Full-disc view of Jupiter in natural color in April 2014
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Designations | |||||||||||||||
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Pronunciation | i/ˈdʒuːpᵻtər/ | ||||||||||||||
Adjectives | |||||||||||||||
Orbital characteristics | |||||||||||||||
Epoch J2000 | |||||||||||||||
Aphelion | 92 AU ( 5.454Gm) 816.04 | ||||||||||||||
Perihelion | 29 AU ( 4.950) 740.55 Gm | ||||||||||||||
60 AU ( 5.202) 778.299 Gm | |||||||||||||||
Eccentricity | 498 0.048 | ||||||||||||||
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398.88 d | |||||||||||||||
Average orbital speed
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13.07 km/s | ||||||||||||||
20.020° | |||||||||||||||
Inclination |
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100.464° | |||||||||||||||
273.867° | |||||||||||||||
Known satellites | 67 (as of 2014[update]) | ||||||||||||||
Physical characteristics | |||||||||||||||
Mean radius
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±6 km 69,911 | ||||||||||||||
Equatorial radius
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Polar radius
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Flattening | 87±0.00015 0.064 | ||||||||||||||
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Volume |
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Mass |
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Mean density
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1.326 g/cm3 | ||||||||||||||
m/s2 24.79 2.528 g |
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(estimate) 0.254 | |||||||||||||||
59.5 km/s | |||||||||||||||
Sidereal rotation period
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9.925 h (9 h 55 m 30 s) | ||||||||||||||
Equatorial rotation velocity
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12.6 km/s 300 km/h 45 |
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3.13° (to orbit) | |||||||||||||||
North pole right ascension
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268.057° 17h 52m 14s |
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North pole declination
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64.496° | ||||||||||||||
Albedo | 0.343 (Bond) 0.52 (geom.) |
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to −1.6 −2.94 | |||||||||||||||
29.8″ to 50.1″ | |||||||||||||||
Atmosphere | |||||||||||||||
Surface pressure
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20–200 kPa (cloud layer) | ||||||||||||||
27 km | |||||||||||||||
Composition by volume |
by volume:
Ices:
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by volume:
Ices:
Jupiter is the fifth planet from the Sun and the largest in the Solar System. It is a giant planet with a mass one-thousandth that of the Sun, but two and a half times that of all the other planets in the Solar System combined. Jupiter and Saturn are gas giants; the other two giant planets, Uranus and Neptune are ice giants. Jupiter was known to astronomers in ancient times. The Romans named it after their god Jupiter. When viewed from Earth, Jupiter can reach an apparent magnitude of −2.94, bright enough for its reflected light to cast shadows, and making it on average the third-brightest object in the night sky after the Moon and Venus.
Jupiter is primarily composed of hydrogen with a quarter of its mass being helium, though helium comprises only about a tenth of the number of molecules. It may also have a rocky core of heavier elements, but like the other giant planets, Jupiter lacks a well-defined solid surface. Because of its rapid rotation, the planet's shape is that of an oblate spheroid (it has a slight but noticeable bulge around the equator). The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. A prominent result is the Great Red Spot, a giant storm that is known to have existed since at least the 17th century when it was first seen by telescope. Surrounding Jupiter is a faint planetary ring system and a powerful magnetosphere. Jupiter has at least 67 moons, including the four large Galilean moons discovered by Galileo Galilei in 1610. Ganymede, the largest of these, has a diameter greater than that of the planet Mercury.