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Himalia (moon): Encyclopedia BETA


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Himalia (moon)

Himalia

Discovery
Discovered byC. D. Perrine
Discovered onDecember 3, 1904
Orbital characteristics
Mean radius11,432,430 km (0.07642 AU)
Eccentricity0.1443
Periapsis9,782,900 km (0.065 AU)
Apoapsis13,082,000 km (0.087 AU)
Orbital period249.726 d (0.704 a)
Orbital circumference71,456,750 km (0.478 AU)
Orbital velocitymax: 3.850 km/s
mean: 3.312 km/s
min: 2.879 km/s
Inclination29.88° (to the ecliptic)
29.59° (to Jupiter's equator)
Is a satellite ofJupiter
Physical characteristics
Mean diameter170 km
Surface area~90,800 km2
Volume~2,570,000 km3
Mass6.7 kg
Mean density2.6 g/cm3
Surface gravity~0.062 m/s2 (0.006 g)
Escape velocity~0.100 km/s
Rotation period~0.4 d (10 h)
Axial tilt
Albedo0.04
Surface temp.
minmean max
KK~124 K
Atmospheric pressure0 kPa
Himalia (hye-mal'-ee-ə, also hi-mahl'-ee-ə, ; Greek Ἱμαλíα) is the largest irregular satellite of Jupiter. It was discovered by Charles Dillon Perrine at the Lick Observatory in 1904 and is named after the nymph Himalia who bore three sons of Zeus.

On December 19, 2000, the Cassini spacecraft, en route to Saturn, captured a very low resolution image of Himalia, but it was too distant to show any surface details.

Himalia did not receive its present name until 1975; before then, it was simply known as Jupiter VI. It was sometimes called "Hestia".

It is the largest member of the group that bears its name, five moons orbiting between 11 and 13 Gm from Jupiter at an inclination of about 27.5°.

Physical characteristics

Cassini pictured Himalia from 4.4 million km as an elongated object with axes 150 ± 20 and 120 ± 20 km, close to the Earth-based estimations. Carolyn C. Porco et al. Cassini Imaging of Jupiter's Atmosphere, Satellites, and Rings , Science, 299(March 2003), pp. 1541 - 1547. It, as the other members of its group, appears neutral (grey) with colour indices B-V=0.62, V-R= 0.4, similar to a C-type asteroid.spectrum, with a slight absorption at 3 μm which could indicate the presence of water.Chamberlain, Matthew A.; Brown, Robert H. Near-infrared spectroscopy of Himalia, Icarus, 172 (2004), pp. 163-169.

External links

* Astronomical Journal, 24 (1905) 154B
* Astronomical Journal, 24 (1905) 160 (same as above)
* Publications of the Astronomical Society of the Pacific, 17 (1905) 22
* Harvard College Observatory Bulletin, 173 (1905) 1
* Harvard College Observatory Bulletin, 175 (1905) 1
* Astronomische Nachrichten, 169 (1905) 43/44

References




... | Leda | Himalia | Lysithea | ...




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