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Satellites of Mars

    

automatic translation

    

astronoo Mercury Mercury the first planet of the solar system in 57,9 million km of the sun is, its diameter is 4880 km. astronoo Venus Venus the second planet of the solar system in 108,2 million km of the sun is, its diameter is 13000 km. astronoo Earth Earth the third planet of the solar system in 149,6 million km of the sun is, its diameter is 12756 km. astronoo Mars Mars the fourth planet of the solar system in 227,9 million km of the sun is, its diameter is 6800 km. astronoo Jupiter Jupiter the fifth planet of the solar system in 778 million km of the sun is, its diameter is 143000 km. astronoo Saturn Saturn the sixth planet of the solar system in 1427 million km of the sun is, its diameter is 120500 km. astronoo Uranus Uranus the seventh planet of the solar system in 2870 million km of the sun is, its diameter is 51120 km.  astronoo Neptune Neptune the eighth planet of the solar system in 4496 million km of the sun is, its diameter is 49530 km. 
astronoo Moon Earth possess that a single natural satellite, the Moon which orbits in 160000 km of the earth.  astronoo satellites of Mars Mars possess 2 known natural satellites, Phobos and Deimos. They orbit near the planet, in some thousand kilometers of this one.  astronoo satellites of Jupiter Jupiter possess more than 60 known natural satellites, among which Ganymede, Io, Callisto, Europe and the others... astronoo satellites of Saturn Saturn possess 59 known natural satellites, of which Titan, Rhea, Iapetus, Dioné, Thetis, Enceladus, Mimas, Hyperion, Phoebe, Janus, Epimetheus, Prometheus, Pandora and the others... astronoo satellites of Uranus Uranus possess at least 27 known natural satellites, among which Titania, Oberon, Umbriel, Ariel... astronoo satellites of Neptune Neptune possess tens of known natural satellites, of which Triton, Proteus, Larissa, Galatea, Despina, Nereid, Thalassa, Naiad...

     

Moons of Mars

    

    

Both moons of the planet are Phobos and Deimos (names pulled by the sons of the god Ares in antique Greece).
They orbit near the planet, in some thousand kilometers of this one.
They are bound in Mars by the strengths of tides, always showing the same face in its direction. As Phobos orbits around Mars more quickly than turns the planet itself, the strengths of tides make decrease its orbital beam in a slow, but constant way, at the rate of 9 cm a year.

 

In 20 in 40 million years, Phobos will crash on the Martian surface. Deimos, on the other hand, is taken away enough so that its orbit tends rather to go away, it in a infinitely slow way.
It is an allusion to a Greek verse, " The God of the war arrives, flanked by its two satellites (hired men) fear and terror " phobos mean in Greek 'fear', and Deimos 'terror'.

 

 

     

Phobos

   

category : satellites of planets


    

Deimos and Phobos is constituted by rocks rich in carbon and by ice (as the asteroids of type - C). Both are strewed with craters of impact as all the telluric objects of the solar system.
The orbit of Phobos is below the beam orbital synchronous. It gets up on the West, moves very quickly through the sky and goes to bed in the East, usually twice a day.
It is if near Mars where he cannot be observed over the horizon completely by the surface. Phobos is condemned because its orbit being below the synchronous height, the strengths of tides decrease gradually its orbital beam at the 1,8 meter rate by century.
In approximately 40 million years, it will break to form a ring around Mars or it will crash on its surface.

 

 
Phobos Lune de Mars
diameter 26,8×21×18,4 km
mass 1,070x1016 kg
discovered in  august 20th 1877
discovered by Asaph Hall
distance of Mars 9 380 km
     

Deimos

   

category : satellites of planets


    

Deimos would be originally a primitive meteorite, because quite as Phobos, her composition differs from that of the Mars.
This moon would have formed in the external belt of asteroids between Mars and Jupiter, because its color and its density are close to asteroids of type C, common in this belt of asteroids.
It is a small rotating, very dark irregular body of shape there 30H18mn on its orbit in 23 460 km.
It is in synchronous rotation, presenting, quite as Phobos or the Moon, always the same in front of the planet.
Too close to Mars, he cannot any more be visible beyond the 82nd parallel.
Deimos seems smooth with its ground swamped with dust of regolith, no crater exceeds 3000 m of diameter.
The surface seems exempt of streak.
Considering his weak gravity 4.10-4g, due to his small size, a man would take off by jumping in 36 kph, what amounts to an escape speed of 10m/s.

 

 
Deimos Lune de Mars
diameter 15×12×10,4 km
mass 0,224x1016 kg
discovered in  august 17th 1877
discovered by Asaph Hall
distance of Mars 23 460 km
     

Related subjects

   

category : satellites of planets


    

Mars

 astronoo Deimos as seen by MRO astronoo Dwarf Planets

Phobos

 

Deimos

  
     

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The universe is all worked up

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Astronomy - october 15th 2007