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Neptune
Orbit:
4,504,000,000 km or (2,798,785,600 miles) or (30.06 AU) from Sun
Diameter: 49,532 km or 30779 miles (equatorial)
Mass: 1.0247 x 1026 kg or 2.069
x 1026 lbs
Neptune is the eighth planet from the sun and the fourth
largest (by diameter). It is smaller in diameter but larger in mass
than Uranus.
In Roman mythology, Neptune (Greek: Poseidon) was the
god of the sea.
After the discovery of Uranus, it was noticed that its
orbit was not as it should be in accordance with Newton's laws. It was
therefore predicted that another more distant planet must be perturbing
Uranus' orbit. Galle and d'Arrest first observed Neptune on Sept. 23,
1846, very near to the locations independently predicted by Adams and
Le Verrier from calculations based on the observed positions of Jupiter,
Saturn and Uranus. An international dispute arose between the English
and French (though not apparently between Adams and Le Verrier personally)
over priority and the right to name the new planet. Adams and Le Verrier
are now jointly credited with Neptune's discovery.
Subsequent observations have shown that the orbits calculated
by Adams and Le Verrier diverge from Neptune's actual orbit fairly quickly.
Had the search for the planet taken place a few years earlier or later,
it would not have been found anywhere near the predicted location.
Neptune has been visited by only one spacecraft, Voyager
2, on Aug. 25, 1989. Almost everything we know about Neptune comes from
this encounter.
Because Pluto's orbit is so eccentric, it sometimes crosses
the orbit of Neptune. Since 1979, Neptune has actually been the most
distant planet from the sun; Pluto will again be the most distant in
1999.
Neptune's composition is probably similar to Uranus':
various "ices" and rock with about 15 percent hydrogen and a little
helium. Like Uranus, but unlike Jupiter and Saturn, it may not have
a distinct internal layering but have a more or less uniform composition.
But there is most likely a small core (about the mass of the Earth)
of rocky material. Its atmosphere is mostly hydrogen and helium with
a small amount of methane.
Neptune's blue color is the result of absorption of red
light by methane in the atmosphere.
Like a typical gas planet, Neptune has rapid winds confined
to bands of latitude and large storms or vortices. Neptune's winds are
the fastest in the solar system, reaching 2,000 km/hour (1,250 miles/hour).
Like Jupiter and Saturn, Neptune has an internal heat
source -- it radiates more than twice as much energy as it receives
from the sun.
At the time of the Voyager encounter, Neptune's most prominent
feature was the Great Dark Spot in the southern hemisphere. It was about
half the size as Jupiter's Great Red Spot (about the same diameter as
Earth). Neptune's winds blew the Great Dark Spot westward at 300 meters/second
(700 mph). Voyager 2 also saw a smaller dark spot in the southern hemisphere
and a small irregular white cloud that zips around Neptune every 16
hours or so now known as "The Scooter" (right). It may be a plume rising
from lower in the atmosphere, but its true nature remains a mystery.
However, HST observations of Neptune in 1994 show that
the Great Dark Spot has disappeared! It has either simply dissipated
or is currently being masked by other aspects of the atmosphere. A few
months later, HST discovered a new dark spot in Neptune's northern hemisphere.
This indicates that Neptune's atmosphere changes rapidly, perhaps due
to slight changes in the temperature differences between the tops and
bottoms of the clouds.
Neptune also has rings. Earth-based observations showed
only faint arcs instead of complete rings, but Voyager 2's images showed
them to be complete rings with bright clumps. One of the rings appears
to have a curious twisted structure.
Like Uranus and Jupiter, Neptune's rings are very dark;
but their composition is unknown.
Neptune's rings have been given names: the outermost is
Adams (which contains three prominent arcs now named Liberty, Equality
and Fraternity), next is an unnamed ring coorbital with Galatea, then
Leverrier (whose outer extensions are called Lassell and Arago), and
finally the faint but broad Galle.
Neptune's magnetic field is, like Uranus', oddly oriented
and probably generated by motions of conductive material (probably water)
in its middle layers.
Neptune can be seen with binoculars (if you know exactly
where to look), but a large telescope is needed to see anything other
than a tiny disk.
Neptune's Satellites
Neptune has eight known moons -- seven small ones and Triton.
| Satellite |
Distance
(000 km) |
Radius
(km)
|
Mass
(kg) |
Discoverer
|
Date
|
| Naiad |
48 |
29 |
? |
Voyager 2 |
1989 |
| Thalassa |
50 |
40 |
? |
Voyager 2 |
1989 |
| Despina |
53 |
74 |
? |
Voyager 2 |
1989 |
| Galatea |
62 |
79 |
? |
Voyager 2 |
1989 |
| Larissa |
74 |
96 |
? |
Voyager 2 |
1989 |
| Proteus |
118 |
209 |
? |
Voyager 2 |
1989 |
| Triton |
355 |
1350 |
2.14e22 |
Lassell |
1946 |
| Nereid |
5509 |
170 |
? |
Kuiper |
1949 |

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