Neptune

 
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Neptune, like its twin, Uranus, has an atmosphere composed of hydrogen, helium, methane, and ammonia. The methane creates the blue color. Neptune's internal structure is also the same as that of Uranus.

The core of Neptune is probably composed of liquid rock. Then, farther up, the liquid rock slowly gives way to an ocean, primarily containing hydrogen, helium, and water, but also ammonia and methane. This "ocean" accounts for most of Neptune's bulk. The ocean slowly thins out into the atmosphere.

This atmosphere contains much more detail than Uranus'. It has swirls of clouds and high-altitude cirrus clouds, as well as gigantic storms.

Neptune also has a faint system of rings. The rings are made of pieces of material the size of a car or truck. There is about one thousandth of the matter in Neptune's rings as in Uranus'. If the rings were all rolled into a ball, the ball would be only a couple of miles across. That matter is spread across 125,000 km (77,500 miles).

In the outermost ring of Neptune, there are three anomalies called the "Three Arcs of Neptune." They are areas where the rings are relatively dense. Over the millions of years that these have existed, the particles in the arcs should have spread out until the ring was a uniform density. However, this has not happened. Scientists now believe that these arcs are shepherded by small moons.

Unique Characteristics

Neptune has a few features that no other planet has. Once Uranus had been discovered, perturbations in its orbit were seen. Calculations were made, and it was predicted that there should be a planet within a certain patch of sky. Within hours, Neptune was discovered in 1846.

The first feature that is unique to Neptune is the Great Dark Spot (left). It is a depression in the atmosphere surrounded by high cirrus clouds. Neptune's Great Dark Spot does not appear to be stable, though. A few years after the Voyagers found it, it had disappeared (Hubble Space Telescope pictures at the right). Then, in 1995, it reappeared in Neptune's northern hemisphere.

When the Great Dark Spot was first discovered, it was thought to be moving very slowly. However, when Neptune's rotation rate was finally determined, it showed that the Great Dark Spot wasn't moving slowly with the planet, but was actually moving in a direction opposite the planet's spin at almost supersonic speeds. These are ten times hurricane speeds on Earth.

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Neptune's Satellite

Neptune has 13 known moons. They are composed of rock and ice. Triton has a retrograde orbit. Nereid has a highly elliptical orbit. Voyager 2 discovered 6 of the moons not observable from Earth. Very recently, three more moons, S/2002 N1-3, were discovered from a ground-based telescope in 2002.The first four moons of Neptune, Naiad, Thalassa, Despina, and Galatea, are so close to Neptune that they orbit within its ring system. Little is known about them.

The next one out, Larissa, was actually discovered in 1981, when it blocked a star. This was attributed to the ring arcs, but later was found to be the moon, being re-discovered by Voyager 2 in 1989.

Proteus is the second-largest moon in orbit around Neptune. It is so close to the planet that Earth-bound telescopes cannot see it.

Triton is next, and is one of the strangest moons in the solar system. First, it is one of only three moons in the solar system that has an atmosphere (Jupiter's Io and Saturn's Titan are the other two). It is thicker than Io's, yet much thinner than Titan's. Its pressure is 1/100,000 of Earth's.

The eighth moon, Nereid, has a highly elliptical orbit that causes it to swing around Neptune at various distances. When closest, it is 1,342,530 km (834,210 miles) from the planet. At the farthest distance, it is 9,667,120 km (6,006,870 miles) from Neptune.

The last five moons were discovered in the first few weeks of and throughout 2003. They have not yet been given official names by the International Astronomical Union. Very little is yet known about them.

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