Adrastea (moon) Guide, Meaning , Facts, Information and Description
| Discovery | |||||||
|---|---|---|---|---|---|---|---|
| Discovered by | David C. Jewitt G. Edward Danielson | ||||||
| Discovered on | July 8 1979 | ||||||
| Orbital characteristics | |||||||
| Mean radius | 129,000 km | ||||||
| Eccentricity | 0.0018 | ||||||
| Revolution period | 7h 9.5m | ||||||
| Inclination | 0.05° | ||||||
| Is a satellite of | Jupiter | ||||||
| Physical characteristics | |||||||
| Mean diameter | 16.4 km | ||||||
| Surface area | km2 | ||||||
| Mass | 1.8894×1016 kg | ||||||
| Mean density | 4.5 g/cm3 | ||||||
| Surface gravity | 0.012 m/s2 | ||||||
| Surface Gravity (Earth = 1) | 0.00122 | ||||||
| Rotation period | 7h 9.5m | ||||||
| Axial tilt | 0° | ||||||
| Albedo | 0.05 | ||||||
| Surface temp |
| ||||||
| Atmospheric pressure | 0 kPa | ||||||
It belongs to the Amalthea group of small inner jovian moons.
Adrastea is inside Jupiter's planetary ring and may be the source of some of its material. Its orbit lies inside Jupiter's synchronous orbit radius, and as a result tidal forces are slowly causing its orbit to decay. It is also within Jupiter's Roche limit, but is small enough to avoid tidal disruption.
, 1979 by Voyager 2. Adrastea is the dot in the very middle, straddling the line of the Jovian rings.]]
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