Themisto (moon)

From Simple English Wikipedia, the free encyclopedia
Discovered byCharles Kowal (1975)

Elizabeth Roemer (1975)
Scott S. Sheppard (2000)
David C. Jewitt (2000)
Yanga R. Fernández (2000)

Eugene A. Magnier (2000)
Discovery dateSeptember 30, 1975
November 21, 2000 rediscovered
Orbital characteristics
Periapsis5,909,000 km (0.039 AU)
Apoapsis8,874,300 km (0.059 AU)
Mean orbit radius
7,391,650 km (0.04941 AU)
129.82761 d (0.3554 a)
4.098 km/s
Inclination45.81° (to the ecliptic)
47.48° (to Jupiter's equator)
Satellite ofJupiter
Physical characteristics
Mean radius
4 km[1]
Circumference~25 km
~200 km²
Volume~270 km³
Mass6.89×1014 kg
Mean density
2.6 g/cm3 assumed[2]
~0.0029 m/s2 (0.0003 g)
~0.0048 km/s
Albedo0.04 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]

Diagram illustrating Themisto's orbit (top left) among those of the other non-spherical moons of Jupiter. The moons above the horizontal axis are prograde, the moons beneath it are retrograde. The yellow segments extend from the pericentre to the apocentre, showing the orbital eccentricity.

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. Ephemeris IAU-MPC NSES
  2. Mean orbital parameters NASA JPL

Other websites[change | change source]