Neptune's Satellites
 
 
 Neptune
 
 
Satellite Period 
(days)
Inclination 
(degrees)
Eccentricity Density 
(kg/m^3)
Albedo
Naiad 0.294396 4.74 0.00 N/A 0.06
Thalassa 0.311485 0.21 0.00 N/A 0.06
Despina 0.334655 0.07 0.00 N/A 0.06
Galatea 0.428745 0.05 0.00 N/A 0.06
Larissa 0.554654 0.20 0.00 N/A 0.06
Proteus 1.122315 0.55 0.00 N/A 0.06
Triton 5.876854 R 156.834 N/A 2,054 0.7
Nereid 360.13619 7.23 0.7512 N/A 0.2
    *R indicates retrograde motion
 
 
 That's great but what is this stuff?
 

Naiad
 
 

    Naiad ( "NAY ed" ) is the innermost of Neptune's known satellites:

            orbit:    48,200 km from Neptune
            diameter: 58 km
            mass:     N/A

    The Naiads were the nymphs who lived in and presided over brooks, springs, and fountains.

    The last of the satellites discovered in 1989 by Voyager 2.

    Naiad, Thalassa, Despina and Galatea are all irregularly shaped.
 
 

Thalassa
 
 

    Thalassa ("tuh LASS eh") is the second of Neptune's known satellites:

            orbit:    50,000 km from Neptune
            diameter: 80 km
            mass:     N/A

    "Thalassa" is the Greek word for "sea".

    Discovered in 1989 by Voyager 2.
 
 
 

Despina
 
 

    Despina is the third of Neptune's known satellites:

            orbit:    52,600 km from Neptune
            diameter: 148 km
            mass:     N/A

    Despina was a nymph, the daughter of Poseidon (Neptune) and Demeter.

    Discovered in 1989 by Voyager 2.
 
 
 

Galatea
 
 

    Galatea ("gal eh TEE eh") is the fourth of Neptune's known satellites:

            orbit:    62,000 km from Neptune
            diameter: 158 km
            mass:     N/A

    Galatea was a Sicilian Nereid loved by the Cyclops Polyphemus. (Not related to the maiden who was
    originally a statue carved by Pygmalion and who was brought to life by Aphrodite.)

    Discovered in 1989 by Voyager 2.
 
 

Larissa
 
 

    Larissa ("LA ree suh") is the fifth of Neptune's known satellites:

            orbit:    73,600 km from Neptune
            diameter: 193 km (208 x 178)
            mass:     N/A

    Larissa was the mother by Poseidon (Neptune) of Pelasgus.

    Larissa was "officially" discovered in 1989 by Voyager 2 though it was observed in 1981 by Dave Tholen
    and colleagues using the stellar occultation method.

    Like Proteus, Larissa is irregular (non-spherical) in shape and appears to be heavily cratered.
 
 

Proteus

    Proteus ("PROH tee us") is the sixth of Neptune's known satellites and the second largest:

            orbit:    117,600 km from Neptune
            diameter: 418 km (436 x 416 x 402)
            mass:     N/A

    Proteus was a sea god who could change his shape at will.

    Discovered in 1989 by Voyager 2. Though it is larger than Nereid, it was not discovered earlier because it
    is very dark and so close to Neptune that it is difficult to see in the glare of the much brighter planet.

    Proteus is irregular (non-spherical) in shape. Proteus is probably about as big as an irregular body can be
    before its gravity pulls it into a more spherical shape.

    The heavily cratered surface shows no signs of geologic activity.
 
 
 

Triton

    Triton ("TRY ton") is the seventh and by far the largest of Neptune's satellites:

            orbit:    354,760 km from Neptune
            diameter: 2700 km
            mass:     2.14e22 kg

    Discovered by Lassell in 1846 only a few weeks after the discovery of Neptune itself.

    In Greek mythology, Triton is a god of the sea, the son of Poseidon (Neptune); usually portrayed as having
    the head and trunk of a man and the tail of a fish.

    Triton has been visited by only one spacecraft, Voyager 2 on Aug 25 1989. Almost everything we know
    about  it comes from this encounter.

    Triton's orbit is retrograde. It is the only large moon to orbit "backwards", the only other moons with
    retrograde orbits are Jupiter's moons Ananke, Carme, Pasiphae and Sinope and Saturn's Phoebe all of
    which are less than 1/10 the diameter of Triton. Triton may may originated elsewhere (perhaps in the Kuiper
    Belt?) and later been captured by Neptune (perhaps involving a collision with another now shattered
    Neptunian moon). A capture scenario could account not only for Triton's orbit but also for the unusual orbit of
    Nereid and provide the energy needed to melt and differentiate Triton's interior.

    Because of its retrograde orbit, tidal interactions between Neptune and Triton remove energy from Triton
    thus  lowering its orbit (and speeding up Neptune's rotation). At some very distant future time it will either
    break up (perhaps forming a ring) or crash into Neptune.

    The unusual nature of Triton's orbit, the similarity of bulk properties between Pluto and Triton, and the highly
    eccentric, Neptune-crossing nature of Pluto's orbit suggest some historical connection between them.
    Exactly what this might be is purely conjecture at this time however.

    Triton's axis of rotation is also unusual, tilted 157 degrees with respect to Neptune's axis   (which is in turn
    inclined 30 degrees from the plane of Neptune's orbit). This adds up to an orientation with respect to the Sun
    somewhat like Uranus's with polar and equatorial regions alternately pointing toward the Sun. This probably
    results in radical seasonal changes as one pole then the other moves into the sunlight. During the Voyager 2
    encounter, Triton's south pole was facing the Sun.

    Triton's density (2.0) is slightly greater than that of Saturn's icy moons (e.g. Rhea). Triton is probably only
    about 25% water ice with remainder rocky material.

    Voyager found that Triton has an atmosphere, albeit a very tenuous one (about 0.01 millibar), composed
    mostly of nitrogen with a small amount of methane. A thin haze extends up 5-10 km.

    The temperature at the surface of Triton is only 34.5 K (-235 C, -391 F), as cold as Pluto. This is due in part
    to its high albedo (.7 - .8) which means that little of the Sun's meager light is absorbed. At this temperature
    methane, nitrogen and carbon dioxide all freeze solid.

    There are very few craters visible; the surface is relatively young. Almost the entire southern hemisphere is
    covered with an "ice cap" of frozen nitrogen and methane.

    There are extensive ridges and valleys in complex patterns all
    over Triton's surface. These are probably the result of
    freezing/thawing cycles (right).

The most interesting (and totally unexpected) features of this unusually interesting world are the ice volcanoes. The eruptive material is probably liquid nitrogen, dust, or methane compounds from beneath the surface. One of Voyager's images shows an actual plume rising 8 km above the surface and extending 140 km "downwind" (left).
 
 

    Triton, Io and Venus are the only bodies in the solar system besides Earth that are known to be volcanically
    active at the present time (though Mars clearly was in the past). It's also interesting to note that very different
    volcanic processes occur in the outer solar system. Earth's and Venus' (and Mars') eruptions are of rocky
    material and are driven by internal heat. Io's eruptions are probably sulfur or sulfur compounds driven by tidal
    interactions with Jupiter. Triton's eruptions are of very volatile compounds like nitrogen or methane driven by
    seasonal heating from the Sun.
 
 
 

Nereid
 
 

    Nereid ( "NEER ee ed"  ) is the outermost of Neptune's known satellites and the third largest:

            orbit:    5,513,400 km distance from Neptune
            diameter: 340 km
            mass:     N/A

    Nereid is any one of the sea nymphs, the 50 daughters of Nereus and Doris.

    Discovered in 1949 by Kuiper.

    Nereid's orbit is the most highly eccentric of any planet or satellite in the solar system; its distance from
    Neptune varies from 1,353,600 to 9,623,700 kilometers.

    Nereid's odd orbit indicates that it may be a captured asteroid or Kuiper Belt object.
 
 
 

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