from the source and directly detects X-rays diffracted or fluoresced by the sample. The CCD can mea... | CheMin | https://en.wikipedia.org/wiki/CheMin |
c000023 | Capacity: CheMin is planned to analyze as many as 74 dry samples, but it is capable of analyzing many more because its sample cells can be emptied and reused for additional analyses. Cross-contamination by cell reuse is expected to be less than 5%. CheMin does not have the capability to store previously analyzed sample... | CheMin | https://en.wikipedia.org/wiki/CheMin |
c000024 | CheMin analyzed many rocks. Some contained carbonates in the form of crystalline siderite (FeCO3). One rock contained over 10 % of the mineral. The rocks also were composed of plagioclase with the elements sodium (Na)–, Ca-, and aluminum (Al)–, as well as Ca- and Mg-bearing silicate mineral pyroxene. Other minera... | CheMin | https://en.wikipedia.org/wiki/CheMin |
c000025 | Chemistry and Camera complex (ChemCam) is a suite of remote sensing instruments on Mars for the Curiosity rover. As the name implies, ChemCam is actually two different instruments combined as one: a laser-induced breakdown spectroscopy (LIBS) and a Remote Micro Imager (RMI) telescope. The purpose of the LIBS instrument... | Chemistry and Camera complex | https://en.wikipedia.org/wiki/Chemistry_and_Camera_complex |
c000026 | Using the same collection optics, the RMI provides context images of the LIBS analysis spots. The RMI resolves 1 mm (0.039 in) objects at 10 m (33 ft) distance, and has a field of view covering 20 cm (7.9 in) at that distance. The RMI has also been used to take images of distant geologic features and landscapes. The Ch... | Chemistry and Camera complex | https://en.wikipedia.org/wiki/Chemistry_and_Camera_complex |
c000027 | The Remote Micro-Imager is primarily used to capture high-resolution, black and white images of ChemCam targets for context and documentation. Usually, an image of the target of interest is captured before and after the laser is fired. Often, the laser makes "LIBS pits" that can be visible in the RMI to show where the ... | Chemistry and Camera complex | https://en.wikipedia.org/wiki/Chemistry_and_Camera_complex |
c000028 | ChemCam has been used, in conjunction with other instruments of the Curiosity rover, to make advancements in understanding the chemical composition of rocks and soils on Mars. LIBS makes it possible to detect and quantify the major oxides: SiO2, Al2O3, FeOT, MgO, TiO2, CaO, Na2O, and K2O of bedrock targets. There are d... | Chemistry and Camera complex | https://en.wikipedia.org/wiki/Chemistry_and_Camera_complex |
c000029 | Cheyava Falls is a rock discovered on Mars in 2024 by NASA's Perseverance rover during its exploration of the Jezero crater. This rock, named after a Grand Canyon waterfall, has drawn significant attention due to its potential as an indicator of ancient life on Mars. The rover's instruments detected organic compounds w... | Cheyava Falls | https://en.wikipedia.org/wiki/Cheyava_Falls |
c000030 | The "arrowhead-shaped rock" was found at the northern edge of Neretva Vallis area, on 18 July 2024, and is 3.2 by 2 feet (0.98 m × 0.61 m). On 21 July 2024, Perseverance took a sample of the rock that became its 22nd core sample that can be delivered to Earth by a future mission. The rover made a "selfie" with a rock o... | Cheyava Falls | https://en.wikipedia.org/wiki/Cheyava_Falls |
c000031 | On 10 September 2025, NASA reported a "potential biosignature" finding in Cheyava Falls: organic-carbon–bearing mudstones hosting sub-millimetre nodules and millimetre-scale reaction fronts enriched in ferrous iron phosphate and iron sulfide, consistent with vivianite and greigite, imply low-temperature, post-depositio... | Cheyava Falls | https://en.wikipedia.org/wiki/Cheyava_Falls |
c000032 | The same organic materials can be produced by non-biological processes which require "hot conditions" like volcanic activity; the rock location suggests that it was underwater, and there is no detected past volcanic activity in that region. Perseverance's SHERLOC, a deep-ultraviolet Raman spectrometer, detected organic... | Cheyava Falls | https://en.wikipedia.org/wiki/Cheyava_Falls |
c000033 | Bright Angel is roughly 3,500 km from Curiosity's organic detections at Gale crater, so finding comparable organics here suggests organic matter may have been geographically widespread on Mars around 3.5 billion years ago. The carbon is confirmed to be not graphite, but its specific type and origin remain unresolved. P... | Cheyava Falls | https://en.wikipedia.org/wiki/Cheyava_Falls |
c000034 | According to the first author of an article in Nature, Joel Hurowitz, "labs on Earth could look for ways of achieving the same effects without either biology or high temperatures"; but even if it can be done, the result might fail the Knoll criterion: "to be evidence of life, an observation has to not just be explicabl... | Cheyava Falls | https://en.wikipedia.org/wiki/Cheyava_Falls |
c000035 | The Columbia Hills are a range of low hills inside Gusev crater on Mars. They were observed by the Mars Exploration Rover Spirit when it landed within the crater in 2004. They were promptly given an unofficial name by NASA since they were the most striking nearby feature on the surface. The hills lie approximately 3 ki... | Columbia Hills (Mars) | https://en.wikipedia.org/wiki/Columbia_Hills_%28Mars%29 |
c000036 | Brown Hill - named after David M. Brown Chawla Hill - named after Kalpana Chawla Clark Hill - named after Laurel Clark Husband Hill - named after Rick Husband McCool Hill - named after William C. McCool Ramon Hill - named after Ilan Ramon With the Spirit rover, scientists found a variety of rock types in the Columbia H... | Columbia Hills (Mars) | https://en.wikipedia.org/wiki/Columbia_Hills_%28Mars%29 |
c000037 | Acid fog is believed to have changed some of the Watchtower rocks. This was in a 200 meter long section of Cumberland Ridge and the Husband Hill summit. Certain places became less crystalline and more amorphous. Acidic water vapor from volcanoes dissolved some minerals forming a gel. When water evaporated a cement... | Columbia Hills (Mars) | https://en.wikipedia.org/wiki/Columbia_Hills_%28Mars%29 |
c000038 | Wishstone contained a great deal of plagioclase, some olivine, and anhydrite (a calcium sulfate). Peace rocks showed sulfur and strong evidence for bound water, so hydrated sulfates are suspected. Watchtower class rocks lack olivine, implying that they may have been altered by water. The Independence class showed so... | Columbia Hills (Mars) | https://en.wikipedia.org/wiki/Columbia_Hills_%28Mars%29 |
c000039 | After Spirit stopped working scientists studied old data from the Miniature Thermal Emission Spectrometer (Mini-TES) and confirmed the presence of large amounts of carbonate-rich rocks, which means that regions of the planet may have once harbored water. The carbonates were discovered in an outcrop of rocks called "Co... | Columbia Hills (Mars) | https://en.wikipedia.org/wiki/Columbia_Hills_%28Mars%29 |
c000040 | The composition of Mars covers the branch of the geology of Mars that describes the make-up of the planet Mars. Mars is differentiated, which—for a terrestrial planet—implies that it has a central core made up of high density matter (mainly metallic iron and nickel) surrounded by a less dense, silicate mantle and crust... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000041 | Much of what we know about the elemental composition of Mars comes from orbiting spacecraft and landers. (See Exploration of Mars for list.) Most of these spacecraft carry spectrometers and other instruments to measure the surface composition of Mars by either remote sensing from orbit or in situ analyses on the surfac... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000042 | Hydrogen is present as water (H2O) ice and in hydrated minerals. Carbon occurs as carbon dioxide (CO2) in the atmosphere and sometimes as dry ice at the poles. An unknown amount of carbon is also stored in carbonates. Molecular nitrogen (N2) makes up 2.7 percent of the atmosphere. As far as we know, organic compounds a... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000043 | Mars is fundamentally an igneous planet. Rocks on the surface and in the crust consist predominantly of minerals that crystallize from magma. Most of our current knowledge about the mineral composition of Mars comes from spectroscopic data from orbiting spacecraft, in situ analyses of rocks and soils from six landing s... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000044 | The dark areas of Mars are characterised by the mafic rock-forming minerals olivine, pyroxene, and plagioclase feldspar. These minerals are the primary constituents of basalt, a dark volcanic rock that also makes up the Earth's oceanic crust and the lunar maria. The mineral olivine occurs all over the planet, but some ... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000045 | Between 1997 and 2006, the Thermal Emission Spectrometer (TES) on the Mars Global Surveyor (MGS) spacecraft mapped the global mineral composition of the planet. TES identified two global-scale volcanic units on Mars. Surface Type 1 (ST1) characterises the Noachian-aged highlands and consists of unaltered plagioclase- a... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000046 | Rocks studied by Spirit rover in Gusev crater can be classified in different ways. The amounts and types of minerals make the rocks primitive basalts—also called picritic basalts. The rocks are similar to ancient terrestrial rocks called basaltic komatiites. Rocks of the plains also resemble the basaltic shergottites, ... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000047 | In the journal Science from September 2013, researchers described a different type of rock called "Jake M" or "Jake Matijevic (rock),” It was the first rock analyzed by the Alpha Particle X-ray Spectrometer instrument on the Curiosity rover, and it was different from other known Martian igneous rocks as it is alkaline ... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000048 | Using SAM's mass spectrometer, scientists measured isotopes of helium, neon, and argon that cosmic rays produce as they go through rock. The fewer of these isotopes they find, the more recently the rock has been exposed near the surface. The 4-billion-year-old lakebed rock drilled by Curiosity was uncovered between 30 ... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000049 | The samples examined were probably once mud that for millions to tens of millions of years could have hosted living organisms. This wet environment had neutral pH, low salinity, and variable redox states of both iron and sulfur species. These types of iron and sulfur could have been used by living organisms. C, H, O, S... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000050 | Much of the Martian surface is deeply covered by dust as fine as talcum powder. The global predominance of dust obscures the underlying bedrock, making spectroscopic identification of primary minerals impossible from orbit over many areas of the planet. The red/orange appearance of the dust is caused by iron(III) oxide... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000051 | Opaline silica and iron sulphate minerals form in acidic (low pH) solutions. Sulphates have been found in a variety of locations, including near Juventae Chasma, Ius Chasma, Melas Chasma, Candor Chasma, and Ganges Chasma. These sites all contain fluvial landforms indicating that abundant water was once present. Spiri... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000052 | While the possibility of carbonates on Mars has been of great interest to astrobiologists and geochemists alike, there was little evidence for significant quantities of carbonate deposits on the surface. In the summer of 2008, the TEGA and WCL experiments on the 2007 Phoenix Mars lander found between 3–5wt% (percent by... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000053 | The rocks on the plains of Gusev are a type of basalt. They contain the minerals olivine, pyroxene, plagioclase, and magnetite, and they look like volcanic basalt as they are fine-grained with irregular holes (geologists would say they have vesicles and vugs). Much of the soil on the plains came from the breakdown of ... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000054 | The dust in Gusev Crater is the same as dust all around the planet. All the dust was found to be magnetic. Moreover, Spirit found the magnetism was caused by the mineral magnetite, especially magnetite that contained the element titanium. One magnet was able to completely divert all dust hence all Martian dust is th... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000055 | Plain's rocks have been very slightly altered, probably by thin films of water because they are softer and contain veins of light colored material that may be bromine compounds, as well as coatings or rinds. It is thought that small amounts of water may have gotten into cracks inducing mineralization processes). Coati... | Composition of Mars | https://en.wikipedia.org/wiki/Composition_of_Mars |
c000056 | Curiosity is a Mars rover that is exploring Gale crater and Mount Sharp on Mars as part of NASA's Mars Science Laboratory (MSL) mission. Launched in 2011 and landed the following year, the car-sized rover continues to operate more than a decade after its original two-year mission. Curiosity was launched from Cape Canav... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000057 | In December 2012, Curiosity's two-year mission was extended indefinitely. On August 6, 2022, a detailed overview of accomplishments by the Curiosity rover for the last ten years was reported. The rover is still operational, and as of July 13, 2026, Curiosity has been active on Mars for 4953 sols (5089 total days; 13 ye... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000058 | Biological Determine the nature and inventory of organic carbon compounds Investigate the chemical building blocks of life (carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur) Identify features that may represent the effects of biological processes (biosignatures and biomolecules) Geological and geochemical Inv... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000059 | About one year into the surface mission, and having assessed that ancient Mars could have been hospitable to microbial life, the MSL mission objectives evolved to developing predictive models for the preservation process of organic compounds and biomolecules; a branch of paleontology called taphonomy. The region it is ... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000060 | Adjusted for inflation, Curiosity has a life-cycle cost of US$3.2 billion in 2020. By comparison, the 2021 Perseverance rover has a life-cycle cost of US$2.9 billion. Curiosity is 2.9 m (9 ft 6 in) long by 2.7 m (8 ft 10 in) wide by 2.2 m (7 ft 3 in) high, larger than Mars Exploration Rovers, which are 1.5 m (4 ft 11 i... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000061 | Curiosity comprised 23% of the mass of the 3,893 kg (8,583 lb) spacecraft at launch. The remaining mass was discarded in the process of transport and landing. Dimensions: Curiosity has a mass of 899 kg (1,982 lb) including 80 kg (180 lb) of scientific instruments. The rover is 2.9 m (9 ft 6 in) long by 2.7 m (8 ft 10 i... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000062 | Curiosity's RTG is the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG), designed and built by Rocketdyne and Teledyne Energy Systems under contract to the U.S. Department of Energy, and fueled and tested by the Idaho National Laboratory. Based on legacy RTG technology, it represents a more flexible and comp... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000063 | Heat rejection system: The temperatures at the landing site vary seasonally and the thermal system warms the rover as needed. The thermal system does so in several ways: passively, through the dissipation to internal components; by electrical heaters strategically placed on key components; and by using the rover heat r... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000064 | The RCE computers use the RAD750 Central processing unit (CPU), which is a successor to the RAD6000 CPU of the Mars Exploration Rovers. The IBM RAD750 CPU, a radiation-hardened version of the PowerPC 750, can execute up to 400 Million instructions per second (MIPS), while the RAD6000 CPU is capable of up to only 35 MIP... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000065 | The rover has four processors. One of them is a SPARC processor that runs the rover's thrusters and descent-stage motors as it descended through the Martian atmosphere. Two others are PowerPC processors: the main processor, which handles nearly all of the rover's ground functions, and that processor's backup. The fourt... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000066 | Jet Propulsion Laboratory (JPL) is the central data distribution hub where selected data products are provided to remote science operations sites as needed. JPL is also the central hub for the uplink process, though participants are distributed at their respective home institutions. At landing, telemetry was monitored ... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000067 | Curiosity can roll over obstacles approaching 65 cm (26 in) in height, and it has a ground clearance of 60 cm (24 in). Based on variables including power levels, terrain difficulty, slippage and visibility, the maximum terrain-traverse speed is estimated to be 200 m (660 ft) per day by automatic navigation. The rover l... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000068 | According to NASA, an estimated 20,000 to 40,000 heat-resistant bacterial spores were on Curiosity at launch, and as many as 1,000 times that number may not have been counted. Previous NASA Mars rovers became active only after the successful entry, descent and landing on the Martian surface. Curiosity, on the other han... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000069 | As of August 16, 2024, the rover had driven 35.5 km (22.1 mi) from its landing site. As of July 13, 2026 it has driven 36.86 km (22.90 mi) from its landing site over 4953 sols (Martian days), and as of January 2025, its elevation had changed over 740 m (2,430 ft) upward. Curiosity has two full sized, vehicle system tes... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000070 | The MastCam, Mars Hand Lens Imager (MAHLI), and Mars Descent Imager (MARDI) cameras were developed by Malin Space Science Systems and they all share common design components, such as on-board digital image processing boxes, 1600 × 1200 charge-coupled device (CCDs), and an RGB Bayer pattern filter. In total, the rover c... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000071 | Each camera has eight gigabytes of flash memory, which is capable of storing over 5,500 raw images, and can apply real time lossless data compression. The cameras have an autofocus capability that allows them to focus on objects from 2.1 m (6 ft 11 in) to infinity. In addition to the fixed RGBG Bayer pattern filter, ea... | Curiosity (rover) | https://en.wikipedia.org/wiki/Curiosity_%28rover%29 |
c000072 | Lady Diana Trujillo Pomerantz (born 1983) is a Colombian-American aerospace engineer at the NASA Jet Propulsion Laboratory. She currently leads the engineering team at JPL responsible for the robotic arm of the Perseverance rover. On February 18, 2021, Trujillo hosted the first ever Spanish-language NASA transmission o... | Diana Trujillo | https://en.wikipedia.org/wiki/Diana_Trujillo |
c000073 | Trujillo enrolled initially at the University of Florida to pursue studies in aerospace engineering, inspired by a magazine article about the role of women working on aerospace missions and having self-confidence in her strong mathematical skills. While studying at the university, she decided to apply for the NASA Acad... | Diana Trujillo | https://en.wikipedia.org/wiki/Diana_Trujillo |
c000074 | Trujillo joined NASA in 2007, working at Goddard Space Flight Center on the Constellation program and the Jet Propulsion Laboratory on human and robotic space missions. She has served many roles, including Surface Sampling System Activity Lead and Dust Removal Tool Lead Systems Engineer. She was responsible for ensurin... | Diana Trujillo | https://en.wikipedia.org/wiki/Diana_Trujillo |
c000075 | Trujillo worked as flight director on the Mars 2020 Perseverance Rover robotic arm and in February 2021, she hosted NASA's first Spanish-language planetary landing show. She has been involved in several initiatives to inspire young women from Latin America and African-American women to pursue a career in science and en... | Diana Trujillo | https://en.wikipedia.org/wiki/Diana_Trujillo |
c000076 | 2021 Awarded the rank of Commander (Comendador) in the Order of Boyaca, the highest honor that can be awarded to Colombian citizens for exceptional service to Colombia 2021 Awarded by the Congress of Colombia the order of merit Policarpa Salavarrieta on March 8, 2021. 2019 City of STEM Icon Award. 2017 Named one of Los... | Diana Trujillo | https://en.wikipedia.org/wiki/Diana_Trujillo |
c000077 | The Dynamic Albedo of Neutrons (DAN) instrument is an experiment mounted on the Mars Science Laboratory's Curiosity rover. It is a pulsed sealed-tube neutron source and detector used to measure hydrogen or ice and water at or near the Martian surface. The instrument consists of the detector element (DE) and a 14.1 MeV... | Dynamic Albedo of Neutrons | https://en.wikipedia.org/wiki/Dynamic_Albedo_of_Neutrons |
c000078 | On August 19, 2015, NASA scientists reported that the DAN instrument on Curiosity detected an unusual hydrogen-rich area, at "Marias Pass," on Mars. The hydrogen found seemed related to water or hydroxyl ions in rocks within 3 feet (0.91 m) beneath the rover, according to the scientists. | Dynamic Albedo of Neutrons | https://en.wikipedia.org/wiki/Dynamic_Albedo_of_Neutrons |
c000079 | Eberswalde, previously known as Holden NE, is a partially buried impact crater in Margaritifer Terra, Mars. Eberswalde crater lies just to the north of Holden, a large crater that may have been a lake. The 65.3-km-diameter crater, centered at 24°S, 33°W, is named after the German town of the same name, in accordance w... | Eberswalde (crater) | https://en.wikipedia.org/wiki/Eberswalde_%28crater%29 |
c000080 | Several sites in the Margaritifer Sinus quadrangle have been proposed as areas to send NASA's major Mars rover, the Mars Science Laboratory (MSL). Eberswalde was shortlisted as one of the final four proposed landing sites for the Curiosity rover, part of the MSL mission. It was voted a close second after Gale crater by... | Eberswalde (crater) | https://en.wikipedia.org/wiki/Eberswalde_%28crater%29 |
c000081 | Many craters once contained lakes. The delta in Eberswalde Crater is strong evidence that a lake once existed here. Based on an estimate by Moore et al. in 2003 of flow volume to the crater at 700 m3/s, it is estimated that it would take twenty years to completely fill the crater, ignoring evaporation and infiltration... | Eberswalde (crater) | https://en.wikipedia.org/wiki/Eberswalde_%28crater%29 |
c000082 | Experience Curiosity is an interactive web application developed by NASA's Jet Propulsion Laboratory to celebrate the third anniversary of the Curiosity rover landing on Mars. This 3D serious game makes it possible to operate the rover, control its cameras and the robotic arm and reproduces some of the prominent events... | Experience Curiosity | https://en.wikipedia.org/wiki/Experience_Curiosity |
c000083 | Gale is a crater, and probable dry lake, at 5.4°S 137.8°E / -5.4; 137.8 in the northwestern part of the Aeolis quadrangle on Mars. It is 154 km (96 mi) in diameter and estimated to be about 3.5–3.8 billion years old. The crater was named after Walter Frederick Gale, an amateur astronomer from Sydney, Australia, who ob... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000084 | Gale, named for Walter F. Gale (1865–1945), an amateur astronomer from Australia, spans 154 km (96 mi) in diameter and holds a mountain, Aeolis Mons (informally named "Mount Sharp" to pay tribute to geologist Robert P. Sharp) rising 18,000 ft (5,500 m) from the crater floor, higher than Mount Rainier rises above Seattl... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000085 | At 10:32 p.m. PDT on August 5, 2012 (1:32 a.m. EDT on August 6, 2012), the Mars Science Laboratory rover Curiosity landed on Mars at 4.5°S 137.4°E / -4.5; 137.4, at the foot of the layered mountain inside Gale. Curiosity landed within a landing ellipse approximately 7 km (4.3 mi) by 20 km (12 mi). The landing ellipse ... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000086 | Orbital THEMIS and topography data, plus visible and near-infrared images, were used to make a geological map of the crater. CRISM data indicated the lower bench unit was composed of interstratified clay and sulfates. Curiosity explored the stratigraphy of the crater consisting of the Bradbury Group and the overlying... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000087 | Observations of possible cross-bedded strata on the upper mound suggest aeolian processes, but the origin of the lower mound layers remains ambiguous. In February 2019, NASA scientists reported that the Mars Curiosity rover had determined, for the first time, the density of Mount Sharp in Gale, thereby establishing a c... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000088 | In December 2012, scientists working on the Mars Science Laboratory mission announced that an extensive soil analysis of Martian soil performed by Curiosity showed evidence of water molecules, sulphur and chlorine, as well as hints of organic compounds. However, terrestrial contamination, as the source of the organic c... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000089 | On December 9, 2013, NASA reported that, based on evidence from Curiosity studying Aeolis Palus, Gale contained an ancient freshwater lake which could have been a hospitable environment for microbial life. On December 16, 2014, NASA reported detecting, by the Curiosity rover at Gale, an unusual increase, then decrease,... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000090 | On August 5, 2017, NASA celebrated the fifth anniversary of the Curiosity rover mission landing, and related exploratory accomplishments, on the planet Mars. (Videos: Curiosity's First Five Years (02:07); Curiosity's POV: Five Years Driving (05:49); Curiosity's Discoveries About Gale Crater (02:54)) On June 7, 2018, NA... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000091 | On November 4, 2018, geologists presented evidence, based on studies in Gale by the Curiosity rover, that there was plenty of water on early Mars. In January 2020, researchers have found certain minerals, made of carbon and oxygen, in rocks at Gale, which may have formed in an ice-covered lake during a cold stage betwe... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000092 | This discovery is significant. Much evidence exists to show that impacts and volcanic activity could melt ground ice to make liquid water. However, that water may not last long enough for life to develop. This new finding shows here it is not the case–water stayed for some time. Also, with water coming and going on... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000093 | Research published in February 2025 described wave ripples in Gale that show that liquid water flowed there. The ripples were found in two different time periods. Calculations based on their shape and sizes revealed that they were formed in shallow moving water. The water could have been as deep as 2 meters. Before... | Gale (crater) | https://en.wikipedia.org/wiki/Gale_%28crater%29 |
c000094 | Glenelg (or Glenelg Intrigue) is a location on Mars near the Mars Science Laboratory (Curiosity rover) landing site (Bradbury Landing) in Gale Crater marked by a natural intersection of three kinds of terrain. The location was named Glenelg by NASA scientists for two reasons: all features in the immediate vicinity were... | Glenelg, Mars | https://en.wikipedia.org/wiki/Glenelg%2C_Mars |
c000095 | Goulburn, also known as Goulburn Scour, is a rock outcrop on the surface of Aeolis Palus, between Peace Vallis and Aeolis Mons ("Mount Sharp"), in Gale crater on the planet Mars. The outcrop was encountered by the Curiosity rover on landing at the Bradbury Landing on August 6, 2012 (the 1st sol of the mission) and is ... | Goulburn (Mars) | https://en.wikipedia.org/wiki/Goulburn_%28Mars%29 |
c000096 | Gusev is a crater on the planet Mars and is located at 14.5°S 175.4°E / -14.5; 175.4 and is in the Aeolis quadrangle. The crater is about 166 kilometers in diameter and formed approximately three to four billion years ago. It was named after Russian astronomer Matvey Gusev (1826–1866) in 1976. Prior to the exploration... | Gusev (Martian crater) | https://en.wikipedia.org/wiki/Gusev_%28Martian_crater%29 |
c000097 | On January 3, 2004, Gusev was the landing site of the first of NASA's two Mars Exploration Rovers, named Spirit. It was hoped that the numerous smaller and more recent craters in this region would have exposed sedimentary material from early eras, although at first the region proved disappointing in its lack of availab... | Gusev (Martian crater) | https://en.wikipedia.org/wiki/Gusev_%28Martian_crater%29 |
c000098 | Much of the soil on the plains came from the breakdown of the local rocks. Fairly high levels of nickel were found in some soils; probably from meteorites. Analysis shows that the rocks have been slightly altered by tiny amounts of water. Outside coatings and cracks inside the rocks suggest water deposited minerals, ... | Gusev (Martian crater) | https://en.wikipedia.org/wiki/Gusev_%28Martian_crater%29 |
c000099 | Observations of rocks on the plains show they contain the minerals pyroxene, olivine, plagioclase, and magnetite. These rocks can be classified in different ways. The amounts and types of minerals make the rocks primitive basalts—also called picritic basalts. The rocks are similar to ancient terrestrial rocks called... | Gusev (Martian crater) | https://en.wikipedia.org/wiki/Gusev_%28Martian_crater%29 |
Wikipedia Gradual-Semantic Retrieval Benchmark
A single fixed Wikipedia corpus (1,655 science / astronomy passages) paired with fifteen query sets of steadily decreasing semantic breadth — from all of science down to a single information need asked in about 300 paraphrases. It is designed to measure how a dense retriever behaves, in both benign utility and vulnerability to corpus-poisoning attacks, as the attacked query distribution narrows.
The fifteen levels form a strictly nested chain,
scope(L1) ⊂ scope(L2) ⊂ … ⊂ scope(L15), so breadth decreases
monotonically the whole way down. Each level has 300 queries (L5 has 298), split
150 held-in / 150 held-out. The layout matches the other PoisonTEB datasets
(msmarco-concepts): configs corpus / queries / qrels, with one split per level
(levels play the role of "concepts") over one shared corpus.
Public and redistributable (the corpus is Wikipedia text, CC BY-SA 4.0). Sibling of the
Harry-Potter proof-of-concept MatanBT/hp-gradual-semantic.
The fifteen levels
Levels L15 → L6 are carved by Wikipedia's category tree: each passage carries a chain-depth equal to the narrowest level whose scope contains it, so the nesting is exact by construction. Levels L5 → L1 keep narrowing below the flagship band, where the category tree bottoms out, by subject instead — one mission ⊃ two robots ⊃ one subject ⊃ a few facets ⊃ one query. The corpus is identical across all levels; only the query scope narrows.
| Level | Label | Scope | Queries | Golds / query |
|---|---|---|---|---|
| L15 | science |
Science in general (any natural-science topic) | 300 | 1.00 |
| L14 | astronomy |
Astronomy and astrophysics | 300 | 1.00 |
| L13 | solar_system |
The Solar System (beyond the planets themselves) | 300 | 1.00 |
| L12 | planets |
Planets (as a class) and the non-terrestrial planets | 300 | 1.00 |
| L11 | terrestrial_planets |
The terrestrial (rocky) planets | 300 | 1.00 |
| L10 | mars |
The planet Mars (the world itself) | 300 | 1.00 |
| L9 | mars_exploration |
Exploration of Mars (all mission types) | 300 | 2.66 |
| L8 | mars_surface_missions |
Missions that operated on the Martian surface | 300 | 2.25 |
| L7 | mars_rovers |
Mars rovers (all of them) | 300 | 2.82 |
| L6 | flagship_rover_ops |
The Curiosity and Perseverance rover missions | 300 | 2.26 |
| L5 | mars2020_mission |
The whole Mars 2020 mission | 298 | 1.28 |
| L4 | perseverance_and_ingenuity |
The Perseverance rover and Ingenuity helicopter | 300 | 1.65 |
| L3 | ingenuity_helicopter |
The Ingenuity helicopter as a subject | 300 | 1.41 |
| L2 | ingenuity_flight_campaign |
A few facets of Ingenuity's flight campaign | 300 | 1.60 |
| L1 | ingenuity_flight_count |
The exact fact: Ingenuity's total flight count | 300 | 2.00 |
Loading
from datasets import load_dataset
corpus = load_dataset("MatanBT/wiki-gradual-semantic", "corpus", split="train")
queries = load_dataset("MatanBT/wiki-gradual-semantic", "queries", split="L1") # narrowest
qrels = load_dataset("MatanBT/wiki-gradual-semantic", "qrels", split="L15") # broadest
From the paper's eval flow: python embedding_evaluators/eval.py run <model> --wiki-semantic-grid
(uses RetrievalEvalDataset.init_from_wiki_semantic).
Files and schema
| Config | Split(s) | One row per… | Fields |
|---|---|---|---|
corpus |
train |
in-domain passage (can be gold) | _id, text, title (source article), url |
corpus |
corpus_additional |
in-domain distractor passage (never gold) | _id, text, title, url |
queries |
L1…L15 |
query | _id, text, level (1-15), level_label, split (held_in/held_out), source_chunk_id |
qrels |
L1…L15 |
gold judgment | query-id, corpus-id, score (=1) |
Multi-gold relevance. Wikipedia states the same fact across near-duplicate chunks and sibling articles, so a query often has several correct answers. Wherever that happens, every passage that directly answers the query is marked relevant (the "Golds / query" column above). On the subject and category levels L3-L9 the extra golds were selected by an impartial LLM judge over a neutral BM25 + dense + same-article candidate pool, so the labels favour no single retriever; the two paraphrase levels L1-L2 use a curated gold set for their target fact(s); the broad category levels L10-L15 keep a single gold. This makes NDCG@10 reward retrieving a correct answer rather than retrieving one arbitrarily-chosen chunk.
Distractors. corpus_additional holds 1,083 extra Wikipedia science/space passages
mined from the same category tree as the corpus (none of which is any query's gold). They are
meant to be added at eval time as genuinely competitive, on-domain noise — off-domain passages
(e.g. random web text) are trivially separable and do not affect retrieval. The eval loader
adds a deterministic prefix of this split via init_from_wiki_semantic(n_random_passages_to_add=N).
Sidecars. groups.json (per-level metadata, including held_in_ids / held_out_ids),
corpus_meta.jsonl (_id, depth, title, url per passage), corpus_stats.json, and
sources.tsv (the full per-article source list, also reproduced below).
Reference baseline (e5-base-v2)
intfloat/e5-base-v2 (queries prefixed with query: , passages with passage: ,
embeddings L2-normalized, cosine scoring), evaluated over the train corpus with all
1,083 corpus_additional distractors added (a 2,738-passage haystack). success@10 is
the fraction of queries with a correct passage in the top 10. NDCG@10 declines toward the
narrow end mainly because many near-duplicate passages tie, not because retrieval fails —
note that success@10 stays high (0.91-1.00) at every level. Reproduce with
python embedding_evaluators/eval.py run intfloat/e5-base-v2 --wiki-semantic-grid.
| Level | Label | NDCG@10 | success@10 |
|---|---|---|---|
| L15 | science |
0.921 | 0.99 |
| L14 | astronomy |
0.915 | 0.99 |
| L13 | solar_system |
0.905 | 0.99 |
| L12 | planets |
0.927 | 0.99 |
| L11 | terrestrial_planets |
0.914 | 0.99 |
| L10 | mars |
0.947 | 0.99 |
| L9 | mars_exploration |
0.872 | 1.00 |
| L8 | mars_surface_missions |
0.901 | 1.00 |
| L7 | mars_rovers |
0.848 | 1.00 |
| L6 | flagship_rover_ops |
0.749 | 0.95 |
| L5 | mars2020_mission |
0.778 | 0.95 |
| L4 | perseverance_and_ingenuity |
0.683 | 0.92 |
| L3 | ingenuity_helicopter |
0.704 | 0.91 |
| L2 | ingenuity_flight_campaign |
0.658 | 0.93 |
| L1 | ingenuity_flight_count |
0.753 | 0.97 |
Sources
Every passage is chunked from English Wikipedia. The benchmark draws on
1,654 distinct articles — 117 scraped in full and 1,537
from the article's lead (intro) section only. The corpus (gold-able) split comes mostly from
the core science / Mars-rover articles taken in full; the corpus_additional distractor split
comes mostly from adjacent articles' lead sections. Each passage also records its own source in
its title / url fields; the machine-readable list is in sources.tsv.
Full list of 1,654 source articles — passages (corpus / distractor), and how much of the article was scraped
| Article | Passages (corpus / distractor) | Scraped |
|---|---|---|
| Composition of Mars | 16 (16 / 0) | full article |
| Curiosity (rover) | 16 (16 / 0) | full article |
| Ingenuity (helicopter) | 16 (16 / 0) | full article |
| Mars 2020 | 16 (16 / 0) | full article |
| Mars Exploration Rover | 16 (16 / 0) | full article |
| Mars Pathfinder | 16 (16 / 0) | full article |
| Mars Science Laboratory | 16 (16 / 0) | full article |
| Meridiani Planum | 16 (16 / 0) | full article |
| Opportunity (rover) | 16 (16 / 0) | full article |
| Perseverance (rover) | 16 (16 / 0) | full article |
| Rosalind Franklin (rover) | 16 (16 / 0) | full article |
| Sojourner (rover) | 16 (16 / 0) | full article |
| Spirit (rover) | 16 (16 / 0) | full article |
| Tianwen-1 | 16 (16 / 0) | full article |
| Timeline of Mars Science Laboratory | 16 (16 / 0) | full article |
| Timeline of Opportunity | 16 (16 / 0) | full article |
| Timeline of Spirit | 16 (16 / 0) | full article |
| Zhurong (rover) | 15 (15 / 0) | full article |
| ExoMars | 13 (13 / 0) | full article |
| Mars sample-return mission | 12 (12 / 0) | full article |
| Mars Society | 12 (12 / 0) | full article |
| European Rover Challenge | 11 (11 / 0) | full article |
| Gale (crater) | 11 (11 / 0) | full article |
| Idefix (rover) | 10 (10 / 0) | full article |
| Mars Astrobiology Explorer-Cacher | 10 (10 / 0) | full article |
| University Rover Challenge | 10 (10 / 0) | full article |
| Endeavour (crater) | 9 (9 / 0) | full article |
| Gusev (Martian crater) | 9 (9 / 0) | full article |
| Jezero (crater) | 9 (9 / 0) | full article |
| Mars Oxygen ISRU Experiment | 9 (9 / 0) | full article |
| Mawrth Vallis | 9 (9 / 0) | full article |
| Mars Geyser Hopper | 8 (8 / 0) | full article |
| Loay Elbasyouni | 7 (7 / 0) | full article |
| Mars 2 | 7 (7 / 0) | full article |
| Mars 3 | 7 (7 / 0) | full article |
| Mars rover | 7 (7 / 0) | full article |
| Mount Sharp | 7 (7 / 0) | full article |
| Astrobiology Field Laboratory | 6 (6 / 0) | full article |
| Cheyava Falls | 6 (6 / 0) | full article |
| Crewed Mars rover | 6 (6 / 0) | full article |
| Northern Light (spacecraft) | 6 (6 / 0) | full article |
| Syrtis Major Planum | 6 (6 / 0) | full article |
| Brightness temperature | 5 (0 / 5) | lead section |
| Columbia Hills (Mars) | 5 (5 / 0) | full article |
| Diana Trujillo | 5 (5 / 0) | full article |
| Fretted terrain | 5 (0 / 5) | lead section |
| Magnetosphere chronology | 5 (0 / 5) | lead section |
| Mars Lander Mission | 5 (5 / 0) | full article |
| Multi-mission radioisotope thermoelectric generator | 5 (5 / 0) | full article |
| NASA's Eyes | 5 (4 / 1) | full article |
| Northeast Syrtis | 5 (5 / 0) | full article |
| Peace Vallis | 5 (5 / 0) | full article |
| Rocker-bogie | 5 (5 / 0) | full article |
| Sample Analysis at Mars | 5 (5 / 0) | full article |
| SuperCam | 5 (5 / 0) | full article |
| Vandi Verma | 5 (5 / 0) | full article |
| Alpha particle X-ray spectrometer | 4 (4 / 0) | full article |
| CheMin | 4 (4 / 0) | full article |
| Chemistry and Camera complex | 4 (4 / 0) | full article |
| History of life | 4 (0 / 4) | lead section |
| Impact event | 4 (0 / 4) | lead section |
| List of Solar System objects by size | 4 (0 / 4) | lead section |
| Mastcam-Z | 4 (4 / 0) | full article |
| MELOS | 4 (4 / 0) | full article |
| Phobos Surveyor | 4 (4 / 0) | full article |
| Regge–Wheeler–Zerilli equations | 4 (0 / 4) | lead section |
| Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals | 4 (4 / 0) | full article |
| Sky crane (landing system) | 4 (4 / 0) | full article |
| Swati Mohan | 4 (4 / 0) | full article |
| UK Centre for Astrobiology | 4 (0 / 4) | lead section |
| Void ratio | 4 (0 / 4) | lead section |
| Adirondack (Mars) | 3 (3 / 0) | lead section |
| Aeolis Palus | 3 (3 / 0) | full article |
| Akshata Krishnamurthy | 3 (3 / 0) | full article |
| Allen Chen | 3 (3 / 0) | full article |
| Anthroposphere | 3 (0 / 3) | lead section |
| AQUAL | 3 (0 / 3) | lead section |
| Astrobiology | 3 (3 / 0) | lead section |
| Atmosphere of Earth | 3 (3 / 0) | lead section |
| Atmosphere of Mars | 3 (3 / 0) | lead section |
| Bacteria | 3 (3 / 0) | lead section |
| Big Bang | 3 (3 / 0) | lead section |
| BLUEsat UNSW | 3 (3 / 0) | full article |
| Bob Balaram | 3 (3 / 0) | full article |
| Bradbury Landing | 3 (3 / 0) | full article |
| Callisto (moon) | 3 (3 / 0) | lead section |
| Climate change | 3 (3 / 0) | lead section |
| Climate of Mars | 3 (2 / 1) | lead section |
| Comet | 3 (3 / 0) | lead section |
| Convective overturn | 3 (0 / 3) | lead section |
| Earth | 3 (3 / 0) | lead section |
| Eberswalde (crater) | 3 (3 / 0) | full article |
| Energetic neutral atom | 3 (0 / 3) | lead section |
| Entropy (astrophysics) | 3 (0 / 3) | lead section |
| Equatorial layered deposits | 3 (3 / 0) | lead section |
| Europa (moon) | 3 (3 / 0) | lead section |
| Evolution | 3 (3 / 0) | lead section |
| Exoplanet | 3 (3 / 0) | lead section |
| Galaxy H-Alpha Fabry-Perot System | 3 (0 / 3) | lead section |
| Geology of Venus | 3 (3 / 0) | lead section |
| Giant-impact hypothesis | 3 (0 / 3) | lead section |
| Glaciers on Mars | 3 (3 / 0) | lead section |
| Gullies on Mars | 3 (3 / 0) | lead section |
| High throughput biology | 3 (0 / 3) | lead section |
| History of Mars observation | 3 (3 / 0) | lead section |
| Holden (Martian crater) | 3 (3 / 0) | full article |
| Hubble Space Telescope | 3 (3 / 0) | lead section |
| Impact crater | 3 (3 / 0) | lead section |
| International Chemical Identifier | 3 (0 / 3) | lead section |
| International Mars Exploration Working Group | 3 (3 / 0) | lead section |
| James Webb Space Telescope | 3 (3 / 0) | lead section |
| Journey to Mars | 3 (0 / 3) | lead section |
| Jupiter | 3 (3 / 0) | lead section |
| Kuiper belt | 3 (3 / 0) | lead section |
| Latitude dependent mantle | 3 (3 / 0) | lead section |
| Life on Mars | 3 (3 / 0) | lead section |
| Linear ridge networks | 3 (3 / 0) | lead section |
| List of Solar System objects | 3 (0 / 3) | lead section |
| Local Group | 3 (3 / 0) | lead section |
| Main sequence | 3 (3 / 0) | lead section |
| Mars | 3 (3 / 0) | lead section |
| Mars Surveyor 2001 | 3 (3 / 0) | full article |
| Mineral | 3 (3 / 0) | lead section |
| Nebular hypothesis | 3 (0 / 3) | lead section |
| Nervous system | 3 (3 / 0) | lead section |
| Noachian | 3 (2 / 1) | lead section |
| Nuclear fission | 3 (3 / 0) | lead section |
| Nucleosynthesis | 3 (0 / 3) | lead section |
| Ocean | 3 (3 / 0) | lead section |
| Oort cloud | 3 (3 / 0) | lead section |
| Optical depth (astrophysics) | 3 (0 / 3) | lead section |
| Oregon State University Mars Rover | 3 (3 / 0) | full article |
| Oxia Palus quadrangle | 3 (0 / 3) | lead section |
| Paleontology | 3 (0 / 3) | lead section |
| Phillips relationship | 3 (0 / 3) | lead section |
| Phobos (moon) | 3 (2 / 1) | lead section |
| Photosynthesis | 3 (3 / 0) | lead section |
| Planet | 3 (3 / 0) | lead section |
| Planetary boundaries | 3 (0 / 3) | lead section |
| Potentially hazardous object | 3 (0 / 3) | lead section |
| Radiation assessment detector | 3 (3 / 0) | full article |
| Random sequential adsorption | 3 (0 / 3) | lead section |
| Ride Report | 3 (3 / 0) | lead section |
| Satellite system (astronomy) | 3 (0 / 3) | lead section |
| Scale (chemistry) | 3 (0 / 3) | lead section |
| Scalloped topography | 3 (3 / 0) | lead section |
| Semiconductor | 3 (3 / 0) | lead section |
| Single-cell nanoencapsulation | 3 (0 / 3) | lead section |
| Solar System | 3 (3 / 0) | lead section |
| Solar transit | 3 (0 / 3) | lead section |
| Speed of light | 3 (3 / 0) | lead section |
| Statistics | 3 (3 / 0) | lead section |
| The central science | 3 (0 / 3) | lead section |
| Timothy Canham | 3 (3 / 0) | full article |
| Tolman–Oppenheimer–Volkoff equation | 3 (0 / 3) | lead section |
| Upper plains unit | 3 (3 / 0) | lead section |
| Victoria (crater) | 3 (3 / 0) | full article |
| Virus | 3 (3 / 0) | lead section |
| Water on Mars | 3 (3 / 0) | lead section |
| 2001 Mars Odyssey | 2 (2 / 0) | lead section |
| 391 Ingeborg | 2 (2 / 0) | lead section |
| 4 Vesta | 2 (2 / 0) | lead section |
| 55 Cancri Ae | 2 (0 / 2) | lead section |
| Abundance of the chemical elements | 2 (0 / 2) | lead section |
| Acid | 2 (2 / 0) | lead section |
| Albedo feature | 2 (0 / 2) | lead section |
| Allotropy | 2 (0 / 2) | lead section |
| Alloy | 2 (0 / 2) | lead section |
| Andromeda Galaxy | 2 (2 / 0) | lead section |
| Annual cycle | 2 (0 / 2) | lead section |
| Arcadia quadrangle | 2 (2 / 0) | lead section |
| Areosynchronous orbit | 2 (2 / 0) | lead section |
| Asteroid | 2 (2 / 0) | lead section |
| Asteroid belt | 2 (2 / 0) | lead section |
| Astronomical constant | 2 (0 / 2) | lead section |
| Astrophysics | 2 (0 / 2) | lead section |
| Atmosphere | 2 (0 / 2) | lead section |
| Atmosphere of Jupiter | 2 (2 / 0) | lead section |
| Atmosphere of Venus | 2 (2 / 0) | lead section |
| Atom | 2 (2 / 0) | lead section |
| Atomic and molecular astrophysics | 2 (0 / 2) | lead section |
| Bidirectional scattering distribution function | 2 (0 / 2) | lead section |
| Binary star | 2 (2 / 0) | lead section |
| Biogeography | 2 (0 / 2) | lead section |
| Biosaline agriculture | 2 (0 / 2) | lead section |
| Black hole | 2 (2 / 0) | lead section |
| Brain terrain | 2 (2 / 0) | lead section |
| Cape York (Mars) | 2 (2 / 0) | lead section |
| Cell (biology) | 2 (2 / 0) | lead section |
| Centaur (small Solar System body) | 2 (2 / 0) | lead section |
| Ceres (dwarf planet) | 2 (2 / 0) | lead section |
| Chamberlin–Moulton planetesimal hypothesis | 2 (0 / 2) | lead section |
| Champagne flow model | 2 (0 / 2) | lead section |
| Chandrasekhar–Kendall function | 2 (0 / 2) | lead section |
| Chemical bond | 2 (2 / 0) | lead section |
| Chemical element | 2 (0 / 2) | lead section |
| Chemical reaction | 2 (0 / 2) | lead section |
| Claimed moons of Earth | 2 (0 / 2) | lead section |
| Clearing the neighbourhood | 2 (0 / 2) | lead section |
| Colonization of Mars | 2 (2 / 0) | lead section |
| Constellation | 2 (2 / 0) | lead section |
| Constellation program | 2 (2 / 0) | lead section |
| Cosmic dust | 2 (0 / 2) | lead section |
| Cosmic microwave background | 2 (2 / 0) | lead section |
| Cosmology | 2 (2 / 0) | lead section |
| Dark energy | 2 (2 / 0) | lead section |
| Dark matter | 2 (2 / 0) | lead section |
| Dark slope streak | 2 (2 / 0) | lead section |
| Darwin–Radau equation | 2 (0 / 2) | lead section |
| Dawn (spacecraft) | 2 (2 / 0) | lead section |
| De Vaucouleurs's law | 2 (0 / 2) | lead section |
| Deep space exploration | 2 (0 / 2) | lead section |
| Descent 3 | 2 (0 / 2) | lead section |
| Detached object | 2 (0 / 2) | lead section |
| Discovery and exploration of the Solar System | 2 (0 / 2) | lead section |
| DNA | 2 (2 / 0) | lead section |
| Doom (1993 video game) | 2 (2 / 0) | lead section |
| Double layer forces | 2 (0 / 2) | lead section |
| Dynamic Albedo of Neutrons | 2 (2 / 0) | full article |
| Earth analog | 2 (0 / 2) | lead section |
| Earth mass | 2 (0 / 2) | lead section |
| Earth radius | 2 (0 / 2) | lead section |
| Earth's energy budget | 2 (0 / 2) | lead section |
| Earth's magnetic field | 2 (2 / 0) | lead section |
| Earthquake | 2 (2 / 0) | lead section |
| Ecology | 2 (2 / 0) | lead section |
| Einasto profile | 2 (0 / 2) | lead section |
| Electricity | 2 (2 / 0) | lead section |
| Electroconductive carbon black | 2 (0 / 2) | lead section |
| Electromagnetism | 2 (2 / 0) | lead section |
| Emirates Mars Mission | 2 (2 / 0) | lead section |
| Enceladus | 2 (2 / 0) | lead section |
| Energy-rich species | 2 (0 / 2) | lead section |
| Enzyme | 2 (2 / 0) | lead section |
| Equivalent weight | 2 (0 / 2) | lead section |
| Eris (dwarf planet) | 2 (2 / 0) | lead section |
| Esdat | 2 (0 / 2) | lead section |
| Europa Clipper | 2 (2 / 0) | lead section |
| Eutectic system | 2 (0 / 2) | lead section |
| Fluorescence | 2 (0 / 2) | lead section |
| Formation and evolution of the Solar System | 2 (2 / 0) | lead section |
| Formation of Jupiter | 2 (0 / 2) | lead section |
| Fossil | 2 (2 / 0) | lead section |
| Galaxy | 2 (2 / 0) | lead section |
| Galilean moons | 2 (2 / 0) | lead section |
| Ganymede (moon) | 2 (2 / 0) | lead section |
| Gas giant | 2 (2 / 0) | lead section |
| Gas torus | 2 (0 / 2) | lead section |
| Genetics | 2 (2 / 0) | lead section |
| Geology | 2 (2 / 0) | lead section |
| Geology of Mercury | 2 (2 / 0) | lead section |
| Geology of solar terrestrial planets | 2 (0 / 2) | lead section |
| Geology of the Moon | 2 (2 / 0) | lead section |
| Geometry | 2 (2 / 0) | lead section |
| Geopark | 2 (0 / 2) | lead section |
| Geophysics | 2 (0 / 2) | lead section |
| GeoRef | 2 (0 / 2) | lead section |
| Geysers on Mars | 2 (2 / 0) | lead section |
| Giant planet | 2 (0 / 2) | lead section |
| Global Standard Stratigraphic Age | 2 (0 / 2) | lead section |
| Global surface temperature | 2 (0 / 2) | lead section |
| Gonggong (dwarf planet) | 2 (0 / 2) | lead section |
| Gravitational compression | 2 (0 / 2) | lead section |
| Gravitational lensing formalism | 2 (0 / 2) | lead section |
| Gravitational memory effect | 2 (0 / 2) | lead section |
| Gravitational wave | 2 (2 / 0) | lead section |
| Gravitational-wave astronomy | 2 (0 / 2) | lead section |
| Gravity | 2 (2 / 0) | lead section |
| Habitability of G-type main-sequence star systems | 2 (0 / 2) | lead section |
| Halley's Comet | 2 (2 / 0) | lead section |
| Haloscope (physics) | 2 (0 / 2) | lead section |
| Haumea | 2 (0 / 2) | lead section |
| Hayashi track | 2 (0 / 2) | lead section |
| Hazcam | 2 (2 / 0) | full article |
| Heliocentric orbit | 2 (2 / 0) | lead section |
| Heliocentrism | 2 (0 / 2) | lead section |
| Heliosphere | 2 (2 / 0) | lead section |
| Home Plate (Mars) | 2 (2 / 0) | full article |
| Human mission to Mars | 2 (2 / 0) | lead section |
| Human spaceflight | 2 (0 / 2) | lead section |
| Husar-rover | 2 (0 / 2) | lead section |
| IAU (1976) System of Astronomical Constants | 2 (0 / 2) | lead section |
| IAU definition of planet | 2 (0 / 2) | lead section |
| Idealized greenhouse model | 2 (0 / 2) | lead section |
| Imagining Mars: A Literary History | 2 (0 / 2) | lead section |
| Immune system | 2 (2 / 0) | lead section |
| Infest the Rats' Nest | 2 (1 / 1) | lead section |
| InSight | 2 (2 / 0) | lead section |
| Instrumental magnitude | 2 (0 / 2) | lead section |
| International Center for Relativistic Astrophysics | 2 (0 / 2) | lead section |
| Interplanetary dust cloud | 2 (0 / 2) | lead section |
| Interstellar medium | 2 (2 / 0) | lead section |
| Intrinsic DNA fluorescence | 2 (0 / 2) | lead section |
| Io (moon) | 2 (2 / 0) | lead section |
| Ismenius Lacus quadrangle | 2 (2 / 0) | lead section |
| Jacob Matijevic | 2 (2 / 0) | full article |
| Jaffe profile | 2 (0 / 2) | lead section |
| Jake Matijevic (rock) | 2 (2 / 0) | full article |
| Jumping-Jupiter scenario | 2 (0 / 2) | lead section |
| Jupiter radius | 2 (0 / 2) | lead section |
| K correction | 2 (0 / 2) | lead section |
| Kepler-452b | 2 (0 / 2) | lead section |
| Kirkwood gap | 2 (2 / 0) | lead section |
| Lane–Emden equation | 2 (0 / 2) | lead section |
| Laniakea Supercluster | 2 (0 / 2) | lead section |
| LARLE crater | 2 (2 / 0) | lead section |
| Laser | 2 (2 / 0) | lead section |
| Leo Rover | 2 (2 / 0) | full article |
| Lineated valley fill | 2 (2 / 0) | lead section |
| List of crewed spacecraft | 2 (0 / 2) | lead section |
| List of Mars-crossing minor planets | 2 (2 / 0) | lead section |
| List of minor planets: 10001–11000 | 2 (1 / 1) | lead section |
| List of minor planets: 1001–2000 | 2 (1 / 1) | lead section |
| List of minor planets: 11001–12000 | 2 (1 / 1) | lead section |
| List of minor planets: 111001–112000 | 2 (1 / 1) | lead section |
| List of minor planets: 120001–121000 | 2 (1 / 1) | lead section |
| List of minor planets: 15001–16000 | 2 (1 / 1) | lead section |
| List of minor planets: 160001–161000 | 2 (1 / 1) | lead section |
| List of minor planets: 164001–165000 | 2 (1 / 1) | lead section |
| List of minor planets: 17001–18000 | 2 (1 / 1) | lead section |
| List of minor planets: 18001–19000 | 2 (1 / 1) | lead section |
| List of minor planets: 19001–20000 | 2 (1 / 1) | lead section |
| List of minor planets: 192001–193000 | 2 (1 / 1) | lead section |
| List of minor planets: 20001–21000 | 2 (1 / 1) | lead section |
| List of minor planets: 2001–3000 | 2 (1 / 1) | lead section |
| List of minor planets: 205001–206000 | 2 (1 / 1) | lead section |
| List of minor planets: 217001–218000 | 2 (1 / 1) | lead section |
| List of minor planets: 229001–230000 | 2 (1 / 1) | lead section |
| List of minor planets: 23001–24000 | 2 (1 / 1) | lead section |
| List of minor planets: 237001–238000 | 2 (1 / 1) | lead section |
| List of minor planets: 24001–25000 | 2 (1 / 1) | lead section |
| List of minor planets: 26001–27000 | 2 (1 / 1) | lead section |
| List of minor planets: 270001–271000 | 2 (1 / 1) | lead section |
| List of minor planets: 27001–28000 | 2 (1 / 1) | lead section |
| List of minor planets: 30001–31000 | 2 (1 / 1) | lead section |
| List of minor planets: 306001–307000 | 2 (1 / 1) | lead section |
| List of minor planets: 31001–32000 | 2 (1 / 1) | lead section |
| List of minor planets: 32001–33000 | 2 (1 / 1) | lead section |
| List of minor planets: 328001–329000 | 2 (1 / 1) | lead section |
| List of minor planets: 39001–40000 | 2 (1 / 1) | lead section |
| List of minor planets: 405001–406000 | 2 (1 / 1) | lead section |
| List of minor planets: 42001–43000 | 2 (1 / 1) | lead section |
| List of minor planets: 474001–475000 | 2 (1 / 1) | lead section |
| List of minor planets: 5001–6000 | 2 (1 / 1) | lead section |
| List of minor planets: 509001–510000 | 2 (1 / 1) | lead section |
| List of minor planets: 51001–52000 | 2 (1 / 1) | lead section |
| List of minor planets: 53001–54000 | 2 (1 / 1) | lead section |
| List of minor planets: 6001–7000 | 2 (1 / 1) | lead section |
| List of minor planets: 814001–815000 | 2 (1 / 1) | lead section |
| List of minor planets: 85001–86000 | 2 (1 / 1) | lead section |
| List of minor planets: 99001–100000 | 2 (1 / 1) | lead section |
| List of ocean worlds in the Solar System | 2 (0 / 2) | lead section |
| List of rocks on Mars | 2 (2 / 0) | full article |
| Lists of minor planets | 2 (0 / 2) | lead section |
| Lobate debris apron | 2 (0 / 2) | lead section |
| Magnetism | 2 (2 / 0) | lead section |
| Magnetosheath | 2 (0 / 2) | lead section |
| Magnetosphere of Jupiter | 2 (2 / 0) | lead section |
| Magnetosphere particle motion | 2 (0 / 2) | lead section |
| Makemake | 2 (0 / 2) | lead section |
| Mare Boreum quadrangle | 2 (0 / 2) | lead section |
| Margaritifer Sinus quadrangle | 2 (2 / 0) | lead section |
| Mars 2M No.521 | 2 (2 / 0) | lead section |
| Mars Cube One | 2 (2 / 0) | lead section |
| Mars Environmental Dynamics Analyzer | 2 (2 / 0) | full article |
| Mars Hand Lens Imager | 2 (2 / 0) | full article |
| Mars in culture | 2 (2 / 0) | lead section |
| Mars Orbiter Mission | 2 (2 / 0) | lead section |
| Mars Reconnaissance Orbiter | 2 (2 / 0) | lead section |
| Mars Space Flight Facility | 2 (2 / 0) | lead section |
| MarsDial | 2 (2 / 0) | full article |
| Marsquake | 2 (2 / 0) | lead section |
| Martian dichotomy | 2 (2 / 0) | lead section |
| Martian polar ice caps | 2 (2 / 0) | lead section |
| Martian spherules | 2 (0 / 2) | lead section |
| Mass deficit | 2 (0 / 2) | lead section |
| Mathematics | 2 (2 / 0) | lead section |
| MAVEN | 2 (2 / 0) | lead section |
| Meanings of minor-planet names | 2 (0 / 2) | lead section |
| Melas Chasma | 2 (2 / 0) | full article |
| Mercury (planet) | 2 (2 / 0) | lead section |
| Meteorite | 2 (2 / 0) | lead section |
| Methane functionalization | 2 (0 / 2) | lead section |
| Michael H. Hecht | 2 (2 / 0) | full article |
| Milky Way | 2 (2 / 0) | lead section |
| Minimum orbit intersection distance | 2 (0 / 2) | lead section |
| Minor planet | 2 (0 / 2) | lead section |
| Miyake event | 2 (0 / 2) | lead section |
| Modern physics | 2 (0 / 2) | lead section |
| Molecule | 2 (2 / 0) | lead section |
| Moon | 2 (2 / 0) | lead section |
| Moons of Jupiter | 2 (2 / 0) | lead section |
| Moons of Neptune | 2 (0 / 2) | lead section |
| Moons of Saturn | 2 (2 / 0) | lead section |
| Moons of Uranus | 2 (0 / 2) | lead section |
| Mud cracks on Mars | 2 (2 / 0) | lead section |
| M–sigma relation | 2 (0 / 2) | lead section |
| Natural product | 2 (0 / 2) | lead section |
| Navarro–Frenk–White profile | 2 (0 / 2) | lead section |
| Near-Earth object | 2 (2 / 0) | lead section |
| Nebula | 2 (2 / 0) | lead section |
| Nemesis (hypothetical star) | 2 (0 / 2) | lead section |
| Neptune | 2 (2 / 0) | lead section |
| Neutron star | 2 (2 / 0) | lead section |
| Nili Fossae | 2 (2 / 0) | full article |
| Nordtvedt effect | 2 (0 / 2) | lead section |
| Nucleation | 2 (0 / 2) | lead section |
| Ocean color | 2 (0 / 2) | lead section |
| Ocean heat content | 2 (0 / 2) | lead section |
| Octavia E. Butler Landing | 2 (2 / 0) | full article |
| Optics | 2 (2 / 0) | lead section |
| Palynology | 2 (0 / 2) | lead section |
| Parsec | 2 (2 / 0) | lead section |
| Periodic Bedrock Ridges | 2 (2 / 0) | lead section |
| Periodic table | 2 (2 / 0) | lead section |
| Phobos monolith | 2 (0 / 2) | lead section |
| Phoenix (spacecraft) | 2 (2 / 0) | lead section |
| Photometry (astronomy) | 2 (0 / 2) | lead section |
| Physical cosmology | 2 (0 / 2) | lead section |
| Planck units | 2 (0 / 2) | lead section |
| Planet Nine | 2 (0 / 2) | lead section |
| Planetary mass | 2 (0 / 2) | lead section |
| Planetary science | 2 (2 / 0) | lead section |
| Plasma (physics) | 2 (0 / 2) | lead section |
| Plasmaron | 2 (0 / 2) | lead section |
| Plate tectonics | 2 (2 / 0) | lead section |
| Pluto | 2 (2 / 0) | lead section |
| Polytrope | 2 (0 / 2) | lead section |
| Precovery | 2 (0 / 2) | lead section |
| PROMISE (rover) | 2 (2 / 0) | full article |
| PrOP-M | 2 (2 / 0) | full article |
| Protein | 2 (2 / 0) | lead section |
| Pulsed accretion | 2 (0 / 2) | lead section |
| Quantum mechanics | 2 (2 / 0) | lead section |
| Quasar | 2 (2 / 0) | lead section |
| Radio Recombination Lines | 2 (0 / 2) | lead section |
| Radioactive decay | 2 (2 / 0) | lead section |
| Rain-out model | 2 (0 / 2) | lead section |
| Rampart crater | 2 (2 / 0) | lead section |
| Red giant | 2 (2 / 0) | lead section |
| Redshift | 2 (2 / 0) | lead section |
| Relativistic beaming | 2 (0 / 2) | lead section |
| RIMFAX | 2 (2 / 0) | full article |
| Ring mold crater | 2 (2 / 0) | lead section |
| Rings of Saturn | 2 (2 / 0) | lead section |
| Robert Zubrin | 2 (2 / 0) | lead section |
| Rock Abrasion Tool | 2 (2 / 0) | full article |
| Rocknest (Mars) | 2 (2 / 0) | full article |
| Rover Environmental Monitoring Station | 2 (2 / 0) | full article |
| Runaway greenhouse effect | 2 (2 / 0) | lead section |
| S-process | 2 (0 / 2) | lead section |
| Sadler effect | 2 (0 / 2) | lead section |
| Saturn | 2 (2 / 0) | lead section |
| Scattered disc | 2 (2 / 0) | lead section |
| Schönberg–Chandrasekhar limit | 2 (0 / 2) | lead section |
| Scientific method | 2 (2 / 0) | lead section |
| Sedna (dwarf planet) | 2 (0 / 2) | lead section |
| Sednoid | 2 (0 / 2) | lead section |
| Shock waves in astrophysics | 2 (0 / 2) | lead section |
| Small Deep Space Transponder | 2 (2 / 0) | full article |
| Small planet radius gap | 2 (0 / 2) | lead section |
| Solar eclipse | 2 (2 / 0) | lead section |
| Solar irradiance | 2 (0 / 2) | lead section |
| Solar System model | 2 (0 / 2) | lead section |
| Solar wind | 2 (2 / 0) | lead section |
| Source function | 2 (0 / 2) | lead section |
| Soviet Mars program | 2 (2 / 0) | lead section |
| Space colonization | 2 (0 / 2) | lead section |
| Space exploration | 2 (0 / 2) | lead section |
| Spaceflight | 2 (0 / 2) | lead section |
| Spacewatch | 2 (0 / 2) | lead section |
| Spiral arm | 2 (0 / 2) | lead section |
| Star | 2 (2 / 0) | lead section |
| Stellar evolution | 2 (2 / 0) | lead section |
| Stellar pulsation | 2 (0 / 2) | lead section |
| Substorm | 2 (0 / 2) | lead section |
| Sun | 2 (2 / 0) | lead section |
| Supernova | 2 (2 / 0) | lead section |
| Supernova nucleosynthesis | 2 (0 / 2) | lead section |
| Superplasticizer | 2 (0 / 2) | lead section |
| Syrtis Major quadrangle | 2 (0 / 2) | lead section |
| Tasmanite (tektite) | 2 (0 / 2) | lead section |
| Tectonics of Mars | 2 (2 / 0) | lead section |
| Terrain softening | 2 (0 / 2) | lead section |
| Thalassogen | 2 (0 / 2) | lead section |
| The Mission (Styx album) | 2 (2 / 0) | lead section |
| Thermodynamics | 2 (2 / 0) | lead section |
| Tidal locking | 2 (2 / 0) | lead section |
| Tides in marginal seas | 2 (0 / 2) | lead section |
| Titan (moon) | 2 (2 / 0) | lead section |
| Tolman–Oppenheimer–Volkoff limit | 2 (0 / 2) | lead section |
| Toomre's stability criterion | 2 (0 / 2) | lead section |
| Toroidal solenoid | 2 (0 / 2) | lead section |
| Trace Gas Orbiter | 2 (2 / 0) | lead section |
| Transit of Venus | 2 (2 / 0) | lead section |
| TRAPPIST-1 | 2 (2 / 0) | lead section |
| Traverse (surveying) | 2 (0 / 2) | lead section |
| Trojan (celestial body) | 2 (0 / 2) | lead section |
| True polar wander on Mars | 2 (2 / 0) | lead section |
| Uncrewed spacecraft | 2 (0 / 2) | lead section |
| University of Hawaiʻi at Mānoa | 2 (0 / 2) | lead section |
| Uranus | 2 (2 / 0) | lead section |
| Vaccine | 2 (2 / 0) | lead section |
| Valley network (Mars) | 2 (2 / 0) | lead section |
| Venus | 2 (2 / 0) | lead section |
| Very Large Telescope | 2 (2 / 0) | lead section |
| Viking program | 2 (2 / 0) | lead section |
| Volcano | 2 (2 / 0) | lead section |
| Vulcanoid | 2 (0 / 2) | lead section |
| Weather | 2 (2 / 0) | lead section |
| White dwarf | 2 (2 / 0) | lead section |
| Woltjer's theorem | 2 (0 / 2) | lead section |
| Zeeman–Doppler imaging | 2 (0 / 2) | lead section |
| Zodiacal light | 2 (2 / 0) | lead section |
| (121514) 1999 UJ7 | 1 (1 / 0) | lead section |
| (155140) 2005 UD | 1 (1 / 0) | lead section |
| (15700) 1987 QD | 1 (1 / 0) | lead section |
| (38063) 1999 FH | 1 (0 / 1) | lead section |
| (5407) 1992 AX | 1 (1 / 0) | lead section |
| (9992) 1997 TG19 | 1 (1 / 0) | lead section |
| 1009 Sirene | 1 (1 / 0) | lead section |
| 10502 Armaghobs | 1 (1 / 0) | lead section |
| 1065 Amundsenia | 1 (1 / 0) | lead section |
| 1131 Porzia | 1 (1 / 0) | lead section |
| 1134 Kepler | 1 (1 / 0) | lead section |
| 1139 Atami | 1 (0 / 1) | lead section |
| 1170 Siva | 1 (1 / 0) | lead section |
| 1198 Atlantis | 1 (1 / 0) | lead section |
| 1204 Renzia | 1 (1 / 0) | lead section |
| 1235 Schorria | 1 (1 / 0) | lead section |
| 1310 Villigera | 1 (0 / 1) | lead section |
| 1316 Kasan | 1 (1 / 0) | lead section |
| 132 Aethra | 1 (1 / 0) | lead section |
| 1374 Isora | 1 (0 / 1) | lead section |
| 142 Polana | 1 (1 / 0) | lead section |
| 1468 Zomba | 1 (1 / 0) | lead section |
| 1474 Beira | 1 (1 / 0) | lead section |
| 1565 Lemaître | 1 (1 / 0) | lead section |
| 1656 Suomi | 1 (1 / 0) | lead section |
| 1727 Mette | 1 (0 / 1) | lead section |
| 1747 Wright | 1 (0 / 1) | lead section |
| 1750 Eckert | 1 (0 / 1) | lead section |
| 19982 Barbaradoore | 1 (1 / 0) | lead section |
| 1MV | 1 (1 / 0) | lead section |
| 2007 WD5 | 1 (1 / 0) | lead section |
| 2014 MV67 | 1 (1 / 0) | lead section |
| 2023 FW14 | 1 (1 / 0) | lead section |
| 2035 Stearns | 1 (1 / 0) | lead section |
| 2044 Wirt | 1 (0 / 1) | lead section |
| 2064 Thomsen | 1 (0 / 1) | lead section |
| 2074 Shoemaker | 1 (0 / 1) | lead section |
| 2204 Lyyli | 1 (1 / 0) | lead section |
| 2253 Espinette | 1 (1 / 0) | lead section |
| 2423 Ibarruri | 1 (1 / 0) | lead section |
| 2449 Kenos | 1 (0 / 1) | lead section |
| 2629 Rudra | 1 (1 / 0) | lead section |
| 26858 Misterrogers | 1 (1 / 0) | lead section |
| 2744 Birgitta | 1 (1 / 0) | lead section |
| 2937 Gibbs | 1 (1 / 0) | lead section |
| 2cDM model of dark matter | 1 (0 / 1) | lead section |
| 3 Juno | 1 (0 / 1) | lead section |
| 3040 Kozai | 1 (1 / 0) | lead section |
| 3200 Phaethon | 1 (1 / 0) | lead section |
| 323 Brucia | 1 (0 / 1) | lead section |
| 3255 Tholen | 1 (1 / 0) | lead section |
| 3267 Glo | 1 (1 / 0) | lead section |
| 3343 Nedzel | 1 (1 / 0) | lead section |
| 3401 Vanphilos | 1 (0 / 1) | lead section |
| 3402 Wisdom | 1 (1 / 0) | lead section |
| 3581 Alvarez | 1 (1 / 0) | lead section |
| 3635 Kreutz | 1 (0 / 1) | lead section |
| 3674 Erbisbühl | 1 (0 / 1) | lead section |
| 3737 Beckman | 1 (1 / 0) | lead section |
| 3800 Karayusuf | 1 (1 / 0) | lead section |
| 3854 George | 1 (1 / 0) | lead section |
| 3873 Roddy | 1 (1 / 0) | lead section |
| 39741 Komm | 1 (1 / 0) | lead section |
| 4142 Dersu-Uzala | 1 (1 / 0) | lead section |
| 4205 David Hughes | 1 (0 / 1) | lead section |
| 4276 Clifford | 1 (1 / 0) | lead section |
| 4435 Holt | 1 (1 / 0) | lead section |
| 4451 Grieve | 1 (1 / 0) | lead section |
| 4587 Rees | 1 (1 / 0) | lead section |
| 512 Taurinensis | 1 (1 / 0) | lead section |
| 5335 Damocles | 1 (0 / 1) | lead section |
| 5641 McCleese | 1 (1 / 0) | lead section |
| 5642 Bobbywilliams | 1 (1 / 0) | lead section |
| 6042 Cheshirecat | 1 (0 / 1) | lead section |
| 61 Virginis b | 1 (0 / 1) | lead section |
| 6141 Durda | 1 (0 / 1) | lead section |
| 6170 Levasseur | 1 (1 / 0) | lead section |
| 6500 Kodaira | 1 (1 / 0) | lead section |
| 699 Hela | 1 (1 / 0) | lead section |
| 7369 Gavrilin | 1 (0 / 1) | lead section |
| 7505 Furusho | 1 (1 / 0) | lead section |
| 7604 Kridsadaporn | 1 (0 / 1) | lead section |
| 7816 Hanoi | 1 (1 / 0) | lead section |
| 9564 Jeffwynn | 1 (1 / 0) | lead section |
| 96P sungrazer family | 1 (0 / 1) | lead section |
| 9969 Braille | 1 (0 / 1) | lead section |
| Abdullah Alamri | 1 (0 / 1) | lead section |
| Acheron Fossae | 1 (1 / 0) | lead section |
| Achondrite | 1 (0 / 1) | lead section |
| Actinide chemistry | 1 (0 / 1) | lead section |
| Active asteroid | 1 (0 / 1) | lead section |
| Aerial Regional-scale Environmental Survey | 1 (1 / 0) | lead section |
| AIC Judd Award | 1 (0 / 1) | lead section |
| Alaknanda Galaxy | 1 (0 / 1) | lead section |
| Algorithm | 1 (1 / 0) | lead section |
| Allan Hills 77005 | 1 (1 / 0) | lead section |
| Allan Hills 84001 | 1 (1 / 0) | lead section |
| Amateur chemistry | 1 (0 / 1) | lead section |
| Amazonian (Mars) | 1 (1 / 0) | lead section |
| Amazonis quadrangle | 1 (0 / 1) | lead section |
| Amenthes Fossae | 1 (1 / 0) | lead section |
| Amenthes quadrangle | 1 (0 / 1) | lead section |
| Amorphous carbonia | 1 (0 / 1) | lead section |
| Andean dark constellations | 1 (0 / 1) | lead section |
| Angular momentum problem | 1 (0 / 1) | lead section |
| Aonia Mons | 1 (1 / 0) | lead section |
| Applegate mechanism | 1 (0 / 1) | lead section |
| Arabia quadrangle | 1 (1 / 0) | lead section |
| Arctic Mars Analog Svalbard Expedition | 1 (1 / 0) | lead section |
| Arens–van Dorp synthesis | 1 (0 / 1) | lead section |
| Areocentric orbit | 1 (1 / 0) | lead section |
| Areography | 1 (1 / 0) | lead section |
| Areostationary orbit | 1 (1 / 0) | lead section |
| Argyre quadrangle | 1 (1 / 0) | lead section |
| Ariadnes Colles | 1 (1 / 0) | lead section |
| ARIANNA Experiment | 1 (0 / 1) | lead section |
| Arnus Vallis | 1 (1 / 0) | lead section |
| Arsia Chasmata | 1 (1 / 0) | lead section |
| Ashen light | 1 (0 / 1) | lead section |
| Asteroid mining | 1 (0 / 1) | lead section |
| Asteroseismology | 1 (0 / 1) | lead section |
| Astrobiophysics | 1 (0 / 1) | lead section |
| Astrochemistry | 1 (0 / 1) | lead section |
| Astroinformatics | 1 (0 / 1) | lead section |
| Astronomer | 1 (0 / 1) | lead section |
| Astronomical transit | 1 (1 / 0) | lead section |
| Astronomical unit | 1 (1 / 0) | lead section |
| Astronomy | 1 (0 / 1) | lead section |
| Astronomy & Geophysics | 1 (0 / 1) | lead section |
| Astrophysical fluid dynamics | 1 (0 / 1) | lead section |
| Astrostatistics | 1 (0 / 1) | lead section |
| Astrotourism | 1 (0 / 1) | lead section |
| Atlantis Chaos | 1 (1 / 0) | lead section |
| Atlas of Terrestrial Group Planets and their Moons | 1 (0 / 1) | lead section |
| Atmospheric chemistry | 1 (0 / 1) | lead section |
| Atmospheric Chemistry Suite | 1 (1 / 0) | lead section |
| Atominstitute | 1 (0 / 1) | lead section |
| Aufeis | 1 (0 / 1) | lead section |
| Auqakuh Vallis | 1 (1 / 0) | lead section |
| Aurora | 1 (0 / 1) | lead section |
| Aurora on Mars | 1 (0 / 1) | lead section |
| Aurora programme | 1 (1 / 0) | lead section |
| Auroral kilometric radiation | 1 (0 / 1) | lead section |
| Austere Human Missions to Mars | 1 (1 / 0) | lead section |
| Australasian strewnfield | 1 (0 / 1) | lead section |
| Australe Montes | 1 (1 / 0) | lead section |
| Australian Journal of Earth Sciences | 1 (0 / 1) | lead section |
| Austrian Space Forum | 1 (1 / 0) | lead section |
| Avernus Colles | 1 (1 / 0) | lead section |
| Axial tilt | 1 (0 / 1) | lead section |
| Axis of evil (cosmology) | 1 (0 / 1) | lead section |
| B2FH paper | 1 (0 / 1) | lead section |
| B612 Foundation | 1 (0 / 1) | lead section |
| Bagnold Dunes | 1 (1 / 0) | full article |
| Bahcall–Wolf cusp | 1 (0 / 1) | lead section |
| Bahram Vallis | 1 (1 / 0) | lead section |
| Bancroft Award | 1 (0 / 1) | lead section |
| Barnacle Bill (Martian rock) | 1 (1 / 0) | lead section |
| Bathurst Inlet (rock) | 1 (1 / 0) | full article |
| Beagle 2 | 1 (1 / 0) | lead section |
| Beagle 3 | 1 (1 / 0) | lead section |
| Bedford Level experiment | 1 (0 / 1) | lead section |
| Benzimidazolone pigments | 1 (0 / 1) | lead section |
| Bi-scalar tensor vector gravity | 1 (0 / 1) | lead section |
| Biblis Tholus | 1 (1 / 0) | lead section |
| Biermann battery | 1 (0 / 1) | lead section |
| Biliprotein | 1 (0 / 1) | lead section |
| Bioactive terrarium | 1 (0 / 1) | lead section |
| Bioconcentration | 1 (0 / 1) | lead section |
| Biological constraints | 1 (0 / 1) | lead section |
| Biological Oxidant and Life Detection | 1 (1 / 0) | lead section |
| Biologist | 1 (0 / 1) | lead section |
| Biology | 1 (1 / 0) | lead section |
| Biology of romantic love | 1 (0 / 1) | lead section |
| Biophysical chemistry | 1 (0 / 1) | lead section |
| Bittern (salt) | 1 (0 / 1) | lead section |
| Blast wave | 1 (0 / 1) | lead section |
| Bonestell (crater) | 1 (1 / 0) | lead section |
| Bosporos Planum | 1 (1 / 0) | lead section |
| Bounce Rock | 1 (0 / 1) | lead section |
| Bow shock | 1 (0 / 1) | lead section |
| Bryan Versteeg | 1 (1 / 0) | lead section |
| Building block (chemistry) | 1 (0 / 1) | lead section |
| C/2013 A1 (Siding Spring) | 1 (0 / 1) | lead section |
| C1 chemistry | 1 (0 / 1) | lead section |
| Calconcarboxylic acid | 1 (0 / 1) | lead section |
| Calculus | 1 (1 / 0) | lead section |
| California Volcano Observatory | 1 (0 / 1) | lead section |
| Calorimetric Electron Telescope | 1 (0 / 1) | lead section |
| Caloris Planitia | 1 (1 / 0) | lead section |
| Cancer exodus hypothesis | 1 (0 / 1) | lead section |
| Carbodiphosphoranes | 1 (0 / 1) | lead section |
| Carbon planet | 1 (0 / 1) | lead section |
| Carbonates on Mars | 1 (1 / 0) | lead section |
| Carryover effect | 1 (0 / 1) | lead section |
| Cascades Volcano Observatory | 1 (0 / 1) | lead section |
| Casius quadrangle | 1 (1 / 0) | lead section |
| Cassini's laws | 1 (0 / 1) | lead section |
| Causal dynamical triangulation | 1 (0 / 1) | lead section |
| Caves of Mars Project | 1 (1 / 0) | lead section |
| CDG-2 | 1 (0 / 1) | lead section |
| Cebrenia quadrangle | 1 (1 / 0) | lead section |
| Celestial police | 1 (0 / 1) | lead section |
| Celestial sphere | 1 (1 / 0) | lead section |
| Centauri Montes | 1 (1 / 0) | lead section |
| Centro de Estudios de Fisica del Cosmos de Aragon | 1 (0 / 1) | lead section |
| Chalce Montes | 1 (1 / 0) | lead section |
| Chandrasekhar limit | 1 (0 / 1) | lead section |
| Chandrasekhar number | 1 (0 / 1) | lead section |
| Chandrasekhar polarization | 1 (0 / 1) | lead section |
| Chandrasekhar potential energy tensor | 1 (0 / 1) | lead section |
| Chandrasekhar–Fermi method | 1 (0 / 1) | lead section |
| Chandrasekhar–Friedman–Schutz instability | 1 (0 / 1) | lead section |
| Chaotic rotation | 1 (0 / 1) | lead section |
| Charged aerosol detector | 1 (0 / 1) | lead section |
| Chasma | 1 (1 / 0) | lead section |
| Chasma Boreale | 1 (1 / 0) | lead section |
| Chassigny (meteorite) | 1 (1 / 0) | lead section |
| Chemical bath deposition | 1 (0 / 1) | lead section |
| Chemical biology | 1 (0 / 1) | lead section |
| Chemical cycling | 1 (0 / 1) | lead section |
| Chemical equation | 1 (0 / 1) | lead section |
| Chemical free | 1 (0 / 1) | lead section |
| Chemical library | 1 (0 / 1) | lead section |
| Chemical similarity | 1 (0 / 1) | lead section |
| Chemical state | 1 (0 / 1) | lead section |
| Chemical synthesis | 1 (0 / 1) | lead section |
| Chemical technologist | 1 (0 / 1) | lead section |
| Chemistry | 1 (1 / 0) | lead section |
| Chemoproteomics | 1 (0 / 1) | lead section |
| Chirgwin–Coulson weights | 1 (0 / 1) | lead section |
| Chloride-bearing deposits on Mars | 1 (0 / 1) | lead section |
| Chlororespiration | 1 (0 / 1) | lead section |
| Chondritic uniform reservoir | 1 (0 / 1) | lead section |
| Chromogen | 1 (0 / 1) | lead section |
| Chronology | 1 (0 / 1) | lead section |
| Chronology of discoveries of water on Mars | 1 (1 / 0) | lead section |
| Chryse Alien | 1 (1 / 0) | lead section |
| CircumArctic Rangifer Monitoring and Assessment Network | 1 (0 / 1) | lead section |
| Clandestine chemistry | 1 (0 / 1) | lead section |
| Climate system | 1 (0 / 1) | lead section |
| CLUPI | 1 (1 / 0) | lead section |
| CNEOS 2014-01-08 | 1 (0 / 1) | lead section |
| Collision-induced absorption and emission | 1 (0 / 1) | lead section |
| Colloidal probe technique | 1 (0 / 1) | lead section |
| Community Surface Dynamics Modeling System | 1 (0 / 1) | lead section |
| Comparative planetary science | 1 (0 / 1) | lead section |
| Comparison of embedded computer systems on board the Mars rovers | 1 (1 / 0) | full article |
| Compliance constants | 1 (0 / 1) | lead section |
| Compound Interest (website) | 1 (0 / 1) | lead section |
| Compton scattering | 1 (0 / 1) | lead section |
| Compton telescope | 1 (0 / 1) | lead section |
| Computational astrophysics | 1 (0 / 1) | lead section |
| Concentric crater fill | 1 (1 / 0) | lead section |
| Coprates quadrangle | 1 (1 / 0) | lead section |
| Core-powered mass loss | 1 (0 / 1) | lead section |
| Core–shell semiconductor nanocrystal | 1 (0 / 1) | lead section |
| Corona | 1 (1 / 0) | lead section |
| Coronae Montes | 1 (1 / 0) | lead section |
| Coronal loop | 1 (0 / 1) | lead section |
| CoRoT-7b | 1 (0 / 1) | lead section |
| Corrosion inhibitors for the petroleum industry | 1 (0 / 1) | lead section |
| Cosmic ray astronomy | 1 (0 / 1) | lead section |
| Cosmic shoreline | 1 (0 / 1) | lead section |
| Cosmochemistry | 1 (0 / 1) | lead section |
| Craig Chester (astronomer) | 1 (0 / 1) | lead section |
| Craters of the Moon | 1 (1 / 0) | lead section |
| Critical ionization velocity | 1 (0 / 1) | lead section |
| Crocco's Multiplanetary Trajectory | 1 (1 / 0) | lead section |
| Crossover experiment (chemistry) | 1 (0 / 1) | lead section |
| Crystallography | 1 (0 / 1) | lead section |
| Cyane Fossae | 1 (1 / 0) | lead section |
| Cyclosiloxane | 1 (0 / 1) | lead section |
| Dao Vallis | 1 (1 / 0) | lead section |
| Darian calendar | 1 (1 / 0) | lead section |
| Dark fluid | 1 (0 / 1) | lead section |
| Dark oxygen | 1 (0 / 1) | lead section |
| David Sobral | 1 (0 / 1) | lead section |
| De Laval nozzle | 1 (0 / 1) | lead section |
| De Sitter effect | 1 (0 / 1) | lead section |
| Debrecen Heliophysical Observatory | 1 (0 / 1) | lead section |
| Decay technique | 1 (0 / 1) | lead section |
| Deep Space 2 | 1 (1 / 0) | lead section |
| Deep Space Transport | 1 (1 / 0) | lead section |
| Definition of planet | 1 (1 / 0) | lead section |
| Deformation bands | 1 (1 / 0) | lead section |
| Deimos (moon) | 1 (1 / 0) | lead section |
| Deimos and Phobos Interior Explorer | 1 (1 / 0) | lead section |
| DePriester chart | 1 (0 / 1) | lead section |
| Depth in a well | 1 (0 / 1) | lead section |
| Dermestarium | 1 (0 / 1) | lead section |
| Desert planet | 1 (0 / 1) | lead section |
| Diacria quadrangle | 1 (1 / 0) | lead section |
| Differential Doppler effect | 1 (0 / 1) | lead section |
| Digital elevation model | 1 (0 / 1) | lead section |
| Direct reduction | 1 (0 / 1) | lead section |
| Dirichlet's ellipsoidal problem | 1 (0 / 1) | lead section |
| Dissociative recombination | 1 (0 / 1) | lead section |
| Disturbance storm time index | 1 (0 / 1) | lead section |
| Dungey Cycle | 1 (0 / 1) | lead section |
| Dust astronomy | 1 (0 / 1) | lead section |
| Dusty plasma | 1 (0 / 1) | lead section |
| Dwarf planet | 1 (1 / 0) | lead section |
| Dynamical friction | 1 (0 / 1) | lead section |
| Dysnomia (moon) | 1 (0 / 1) | lead section |
| Earth ellipsoid | 1 (0 / 1) | lead section |
| Earth science | 1 (0 / 1) | lead section |
| Earth Science Decadal Survey | 1 (0 / 1) | lead section |
| Earth Similarity Index | 1 (0 / 1) | lead section |
| Earth trojan | 1 (0 / 1) | lead section |
| Earth's crustal evolution | 1 (0 / 1) | lead section |
| Eddington Medal | 1 (0 / 1) | lead section |
| Eddington number | 1 (0 / 1) | lead section |
| Eden Patera | 1 (1 / 0) | lead section |
| Effective temperature | 1 (0 / 1) | lead section |
| Effects of Planet Nine on trans-Neptunian objects | 1 (0 / 1) | lead section |
| Ejecta | 1 (0 / 1) | lead section |
| El Capitan (Mars) | 1 (0 / 1) | lead section |
| Electris deposits | 1 (1 / 0) | lead section |
| Electrolysed water | 1 (0 / 1) | lead section |
| Electrostatic solitary wave | 1 (0 / 1) | lead section |
| Elephant Moraine 79001 | 1 (0 / 1) | lead section |
| Elephant trunk (astronomy) | 1 (0 / 1) | lead section |
| Elysium (volcanic province) | 1 (1 / 0) | lead section |
| Elysium quadrangle | 1 (1 / 0) | lead section |
| Empirical evidence for the spherical shape of Earth | 1 (0 / 1) | lead section |
| Endogeny (biology) | 1 (0 / 1) | lead section |
| Enduring Quests and Daring Visions | 1 (0 / 1) | lead section |
| Energy | 1 (1 / 0) | lead section |
| Environmental chemistry | 1 (0 / 1) | lead section |
| Environmental science | 1 (0 / 1) | lead section |
| Eos Chasma | 1 (1 / 0) | lead section |
| Epicentral distance | 1 (0 / 1) | lead section |
| Equatorial bulge | 1 (0 / 1) | lead section |
| Eridania Lake | 1 (1 / 0) | lead section |
| Eridania Planitia | 1 (1 / 0) | lead section |
| Eridania quadrangle | 1 (1 / 0) | lead section |
| Erinacin | 1 (0 / 1) | lead section |
| Eucrite | 1 (0 / 1) | lead section |
| European Solar Telescope | 1 (0 / 1) | lead section |
| Europlanet | 1 (0 / 1) | lead section |
| Evidence of water on Mars found by Mars Reconnaissance Orbiter | 1 (1 / 0) | lead section |
| Exometeorology | 1 (0 / 1) | lead section |
| ExoMol | 1 (0 / 1) | lead section |
| Exoplanet Explorers | 1 (0 / 1) | lead section |
| Experience Curiosity | 1 (1 / 0) | full article |
| Exploration of Mars | 1 (1 / 0) | lead section |
| Extragalactic cosmic ray | 1 (0 / 1) | lead section |
| Extraterrestrial atmosphere | 1 (0 / 1) | lead section |
| Extraterrestrial materials | 1 (0 / 1) | lead section |
| Extraterrestrial sample curation | 1 (0 / 1) | lead section |
| Extraterrestrial Sample Curation Center | 1 (0 / 1) | lead section |
| Extraterrestrial sky | 1 (0 / 1) | lead section |
| Extreme trans-Neptunian object | 1 (0 / 1) | lead section |
| Fermi Gamma-ray Space Telescope | 1 (0 / 1) | lead section |
| Ferric hydroxysulfate | 1 (0 / 1) | lead section |
| Field effect (chemistry) | 1 (0 / 1) | lead section |
| Fifth Giant | 1 (0 / 1) | lead section |
| Fine-Resolution Epithermal Neutron Detector | 1 (1 / 0) | lead section |
| Firehose instability | 1 (0 / 1) | lead section |
| First point of Aries | 1 (0 / 1) | lead section |
| Fiske Planetarium | 1 (0 / 1) | lead section |
| Five-planet Nice model | 1 (0 / 1) | lead section |
| Fluvioglacial landform | 1 (0 / 1) | lead section |
| Flux transfer event | 1 (0 / 1) | lead section |
| Fobos-Grunt | 1 (1 / 0) | lead section |
| Forensic chemistry | 1 (0 / 1) | lead section |
| Fractal cosmology | 1 (0 / 1) | lead section |
| Fragmentomics | 1 (0 / 1) | lead section |
| Francesca E. DeMeo | 1 (0 / 1) | lead section |
| Free element | 1 (0 / 1) | lead section |
| Free-return trajectory | 1 (1 / 0) | lead section |
| Frenesy (physics) | 1 (0 / 1) | lead section |
| Frento Vallis | 1 (1 / 0) | lead section |
| Frequency separation | 1 (0 / 1) | lead section |
| Frost line (astrophysics) | 1 (0 / 1) | lead section |
| Galactic Bridges and Tails | 1 (0 / 1) | lead section |
| Galactic Center | 1 (1 / 0) | lead section |
| Galaxias Fossae | 1 (1 / 0) | lead section |
| Galaxius Mons | 1 (1 / 0) | lead section |
| Galaxy cluster | 1 (1 / 0) | lead section |
| Gauge vector–tensor gravity | 1 (0 / 1) | lead section |
| General Coordinates Network | 1 (0 / 1) | lead section |
| GEOBASE | 1 (0 / 1) | lead section |
| Geochemistry | 1 (0 / 1) | lead section |
| Geodesy | 1 (0 / 1) | lead section |
| Geology of Mars | 1 (1 / 0) | lead section |
| Geomechanics | 1 (0 / 1) | lead section |
| Geomorphology | 1 (0 / 1) | lead section |
| GeoNet (New Zealand) | 1 (0 / 1) | lead section |
| Geophysical definition of planet | 1 (0 / 1) | lead section |
| Geoscience education | 1 (0 / 1) | lead section |
| Geoscientist (magazine) | 1 (0 / 1) | lead section |
| Gerard 't Hooft | 1 (1 / 0) | lead section |
| Geryon Montes | 1 (1 / 0) | lead section |
| Giant impacts phase of planetary formation | 1 (0 / 1) | lead section |
| Giuseppe Donatiello | 1 (0 / 1) | lead section |
| Glass with embedded metal and sulfides | 1 (0 / 1) | lead section |
| Glenelg, Mars | 1 (1 / 0) | full article |
| Gliese 15 Ab | 1 (0 / 1) | lead section |
| Gliese 176 b | 1 (0 / 1) | lead section |
| Gliese 486 b | 1 (0 / 1) | lead section |
| Gliese 581e | 1 (0 / 1) | lead section |
| Gliese 876 d | 1 (0 / 1) | lead section |
| Global Boundary Stratotype Section and Point | 1 (0 / 1) | lead section |
| Glossary of astronomy | 1 (0 / 1) | lead section |
| Glossary of chemistry terms | 1 (0 / 1) | lead section |
| GNS Science | 1 (0 / 1) | lead section |
| Goldschmidt classification | 1 (0 / 1) | lead section |
| Goulburn (Mars) | 1 (1 / 0) | full article |
| Grand tack hypothesis | 1 (0 / 1) | lead section |
| Granicus Valles | 1 (1 / 0) | lead section |
| Gravitational scattering | 1 (0 / 1) | lead section |
| Gravitational self-force | 1 (0 / 1) | lead section |
| Gravity of Mars | 1 (0 / 1) | lead section |
| GravitySimulator | 1 (0 / 1) | lead section |
| Great Red Spot | 1 (1 / 0) | lead section |
| Green chemistry | 1 (0 / 1) | lead section |
| Grey atmosphere | 1 (0 / 1) | lead section |
| Groundwater on Mars | 1 (1 / 0) | lead section |
| Grupo de Astronomía y Ciencias del Espacio | 1 (0 / 1) | lead section |
| Grupo Fertiberia | 1 (0 / 1) | lead section |
| Gusev | 1 (1 / 0) | full article |
| Habitability, Brine Irradiation and Temperature | 1 (0 / 1) | lead section |
| Hadriacus Mons | 1 (1 / 0) | lead section |
| Half-month | 1 (0 / 1) | lead section |
| Harmakhis Vallis | 1 (1 / 0) | lead section |
| Harvard Plate Stacks | 1 (0 / 1) | lead section |
| Hawking radiation | 1 (0 / 1) | lead section |
| HD 181433 b | 1 (0 / 1) | lead section |
| HD 215497 b | 1 (0 / 1) | lead section |
| HD 219134 b | 1 (0 / 1) | lead section |
| HD 7924 b | 1 (0 / 1) | lead section |
| Heat Shield Rock | 1 (1 / 0) | lead section |
| HED meteorite | 1 (0 / 1) | lead section |
| Heinlein (crater) | 1 (1 / 0) | lead section |
| Heliophysics | 1 (0 / 1) | lead section |
| Hellas Montes | 1 (1 / 0) | lead section |
| Hellas quadrangle | 1 (1 / 0) | lead section |
| Hellespontus Montes | 1 (1 / 0) | lead section |
| Hephaestus Fossae | 1 (1 / 0) | lead section |
| Her Desher Vallis | 1 (1 / 0) | lead section |
| Hera (space mission) | 1 (1 / 0) | lead section |
| Hereford Arizona Observatory | 1 (0 / 1) | lead section |
| High Altitude Observatory | 1 (0 / 1) | lead section |
| High energy density physics | 1 (0 / 1) | lead section |
| High Resolution Stereo Camera | 1 (1 / 0) | lead section |
| Highly charged ion | 1 (0 / 1) | lead section |
| Hills cloud | 1 (0 / 1) | lead section |
| HiRISE | 1 (1 / 0) | lead section |
| Historical models of the Solar System | 1 (0 / 1) | lead section |
| History of Solar System formation and evolution hypotheses | 1 (0 / 1) | lead section |
| History of synthetic-aperture radar | 1 (0 / 1) | lead section |
| Hot Jupiter | 1 (1 / 0) | lead section |
| Hottah (Mars) | 1 (1 / 0) | full article |
| Hrad Vallis | 1 (1 / 0) | lead section |
| Hubble–Reynolds law | 1 (0 / 1) | lead section |
| Huihui Lifa | 1 (0 / 1) | lead section |
| Human spaceflight programs | 1 (0 / 1) | lead section |
| HUN-REN Wigner Research Centre for Physics | 1 (0 / 1) | lead section |
| Hunveyor | 1 (0 / 1) | lead section |
| Huo Hsing Vallis | 1 (1 / 0) | lead section |
| Hydraotes Chaos | 1 (1 / 0) | lead section |
| Hydrogen anion | 1 (0 / 1) | lead section |
| Hyperspectral Imager for the Coastal Ocean | 1 (0 / 1) | lead section |
| Iapygia quadrangle | 1 (1 / 0) | lead section |
| Ice cloud | 1 (1 / 0) | lead section |
| Ice giant | 1 (1 / 0) | lead section |
| Ice planet | 1 (0 / 1) | lead section |
| Icebreaker Life | 1 (1 / 0) | lead section |
| ICRANet | 1 (0 / 1) | lead section |
| Icy moonquakes | 1 (0 / 1) | lead section |
| Illustris project | 1 (0 / 1) | lead section |
| Impact events on Mars | 1 (1 / 0) | lead section |
| In situ resource utilization | 1 (1 / 0) | lead section |
| Index of Earth science articles | 1 (0 / 1) | lead section |
| Indian Mars exploration missions | 1 (1 / 0) | lead section |
| Indoloquinolizidine alkaloids | 1 (0 / 1) | lead section |
| Indus Vallis | 1 (1 / 0) | lead section |
| Inspiration Mars Foundation | 1 (1 / 0) | lead section |
| Institute for Earth & Space Exploration | 1 (0 / 1) | lead section |
| Institute of Physics Edward Appleton Medal and Prize | 1 (0 / 1) | lead section |
| Instituto de Astrofísica de Andalucía | 1 (0 / 1) | lead section |
| Internal heating | 1 (0 / 1) | lead section |
| International Mars Ice Mapper Mission | 1 (1 / 0) | lead section |
| International Polar Year | 1 (0 / 1) | lead section |
| International Year of Planet Earth | 1 (0 / 1) | lead section |
| Interplanetary magnetic field | 1 (0 / 1) | lead section |
| Interplanetary medium | 1 (1 / 0) | lead section |
| Inverted relief | 1 (1 / 0) | lead section |
| Ioliomics | 1 (0 / 1) | lead section |
| IRAP PhD Program | 1 (0 / 1) | lead section |
| IRAS 20324+4057 | 1 (0 / 1) | lead section |
| Iron catastrophe | 1 (0 / 1) | lead section |
| Iron peak | 1 (0 / 1) | lead section |
| Iron planet | 1 (0 / 1) | lead section |
| Is Mars Habitable? | 1 (1 / 0) | lead section |
| Ismenia Patera | 1 (0 / 1) | lead section |
| Jack B. Newton | 1 (0 / 1) | lead section |
| Jacobi ellipsoid | 1 (0 / 1) | lead section |
| James B. Garvin | 1 (1 / 0) | lead section |
| Jeans's theorem | 1 (0 / 1) | lead section |
| Joanna V. Clark | 1 (1 / 0) | lead section |
| Jovis Tholus | 1 (1 / 0) | lead section |
| Jupiter mass | 1 (0 / 1) | lead section |
| Jupiter's South Pole | 1 (0 / 1) | lead section |
| K2-288Bb | 1 (0 / 1) | lead section |
| Kaidun meteorite | 1 (0 / 1) | lead section |
| Kathryn's Wheel | 1 (0 / 1) | lead section |
| Kavli Prize | 1 (0 / 1) | lead section |
| Kazachok | 1 (1 / 0) | lead section |
| Kepler-10b | 1 (0 / 1) | lead section |
| Kepler-186f | 1 (1 / 0) | lead section |
| Kepler-37b | 1 (0 / 1) | lead section |
| Kepler-409b | 1 (0 / 1) | lead section |
| Kepler-59b | 1 (0 / 1) | lead section |
| Kepler-68b | 1 (0 / 1) | lead section |
| Kepler-68c | 1 (0 / 1) | lead section |
| Kepler-78b | 1 (0 / 1) | lead section |
| Kepler-9d | 1 (0 / 1) | lead section |
| Kirkhill Astronomical Pillar | 1 (0 / 1) | lead section |
| Komabayashi–Ingersoll limit | 1 (0 / 1) | lead section |
| Korolev (Martian crater) | 1 (1 / 0) | lead section |
| Kosmos 419 | 1 (1 / 0) | lead section |
| Kythira | 1 (0 / 1) | lead section |
| Labeatis Fossae | 1 (1 / 0) | lead section |
| Laboratoire atmosphères, milieux, observations spatiales | 1 (0 / 1) | lead section |
| Labou Vallis | 1 (1 / 0) | lead section |
| Ladon Valles | 1 (1 / 0) | lead section |
| Lakes on Mars | 1 (1 / 0) | lead section |
| Land change science | 1 (0 / 1) | lead section |
| Laplace plane | 1 (0 / 1) | lead section |
| LaRa | 1 (1 / 0) | lead section |
| Large Enriched Germanium Experiment for Neutrinoless BB Decay | 1 (0 / 1) | lead section |
| Larklight | 1 (1 / 0) | lead section |
| Last Chance (Mars) | 1 (1 / 0) | lead section |
| Lava planet | 1 (0 / 1) | lead section |
| Lethe Vallis | 1 (1 / 0) | lead section |
| LHS 3844 b | 1 (0 / 1) | lead section |
| Licus Vallis | 1 (1 / 0) | lead section |
| Light curve | 1 (0 / 1) | lead section |
| Light-year | 1 (1 / 0) | lead section |
| LightShip (spacecraft) | 1 (1 / 0) | lead section |
| Link (Mars) | 1 (1 / 0) | full article |
| Liquid nitrogen wash | 1 (0 / 1) | lead section |
| List of areas of chaos terrain on Mars | 1 (0 / 1) | lead section |
| List of artificial objects on Mars | 1 (1 / 0) | lead section |
| List of centaurs (small Solar System bodies) | 1 (0 / 1) | lead section |
| List of crewed Mars mission plans | 1 (1 / 0) | lead section |
| List of Earth observation satellites | 1 (0 / 1) | lead section |
| List of extraterrestrial dune fields | 1 (1 / 0) | lead section |
| List of former planets | 1 (0 / 1) | lead section |
| List of galaxies by surface brightness | 1 (0 / 1) | lead section |
| List of gravitationally rounded objects of the Solar System | 1 (0 / 1) | lead section |
| List of hypothetical Solar System objects | 1 (0 / 1) | lead section |
| List of Indian astronomical treatises | 1 (0 / 1) | lead section |
| List of Ingenuity flights | 1 (1 / 0) | full article |
| List of Labes on Mars | 1 (1 / 0) | lead section |
| List of landing ellipses on extraterrestrial bodies | 1 (1 / 0) | lead section |
| List of largest craters in the Solar System | 1 (0 / 1) | lead section |
| List of Mars landers | 1 (1 / 0) | lead section |
| List of Mars orbiters | 1 (1 / 0) | lead section |
| List of minor planets: 100001–101000 | 1 (1 / 0) | lead section |
| List of minor planets: 101001–102000 | 1 (1 / 0) | lead section |
| List of minor planets: 121001–122000 | 1 (1 / 0) | lead section |
| List of minor planets: 124001–125000 | 1 (1 / 0) | lead section |
| List of minor planets: 129001–130000 | 1 (1 / 0) | lead section |
| List of minor planets: 13001–14000 | 1 (1 / 0) | lead section |
| List of minor planets: 132001–133000 | 1 (1 / 0) | lead section |
| List of minor planets: 134001–135000 | 1 (0 / 1) | lead section |
| List of minor planets: 14001–15000 | 1 (1 / 0) | lead section |
| List of minor planets: 145001–146000 | 1 (0 / 1) | lead section |
| List of minor planets: 152001–153000 | 1 (0 / 1) | lead section |
| List of minor planets: 155001–156000 | 1 (1 / 0) | lead section |
| List of minor planets: 16001–17000 | 1 (1 / 0) | lead section |
| List of minor planets: 168001–169000 | 1 (1 / 0) | lead section |
| List of minor planets: 172001–173000 | 1 (0 / 1) | lead section |
| List of minor planets: 183001–184000 | 1 (1 / 0) | lead section |
| List of minor planets: 185001–186000 | 1 (1 / 0) | lead section |
| List of minor planets: 21001–22000 | 1 (0 / 1) | lead section |
| List of minor planets: 218001–219000 | 1 (1 / 0) | lead section |
| List of minor planets: 22001–23000 | 1 (1 / 0) | lead section |
| List of minor planets: 223001–224000 | 1 (1 / 0) | lead section |
| List of minor planets: 225001–226000 | 1 (0 / 1) | lead section |
| List of minor planets: 233001–234000 | 1 (1 / 0) | lead section |
| List of minor planets: 240001–241000 | 1 (1 / 0) | lead section |
| List of minor planets: 255001–256000 | 1 (1 / 0) | lead section |
| List of minor planets: 283001–284000 | 1 (1 / 0) | lead section |
| List of minor planets: 290001–291000 | 1 (1 / 0) | lead section |
| List of minor planets: 3001–4000 | 1 (1 / 0) | lead section |
| List of minor planets: 304001–305000 | 1 (0 / 1) | lead section |
| List of minor planets: 308001–309000 | 1 (1 / 0) | lead section |
| List of minor planets: 322001–323000 | 1 (0 / 1) | lead section |
| List of minor planets: 331001–332000 | 1 (1 / 0) | lead section |
| List of minor planets: 333001–334000 | 1 (1 / 0) | lead section |
| List of minor planets: 34001–35000 | 1 (1 / 0) | lead section |
| List of minor planets: 35001–36000 | 1 (0 / 1) | lead section |
| List of minor planets: 37001–38000 | 1 (0 / 1) | lead section |
| List of minor planets: 376001–377000 | 1 (1 / 0) | lead section |
| List of minor planets: 378001–379000 | 1 (1 / 0) | lead section |
| List of minor planets: 40001–41000 | 1 (1 / 0) | lead section |
| List of minor planets: 4001–5000 | 1 (1 / 0) | lead section |
| List of minor planets: 431001–432000 | 1 (1 / 0) | lead section |
| List of minor planets: 442001–443000 | 1 (1 / 0) | lead section |
| List of minor planets: 464001–465000 | 1 (1 / 0) | lead section |
| List of minor planets: 469001–470000 | 1 (0 / 1) | lead section |
| List of minor planets: 52001–53000 | 1 (1 / 0) | lead section |
| List of minor planets: 524001–525000 | 1 (1 / 0) | lead section |
| List of minor planets: 54001–55000 | 1 (1 / 0) | lead section |
| List of minor planets: 58001–59000 | 1 (1 / 0) | lead section |
| List of minor planets: 591001–592000 | 1 (1 / 0) | lead section |
| List of minor planets: 618001–619000 | 1 (1 / 0) | lead section |
| List of minor planets: 65001–66000 | 1 (1 / 0) | lead section |
| List of minor planets: 66001–67000 | 1 (0 / 1) | lead section |
| List of minor planets: 667001–668000 | 1 (0 / 1) | lead section |
| List of minor planets: 69001–70000 | 1 (1 / 0) | lead section |
| List of minor planets: 7001–8000 | 1 (1 / 0) | lead section |
| List of minor planets: 73001–74000 | 1 (1 / 0) | lead section |
| List of minor planets: 77001–78000 | 1 (1 / 0) | lead section |
| List of minor planets: 79001–80000 | 1 (1 / 0) | lead section |
| List of minor planets: 8001–9000 | 1 (1 / 0) | lead section |
| List of minor planets: 836001–837000 | 1 (0 / 1) | lead section |
| List of minor planets: 9001–10000 | 1 (1 / 0) | lead section |
| List of minor planets: 96001–97000 | 1 (1 / 0) | lead section |
| List of named Solar System objects | 1 (0 / 1) | lead section |
| List of oceanographic institutions and programs | 1 (0 / 1) | lead section |
| List of physiographic regions | 1 (0 / 1) | lead section |
| List of possible dwarf planets | 1 (0 / 1) | lead section |
| List of Saturn-crossing minor planets | 1 (0 / 1) | lead section |
| List of Solar System objects most distant from the Sun | 1 (0 / 1) | lead section |
| List of surface features of Mars visited by Spirit and Opportunity | 1 (1 / 0) | lead section |
| List of tallest mountains in the Solar System | 1 (0 / 1) | lead section |
| Ljubinka Nikolić | 1 (1 / 0) | lead section |
| Local Bubble | 1 (0 / 1) | lead section |
| Los Angeles (meteorite) | 1 (1 / 0) | lead section |
| Louth (crater) | 1 (1 / 0) | lead section |
| Low-Density Supersonic Decelerator | 1 (1 / 0) | lead section |
| Lucus Planum | 1 (1 / 0) | lead section |
| Lunae Palus quadrangle | 1 (1 / 0) | lead section |
| Lunar fluorescence | 1 (0 / 1) | lead section |
| Lunar mare | 1 (1 / 0) | lead section |
| Lunarcrete | 1 (1 / 0) | lead section |
| Lycus Sulci | 1 (1 / 0) | lead section |
| Maclaurin spheroid | 1 (0 / 1) | lead section |
| Mad Vallis | 1 (1 / 0) | lead section |
| Magma ocean | 1 (0 / 1) | lead section |
| Magnetic field of Mars | 1 (0 / 1) | lead section |
| Magnetic helicity | 1 (0 / 1) | lead section |
| Magnetic mirror point | 1 (0 / 1) | lead section |
| Magnetochemistry | 1 (0 / 1) | lead section |
| Magnetogravity wave | 1 (0 / 1) | lead section |
| Magnetosphere | 1 (0 / 1) | lead section |
| Magnetotellurics | 1 (0 / 1) | lead section |
| Malea Planum | 1 (1 / 0) | lead section |
| Mangala Dosha | 1 (1 / 0) | lead section |
| Mantle (geology) | 1 (1 / 0) | lead section |
| Mare Acidalium quadrangle | 1 (1 / 0) | lead section |
| Mare Australe quadrangle | 1 (1 / 0) | lead section |
| Mare Tyrrhenum quadrangle | 1 (1 / 0) | lead section |
| Mareotis Fossae | 1 (1 / 0) | lead section |
| Mariner 4 | 1 (1 / 0) | lead section |
| Mariner 6 and 7 | 1 (1 / 0) | lead section |
| Mariner 9 | 1 (1 / 0) | lead section |
| Mariner program | 1 (1 / 0) | lead section |
| Mars 1 | 1 (1 / 0) | lead section |
| Mars 2M No.522 | 1 (1 / 0) | lead section |
| Mars 2MV-3 No.1 | 1 (1 / 0) | lead section |
| Mars 4 | 1 (1 / 0) | lead section |
| Mars 5 | 1 (1 / 0) | lead section |
| Mars 6 | 1 (1 / 0) | lead section |
| Mars 7 | 1 (1 / 0) | lead section |
| Mars 96 | 1 (1 / 0) | lead section |
| Mars aircraft | 1 (1 / 0) | lead section |
| Mars analog habitat | 1 (1 / 0) | lead section |
| Mars and Beyond | 1 (1 / 0) | lead section |
| Mars atmospheric entry | 1 (1 / 0) | lead section |
| Mars Base Camp | 1 (1 / 0) | lead section |
| Mars carbon dioxide ice cloud | 1 (0 / 1) | lead section |
| Mars carbonate catastrophe | 1 (1 / 0) | lead section |
| Mars Color Imager | 1 (1 / 0) | lead section |
| Mars cycler | 1 (1 / 0) | lead section |
| Mars Design Reference Mission | 1 (1 / 0) | lead section |
| Mars Direct | 1 (1 / 0) | lead section |
| Mars Excursion Module | 1 (1 / 0) | lead section |
| Mars Exploration Joint Initiative | 1 (1 / 0) | lead section |
| Mars Exploration Program | 1 (1 / 0) | lead section |
| Mars Express | 1 (1 / 0) | lead section |
| Mars flyby | 1 (1 / 0) | lead section |
| Mars general circulation model | 1 (1 / 0) | lead section |
| Mars Global Surveyor | 1 (1 / 0) | lead section |
| Mars Gravity Biosatellite | 1 (1 / 0) | lead section |
| Mars habitat | 1 (1 / 0) | lead section |
| Mars hoax email | 1 (0 / 1) | lead section |
| Mars Institute | 1 (1 / 0) | lead section |
| Mars jar | 1 (0 / 1) | lead section |
| Mars landing | 1 (1 / 0) | lead section |
| Mars MetNet | 1 (1 / 0) | lead section |
| Mars Micro Orbiter | 1 (1 / 0) | lead section |
| Mars Microspacecraft Missions | 1 (1 / 0) | lead section |
| Mars monolith | 1 (1 / 0) | lead section |
| Mars Multispectral Imager for Subsurface Studies | 1 (1 / 0) | lead section |
| Mars Observer | 1 (1 / 0) | lead section |
| Mars ocean hypothesis | 1 (1 / 0) | lead section |
| Mars One | 1 (1 / 0) | lead section |
| Mars Orbiter Camera | 1 (1 / 0) | lead section |
| Mars Outpost | 1 (0 / 1) | lead section |
| Mars Piloted Orbital Station | 1 (1 / 0) | lead section |
| Mars Plant Experiment | 1 (1 / 0) | full article |
| Mars Polar Lander | 1 (1 / 0) | lead section |
| Mars race | 1 (1 / 0) | lead section |
| Mars regional atmospheric modeling system | 1 (1 / 0) | lead section |
| Mars Sample Recovery Helicopter | 1 (1 / 0) | lead section |
| Mars suit | 1 (1 / 0) | lead section |
| Mars surface color | 1 (0 / 1) | lead section |
| Mars Surveyor '98 | 1 (1 / 0) | lead section |
| Mars Telecommunications Orbiter | 1 (1 / 0) | lead section |
| Mars to Stay | 1 (1 / 0) | lead section |
| MARS-500 | 1 (1 / 0) | lead section |
| Mars-Aster | 1 (1 / 0) | full article |
| Mars-Grunt | 1 (1 / 0) | lead section |
| Marsification | 1 (1 / 0) | lead section |
| Marsokhod | 1 (1 / 0) | full article |
| Martian canals | 1 (1 / 0) | lead section |
| Martian chaos terrain | 1 (0 / 1) | lead section |
| Martian dust devils | 1 (0 / 1) | lead section |
| Martian language | 1 (0 / 1) | lead section |
| Martian lava tube | 1 (1 / 0) | lead section |
| Martian meteorite | 1 (1 / 0) | lead section |
| Martian Moons eXploration | 1 (1 / 0) | lead section |
| Martian packet | 1 (1 / 0) | lead section |
| Martian Piloted Complex | 1 (1 / 0) | lead section |
| Martian regolith | 1 (1 / 0) | lead section |
| Martian regolith simulant | 1 (1 / 0) | lead section |
| Martian Summer | 1 (0 / 1) | lead section |
| Martian surface | 1 (0 / 1) | lead section |
| Mary Roach | 1 (1 / 0) | lead section |
| Mass segregation (astronomy) | 1 (0 / 1) | lead section |
| Mass–metallicity relation | 1 (0 / 1) | lead section |
| Matijevic Hill | 1 (1 / 0) | lead section |
| Maʼadim Vallis | 1 (1 / 0) | lead section |
| MBR Explorer | 1 (1 / 0) | lead section |
| Mechanical hemolytic anemia | 1 (0 / 1) | lead section |
| Mechanochemistry | 1 (0 / 1) | lead section |
| MEDA | 1 (1 / 0) | full article |
| Medea hypothesis | 1 (0 / 1) | lead section |
| Medusae Fossae Formation | 1 (1 / 0) | lead section |
| Mega-Earth | 1 (0 / 1) | lead section |
| Meitei astronomy | 1 (0 / 1) | lead section |
| Memphis Facula | 1 (0 / 1) | lead section |
| Mercury's magnetic field | 1 (1 / 0) | lead section |
| Metal assisted chemical etching | 1 (0 / 1) | lead section |
| Metallicity distribution function | 1 (0 / 1) | lead section |
| Meteor shower | 1 (1 / 0) | lead section |
| Meteoroid | 1 (1 / 0) | lead section |
| Methone (moon) | 1 (0 / 1) | lead section |
| Micro-X-ray fluorescence | 1 (0 / 1) | lead section |
| Microfluidic cell culture | 1 (0 / 1) | lead section |
| MicrOmega-IR | 1 (1 / 0) | lead section |
| Micrometeorite | 1 (0 / 1) | lead section |
| Micrometeoroid | 1 (0 / 1) | lead section |
| Microscale chemistry | 1 (0 / 1) | lead section |
| Mineralogy of Mars | 1 (1 / 0) | lead section |
| Minor-planet moon | 1 (0 / 1) | lead section |
| Mission to Mars: My Vision for Space Exploration | 1 (1 / 0) | lead section |
| Mixed oxidant | 1 (0 / 1) | lead section |
| Mixture | 1 (0 / 1) | lead section |
| MOA-2007-BLG-192Lb | 1 (0 / 1) | lead section |
| Mobile mapping | 1 (0 / 1) | lead section |
| MOC Public Targeting Program | 1 (1 / 0) | lead section |
| Modified Newtonian dynamics | 1 (0 / 1) | lead section |
| Moment of inertia factor | 1 (0 / 1) | lead section |
| Monochrome astrophotography techniques | 1 (0 / 1) | lead section |
| Moons of Haumea | 1 (0 / 1) | lead section |
| Moons of Mars | 1 (0 / 1) | lead section |
| Moons of Pluto | 1 (0 / 1) | lead section |
| Morphs collaboration | 1 (0 / 1) | lead section |
| Moss meteorite | 1 (0 / 1) | lead section |
| Multi-messenger astronomy | 1 (0 / 1) | lead section |
| N-Sulfonylimine | 1 (0 / 1) | lead section |
| N165 | 1 (1 / 0) | full article |
| Nakhla meteorite | 1 (1 / 0) | lead section |
| Nakhlite | 1 (1 / 0) | lead section |
| Naktong Vallis | 1 (1 / 0) | lead section |
| Nanedi Valles | 1 (1 / 0) | lead section |
| Nanogeoscience | 1 (0 / 1) | lead section |
| NASA Design Reference Mission 3.0 | 1 (1 / 0) | lead section |
| NASA-ESA Mars Sample Return | 1 (1 / 0) | lead section |
| Natural satellite | 1 (0 / 1) | lead section |
| Navcam | 1 (1 / 0) | full article |
| Naïve physics | 1 (0 / 1) | lead section |
| Nepenthes Mensae | 1 (1 / 0) | lead section |
| Neptunian desert | 1 (0 / 1) | lead section |
| Nereidum Montes | 1 (1 / 0) | lead section |
| NetLander | 1 (1 / 0) | lead section |
| Neukum (Martian crater) | 1 (1 / 0) | lead section |
| Neuroscience | 1 (1 / 0) | lead section |
| Next Mars Orbiter | 1 (1 / 0) | lead section |
| NGC 1875 | 1 (0 / 1) | lead section |
| NGC 2525 | 1 (0 / 1) | lead section |
| Nichts von euch auf Erden | 1 (1 / 0) | lead section |
| Nilo Syrtis | 1 (1 / 0) | lead section |
| Nilokeras Scopulus | 1 (1 / 0) | lead section |
| Nirig | 1 (0 / 1) | lead section |
| Northwest Africa 16788 | 1 (1 / 0) | lead section |
| Northwest Africa 7034 | 1 (1 / 0) | lead section |
| Nottingham effect | 1 (0 / 1) | lead section |
| Nozomi (spacecraft) | 1 (1 / 0) | lead section |
| Nuclear astrophysics | 1 (0 / 1) | lead section |
| Nucleocosmochronology | 1 (0 / 1) | lead section |
| Nuker Team | 1 (0 / 1) | lead section |
| Observatory | 1 (1 / 0) | lead section |
| Ocean optics | 1 (0 / 1) | lead section |
| Ocean world | 1 (0 / 1) | lead section |
| Oceanography | 1 (0 / 1) | lead section |
| Octantis Mons | 1 (1 / 0) | lead section |
| OGLE-2005-BLG-390Lb | 1 (0 / 1) | lead section |
| OGLE-2016-BLG-1195Lb | 1 (0 / 1) | lead section |
| Olympus Mons | 1 (1 / 0) | lead section |
| Oppenheimer–Snyder model | 1 (0 / 1) | lead section |
| Orbit of Mars | 1 (1 / 0) | lead section |
| Orcus Patera | 1 (1 / 0) | lead section |
| Ore resources on Mars | 1 (1 / 0) | lead section |
| Organic chemistry | 1 (0 / 1) | lead section |
| Organoantimony chemistry | 1 (0 / 1) | lead section |
| Organolithium chemistry | 1 (0 / 1) | lead section |
| Osipkov–Merritt model | 1 (0 / 1) | lead section |
| Oti Fossae | 1 (1 / 0) | lead section |
| Outerra | 1 (1 / 0) | lead section |
| Outflow channels | 1 (1 / 0) | lead section |
| Outline of astronomy | 1 (0 / 1) | lead section |
| Outline of astrophysics | 1 (0 / 1) | lead section |
| Outline of Earth science | 1 (0 / 1) | lead section |
| Outline of Mars | 1 (1 / 0) | lead section |
| Outline of the Solar System | 1 (0 / 1) | lead section |
| Padus Vallis | 1 (1 / 0) | lead section |
| Pale Blue Dot | 1 (0 / 1) | lead section |
| Paleogeoscience | 1 (0 / 1) | lead section |
| Paleointensity | 1 (0 / 1) | lead section |
| PanCam | 1 (1 / 0) | lead section |
| Pancam | 1 (1 / 0) | lead section |
| Panguite | 1 (0 / 1) | lead section |
| Paraná Valles | 1 (1 / 0) | lead section |
| Particle deposition | 1 (0 / 1) | lead section |
| Perfect fluid | 1 (0 / 1) | lead section |
| Perpendicular paramagnetic bond | 1 (0 / 1) | lead section |
| Peryton (astronomy) | 1 (0 / 1) | lead section |
| Petrie Prize Lecture | 1 (0 / 1) | lead section |
| Phaethontis quadrangle | 1 (1 / 0) | lead section |
| Phaeton (hypothetical planet) | 1 (0 / 1) | lead section |
| Phenol sulfur transferase deficiency | 1 (0 / 1) | lead section |
| Philosophy of chemistry | 1 (0 / 1) | lead section |
| Phippsaksla | 1 (1 / 0) | lead section |
| Phlegra Dorsa | 1 (1 / 0) | lead section |
| Phobos 1 | 1 (1 / 0) | lead section |
| Phobos 2 | 1 (1 / 0) | lead section |
| Phobos And Deimos & Mars Environment | 1 (1 / 0) | lead section |
| Phobos program | 1 (1 / 0) | lead section |
| Phoenicis Lacus quadrangle | 1 (1 / 0) | lead section |
| Phootprint | 1 (1 / 0) | lead section |
| Phosphorimidazolide | 1 (0 / 1) | lead section |
| Photo-erosion | 1 (0 / 1) | lead section |
| Photo-meson | 1 (0 / 1) | lead section |
| Photochemistry | 1 (0 / 1) | lead section |
| Photodissociation region | 1 (0 / 1) | lead section |
| Photographic magnitude | 1 (0 / 1) | lead section |
| Photopharmacology | 1 (0 / 1) | lead section |
| Photosphere | 1 (1 / 0) | lead section |
| Physical geography | 1 (0 / 1) | lead section |
| Physics | 1 (1 / 0) | lead section |
| Physics of Life | 1 (0 / 1) | lead section |
| Physiographic region | 1 (0 / 1) | lead section |
| Phytochemistry | 1 (0 / 1) | lead section |
| Planet Patrol (project) | 1 (0 / 1) | lead section |
| Planet V | 1 (0 / 1) | lead section |
| Planetary cartography | 1 (0 / 1) | lead section |
| Planetary coordinate system | 1 (0 / 1) | lead section |
| Planetary core | 1 (1 / 0) | lead section |
| Planetary differentiation | 1 (0 / 1) | lead section |
| Planetary equilibrium temperature | 1 (0 / 1) | lead section |
| Planetary geology | 1 (1 / 0) | lead section |
| Planetary habitability | 1 (1 / 0) | lead section |
| Planetary habitability in the Solar System | 1 (0 / 1) | lead section |
| Planetary Instrument for X-Ray Lithochemistry | 1 (1 / 0) | full article |
| Planetary migration | 1 (1 / 0) | lead section |
| Planetary mnemonic | 1 (0 / 1) | lead section |
| Planetary Observer program | 1 (1 / 0) | lead section |
| Planetary parade | 1 (0 / 1) | lead section |
| Planetary Science Decadal Survey | 1 (0 / 1) | lead section |
| Planetary Science Institute | 1 (0 / 1) | lead section |
| Planetary system | 1 (1 / 0) | lead section |
| Planetary-mass moon | 1 (0 / 1) | lead section |
| Planetary-mass object | 1 (0 / 1) | lead section |
| Plasma parameters | 1 (0 / 1) | lead section |
| Plasma sheet | 1 (0 / 1) | lead section |
| Plasmagene | 1 (0 / 1) | lead section |
| Plastic-to-Liquid | 1 (0 / 1) | lead section |
| Plummer model | 1 (0 / 1) | lead section |
| Plutino | 1 (0 / 1) | lead section |
| Poison exon | 1 (0 / 1) | lead section |
| Polygonal patterned ground | 1 (1 / 0) | lead section |
| Polylecty | 1 (0 / 1) | lead section |
| Pot of Gold (Mars) | 1 (0 / 1) | lead section |
| Pranav Sharma | 1 (0 / 1) | lead section |
| Pre-Noachian | 1 (1 / 0) | lead section |
| Pressure-induced hydration | 1 (0 / 1) | lead section |
| Press–Schechter formalism | 1 (0 / 1) | lead section |
| Probico | 1 (0 / 1) | lead section |
| Project Boreas | 1 (1 / 0) | lead section |
| Project Eagle | 1 (1 / 0) | lead section |
| Project Mars: A Technical Tale | 1 (1 / 0) | lead section |
| Przybylski's Star | 1 (0 / 1) | lead section |
| PSR B1257+12 A | 1 (0 / 1) | lead section |
| PSR B1257+12 B | 1 (0 / 1) | lead section |
| PSR B1257+12 C | 1 (0 / 1) | lead section |
| Psyche (spacecraft) | 1 (1 / 0) | lead section |
| Pulsar | 1 (1 / 0) | lead section |
| Pycnonuclear fusion | 1 (0 / 1) | lead section |
| Q-PACE | 1 (0 / 1) | lead section |
| Quake (natural phenomenon) | 1 (0 / 1) | lead section |
| Quaoar | 1 (0 / 1) | lead section |
| Quasi-isodynamic stellarator | 1 (0 / 1) | lead section |
| Radio astronomy | 1 (1 / 0) | lead section |
| Radio Galaxy Zoo | 1 (0 / 1) | lead section |
| Radio object with continuous optical spectrum | 1 (0 / 1) | lead section |
| Radio occultation | 1 (0 / 1) | lead section |
| Radiophysical Research Institute | 1 (0 / 1) | lead section |
| Rafael Navarro-Gonzalez | 1 (1 / 0) | full article |
| Rahway Valles | 1 (1 / 0) | lead section |
| Raman Laser Spectrometer | 1 (1 / 0) | lead section |
| RAPID-L | 1 (1 / 0) | lead section |
| Raye Kass | 1 (1 / 0) | lead section |
| Rayleigh fractionation | 1 (0 / 1) | lead section |
| Reducing atmosphere | 1 (0 / 1) | lead section |
| Regional Planetary Image Facility | 1 (0 / 1) | lead section |
| Regius Professor of Astronomy (Edinburgh) | 1 (0 / 1) | lead section |
| Reionization | 1 (0 / 1) | lead section |
| Resonant trans-Neptunian object | 1 (0 / 1) | lead section |
| Retrograde and prograde motion | 1 (1 / 0) | lead section |
| Reull Vallis | 1 (1 / 0) | lead section |
| Reverse weathering | 1 (0 / 1) | lead section |
| Richtmyer–Meshkov instability | 1 (0 / 1) | lead section |
| Ring system | 1 (1 / 0) | lead section |
| Rings of Chariklo | 1 (0 / 1) | lead section |
| Rings of Earth | 1 (0 / 1) | lead section |
| Rings of Rhea | 1 (0 / 1) | lead section |
| River Styles Framework | 1 (0 / 1) | lead section |
| Roche limit | 1 (0 / 1) | lead section |
| Rock analogs for structural geology | 1 (0 / 1) | lead section |
| Rocknest 3 | 1 (1 / 0) | full article |
| Rodriguez well | 1 (1 / 0) | lead section |
| Rosetta (spacecraft) | 1 (1 / 0) | lead section |
| Rosgen Stream Classification | 1 (0 / 1) | lead section |
| Rossiter–McLaughlin effect | 1 (0 / 1) | lead section |
| Rotation and Interior Structure Experiment | 1 (1 / 0) | lead section |
| Rotation period (astronomy) | 1 (0 / 1) | lead section |
| Rubble pile | 1 (0 / 1) | lead section |
| Sabis Vallis | 1 (1 / 0) | lead section |
| Sabrina Vallis | 1 (1 / 0) | lead section |
| SAGES Legacy Unifying Globulars and GalaxieS Survey | 1 (0 / 1) | lead section |
| Sample Collection for Investigation of Mars | 1 (1 / 0) | lead section |
| Santos-Dumont (moonlet) | 1 (0 / 1) | lead section |
| Saturn's hexagon | 1 (0 / 1) | lead section |
| Scalar–tensor–vector gravity | 1 (0 / 1) | lead section |
| Scamander Vallis | 1 (1 / 0) | lead section |
| Schiaparelli EDM | 1 (1 / 0) | lead section |
| School of Molecular Sciences | 1 (0 / 1) | lead section |
| Seasonal flows on warm Martian slopes | 1 (1 / 0) | lead section |
| Sedimentation | 1 (0 / 1) | lead section |
| Sedimentology | 1 (0 / 1) | lead section |
| Seismic Experiment for Interior Structure | 1 (1 / 0) | lead section |
| Seismic oceanography | 1 (0 / 1) | lead section |
| Settling | 1 (0 / 1) | lead section |
| Shape of the atomic nucleus | 1 (0 / 1) | lead section |
| Sheikh Muszaphar Shukor | 1 (1 / 0) | lead section |
| Shockwave cosmology | 1 (0 / 1) | lead section |
| Sigma Gamma Epsilon | 1 (0 / 1) | lead section |
| Sigma-D relation | 1 (0 / 1) | lead section |
| SigMF | 1 (0 / 1) | lead section |
| Siloe Patera | 1 (1 / 0) | lead section |
| Siltation | 1 (0 / 1) | lead section |
| Simud Valles | 1 (1 / 0) | lead section |
| Sinner's circle | 1 (0 / 1) | lead section |
| Sinus Sabaeus quadrangle | 1 (1 / 0) | lead section |
| Small Solar System body | 1 (0 / 1) | lead section |
| Soil solarization | 1 (0 / 1) | lead section |
| Solar flare | 1 (1 / 0) | lead section |
| Solar longitude | 1 (0 / 1) | lead section |
| Solar observation | 1 (0 / 1) | lead section |
| Solar physics | 1 (0 / 1) | lead section |
| Solar radio emission | 1 (0 / 1) | lead section |
| Solid earth | 1 (0 / 1) | lead section |
| Solid-state electrolyte | 1 (0 / 1) | lead section |
| Songline | 1 (0 / 1) | lead section |
| Sound | 1 (1 / 0) | lead section |
| Space climate | 1 (0 / 1) | lead section |
| Space dust measurement | 1 (0 / 1) | lead section |
| Space Exploration Initiative | 1 (1 / 0) | lead section |
| Space weather | 1 (0 / 1) | lead section |
| Space weathering | 1 (0 / 1) | lead section |
| SpaceX Mars colonization program | 1 (1 / 0) | lead section |
| SpaceX Red Dragon | 1 (1 / 0) | lead section |
| Spatial biology | 1 (0 / 1) | lead section |
| Spectral slope | 1 (0 / 1) | lead section |
| Spectroscopy | 1 (1 / 0) | lead section |
| SPECULOOS-3 b | 1 (0 / 1) | lead section |
| Speleology | 1 (0 / 1) | lead section |
| Stable phosphorus radicals | 1 (0 / 1) | lead section |
| Standard solar model | 1 (0 / 1) | lead section |
| Star formation | 1 (1 / 0) | lead section |
| Stationary orbit | 1 (0 / 1) | lead section |
| Stellar archaeology | 1 (0 / 1) | lead section |
| Stellar chemistry | 1 (0 / 1) | lead section |
| Stellar engulfment | 1 (0 / 1) | lead section |
| STEVE | 1 (0 / 1) | lead section |
| Structural chemistry | 1 (0 / 1) | lead section |
| Strömgren integral | 1 (0 / 1) | lead section |
| Subglacial lakes on Mars | 1 (1 / 0) | lead section |
| Substellar object | 1 (0 / 1) | lead section |
| Sudden ionospheric disturbance | 1 (0 / 1) | lead section |
| Sulci Gordii | 1 (1 / 0) | lead section |
| Sunspot | 1 (1 / 0) | lead section |
| Super-dense water | 1 (0 / 1) | lead section |
| Super-Earth | 1 (1 / 0) | lead section |
| Superelectrophilic anion | 1 (0 / 1) | lead section |
| Supergalactic plane | 1 (0 / 1) | lead section |
| Superluminal motion | 1 (0 / 1) | lead section |
| Supra-arcade downflows | 1 (0 / 1) | lead section |
| Supramolecular chemistry | 1 (0 / 1) | lead section |
| Supramolecular coordination complex | 1 (0 / 1) | lead section |
| Surface stress | 1 (0 / 1) | lead section |
| Svein-Erik Hamran | 1 (1 / 0) | full article |
| Swift (Deimian crater) | 1 (1 / 0) | lead section |
| Swiss cheese features | 1 (1 / 0) | lead section |
| Synchronous lateral excitation | 1 (0 / 1) | lead section |
| Synodic day | 1 (0 / 1) | lead section |
| Syria Planum | 1 (1 / 0) | lead section |
| Sérsic profile | 1 (0 / 1) | lead section |
| Tanaica Montes | 1 (1 / 0) | lead section |
| Tarsus (crater) | 1 (1 / 0) | lead section |
| Telecoupling | 1 (0 / 1) | lead section |
| Telescope | 1 (1 / 0) | lead section |
| Tensor–vector–scalar gravity | 1 (0 / 1) | lead section |
| Tera-hertz Explorer | 1 (1 / 0) | lead section |
| Terra Formars (film) | 1 (1 / 0) | lead section |
| Terraforming of Mars | 1 (1 / 0) | lead section |
| Terrestrial planet | 1 (1 / 0) | lead section |
| Thais Russomano | 1 (1 / 0) | lead section |
| Tharsis | 1 (1 / 0) | lead section |
| Tharsis quadrangle | 1 (1 / 0) | lead section |
| Thaumasia Plateau | 1 (1 / 0) | lead section |
| Thaumasia quadrangle | 1 (1 / 0) | lead section |
| The Case for Mars | 1 (1 / 0) | lead section |
| The Mars Project | 1 (1 / 0) | lead section |
| The Martians (scientists) | 1 (1 / 0) | lead section |
| The Millennial Project | 1 (1 / 0) | lead section |
| The Things that Live on Mars | 1 (0 / 1) | lead section |
| The Tower (tarot card) | 1 (1 / 0) | lead section |
| Theia (hypothetical planet) | 1 (0 / 1) | lead section |
| Theoretical planetology | 1 (0 / 1) | lead section |
| Theory of relativity | 1 (1 / 0) | lead section |
| Theory of tides | 1 (0 / 1) | lead section |
| Thermal Emission Imaging System | 1 (1 / 0) | lead section |
| Thermal energy | 1 (0 / 1) | lead section |
| Tholus | 1 (0 / 1) | lead section |
| Tianwen-3 | 1 (1 / 0) | lead section |
| Tidal downsizing | 1 (0 / 1) | lead section |
| Tidal heating | 1 (0 / 1) | lead section |
| Timekeeping on Mars | 1 (1 / 0) | lead section |
| Timeline of discovery of Solar System planets and their moons | 1 (0 / 1) | lead section |
| Timeline of Earth estimates | 1 (0 / 1) | lead section |
| Timeline of Mars 2020 | 1 (1 / 0) | lead section |
| Timeline of Solar System exploration | 1 (0 / 1) | lead section |
| Tinia Valles | 1 (1 / 0) | lead section |
| Tinjar Valles | 1 (1 / 0) | lead section |
| Tintina (rock) | 1 (1 / 0) | full article |
| Tissint meteorite | 1 (1 / 0) | lead section |
| Titius–Bode law | 1 (0 / 1) | lead section |
| TMK | 1 (1 / 0) | lead section |
| Tokogeny | 1 (0 / 1) | lead section |
| TOP Assay | 1 (0 / 1) | lead section |
| Torpor Inducing Transfer Habitat For Human Stasis To Mars | 1 (1 / 0) | lead section |
| TRACE (computer program) | 1 (0 / 1) | lead section |
| Trans-Neptunian object | 1 (1 / 0) | lead section |
| Transit of Deimos from Mars | 1 (1 / 0) | lead section |
| Transit of Earth from Mars | 1 (1 / 0) | lead section |
| Transit of Mercury from Mars | 1 (1 / 0) | lead section |
| Triboluminescence | 1 (0 / 1) | lead section |
| Tyche (hypothetical planet) | 1 (0 / 1) | lead section |
| Tyras Vallis | 1 (1 / 0) | lead section |
| Ulysses Colles | 1 (1 / 0) | lead section |
| Ulysses Fossae | 1 (1 / 0) | lead section |
| Ulysses Tholus | 1 (1 / 0) | lead section |
| Umov effect | 1 (0 / 1) | lead section |
| Universality–diversity paradigm | 1 (0 / 1) | lead section |
| UniverseMachine | 1 (0 / 1) | lead section |
| Uranius Mons | 1 (1 / 0) | lead section |
| Vaidya metric | 1 (0 / 1) | lead section |
| Valles Marineris | 1 (1 / 0) | lead section |
| Venus in culture | 1 (0 / 1) | lead section |
| Vesta (spacecraft) | 1 (1 / 0) | lead section |
| Vicarious Hypothesis | 1 (1 / 0) | lead section |
| Viking 1 | 1 (1 / 0) | lead section |
| Viking 2 | 1 (1 / 0) | lead section |
| Viking lander biological experiments | 1 (1 / 0) | lead section |
| Virbhadra–Ellis lens equation | 1 (0 / 1) | lead section |
| Virgocentric flow | 1 (0 / 1) | lead section |
| Vision for Space Exploration | 1 (1 / 0) | lead section |
| Visual Monitoring Camera | 1 (1 / 0) | lead section |
| Volcanism on Mars | 1 (1 / 0) | lead section |
| Volcanism on Venus | 1 (1 / 0) | lead section |
| Volcanology | 1 (0 / 1) | lead section |
| Voltaire (crater) | 1 (1 / 0) | lead section |
| Voyager program (Mars) | 1 (1 / 0) | lead section |
| Vulcan (hypothetical planet) | 1 (0 / 1) | lead section |
| WaLSA Team | 1 (0 / 1) | lead section |
| Warrego Valles | 1 (1 / 0) | lead section |
| Water on terrestrial planets of the Solar System | 1 (0 / 1) | lead section |
| Water remote sensing | 1 (0 / 1) | lead section |
| WAVAR | 1 (1 / 0) | lead section |
| Weathering | 1 (0 / 1) | lead section |
| Wet chemistry | 1 (0 / 1) | lead section |
| Wetted perimeter | 1 (0 / 1) | lead section |
| Weyl's postulate | 1 (0 / 1) | lead section |
| White hole | 1 (0 / 1) | lead section |
| Whole Earth Blazar Telescope | 1 (0 / 1) | lead section |
| Wohlfarth Lectureship | 1 (0 / 1) | lead section |
| Wouthuysen–Field coupling | 1 (0 / 1) | lead section |
| X-factor (astrophysics) | 1 (0 / 1) | lead section |
| Xanthe Terra | 1 (1 / 0) | lead section |
| XMM Cluster Survey | 1 (0 / 1) | lead section |
| Yajnavalkya 95 Years Cycle | 1 (0 / 1) | lead section |
| Yamato 000593 | 1 (1 / 0) | lead section |
| Yardangs on Mars | 1 (1 / 0) | lead section |
| Yinghuo-1 | 1 (1 / 0) | lead section |
| Yogi Rock | 1 (1 / 0) | lead section |
| Zagami meteorite | 1 (1 / 0) | lead section |
| Zanstra method | 1 (0 / 1) | lead section |
| Zeldovich approximation | 1 (0 / 1) | lead section |
| Zeldovich equation of state | 1 (0 / 1) | lead section |
| Zond 2 | 1 (1 / 0) | lead section |
Generation and reproducibility
The corpus is a fixed snapshot scraped from English Wikipedia (via the MediaWiki API) in
July 2026 and shipped with the dataset, so retrieval results reproduce from the released
files regardless of later Wikipedia edits. Articles are chunked into passages of roughly 160
words — core/deep articles from their full text, broader articles from the lead section only
(see Sources). Queries were authored by an LLM (Claude) from those passages: levels L6-L15
from corpus passages within each level's category scope; levels L3-L5 from the flagship
articles (Ingenuity, Perseverance, the Mars 2020 mission); levels L1-L2 as paraphrase sets
around Ingenuity's flight campaign. Golds were then expanded and verified as described under
Multi-gold relevance (the same-fact judge is also an LLM, run over a retriever-neutral
candidate pool). Query sampling and the held-in / held-out split use a fixed seed = 42.
Full pipeline: scripts/gradual-semantic-exp/wiki-data-gen/.
Attribution
Corpus text is from English Wikipedia, licensed CC BY-SA 4.0 — attribute
"Wikipedia contributors". Every passage records its source article in its title / url
fields; the complete list is under Sources and in sources.tsv.
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