Mars's Moon - Deimos

D eimos (panic) is a moon of Mars and was named after an attendant of the Roman war god Mars. It was discovered by Asaph Hall in 1877. Deimos is a dark body that appears to be composed of C-type surface materials. It is similar to the C-type (blackish carbonaceous chondrite) asteroids that exist in the outer asteroid belt. Some scientists speculate that Deimos and Phobos (the other martian moon), are captured asteroids; however, other scientists present arguments counter to this theory. Both Deimos and Phobos are saturated with craters. Deimos has a smoother appearance caused by partial filling of some of its craters.

PHYSICAL DATA FOR DEIMOS
 Mass (kg) 1.8e + 15
 Mass (Earth = 1) 3.0120e - 10
 Radius (km) 7.5 x 6.1 x 5.5
 Radius (Earth = 1) 1.1759e - 03
 Mean Density (g/cm3) 1.7
 Mean Distance from Jupiter (km) 23,460
 Magnitude (V0) 12.40


ORBITAL DATA FOR DEIMOS
 Rotational period (days) 1.26244
 Orbital period (days) 1.26244
 Mean orbital velocity (km/s) 1.36
 Orbital eccentricity 0.00
 Orbital inclination (degrees) 0.9 - 2.7
 Escape (km/s) 0.0057
 Albedo 0.07


Physical Data Key
 
Mass Mass
Mass Mass compared to that of Earth.
Radius Radius
Radius Radius compared to that of Earth.
Mean Density Average Density.
Distance Distance to the planet's center.
Magnitude The brightness of a star or object.
 
 
Orbital Data Key
 
Rotational Period Number of days to make one complete rotation.
Orbital Period Number of days to obital the planet.
Mean Orbital Velocity Average obital speed.
Orbital Eccentricity Eccentricity.
Orbital Inclination The tilt of the moon or planet.
Escape Escape Velocity.
Albedo Visual geometric albedo.

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