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Satellites of Neptune

    
automatic translation Automatic translation    

Moons of Neptune

   

category : satellites of planets

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Before the flying over Neptune by the American probe Voyager-2, in 1989, only two satellites, Triton and Nereid, were known. Since thanks to this flying unless 5000 km of distance to Travel 2, Neptune is much better known.
It is surrounded with a thick atmosphere on base of hydrogen, with helium and with methane. The absorption of the red radiations, by the methane is responsible, some blue tint of the planet.
As we presumed it since observations made from the Earth in 1984 and 1985, Neptune is surrounded with a system of rings formed by rocks and by dusts.
Five different rings were identified, among which very diffuse two, at distances included between 42900 and 62900 km of the planet.

 

The most outside contain three regions of stronger density which correspond to bows observed since the Earth. In 1989, the images taken by Voyager-2 revealed new satellites which form a regular system turning on circular and little tilted orbits. The probe also showed that the planet was surrounded with a complete system of fine rings crimped by brilliant bows. In 2003 the number of satellites of Neptune was 13.

 
NameDiameter kmMass kg
   
Triton2706,82,140×1022
Proteus436×416×4025 ×1019
Larissa 208×1785 ×1018
Galatea204×184×1444 ×1018
Despina180×148×1282 ×1018
Nereid1702 ×1018
Thalassa104×100×524 ×1017
Naiad96×60×522 ×1017
     

Triton

    
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Triton is seventh and bigger of the satellites of Neptune. It carries the name of the god of the Greek mythology. Its orbit is reactionary that is that its sense of rotation is set against that of the rotation of Neptune, it supposes that Triton is an outside body which was captured. The moons which have a reactionary orbit cannot have been formed in the same region of the primitive solar nebula as the planets all around of which they turn: they are thus the captured moons. This scenario because of the mass of Triton, is exceptional in the solar system, the known cases have much smaller sizes.

* [photography taker in 1989 by the probe Voyager 2]

 

 
Triton Lune de Neptune
diameter 2706,8 km
mass 2,140 ×1019 kg
discovered in October 10th 1846
discovered  by William Lassell
     

Proteus

    
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Proteus of irregular shape, is the second biggest moon of Neptune. Protée is an object very dark, looking like the soot, he reflects only 10 % of the light which strikes it. It was discovered on May 24th, 1981 by Harold J. Reitsema, William B. Hubbard, Larry A. Lebofsky and David J. Tholen during an eclipse of star.
Its existence was confirmed in 1989 by Stephen p. Bradford A Synnott and. Smith during the passage of the Voyager probe 2 near Neptune.
Proteus is a celestial body covered with craters of impact. Proteus is the name of a marine god of the Greek mythology who could change at will shape, son of Poseidon.

* [photography taken in august 25th 1989 by the probe Voyager 2]

 

 
Proteus Lune de Neptune
diameter 436×416×402 km
mass 5 ×1019 kg
discovered in may 24th 1981
discovered  by Harold J. Reitsema William B. Hubbard Larry A. Lebofsky David J. Tholen
     

Larissa

    
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Larissa of irregular shape, is the fifth moon of Neptune. It was discovered by Harold J. Reitsema, William B. Hubbard, Larry A. Lebofsky and David J. Tholen during an eclipse of star by Neptune May 24th, 1981. Its existence was confirmed by Stephen p. Synnott during the passage of the Voyager probe 2 near Neptune in 1989. The orbit of Larissa, close to the planet, is unstable and declines towards Neptune.
Larissa will form a new ring or will be absorbed by Neptune. In the Greek mythology, Larissa is a girl of Triopas, a king of Argos.

* [photography taken in august 24th 1989 by the probe Voyager 2]

 

 
Larissa Lune de Neptune
diameter 208×178 km
mass 5 ×1018 kg
discovered in may 24th 1981
discovered  by Harold J. Reitsema
William B. Hubbard
Larry A. Lebofsky
David J. Tholen
     

Galatea

    
astronoo    

Galatea of irregular shape, is the fourth moon of Neptune. It was discovered during the passage of the Voyager probe 2 in 1989.
Its name comes from a Nereid (marine nymph) of the Greek mythology. The orbit of Galatea, close to the planet, is unstable and declines towards Neptune. Galatea will form a new ring or will be absorbed by Neptune.

* [photography taken in 1989 by the probe Voyager 2]

 

 
Galatea Lune de Neptune
diameter 204×184×144 km
mass 4 ×1018 kg
discovered in 1989
discovered  by Stephen P. Synnott
 
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