Sample-return mission

File:Apollo 15 Genesis Rock.jpg   File:As17-137-21009.jpg  A **sample-return mission** is a spacecraft mission with the goal of collecting and returning samples from an extraterrestrial location to Earth for analysis. Sample-return missions may bring back merely atoms and molecules or a deposit of complex compounds such as loose material ("soil") and rocks. These samples may be obtained in a number of ways, such as soil and rock excavation or a collector array used for capturing particles of solar wind or cometary debris.

To date, samples of Moon rock from Earth's Moon have been collected by robotic and crewed missions, the comet Wild 2 and the asteroids 25143 Itokawa and 162173 Ryugu have been visited by robotic spacecraft which returned samples to Earth, and samples of the solar wind have been returned by the robotic *Genesis* mission. Samples from the asteroid 101955 Bennu have been obtained and will start back to Earth in March 2021.

In addition to sample-return missions, samples from three identified non-terrestrial bodies have been collected by means other than sample-return missions: samples from the Moon in the form of Lunar meteorites, samples from Mars in the form of Martian meteorites, and samples from Vesta in the form of HED meteorites.

## Scientific use

 File:Motif de "Widmanstätten" ©dada 677.jpg   File:Bilanga meteorite, 4.3g slice.jpg   File:MarsMeteorite-NWA7034-716969main black beauty full.jpg  Samples available on Earth can be analyzed in laboratories, so we can further our understanding and knowledge as part of the discovery and exploration of the Solar System. Until now, many important scientific discoveries about the Solar System were made remotely with telescopes, and some Solar System bodies were visited by orbiting or even landing spacecraft with instruments capable of remote sensing or sample analysis. While such an investigation of the Solar System is technically easier than a sample-return mission, the scientific tools available on Earth to study such samples are far more advanced and diverse than those that can go on spacecraft. Further, analysis of samples on Earth allows follow up of any findings with different tools, including tools that can tell intrinsic extraterrestrial material from terrestrial contamination, and those that have yet to be developed; in contrast, a spacecraft can carry only a limited set of analytic tools, and these have to be chosen and built long before launch.

Samples analyzed on Earth can be matched against findings of remote sensing for more insight into the processes that formed the Solar System. This was done, for example, with findings by the *Dawn* spacecraft, which visited the asteroid Vesta from 2011 to 2012 for imaging, and samples from HED meteorites (collected on Earth until then), which were compared to data gathered by Dawn. These meteorites could then be identified as material ejected from the large impact crater Rheasilvia on Vesta. This allowed deducing the composition of crust, mantle and core of Vesta. Similarly, some differences in composition of asteroids (and, to a lesser extent, different compositions of comets) can be discerned by imaging alone. However, for a more precise inventory of the material on these different bodies, more samples will be collected and returned in the future, to match their compositions with the data gathered through telescopes and astronomical spectroscopy.

One further focus of such investigation—besides the basic composition and geologic history of the various Solar System bodies—is the presence of the building blocks of life on comets, asteroids, Mars or the moons of the gas giants. Several sample-return missions to asteroids and comets are currently in the works. More samples from asteroids and comets will help determine whether life formed in space and was carried to Earth by meteorites. Another question under investigation is whether extraterrestrial life formed on other Solar System bodies like Mars or on the moons of the gas giants, and whether life might even exist there. The result of NASA's last "Decadal Survey" was to prioritize a Mars sample-return mission, as Mars has a special importance: it is comparatively "nearby", might have harbored life in the past, and might even continue to sustain life. Jupiter's moon Europa is another important focus in the search for life in the Solar System. However, due to the distance and other constraints, Europa might not be the target of a sample-return mission in the foreseeable future.

## Planetary protection

Further information: Planetary protection and Extraterrestrial sample curation
Planetary protection aims to prevent biological contamination of both the target celestial body and the Earth—in the case of sample-return missions. No sample has yet been returned with alien life in it. A sample-return from Mars or other location with potential to host life, is a category V mission under COSPAR which directs to containment of any unsterilized sample returned to Earth. This is because it is unknown the effects of such hypothetical life would be on humans or on the biosphere of Earth. For this reason, Carl Sagan and Joshua Lederberg argued in the 1970s that we should do sample-return missions classified as category V missions with extreme caution, and later studies by the NRC and ESF agreed.

## Sample-return missions

### First missions

 File:Apollo 11 2004 scan.jpg   File:Moon rock from Apollo 15 interpretive sign.jpg   File:Moon rock from Apollo 15 side.jpg  The Apollo program returned over Template:Convert of lunar rocks and regolith (including lunar 'soil') to the Lunar Receiving Laboratory in Houston. Today, 75% of the samples are stored at the Lunar Sample Laboratory Facility built in 1979. In July 1969, Apollo 11 achieved the first successful sample return from another Solar System body. It returned approximately Template:Convert of Lunar surface material. This was followed by Template:Convert of material from Apollo 12, Template:Convert of material from Apollo 14, Template:Convert of material from Apollo 15, Template:Convert of material from Apollo 16, and Template:Convert of material from Apollo 17.Template:Citation needed

One of the most significant advances in sample-return missions occurred in 1970 when the robotic Soviet mission known as Luna 16 successfully returned Template:Convert of lunar soil. Likewise, Luna 20 returned Template:Convert in 1974, and Luna 24 returned Template:Convert in 1976. Although they recovered far less than the Apollo missions, they did this fully automatically. Apart from these three successes, other attempts under the Luna programme failed. The first two missions were intended to outstrip Apollo 11 and were undertaken shortly before them in June and July 1969: Luna E-8-5 No. 402 failed at start, and Luna 15 crashed on the Moon. Later, other sample-return missions failed: Kosmos 300 and Kosmos 305 in 1969, Luna E-8-5 No. 405 in 1970, Luna E-8-5M No. 412 in 1975 had unsuccessful launches, and Luna 18 in 1971 and Luna 23 in 1974 had unsuccessful landings on the Moon.

In 1970, the Soviet Union planned for a 1975 first Martian sample-return mission in the Mars 5NM project. This mission was planned to use an N1 rocket, but as this rocket never flew successfully, the mission evolved into the Mars 5M project, which would use a double launch with the smaller Proton rocket and an assembly at a Salyut space station. This Mars 5M mission was planned for 1979, but was canceled in 1977 due to technical problems and complexity; all hardware was ordered destroyed.

### 1990s

The Earth-Orbital Debris Collection (ODC) experiment was deployed on the Mir space station for 18 months during 1996–97 and used aerogel to capture particles from low Earth orbit, consisting of interplanetary dust and man-made particles. Far from being "the last sample-return mission... in... twenty years", ODC was a portable version of an LDEF collector, decreasing collection time significantly, and effective area by orders of magnitude.

### 2000s

 File:GenSC collection2 150dpi.jpg  The next mission to return extraterrestrial samples was the *Genesis* mission, which returned solar wind samples to Earth from beyond Earth orbit in 2004. Unfortunately, the *Genesis* capsule failed to open its parachute while re-entering the Earth's atmosphere and crash-landed in the Utah desert. There were fears of severe contamination or even total mission loss, but scientists managed to save many of the samples. They were the first to be collected from beyond lunar orbit. *Genesis* used a collector array made of wafers of ultra-pure silicon, gold, sapphire, and diamond. Each different wafer was used to collect a different part of the solar wind.Template:Citation needed

 File:Stardust Capsule on Ground.jpg  *Genesis* was followed by NASA's *Stardust* spacecraft, which returned comet samples to Earth on January 15, 2006. It safely passed by Comet Wild 2 and collected dust samples from the comet's coma while imaging the comet's nucleus. *Stardust* used a collector array made of low-density aerogel (99% of which is empty space), which has about 1/1000 of the density of glass. This enables the collection of cometary particles without damaging them due to high impact velocities. Particle collisions with even slightly porous solid collectors would result in destruction of those particles and damage to the collection apparatus. During cruise, the second side of the array collected at least seven interstellar dust particles.

### 2010s and 2020s

In June 2010 the Japan Aerospace Exploration Agency (JAXA) Hayabusa probe returned asteroid samples to Earth after a rendezvous with (and a landing on) S-type asteroid 25143 Itokawa. In November 2010, scientists at the agency confirmed that, despite failure of the sampling device, the probe retrieved micrograms of dust from the asteroid, the first brought back to Earth in pristine condition.

The Russian Fobos-Grunt was a failed sample-return mission designed to return samples from Phobos, one of the moons of Mars. It was launched on November 8, 2011, but failed to leave Earth orbit and crashed after several weeks into the southern Pacific Ocean.

 File:OSIRIS-REX SamCam TAGSAM Event 2020-10-20 small.gif  The Japan Aerospace Exploration Agency (JAXA) launched the improved *Hayabusa2* space probe on December 3, 2014. *Hayabusa2* arrived at the target near-Earth C-type asteroid 162173 Ryugu (previously designated Template:Mpl) on 27 June 2018. It surveyed the asteroid for a year and a half and took samples. It left the asteroid in November 2019 and returned to Earth on December 6, 2020.

The OSIRIS-REx mission was launched in September 2016 on a mission to return samples from the asteroid 101955 Bennu. The samples are expected to enable scientists to learn more about the time before the birth of the Solar System, initial stages of planet formation, and the source of organic compounds that led to the formation of life. It reached the proximity of Bennu on 3 December 2018, where it began analyzing its surface for a target sample area over the next several months. It collected its sample on 20 October 2020, and is expected to return to Earth on 24 September 2023.

China launched the Chang'e 5 lunar sample return mission on November 23, 2020 which returned to Earth with 2 kilograms of lunar soil on December 16, 2020. It was first lunar sample return in over 40 years.

### Future missions

 File:Mars-sample-return-Mars-ascent-vehicule.jpg  See also: Mars sample return mission
Russia has plans for Luna-Glob missions to return samples from the Moon by 2027 and Mars-Grunt to return samples from Mars in the late 2020s.

JAXA is developing the MMX mission, a sample-return mission to Phobos that will be launched in 2024. MMX will study both moons of Mars, but the landing and the sample collection will be on Phobos. This selection was made because of the two moons, Phobos's orbit is closer to Mars and its surface may have particles blasted from Mars. Thus the sample may contain material originating on Mars itself. A propulsion module carrying the sample is expected to return to Earth in approximately September 2029.

China has plans for a Mars sample return mission by 2030. Also, the Chinese Space Agency is designing a sample-retrieval mission from Ceres that would take place during the 2020s.

NASA has long planned a Martian sample-return mission, but has yet to secure the budget to successfully design, build, launch, and land such a probe. The mission remained on NASA's roadmap for planetary science as of the 2013 Planetary Science Decadal Survey. The *Perseverance* rover, launched in 2020, will collect drill core samples and stash them on Mars' surface by 2023, but it remains unclear how they will be retrieved from the stash and returned to Earth.

Comet sample-return missions continue to be a NASA priority. Comet Surface Sample Return was one of the six themes for proposals for NASA's fourth New Frontiers mission. Template:Multipleimage Template:Multipleimage

## Methods of sample return

 File:Tagsamlast.gif  Sample-return methods include, but are not restricted to the following:

 File:Genesis Collector Array.jpg
### Collector array

A collector array may be used to collect millions or billions of atoms, molecules, and fine particulates by using a number of wafers made of different elements. The molecular structure of these wafers allows the collection of various sizes of particles. Collector arrays, such as those flown on *Genesis*, are ultra-pure in order to ensure maximal collection efficiency, durability, and analytical distinguishability.

Collector arrays are useful for collecting tiny, fast-moving atoms such as those expelled by the Sun through the solar wind, but can also be used for collection of larger particles such as those found in the coma of a comet. The NASA spacecraft known as *Stardust* implemented this technique. However, due to the high speeds and size of the particles that make up the coma and the area nearby, a dense solid-state collector array was not viable. As a result, another means for collecting samples had to be designed as to preserve the safety of the spacecraft and the samples themselves.

#### Aerogel

Main article: Aerogel
 File:Meteoroid track through aerogel from EURECA mission.jpg  Aerogel is a silica-based porous solid with a sponge-like structure, 99.8% of whose volume is empty space. Aerogel has about 1/1000 of the density of glass. An aerogel was used in the *Stardust* spacecraft because the dust particles the spacecraft was to collect would have an impact speed of about 6 km/s. A collision with a dense solid at that speed could alter their chemical composition or perhaps vaporize them completely.
Since the aerogel is mostly transparent, and the particles leave a carrot-shaped path once they penetrate the surface, scientists can easily find and retrieve them. Since its pores are on the nanometer scale, particles, even ones smaller than a grain of sand, do not merely pass through the aerogel completely. Instead, they slow to a stop and then are embedded within it.

 File:Mars 5NM.jpg   File:Mars 5NM - Ilustration.jpg  The *Stardust* spacecraft has a tennis-racket-shaped collector with aerogel fitted to it. The collector is retracted into its capsule for safe storage and delivery back to Earth. Aerogel is quite strong and easily survives both launching and outer-space environments.

### Robotic excavation and return

Some of the most risky and difficult types of sample-return missions are those that require landing on an extraterrestrial body such as an asteroid, moon, or planet. It takes a great deal of time, money, and technical ability in order to even initiate such plans. It is a difficult feat that requires that everything from launch to landing to retrieval and launch back to Earth is planned out with high precision and accuracy.

This type of sample return, although having the most risks, is the most rewarding for planetary science. Furthermore, such missions carry a great deal of public outreach potential, which is an important attribute for space exploration when it comes to public support. The only successful robotic sample-return missions of this type have been the Soviet Luna landers and Chinese Chang'e 5.Template:Citation needed

## See also

Template:Div col

* Asteroid mining
* Exploration of Mars
* Exploration of the Moon
* Extraterrestrial sample curation
* List of lunar probes
* Robotic exploration of the Moon
* Timeline of Solar System exploration

Template:Div col end

## References

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## External links

* Mars Exploration: *Sample Returns* Jet Propulsion Laboratory Mars Exploration Program on sample return missions.
* Stardust *Homepage* Jet Propulsion Laboratory *Stardust* mission website.
* Genesis Mission *Homepage* Jet Propulsion Laboratory *Genesis* mission website.
* Stardust: *Aerogel* *Stardust* website on aerogel technology.
* JAXA *Hayabusa* JAXA *Hayabusa* project update.
* MarsNews.com: *Mars Sample Return* MarsNews.com on Mars Sample Return missions.
* Texas Space Grant Consortium: *Missions to the Moon* A list of missions to the Moon from 1958 to 1998.
* Evaluating the Biological Potential in Samples Returned from Planetary Satellites and Small Solar System Bodies The National Academies, Space Science Board 1998

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