Himalia (moon)

Himalia
Low-resolution image of Himalia from Cassini, December 2000
Discovery
Discovered byCharles D. Perrine
Discovery siteLick Observatory
Discovery date3 December 1904
Designations
Designation
Jupiter VI
Pronunciation/hɪˈmliə/ or /hɪˈmɑːliə/
Named after
Ἱμαλία Himalia
AdjectivesHimalian
Orbital characteristics
Epoch 27 April 2019 (JD 2458600.5)
Observation arc114.25 yr (41,728 days)
0.0761287 AU (11,388,690 km)
Eccentricity0.1537860
+248.29 d
94.30785°
1° 26m 59.616s / day
Inclination29.90917° (to the ecliptic)
44.99935°
21.60643°
Satellite ofJupiter
GroupHimalia group
Physical characteristics
Dimensions205.6 × 141.3 km (occultation, projected)
(150 × 120) ± 20 km (Cassini estimate)
139.6±1.7 km
170±20 km
Mass(4.2±0.6)×1018 kg
(1.9–4.2)×1018 kg
Mean density
3.33±0.47 g/cm3 (assuming radius 67 km)
1.63 g/cm3 (assuming radius 85 km)
7.7819±0.0005 h
Albedo0.057±0.008
0.05±0.01
Spectral type
C
14.6
7.9

Himalia (/hɪˈmliə, hɪˈmɑːliə/), also known as Jupiter VI, is the largest irregular satellite of Jupiter. With a diameter of around 140 km (90 mi), it is the sixth largest Jovian satellite, after the four Galilean moons and Amalthea. It was discovered by Charles Dillon Perrine at the Lick Observatory on 3 December 1904 and is named after the nymph Himalia, who bore three sons of Zeus (the Greek equivalent of Jupiter). It is the largest member of the Himalia group, a group of moons that orbit in the prograde direction around Jupiter, likely a collisional family originating from a captured asteroid.