Themisto (moon)
Discovery | |
---|---|
Discovered by | Charles Kowal (1975) Elizabeth Roemer (1975) |
Discovery date | September 30, 1975 November 21, 2000 rediscovered |
Orbital characteristics | |
Periapsis | 5,909,000 km (0.039 AU) |
Apoapsis | 8,874,300 km (0.059 AU) |
Mean orbit radius | 7,391,650 km (0.04941 AU) |
Eccentricity | 0.2006 |
129.82761 d (0.3554 a) | |
Average orbital speed | 4.098 km/s |
Inclination | 45.81° (to the ecliptic) 47.48° (to Jupiter's equator) |
Satellite of | Jupiter |
Physical characteristics | |
Mean radius | 4 km[1] |
Circumference | ~25 km |
~200 km² | |
Volume | ~270 km³ |
Mass | 6.89×1014 kg |
Mean density | 2.6 g/cm3 assumed[2] |
~0.0029 m/s2 (0.0003 g) | |
~0.0048 km/s | |
Albedo | 0.04 assumed[1] |
Temperature | ~124 K |
Themisto or Jupiter XVIII, is a small prograde non-spherical moon of Jupiter. It was found in 1975, lost, and then refound in 2000.
Discovery and naming
[change | change source]Themisto was first found by Charles T. Kowal and Elizabeth Roemer on September 30, 1975, reported on October 3, 1975[3] and designated S/1975 J 1. However, not enough observations were made to establish an orbit and it was subsequently lost.
Themisto appeared as a footnote in astronomy textbooks into the 1980s. Then, in 2000, a seemingly new moon was found by Scott S. Sheppard, David C. Jewitt, Yanga R. Fernández and Eugene A. Magnier, and was designated S/2000 J 1. It was soon confirmed that this was the same as the 1975 object. The Sheppard et al. announcement[4] was immediately correlated with an August 6 2000 observation by the team of Brett J. Gladman, John J. Kavelaars, Jean-Marc Petit, Hans Scholl, Matthew J. Holman, Brian G. Marsden, Philip D. Nicholson and Joseph A. Burns — an observation that was reported to the Minor Planet Center but not published as an IAU Circular (IAUC).[5]
In October 2002 it was officially named after Themisto,[6] daughter of the river god Inachus by Zeus (Jupiter) in Greek mythology.
Characteristics
[change | change source]Themisto's orbit is unusual. Unlike most of Jupiter's moons, which orbit in groups, Themisto orbits alone, midway between the Galilean moons and the first group of prograde irregulars.
Themisto is about 8 kilometers in diameter (assuming an albedo of 0.04)[1]
References
[change | change source]- ↑ 1.0 1.1 1.2 Sheppard, S. S.; Jewitt, D. C.; An abundant population of small irregular satellites around Jupiter, Nature, 423 (May 2003), pp. 261-263
- ↑ Physical parameters from JPL
- ↑ IAUC 2845: Probable New Satellite of Jupiter 1975 October 3 (discovery)
- ↑ IAUC 7525: S/1975 J 1 = S/2000 J 1 2000 November 25 (recovery)
- ↑ MPEC 2000-Y16: S/1975 J 1 = S/2000 J 1, S/1999 J 1 2000 December 19 (recovery and ephemeris)
- ↑ IAUC 7998: Satellites of Jupiter 2002 October 22 (naming the moon)
- Ephemeris IAU-MPC NSES
- Mean orbital parameters NASA JPL