Himalia (moon) facts for kids
Himalia as seen by Cassini-Huygens
|
|
| Discovery | |
|---|---|
| Discovered by | C. D. Perrine |
| Discovery date | December 3, 1904 |
| Orbital characteristics | |
| Periapsis | 9,782,900 km |
| Apoapsis | 13,082,000 km |
|
Mean orbit radius
|
11,460,000 km |
| Eccentricity | 0.16 |
| 250.56 d (0.704 a) | |
|
Average orbital speed
|
3.312 km/s |
| Inclination | 27.50° (to the ecliptic) 29.59° (to Jupiter's equator) |
| Satellite of | Jupiter |
| Physical characteristics | |
|
Mean radius
|
85 km |
| ~90,800 km² | |
| Volume | ~2,570,000 km³ |
| Mass | 6.7×1018 kg |
|
Mean density
|
2.6 g/cm³ (assumed) |
| ~0.062 m/s2 (0.006 g) | |
| ~0.100 km/s | |
|
Sidereal rotation period
|
7.782 h |
| Albedo | 0.04 |
| Temperature | ~124 K |
Himalia is the biggest non-spherical moon of Jupiter. It was found by Charles Dillon Perrine at the Lick Observatory on December 3, 1904. It is named after the nymph Himalia who bore three sons of Zeus (the Greek equivalent of Jupiter).
Name
Himalia did not get its present name until 1975; before then, it was simply known as Jupiter VI or Jupiter Satellite VI, although calls for a full name appeared shortly after its and Elara's discovery; A.C.D. Crommelin wrote in 1905,
Unfortunately the numeration of Jupiter's satellites is now in precisely the same confusion as that of Saturn's system was before the numbers were abandoned and names substituted. A similar course would seem to be advisable here; the designation V for the inner satellite was tolerated for a time, as it was considered to be in a class by itself; but it has now got companions, so that this subterfuge disappears. The substitution of names for numerals is certainly more poetic.
The moon was sometimes called Hestia, after the Greek goddess, from 1955 to 1975.
Orbit
It is the biggest member of the group that bears its name, the moons orbiting between 11.4 and 13 million kilometers from Jupiter at an inclination of about 27.5°. The orbital elements are as of January 2000. They are changing a lot due to Solar and planetary perturbations.
Physical characteristics
A day on Himalia is only about 7 3/4 hours long. Himalia appears grey, like the other members of its group, similar to a C-type asteroid. Measurements by Cassini confirm a featureless spectrum, with a slight absorption at 3 μm which could indicate the presence of water.
Exploration
In November 2000, the Cassini spacecraft, going to Saturn, made a number of pictures of Himalia, including photos from a distance as close as 4.4 million km. The moon covers only a few pixels, but seems to be a stretched object with axes 150 ± 20 and 120 ± 20 km, close to the Earth-based estimations.
In February and March 2007, the New Horizons spacecraft to Pluto made a series of pictures of Himalia, culminating in photos from a distance of eight million km. Again, Himalia appears only a few pixels across.
Images for kids
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Animation of Himalia's orbit. Jupiter · Himalia · Callisto
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Himalia's rotational light curve from Earth-based observations taken between August and October 2010.
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Himalia observed by the Wide-field Infrared Survey Explorer (WISE) spacecraft in 2014
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Cassini image of Himalia, taken in December 2000 from a distance of 4.4 million kilometres
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Phases of Himalia imaged by the LORRI instrument aboard New Horizons
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Composite of six New Horizons images of the possible Himalia ring. The double exposure of Himalia is circled. The arrow points to Jupiter.
See also
In Spanish: Himalia (satélite) para niños
