sentence-transformers/squad huggingface dataset:
Passage: Guests ascending to the 67th, 69th, and 70th level observation decks (dubbed "Top of the Rock") atop the GE Building at Rockefeller Center in New York City ride a high-speed glass-top elevator. When entering the cab, it appears to be any normal elevator ride. However, once the cab begins moving, the interior lights turn off and a special blue light above the cab turns on. This lights the entire shaft, so riders can see the moving cab through its glass ceiling as it rises and lowers through the shaft. Music plays and various animations are also displayed on the ceiling. The entire ride takes about 60 seconds.

Question: What are the 67th, 69th, and 70th floors of the GE Building at Rockerfeller Center nicknamed?

Question: What do these floors serve as?

Question: What type of elevator is featured?

Question: How long is the short trip?

Question: The special effects include blue light, music playing and what else?
Passage: Part of the Haunted Mansion attraction at Disneyland in Anaheim, California, and Disneyland in Paris, France, takes place on an elevator. The "stretching room" on the ride is actually an elevator that travels downwards, giving access to a short underground tunnel which leads to the rest of the attraction. The elevator has no ceiling and its shaft is decorated to look like walls of a mansion. Because there is no roof, passengers are able to see the walls of the shaft by looking up, which gives the illusion of the room stretching.

Question: The Haunted Mansion at Disneyland in California and the one in Paris, France sharewhat attribute?

Question: What is the name of area that is really an elevator?

Question: What is included in the elevator's design?

Question: What is the illusion given by these effects?
Passage: Neptune is the eighth and farthest known planet from the Sun in the Solar System. It is the fourth-largest planet by diameter and the third-largest by mass. Among the giant planets in the Solar System, Neptune is the most dense. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 times the mass of Earth and slightly larger than Neptune.[c] Neptune orbits the Sun once every 164.8 years at an average distance of 30.1 astronomical units (4.50×109 km). Named after the Roman god of the sea, its astronomical symbol is ♆, a stylised version of the god Neptune's trident.

Question: What planet is Neptune's near-twin?

Question: What is Neptune named after?

Question: How much more dense is Neptune compared to Earth?

Question: What does the astronomical sign of Neptune represent?

Question: How many Earth years does Neptune orbit the sun?
Passage: Neptune is not visible to the unaided eye and is the only planet in the Solar System found by mathematical prediction rather than by empirical observation. Unexpected changes in the orbit of Uranus led Alexis Bouvard to deduce that its orbit was subject to gravitational perturbation by an unknown planet. Neptune was subsequently observed with a telescope on 23 September 1846 by Johann Galle within a degree of the position predicted by Urbain Le Verrier. Its largest moon, Triton, was discovered shortly thereafter, though none of the planet's remaining known 14 moons were located telescopically until the 20th century. The planet's distance from Earth gives it a very small apparent size, making it challenging to study with Earth-based telescopes. Neptune was visited by Voyager 2, when it flew by the planet on 25 August 1989. The advent of Hubble Space Telescope and large ground-based telescopes with adaptive optics has recently allowed for additional detailed observations from afar.

Question: How was Neptune found?

Question: When was Neptune first observed?

Question: Who discovered Neptune?

Question: What is Neptune's largest moon?

Question: What flew by Neptune in 1989?
Passage: Neptune is similar in composition to Uranus, and both have compositions that differ from those of the larger gas giants, Jupiter and Saturn. Like Jupiter and Saturn, Neptune's atmosphere is composed primarily of hydrogen and helium, along with traces of hydrocarbons and possibly nitrogen, but contains a higher proportion of "ices" such as water, ammonia, and methane. However, its interior, like that of Uranus, is primarily composed of ices and rock, and hence Uranus and Neptune are normally considered "ice giants" to emphasise this distinction. Traces of methane in the outermost regions in part account for the planet's blue appearance.

Question: Which planet is compositionally similar to Neptune?

Question: What is Neptune's atmosphere primarily composed of?

Question: What is the interior of Neptune composed of?

Question: What makes Neptune blue?

Question: What "ices" makes up Neptune?
Passage: In contrast to the hazy, relatively featureless atmosphere of Uranus, Neptune's atmosphere has active and visible weather patterns. For example, at the time of the Voyager 2 flyby in 1989, the planet's southern hemisphere had a Great Dark Spot comparable to the Great Red Spot on Jupiter. These weather patterns are driven by the strongest sustained winds of any planet in the Solar System, with recorded wind speeds as high as 2,100 kilometres per hour (580 m/s; 1,300 mph). Because of its great distance from the Sun, Neptune's outer atmosphere is one of the coldest places in the Solar System, with temperatures at its cloud tops approaching 55 K (−218 °C). Temperatures at the planet's centre are approximately 5,400 K (5,100 °C). Neptune has a faint and fragmented ring system (labelled "arcs"), which was first detected during the 1960s and confirmed by Voyager 2.

Question: What weather did Voyager 2 observe on Neptune?

Question: What weather feature does Neptune have stronger than any other planet?

Question: What were the wind speeds recorded on Neptune?

Question: What is the cloud tops on Neptune temperature?

Question: What is Neptune's planet center temperature?
Passage: Some of the earliest recorded observations ever made through a telescope, Galileo's drawings on 28 December 1612 and 27 January 1613, contain plotted points that match up with what is now known to be the position of Neptune. On both occasions, Galileo seems to have mistaken Neptune for a fixed star when it appeared close—in conjunction—to Jupiter in the night sky; hence, he is not credited with Neptune's discovery. At his first observation in December 1612, Neptune was almost stationary in the sky because it had just turned retrograde that day. This apparent backward motion is created when Earth's orbit takes it past an outer planet. Because Neptune was only beginning its yearly retrograde cycle, the motion of the planet was far too slight to be detected with Galileo's small telescope. In July 2009, University of Melbourne physicist David Jamieson announced new evidence suggesting that Galileo was at least aware that the 'star' he had observed had moved relative to the fixed stars.

Question: Who drew Neptune after observing it with a telescope?

Question: What was Neptune mistaken for at first?

Question: What happens when Neptune goes retrograde?

Question: What date was Neptune drawn first?

Question: Who recently researched the original observation of Neptune?
Passage: In 1821, Alexis Bouvard published astronomical tables of the orbit of Neptune's neighbour Uranus. Subsequent observations revealed substantial deviations from the tables, leading Bouvard to hypothesise that an unknown body was perturbing the orbit through gravitational interaction. In 1843, John Couch Adams began work on the orbit of Uranus using the data he had. Via Cambridge Observatory director James Challis, he requested extra data from Sir George Airy, the Astronomer Royal, who supplied it in February 1844. Adams continued to work in 1845–46 and produced several different estimates of a new planet.

Question: What year did Alexis Bouvard publish relevant astronomical tables?

Question: What did Alexis Bouvard study?

Question: When did John Couch Adams begin working on the orbit of Uranus?

Question: Who gave John Couch Adams extra data?

Question: What did the extra data John Couch Adams received produce?
Passage: Meanwhile, Le Verrier by letter urged Berlin Observatory astronomer Johann Gottfried Galle to search with the observatory's refractor. Heinrich d'Arrest, a student at the observatory, suggested to Galle that they could compare a recently drawn chart of the sky in the region of Le Verrier's predicted location with the current sky to seek the displacement characteristic of a planet, as opposed to a fixed star. On the evening of 23 September 1846, the day Galle received the letter, he discovered Neptune within 1° of where Le Verrier had predicted it to be, about 12° from Adams' prediction. Challis later realised that he had observed the planet twice, on 4 and 12 August, but did not recognise it as a planet because he lacked an up-to-date star map and was distracted by his concurrent work on comet observations.

Question: Who was Henrich d'Arrest?

Question: When did Galle discover Neptune?

Question: How many degrees off was Adams' prediction?

Question: What did Henrich d'Arrest seek to find?

Question: What was Challis looking for when he saw Neptune the first two times?
Passage: In the wake of the discovery, there was much nationalistic rivalry between the French and the British over who deserved credit for the discovery. Eventually, an international consensus emerged that both Le Verrier and Adams jointly deserved credit. Since 1966, Dennis Rawlins has questioned the credibility of Adams's claim to co-discovery, and the issue was re-evaluated by historians with the return in 1998 of the "Neptune papers" (historical documents) to the Royal Observatory, Greenwich. After reviewing the documents, they suggest that "Adams does not deserve equal credit with Le Verrier for the discovery of Neptune. That credit belongs only to the person who succeeded both in predicting the planet's place and in convincing astronomers to search for it."

Question: What two countries argued over credit for the discovery of Neptune?

Question: Who ultimately deserved credit for the discovery of Neptune?

Question: Who questioned Adams's claim to co-discovery of Neptune?

Question: Who predicted Neptune's place and convinced astronomer's to search for it?

Question: Who did not deserve credit to co-discovery of Neptune?
Passage: Claiming the right to name his discovery, Le Verrier quickly proposed the name Neptune for this new planet, though falsely stating that this had been officially approved by the French Bureau des Longitudes. In October, he sought to name the planet Le Verrier, after himself, and he had loyal support in this from the observatory director, François Arago. This suggestion met with stiff resistance outside France. French almanacs quickly reintroduced the name Herschel for Uranus, after that planet's discoverer Sir William Herschel, and Leverrier for the new planet.

Question: Who claimed the right to name Neptune?

Question: What country approved Neptune's first name?

Question: What did the discoverer want to name Neptune first?

Question: What first introduced Neptune and Uranus's names?

Question: Who did not approve of the first name for Neptune?
Passage: Most languages today, even in countries that have no direct link to Greco-Roman culture, use some variant of the name "Neptune" for the planet. However, in Chinese, Japanese, and Korean, the planet's name was translated as "sea king star" (海王星), because Neptune was the god of the sea. In Mongolian, Neptune is called Dalain Van (Далайн ван), reflecting its namesake god's role as the ruler of the sea. In modern Greek the planet is called Poseidon (Ποσειδώνας, Poseidonas), the Greek counterpart of Neptune. In Hebrew, "Rahab" (רהב), from a Biblical sea monster mentioned in the Book of Psalms, was selected in a vote managed by the Academy of the Hebrew Language in 2009 as the official name for the planet, even though the existing Latin term "Neptun" (נפטון) is commonly used. In Māori, the planet is called Tangaroa, named after the Māori god of the sea. In Nahuatl, the planet is called Tlāloccītlalli, named after the rain god Tlāloc.

Question: What is the Chinese, Japanese, and Korean translations for Neptune?

Question: What god was Neptune?

Question: What is the Mongolian name for Neptune?

Question: What did the Greeks call Neptune?

Question: What was the Biblical sea monster that Neptune is named in Hebrew?
Passage: From its discovery in 1846 until the subsequent discovery of Pluto in 1930, Neptune was the farthest known planet. When Pluto was discovered it was considered a planet, and Neptune thus became the penultimate known planet, except for a 20-year period between 1979 and 1999 when Pluto's elliptical orbit brought it closer to the Sun than Neptune. The discovery of the Kuiper belt in 1992 led many astronomers to debate whether Pluto should be considered a planet or as part of the Kuiper belt. In 2006, the International Astronomical Union defined the word "planet" for the first time, reclassifying Pluto as a "dwarf planet" and making Neptune once again the outermost known planet in the Solar System.

Question: What was Neptune before Pluto was discovered?

Question: What discovery made astronomer's debate Pluto's status as a planet?

Question: What year did the International Astronomical Union define the word planet?

Question: Now that Pluto isn't a planet, what is Neptune known for in our solar system?

Question: What period was Pluto closer to the sun than Neptune?
Passage: Neptune's mass of 1.0243×1026 kg, is intermediate between Earth and the larger gas giants: it is 17 times that of Earth but just 1/19th that of Jupiter.[d] Its gravity at 1 bar is 11.15 m/s2, 1.14 times the surface gravity of Earth, and surpassed only by Jupiter. Neptune's equatorial radius of 24,764 km is nearly four times that of Earth. Neptune, like Uranus, is an ice giant, a subclass of giant planet, due to their smaller size and higher concentrations of volatiles relative to Jupiter and Saturn. In the search for extrasolar planets, Neptune has been used as a metonym: discovered bodies of similar mass are often referred to as "Neptunes", just as scientists refer to various extrasolar bodies as "Jupiters".

Question: What is Neptune's mass?

Question: How much more mass does Neptune have compared to Earth?

Question: What is Neptune's gravity at 1 bar?

Question: What is Neptune's equatorial radius?

Question: What is Neptune referred to due to it's size and concentration of volatiles?
Passage: The mantle is equivalent to 10 to 15 Earth masses and is rich in water, ammonia and methane. As is customary in planetary science, this mixture is referred to as icy even though it is a hot, dense fluid. This fluid, which has a high electrical conductivity, is sometimes called a water–ammonia ocean. The mantle may consist of a layer of ionic water in which the water molecules break down into a soup of hydrogen and oxygen ions, and deeper down superionic water in which the oxygen crystallises but the hydrogen ions float around freely within the oxygen lattice. At a depth of 7000 km, the conditions may be such that methane decomposes into diamond crystals that rain downwards like hailstones. Very-high-pressure experiments at the Lawrence Livermore National Laboratory suggest that the base of the mantle may comprise an ocean of liquid carbon with floating solid 'diamonds'.

Question: What is Neptune's mantle rich in?

Question: What is the hot, dense fluid in Neptune referred to as?

Question: What does the fluid in Neptune have a high conductivity of?

Question: How deep does Neptune's water-ammonia ocean go?

Question: What rains on Neptune?
Passage: At high altitudes, Neptune's atmosphere is 80% hydrogen and 19% helium. A trace amount of methane is also present. Prominent absorption bands of methane exist at wavelengths above 600 nm, in the red and infrared portion of the spectrum. As with Uranus, this absorption of red light by the atmospheric methane is part of what gives Neptune its blue hue, although Neptune's vivid azure differs from Uranus's milder cyan. Because Neptune's atmospheric methane content is similar to that of Uranus, some unknown atmospheric constituent is thought to contribute to Neptune's colour.

Question: What is Neptune's atmosphere made of?

Question: Where are absorption bands of methane on Neptune?

Question: What gives Neptune it's blue hue?

Question: What planet also gets it's color from atmospheric constituent?

Question: What color is Uranus, compared to Neptune?
Passage: Models suggest that Neptune's troposphere is banded by clouds of varying compositions depending on altitude. The upper-level clouds lie at pressures below one bar, where the temperature is suitable for methane to condense. For pressures between one and five bars (100 and 500 kPa), clouds of ammonia and hydrogen sulfide are thought to form. Above a pressure of five bars, the clouds may consist of ammonia, ammonium sulfide, hydrogen sulfide and water. Deeper clouds of water ice should be found at pressures of about 50 bars (5.0 MPa), where the temperature reaches 273 K (0 °C). Underneath, clouds of ammonia and hydrogen sulfide may be found.

Question: What is Neptune's clouds competition variants dependent on?

Question: Which clouds on Neptune are suitable for methane to condense?

Question: What clouds form between one and five bars on Neptune?

Question: On Neptune, what do clouds above five bars consist of?

Question: What is the temperature on Neptune's clouds that are at 50 bars?
Passage: High-altitude clouds on Neptune have been observed casting shadows on the opaque cloud deck below. There are also high-altitude cloud bands that wrap around the planet at constant latitude. These circumferential bands have widths of 50–150 km and lie about 50–110 km above the cloud deck. These altitudes are in the layer where weather occurs, the troposphere. Weather does not occur in the higher stratosphere or thermosphere. Unlike Uranus, Neptune's composition has a higher volume of ocean, whereas Uranus has a smaller mantle.

Question: On Neptune, which clouds cast shadows on the cloud deck below it?

Question: What are the widths of the cloud bands on Neptune?

Question: Where are the high altitude bands of clouds on Neptune?

Question: What does Neptune have more of compared to Uranus?

Question: Where on Neptune does weather not occur?
Passage: For reasons that remain obscure, the planet's thermosphere is at an anomalously high temperature of about 750 K. The planet is too far from the Sun for this heat to be generated by ultraviolet radiation. One candidate for a heating mechanism is atmospheric interaction with ions in the planet's magnetic field. Other candidates are gravity waves from the interior that dissipate in the atmosphere. The thermosphere contains traces of carbon dioxide and water, which may have been deposited from external sources such as meteorites and dust.

Question: What is Neptune's temperature in the thermosphere?

Question: What would interact with Neptune's magnetic field to make it warm?

Question: Where would gravity waves in Neptune's interior dissipate?

Question: What does Neptune's thermosphere containers traces of?
Passage: Neptune also resembles Uranus in its magnetosphere, with a magnetic field strongly tilted relative to its rotational axis at 47° and offset at least 0.55 radii, or about 13500 km from the planet's physical centre. Before Voyager 2's arrival at Neptune, it was hypothesised that Uranus's tilted magnetosphere was the result of its sideways rotation. In comparing the magnetic fields of the two planets, scientists now think the extreme orientation may be characteristic of flows in the planets' interiors. This field may be generated by convective fluid motions in a thin spherical shell of electrically conducting liquids (probably a combination of ammonia, methane and water) resulting in a dynamo action.

Question: What is the rotational axis of Neptune's magnetic field?

Question: Where is Neptune's magnetic field offset from the physical centre?

Question: What planet besides Neptune has a sideways rotation?

Question: What might cause Neptune's extreme orientation?

Question: What fluids are in Neptune's interior?
Passage: The dipole component of the magnetic field at the magnetic equator of Neptune is about 14 microteslas (0.14 G). The dipole magnetic moment of Neptune is about 2.2 × 1017 T·m3 (14 μT·RN3, where RN is the radius of Neptune). Neptune's magnetic field has a complex geometry that includes relatively large contributions from non-dipolar components, including a strong quadrupole moment that may exceed the dipole moment in strength. By contrast, Earth, Jupiter and Saturn have only relatively small quadrupole moments, and their fields are less tilted from the polar axis. The large quadrupole moment of Neptune may be the result of offset from the planet's centre and geometrical constraints of the field's dynamo generator.

Question: What is Neptune's dipole magnetic moment?

Question: What is one of Neptune's non-dipolar component what may exceed the dipole moment in strength?

Question: Which three planets have small quadrupole moments compared to Neptune?

Question: Besides the geometrical constraints of Neptune's dynamo generator, what is another result of the quadrupole moment?

Question: What is the dipole component of the magnetic field at the magnetic equator of neptune?
Passage: Neptune has a planetary ring system, though one much less substantial than that of Saturn. The rings may consist of ice particles coated with silicates or carbon-based material, which most likely gives them a reddish hue. The three main rings are the narrow Adams Ring, 63,000 km from the centre of Neptune, the Le Verrier Ring, at 53,000 km, and the broader, fainter Galle Ring, at 42,000 km. A faint outward extension to the Le Verrier Ring has been named Lassell; it is bounded at its outer edge by the Arago Ring at 57,000 km.

Question: What system, like Saturn, does Neptune have?

Question: What might Neptune's rings consist of?

Question: What might the ice particles of Neptune's rings be coated with?

Question: Where is Adams ring from the center of Neptune?

Question: Where is the La Verrier ring from the center of Neptune?
Passage: Neptune's weather is characterised by extremely dynamic storm systems, with winds reaching speeds of almost 600 m/s (2,200 km/h; 1,300 mph)—nearly reaching supersonic flow. More typically, by tracking the motion of persistent clouds, wind speeds have been shown to vary from 20 m/s in the easterly direction to 325 m/s westward. At the cloud tops, the prevailing winds range in speed from 400 m/s along the equator to 250 m/s at the poles. Most of the winds on Neptune move in a direction opposite the planet's rotation. The general pattern of winds showed prograde rotation at high latitudes vs. retrograde rotation at lower latitudes. The difference in flow direction is thought to be a "skin effect" and not due to any deeper atmospheric processes. At 70° S latitude, a high-speed jet travels at a speed of 300 m/s.

Question: What dynamic weather does Neptune have?

Question: What does Neptune's wind speeds reach?

Question: What is the high wind speed on Neptune's cloud tops?

Question: Which direction does Neptune's winds move relevant to the plant's rotation?

Question: What is the effect called that describes the flow direction on Neptune?