Euanthe (moon) explained

Euanthe
Adjective:Euanthean
Named After:Ευάνθη Eyanthē
Discoverer:Scott S. Sheppard et al.
Discovered:11 December 2001
Discovery Site:Mauna Kea Obs.
Mpc Name:Jupiter XXXIII
Alt Names:S/2001 J 7
Orbit Ref: [1]
Inclination:148.9°
Eccentricity:0.232
Arg Peri:316.0°
Asc Node:271.0°
Mean Anomaly:130.5°
Period:−602.81 days
Satellite Of:Jupiter
Group:Ananke group
Magnitude:22.8
Mean Diameter:3 km

Euanthe, also known as , is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2001, and given the temporary designation .[2] [3]

Euanthe is about 3 kilometres in diameter, and orbits Jupiter at an average distance of 20,465 Mm in 602.81 days, at an inclination of 143° to the ecliptic (142° to Jupiter's equator) with an eccentricity of 0.2001.

It was named in August 2003 after Euanthe, who was the mother of the Graces, according to some Greek writers.[4]

Euanthe belongs to the Ananke group, retrograde irregular moons that orbit Jupiter between 19.3 and 22.7 Gm, at inclinations of roughly 150°.

Notes and References

  1. https://sites.google.com/carnegiescience.edu/sheppard/moons/jupitermoons S.S. Sheppard (2019), Moons of Jupiter, Carnegie Science, on line
  2. Web site: Daniel W. E. Green . IAUC 7900: Satellites of Jupiter . May 16, 2002 . International Astronomical Union.
  3. Web site: Brian G. Marsden . MPEC 2002-J54: Eleven New Satellites of Jupiter . May 15, 2002 . International Astronomical Union Minor Planet Center.
  4. Web site: Daniel W. E. Green . IAUC 8177: Satellites of Jupiter, Saturn, Uranus . August 8, 2003 . International Astronomical Union . dead . https://web.archive.org/web/20120327153049/http://www.cbat.eps.harvard.edu/iauc/08100/08177.html . March 27, 2012 .