 |
|
 |
 |
|
 |
 |
|
|
|
 |
|
Neptune |
 |
|
 |
|
 |
Voyager 2 photo of the
blue planet Neptune
(NASA/JPL) |
|
Voyager 2 close-up of Neptune showing cloud details
(NASA/JPL) |
|
Voyager 2 close-up of Neptune and its great dark spot
(NASA/JPL) |
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 great gas 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 13 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).
 |
|
 |
|
 |
Voyager 2 closeup of Neptune showing cloud formations
(NASA/JPL) |
|
Voyager 2 close-up of upper level clouds in Neptune's atmosphere
(NASA/JPL) |
|
Voyager 2 close-up image of Neptune's great dark spot
(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".
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.
| Statistics for Neptune |
| Discovered by |
...... |
Johann Gottfried Galle |
| Year of Discovery |
...... |
1846 |
| Diameter |
...... |
30,744 miles (49,492 km) |
| Number of Natural Satellites |
...... |
8 |
| Mean Distance from the Sun |
...... |
2,798,116,000 miles (4,504,300,000 km) |
| Rotational Period |
...... |
15.8 hours |
| Orbital Period |
...... |
165 years |
| Orbital Eccentricity |
...... |
0.009 |
| Orbital Inclination |
...... |
1.774 degrees |
| Inclination of Axis |
...... |
29.31 degrees |
| Mean Cloud Temperature |
...... |
-315° F (-193° C) |
| Main Atmospheric Component |
...... |
Hydrogen |
| Atmospheric Pressure |
...... |
2 bars |
| Apparent Magnitude |
...... |
7.84 |
|
|
|
The Moons of Neptune
Listed in order of distance from Neptune
Click on linked names for more information
|
| Name |
Diameter (km) |
Distance (km) |
Year
Discovered |
| Naiad |
67 |
48,200 |
1989 |
| Thalassa |
83 |
50,000 |
1989 |
| Despina |
152 |
52,500 |
1989 |
| Galatea |
175 |
62,000 |
1989 |
| Larissa |
195 |
73,500 |
1989 |
| Proteus |
418 |
117,600 |
1989 |
| Triton |
2707 |
354,800 |
1846 |
| Nereid |
340 |
5,513,400 |
1949 |
| Halimede |
60 |
15,782,000 |
2002 |
| Sao |
38 |
22,422,000 |
2002 |
| Laomedeia |
38 |
23,571,000 |
2002 |
| Psamathe |
28 |
46,695,000 |
2002 |
| Neso |
60 |
48,387,000 |
2003 |
|
|
|

|
|
 |
|