romikgosai/squad_modified_2 huggingface dataset:
Most elevators have a location in which the permit for the building owner to operate the elevator is displayed. While some jurisdictions require the permit to be displayed in the elevator cab, other jurisdictions allow for the operating permit to be kept on file elsewhere – such as the maintenance office – and to be made available for inspection on demand. In such cases instead of the permit being displayed in the elevator cab, often a notice is posted in its place informing riders of where the actual permits are kept.

Q1: Whose name is on the permit required for operation of an elevator?
A1: the building owner
Q2: Do all jurisdictions require the permit to be displayed in the elevator?
A2: some jurisdictions require the permit to be displayed in the elevator cab, other jurisdictions allow for the operating permit to be kept on file elsewhere
Q3: Aside from the elevator, where else might a permit be displayed?
A3: the maintenance office
Q4: What type of notice can be displayed in the elevator in lieu of the permit?
A4: a notice is posted in its place informing riders of where the actual permits are kept.
As of January 2008, Spain is the nation with the most elevators installed in the world, with 950,000 elevators installed that run more than one hundred million lifts every day, followed by United States with 700,000 elevators installed and China with 610,000 elevators installed since 1949. In Brazil, it is estimated that there are approximately 300,000 elevators currently in operation. The world's largest market for elevators is Italy, with more than 1,629 million euros of sales and 1,224 million euros of internal market.

Q1: What country had the second most elevators installed?
A1: United States
Q2: In 2008, what country had the largest number of elevators?
A2: Spain
Q3: How many elevators had China installed since 1949?
A3: 610,000
Q4: What country boasts the worlds largest market for elevators?
A4: Italy
Q5: How many elevators are in Brazil?
A5: 300,000
Double deck elevators are used in the Taipei 101 office tower. Tenants of even-numbered floors first take an escalator (or an elevator from the parking garage) to the 2nd level, where they will enter the upper deck and arrive at their floors. The lower deck is turned off during low-volume hours, and the upper deck can act as a single-level elevator stopping at all adjacent floors. For example, the 85th floor restaurants can be accessed from the 60th floor sky-lobby. Restaurant customers must clear their reservations at the reception counter on the 2nd floor. A bank of express elevators stop only on the sky lobby levels (36 and 60, upper-deck car), where tenants can transfer to "local" elevators.

Q1: What type of elevators are used in the Taipei 101 office tower?
A1: Double deck elevators
Q2: During what hours is the lower deck turned off?
A2: low-volume hours
Q3: During the low volume hours, what can the upper deck function as?
A3: a single-level elevator stopping at all adjacent floors
Q4: On what floor must restaurant customers clear their reservations?
A4: at the reception counter on the 2nd floor
Q5: What levels make up the "sky lobby"?
A5: 36 and 60, upper-deck car
The high-speed observation deck elevators accelerate to a world-record certified speed of 1,010 metres per minute (61 km/h) in 16 seconds, and then it slows down for arrival with subtle air pressure sensations. The door opens after 37 seconds from the 5th floor. Special features include aerodynamic car and counterweights, and cabin pressure control to help passengers adapt smoothly to pressure changes. The downwards journey is completed at a reduced speed of 600 meters per minute, with the doors opening at the 52nd second.

Q1: How fast do the observation deck elevators travel?
A1: 1,010 metres per minute (61 km/h) in 16 seconds
Q2: This speed holds what record?
A2: world-record certified speed
Q3: What does cabin pressure control do?
A3: help passengers adapt smoothly to pressure changes
Q4: How fast does the elevator drop down?
A4: 600 meters per minute
Q5: At what floor do the doors open on the way down?
A5: 52nd
The Twilight Zone Tower of Terror is the common name for a series of elevator attractions at the Disney's Hollywood Studios park in Orlando, the Disney California Adventure Park park in Anaheim, the Walt Disney Studios Park in Paris and the Tokyo DisneySea park in Tokyo. The central element of this attraction is a simulated free-fall achieved through the use of a high-speed elevator system. For safety reasons, passengers are seated and secured in their seats rather than standing. Unlike most traction elevators, the elevator car and counterweight are joined using a rail system in a continuous loop running through both the top and the bottom of the drop shaft. This allows the drive motor to pull down on the elevator car from underneath, resulting in downward acceleration greater than that of normal gravity. The high-speed drive motor is used to rapidly lift the elevator as well.

Q1: What is the name of the elevator attraction at the Disney World parks across the world?
A1: The Twilight Zone Tower of Terror
Q2: What is the main feature of this attraction?
A2: a simulated free-fall achieved through the use of a high-speed elevator system
Q3: Do ride goers stand or sit?
A3: passengers are seated and secured in their seats rather than standing
Q4: What unique feature does this ride provide guests?
A4: downward acceleration greater than that of normal gravity
Q5: What type of motor is used?
A5: high-speed drive motor
The passenger cabs are mechanically separated from the lift mechanism, thus allowing the elevator shafts to be used continuously while passengers board and embark from the cabs, as well as move through show scenes on various floors. The passenger cabs, which are automated guided vehicles or AGVs, move into the vertical motion shaft and lock themselves in before the elevator starts moving vertically. Multiple elevator shafts are used to further improve passenger throughput. The doorways of the top few "floors" of the attraction are open to the outdoor environment, thus allowing passengers to look out from the top of the structure.

Q1: How are passenger cabs separated from the lift?
A1: mechanically
Q2: What type of vehicles are the passenger cabs?
A2: automated guided vehicles or AGVs
Q3: What action do the cabs take before the elevator begins to move?
A3: move into the vertical motion shaft and lock themselves in
Q4: What is special about the doorways of the top floors?
A4: The doorways of the top few "floors" of the attraction are open to the outdoor environment
Q5: What does this allow riders to do at the top?
A5: look out from the top of the structure
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.

Q1: What are the 67th, 69th, and 70th floors of the GE Building at Rockerfeller Center nicknamed?
A1: "Top of the Rock"
Q2: What do these floors serve as?
A2: observation decks
Q3: What type of elevator is featured?
A3: high-speed glass-top
Q4: How long is the short trip?
A4: about 60 seconds
Q5: The special effects include blue light, music playing and what else?
A5: various animations are also displayed on the ceiling
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.

Q1:  The Haunted Mansion at Disneyland in California and the one in Paris, France sharewhat attribute?
A1: takes place on an elevator
Q2: What is the name of area that is really an elevator?
A2: The "stretching room"
Q3: What is included in the elevator's design?
A3: The elevator has no ceiling and its shaft is decorated to look like walls of a mansion
Q4: What is the illusion given by these effects?
A4: the illusion of the room stretching
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.

Q1: What planet is Neptune's near-twin?
A1: Uranus
Q2: What is Neptune named after?
A2: Roman god of the sea
Q3: How much more dense is Neptune compared to Earth?
A3: 17 times
Q4: What does the astronomical sign of Neptune represent?
A4: god Neptune's trident
Q5: How many Earth years does Neptune orbit the sun?
A5: 164.8 years
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.

Q1: How was Neptune found?
A1: mathematical prediction
Q2: When was Neptune first observed?
A2: 23 September 1846
Q3: Who discovered Neptune?
A3: Alexis Bouvard
Q4: What is Neptune's largest moon?
A4: Triton
Q5: What flew by Neptune in 1989?
A5: Voyager 2
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.

Q1: Which planet is compositionally similar to Neptune?
A1: Uranus
Q2: What is Neptune's atmosphere primarily composed of?
A2: hydrogen and helium
Q3: What is the interior of Neptune composed of?
A3: ices and rock
Q4: What makes Neptune blue?
A4: methane
Q5: What "ices" makes up Neptune?
A5: water, ammonia, and methane
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.

Q1: What weather did Voyager 2 observe on Neptune?
A1: Great Dark Spot
Q2: What weather feature does Neptune have stronger than any other planet?
A2: sustained winds
Q3: What were the wind speeds recorded on Neptune?
A3: 2,100 kilometres per hour
Q4: What is the cloud tops on Neptune temperature?
A4: 55 K (−218 °C).
Q5: What is Neptune's planet center temperature?
A5: 5,400 K (5,100 °C)
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.

Q1: Who drew Neptune after observing it with a telescope?
A1: Galileo
Q2: What was Neptune mistaken for at first?
A2: a fixed star
Q3: What happens when Neptune goes retrograde?
A3: Earth's orbit takes it past an outer planet
Q4: What date was Neptune drawn first?
A4: 28 December 1612
Q5: Who recently researched the original observation of Neptune?
A5: David Jamieson
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.

Q1: What year did Alexis Bouvard publish relevant astronomical tables?
A1: 1821
Q2: What did Alexis Bouvard study?
A2: the orbit of Neptune's neighbour Uranus
Q3: When did John Couch Adams begin working on the orbit of Uranus?
A3: 1843
Q4: Who gave John Couch Adams extra data?
A4: Sir George Airy
Q5: What did the extra data John Couch Adams received produce?
A5: several different estimates of a new planet
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.

Q1: Who was Henrich d'Arrest?
A1: student at the observatory
Q2: When did Galle discover Neptune?
A2: 23 September 1846
Q3: How many degrees off was Adams' prediction?
A3: 12°
Q4: What did Henrich d'Arrest seek to find?
A4: the displacement characteristic of a planet
Q5: What was Challis looking for when he saw Neptune the first two times?
A5: comet observations
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."

Q1: What two countries argued over credit for the discovery of Neptune?
A1: French and the British
Q2: Who ultimately deserved credit for the discovery of Neptune?
A2: Le Verrier and Adams
Q3: Who questioned Adams's claim to co-discovery of Neptune?
A3: Dennis Rawlins
Q4: Who predicted Neptune's place and convinced astronomer's to search for it?
A4: Le Verrier
Q5: Who did not deserve credit to co-discovery of Neptune?
A5: Adams
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.

Q1: Who claimed the right to name Neptune?
A1: Le Verrier
Q2: What country approved Neptune's first name?
A2: France
Q3: What did the discoverer want to name Neptune first?
A3: Le Verrier
Q4: What first introduced Neptune and Uranus's names?
A4: French almanacs
Q5: Who did not approve of the first name for Neptune?
A5: French Bureau des Longitudes
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.

Q1: What is the Chinese, Japanese, and Korean translations for Neptune?
A1: sea king star
Q2: What god was Neptune?
A2: god of the sea
Q3: What is the Mongolian name for Neptune?
A3: Dalain Van
Q4: What did the Greeks call Neptune?
A4: Poseidon
Q5: What was the Biblical sea monster that Neptune is named in Hebrew?
A5: Rahab
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.

Q1: What was Neptune before Pluto was discovered?
A1: farthest known planet
Q2: What discovery made astronomer's debate Pluto's status as a planet?
A2: the Kuiper belt
Q3: What year did the International Astronomical Union define the word planet?
A3: 2006
Q4: Now that Pluto isn't a planet, what is Neptune known for in our solar system?
A4: the outermost known planet
Q5: What period was Pluto closer to the sun than Neptune?
A5: between 1979 and 1999
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".

Q1: What is Neptune's mass?
A1: 1.0243×1026 kg
Q2: How much more mass does Neptune have compared to Earth?
A2: 17 times
Q3: What is Neptune's gravity at 1 bar?
A3: 11.15 m/s2
Q4: What is Neptune's equatorial radius?
A4: 24,764 km
Q5: What is Neptune referred to due to it's size and concentration of volatiles?
A5: ice giant
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'.

Q1: What is Neptune's mantle rich in?
A1: water, ammonia and methane
Q2: What is the hot, dense fluid in Neptune referred to as?
A2: icy
Q3: What does the fluid in Neptune have a high conductivity of?
A3: electrical
Q4: How deep does Neptune's water-ammonia ocean go?
A4: 7000 km
Q5: What rains on Neptune?
A5: diamond crystals