Himalia

Also known as Jupiter VI, Hestia

moon of Jupiter

AI overview

Himalia is a moon of Jupiter, one of the many natural satellites that orbit the giant planet. While it's relatively small and distant compared to Jupiter's largest moons, it contributes to our understanding of the diverse collection of objects in Jupiter's orbit and the formation history of the Jupiter system.

AI-generated from the Wikipedia summary — may contain errors.

Wikidata facts

Instance of: irregular moon
Named after: Himalia
Parent body: Jupiter
Radius: 85
Mass: 6.7
Orbital period: 248.29
Image: Himalia.png

Show 11 more facts

semi-major axis of an orbit: 11493550
discoverer or inventor: Charles Dillon Perrine
site of astronomical discovery: Lick Observatory
time of discovery or invention: 1904-12-03
Commons category: Himalia (moon)
orbital eccentricity: 0.16
albedo: 0.04
apparent magnitude: 14.6
orbital inclination: 29.90917
surface gravity: 0.062
different from: Himalia

Sources (5)

via Wikidata · CC0

~9 min read

Encyclopedic overview

Himalia (/hɪˈmeɪliə, 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.

Discovery and naming

Excerpted from Wikipedia’s “Himalia” article, available under the CC BY-SA 4.0 licence.

Himalia

Wikidata facts

Encyclopedic overview

Gallery (7)

Available in 68 languages

What links here128 pages

What links here128 pages