Pasiphae (moon)

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 1908 CJ, 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 Jupiter VIII. It was sometimes called "Poseidon" between 1955 and 1975.

Orbit

Pasiphae orbits Jupiter on a high eccentricity (0.490) and high inclination (about 157°) 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 0.2494 AU 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 (tying the longitude of its perijove with the longitude of perihelion of Jupiter).{{cite journal

Physical characteristics

With a diameter estimated at 58 km (Albedo 4.4%), 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 (colour indices V=17.22 B-V=0.74, R-V=0.38) 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.

References

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References

1. Noah Webster. (1884). "A Practical Dictionary of the English Language".
2. {{Dict.com. Pasiphae
3. Laurent Milesi. (2003). "James Joyce and the difference of language".
4. (2023-12-23). ""Life" of dust originating from the irregular satellites of Jupiter". Monthly Notices of the Royal Astronomical Society.
5. "Planetary Names: Planet and Satellite Names and Discoverers".
6. Melotte, P. J.. (1908). "Note on the Newly Discovered Eighth Satellite of Jupiter, Photographed at the Royal Observatory, Greenwich". [[Monthly Notices of the Royal Astronomical Society]].
7. (June 1908). "Recent Observations of the Moving Object Near Jupiter, Discovered at Greenwich by Mr. J. Melotte". Publications of the Astronomical Society of the Pacific.
8. Cowell, P. H.. (1908). "Note on the Discovery of a Moving Object Near Jupiter". Monthly Notices of the Royal Astronomical Society.
9. [http://www.cbat.eps.harvard.edu/iauc/02800/02846.html IAUC 2846: ''Satellites of Jupiter''] 7 October 1974 (naming the moon)
10. Payne-Gaposchkin, Cecilia. (1970). "Introduction to Astronomy". Prentice-Hall.
11. [[Tommy Grav. Grav, T.]]; [[Matthew J. Holman. Holman, M. J.]]; [[Brett J. Gladman. Gladman, B. J.]]; and [[Kaare Aksnes. Aksnes, K.]]; [https://arxiv.org/abs/astro-ph/0301016 ''Photometric Survey of the Irregular Satellites''], Icarus, Vol. 166 (2003), pp. 33-45
12. Brown, M. E.. (2000). "Near-Infrared Spectroscopy of Centaurs and Irregular Satellites". The American Astronomical Society.
13. Sheppard, S. S.; and Jewitt, D. C.; [http://www.ifa.hawaii.edu/~jewitt/papers/JSATS/SJ2003.pdf ''An Abundant Population of Small Irregular Satellites Around Jupiter''] {{Webarchive. link. (5 August 2003, Nature, Vol. 423 (May 2003), pp. 261-263)