Himalia (moon)

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).

[b] Himalia was discovered by Charles Dillon Perrine at the Lick Observatory on 3 December 1904 in photographs taken with the 36-inch Crossley reflecting telescope which he had recently rebuilt.

[1] Himalia is Jupiter's most easily observed small satellite; though Amalthea is brighter, its proximity to the planet's brilliant disk makes it a far more difficult object to view.

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.

[10] In November 2000, the Cassini spacecraft, en route to Saturn, made a number of images of Himalia, including photos from a distance of 4.4 million km.

[6] In February and March 2007, the New Horizons spacecraft en route to Pluto made a series of images of Himalia, culminating in photos from a distance of 8 million km.

[21] In September 2006, as NASA's New Horizons mission to Pluto approached Jupiter for a gravity assist, it photographed what appeared to be a faint new planetary ring parallel with and slightly inside Himalia's orbit.

Animation of Himalia's orbit.
Jupiter · Himalia · Callisto
Himalia's rotational light curve from Earth-based observations taken between August and October 2010. [ 9 ]
Himalia observed by the Wide-field Infrared Survey Explorer (WISE) spacecraft in 2014
Cassini image of Himalia, taken in December 2000 from a distance of 4.4 million kilometres
Phases of Himalia imaged by the LORRI instrument aboard New Horizons
Composite of six New Horizons images of the possible Himalia ring. The double exposure of Himalia is circled. The arrow points to Jupiter.