| name = Pasiphae
| image = Pasiphaé.jpg
| bgcolour = #ffc0c0
| discovery = yes
| discoverer = P. J. Melotte
| discovered = January 27, 1908
| mean_orbit_radius = 24,094,770 km
| eccentricity = 0.2953
| periapsis = 16,980,250 km
| apoapsis = 31,209,300 km
| period = 764.082032 d (2.092 a)
| avg_speed = 2.242 km/s
| inclination = 145.24° (to the ecliptic)
143.04° (to Jupiter's equator)
| satellite_of = Jupiter
| physical_characteristics = yes
| mean_radius = 20 km
| surface_area = ~11,300 km²
| volume = ~113,000 km³
| mass = 3.0Template:E kg
| density = 2.6 g/cm³ (assumed)
| surface_grav = ~0.022 m/s2 (0.002 g)
| escape_velocity = ~0.036 km/s
| albedo = 0.04 (assumed)
| single_temperature = ~124 K
Pasiphae (Template:IPAc-en Template:Respell; Template:Lang-el; formerly Pasiphaë) is a retrograde irregular satellite of Jupiter. It was discovered in 1908 by Philibert Jacques Melotte and later named after the mythological Pasiphaë, wife of Minos and mother of the Minotaur from Greek legend.
It was first spotted on a plate taken at the Royal Greenwich Observatory on the night of February 28, 1908. Inspection of previous plates found it as far back as January 27. It received the provisional designation Template:Nowrap, 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.
Pasiphae orbits Jupiter on a high eccentricity and high inclination retrograde orbit. It gives its name to the Pasiphae group, irregular retrograde moons orbiting Jupiter at distances ranging between 22.8 and 24.1 million km, and with inclinations ranging between 144.5° and 158.3°. The orbital elements are as of January 2000. They are continuously changing due to solar and planetary perturbations. 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.
Spectroscopical measurements in infrared indicate that Pasiphae is a spectrally featureless object, consistent with the suspected asteroidal origin of the object. Pasiphae is believed to be a fragment from a captured asteroid along with other Pasiphae group satellites.
<ref>tags exist, but no
<references/>tag was found