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hor_green_bar1.jpg Ariel hor_green_bar1.jpg


Uranus' Moon: ArielDiscovered in 1851 by William Lassell, Ariel is the brightest satellite of Uranus. Ariel is 191,240 kilometers from Uranus and has an equatorial radius of 578.9 kilometers. The surface bears many heavy impact craters from millions of years of meteorite impact.

In addition, there are long, deep rift valleys that extend across the surface, much like that on Mars. The bases of the valleys have been smoothed by a fluid (not water), possibly ammonia, methane or carbon monoxide.



PHYSICAL DATA FOR ARIEL
 Mass (kg) 1.27e + 21
 Mass (Earth = 1) 2.1252e - 04
 Radius (km) 578.9
 Radius (Earth = 1) 9.0765e - 02
 Mean Density (g/cm3) 1.56
 Mean Distance from Uranus (km) 191,240
 Magnitude (V0) 14.16

 

ORBITAL DATA FOR ARIEL
 Rotational period (days) 2.520379
 Orbital period (days) 2.520379
 Mean orbital velocity (km/s) 5.52
 Orbital eccentricity 0.0034
 Orbital inclination (degrees) 0.31
 Escape (km/s) 0.541
 Albedo 0.34

 

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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