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| Voyager 2 image of the blue planet Neptune (NASA/JPL) | Voyager 2 close-up of Neptune showing cloud details and the great dark spot (NASA/JPL) | Voyager 2 view of Neptune and its great dark spot (NASA/JPL) |
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Neptune | Continue Tour to Triton |
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God of the Seas
Leaving Uranus and its moons behind us, we next encounter Uranus's sister planet, Neptune, and its system of moons. Neptune is nearly the same size as Uranus, and its composition is extremely similar. It is also the outermost of the two ice giants. Neptune was named after the Roman god of the seas. It was discovered in 1846 by Johann Gottfried Galle of the Berlin Observatory. Neptune has 14 known moons, most of which were not discovered until after Voyager 2's encounter with the planet in 1989. Most of these moons are quite tiny and are probably captured asteroids. The largest of these moons however, has a diameter of 1,680 miles (2,700 kilometers).
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| Voyager 2 close-up of Neptune showing cloud formations (NASA/JPL) |
Voyager 2 close-up image of Neptune's great dark spot (NASA/JPL) |
Voyager 2 close-up of upper level clouds in Neptune's atmosphere (NASA/JPL) |
The Big Blue Spot
Since Neptune was known to be so similar to Uranus, astronomers were expecting to find another bland and featureless world when Voyager 2 arrived there in August of 1989. Much to the surprise of everyone on the Voyager team, Neptune would turn out to be anything but bland. The most startling feature to be discovered was a giant blue spot in the planet's southern hemisphere. It was very similar in appearance to the famous red spot on Jupiter, and about half the size. In 1994, observations of Neptune by the Hubble space telescope have revealed that the giant blue spot has disappeared. Recently, a new blue spot was observed in the planet's northern hemisphere. Astronomers are not sure why the spot on Neptune was relatively short-lived, while the great red spot on Jupiter has bee present for hundreds of years. This indicates that the Neptune's atmosphere is highly active and prone to sudden and severe changes. Several smaller spots were also noted, as was a small, fast-moving, cloud that astronomers named "scooter".
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| This Voyager 2 close-up of Neptune shows upper level clouds in the atmosphere. This was a surprise to astronomers who were expecting a more uniform atmosphere similar to that of Uranus. (NASA/JPL) |
Features of Neptune
Nearly everything we know about Neptune was learned from the Voyager 2 encounter. Like Uranus, Neptune's blue color is the result of red light being absorbed by methane gas in the planet's upper atmosphere. Neptune's composition is believed to be very similar to that of Uranus. It probably has a small, rocky core about the size of the Earth. This core is thought to be surrounded by an extremely thick layer gases composed mainly of hydrogen and helium with a little methane. Besides the mysterious dark and light spots were other fascinating discoveries. Long, white clouds were seen floating in the planet's upper atmosphere. Neptune has the fastest winds in the Solar System, reaching speeds of 1,200 miles (2,000 kilometers) per hour. Voyager 2 also revealed Neptune's system of delicate rings. There are 4 narrow rings, which are extremely faint. Astronomers think they may be composed of dust particles formed from meteorites smashing into the planet's moons. Like Uranus, Neptune's magnetic field is tilted 47 degrees from its rotational axis. Astronomers believe this is caused by internal forces deep within the planet.
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Jupiter
Saturn
Uranus
Neptune
Pluto
Asteroids
Comets
Interstellar Space
Your Weight on Other Planets
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The Moons of Neptune |
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Name |
Pronunciation |
Order |
Diameter |
Orbital Period |
Distance |
Year |
|
Hippocamp Halimede Sao Laomedeia Psamathe Neso |
NAH-yad tha-LAS-uh des-PEEN-uh gal-uh-TEE-uh la-RISS-uh HIP-uh-kamp PROTE-yoos TRY-tun NEER-ee-id HAL-i-MEE-dee SAY-oh LAY-o-mə-DEE-uh SAM-uh-thee NEE-soh |
1 2 3 4 5 6 7 8 9 10 11 12 13 14 |
66 82 150 176 194 34.8 420 2,707 340 62 44 42 38 60 |
0.29 0.31 0.34 0.43 0.56 0.94 1.12 −5.88 360.13 1,879.08 2,912.72 3,171.33 9,074.30 9,740.73 |
48,227 50,074 52,526 61,953 73,548 105,283 117,646 354,759 5,513,818 16,611,000 22,228,000 23,567,000 48,096,000 49,285,000 |
1989 1989 1989 1989 1981 2013 1989 1846 1949 2002 2002 2002 2003 2002 |
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