Ananke (moon)

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Ananke
Ananké.jpg
Ananke on August 15, 1998 at 00:47 UTC from the OHP (Observatoire de Haute-Provence) with a 120-centimeter telescope
Provisional or systematic name Jupiter XII
Central body Jupiter
Properties of the orbit
Major semi-axis 21,276,000 km
Periapsis 16,095,000 km
Apoapsis 26,457,000 km
eccentricity 0.2435
Orbit inclination 148.89 °°
Orbital time 629,770 d
Mean orbital velocity 2.42 km / s
Physical Properties
Albedo 0.04
Apparent brightness 18.75 likes
Medium diameter 28.0 km
Dimensions 3.0  x  10 16 kg
surface 2,463 km 2
Medium density 2.6 g / cm 3
Acceleration of gravity on the surface ≈ 0.010 m / s 2
Escape speed ≈ 16.9 m / s
discovery
Explorer

SB Nicholson

Date of discovery September 28, 1951

Ananke (also Jupiter XII ) is one of the outer moons of the planet Jupiter .

discovery

Ananke was discovered on September 28, 1951 by the astronomer Seth Barnes Nicholson at the Mount Wilson Observatory in California .

The moon was named after Ananke , a lover of Zeus from Greek mythology . It received its official name in 1975. Previously it was referred to as Jupiter's moon XII , as it was the twelfth discovered moon on the planet.

Orbit data

Ananke orbits Jupiter at an average distance of 21.28 million km in 629 days, 18 hours and 29 minutes. The track has an eccentricity of 0.2435. With an inclination of 148.9 ° to the local Laplace plane , the orbit is retrograde , that is, the moon moves around the planet against the direction of rotation of Jupiter.

Ananke is the namesake of a group of moons that move on similar orbits around Jupiter. The Ananke group comprises eight to sixteen moons, with Ananke being the largest member.

Physical data

Ananke has a mean diameter of about 28 km. Their density is estimated at 2.6 g / cm³. It is probably made up mainly of silicate rock. Ananke has a very dark surface with an albedo of 0.04. Their apparent brightness is 18.8 m .

Remarks

  1. The Laplace Plain of Ananke deviates quite clearly from the ecliptic for an outer moon with about 2.4 ° . The reason for this are external disturbances , especially from the large neighboring planet Saturn . The Laplace plane is inclined by about 4.9 ° to the equatorial plane of Jupiter.

Web links

Individual evidence

  1. ^ A b R. A. Jacobson: The Orbits of Outer Jovian Satellites . In: Astronomical Journal . 120, 2000, pp. 2679-2686. doi : 10.1086 / 316817 .
before Jupiter moons after that
Carme Ananke
Leda