Pasiphae (moon)

Pasiphae, formerly spelled Pasiphaë, also known as is one of the outermost and the biggest of retrograde irregular satellite of Jupiter. As an irregular moon with an eccentric orbit, it gets as far as 35.9 million km from Jupiter.

Discovery and Naming

It was discovered in 1908 by Philibert Jacques Melotte.
The moon was first spotted on a plate taken at the Royal Greenwich Observatory on the night of 28 February 1908. Inspection of previous plates found it as far back as January 27. It received the provisional designation ', as it was not clear whether it was an asteroid or a moon of Jupiter. The recognition of the latter case came by April 10.
Later named after the mythological Pasiphaë, wife of Minos and mother of the Minotaur from Greek legend.
Pasiphae did not receive its present name until 1975; before then, it was simply known as '. It was sometimes called "Poseidon" between 1955 and 1975.

Orbit

Image:TheIrregulars [JUPITER retro.svg|thumb|left|300px|The diagram illustrates its orbit in relation to other retrograde irregular satellites of Jupiter. The eccentricity of selected orbits is represented by the yellow segments (extending from the pericentre to the apocentre). The outermost regular satellite Callisto is located for reference..]
Pasiphae orbits Jupiter on a high eccentricity and high inclination on a retrograde orbit with an average distance of 24.1 million km, but it gets as far as 35.9 million km from Jupiter. The orbital elements are continuously changing due to solar and planetary perturbations. In December 2023 the moon reached from Jupiter.
It gives its name to the Pasiphae group, a group of retrograde moons of Jupiter with semi-major axes spread over 22–25 million km, inclinations between 141° and 158°, and higher eccentricities between 0.22 and 0.44.
Pasiphae is also known to be in a secular resonance with Jupiter.

Physical characteristics

With a diameter estimated at 58 km, Pasiphae is the largest retrograde and third largest irregular satellite after Himalia and Elara.
Spectroscopical measurements in infrared indicate that Pasiphae is a spectrally featureless object, consistent with the suspected asteroidal origin of the object.
The satellite appears pale red though it falls into the grey color-class of C-type asteroids.

Origin

Pasiphae probably did not form near Jupiter but was captured by Jupiter later. Pasiphae is believed to be a fragment from a captured asteroid along with other Pasiphae group satellites.