S/2003 J 9 Explained

S/2003 J 9
Discovery Ref: 
Discoverer:Scott S. Sheppard
David C. Jewitt
Jan T. Kleyna
Yanga R. Fernández
Discovery Site:Mauna Kea Obs.
Discovered:6 February 2003
Orbit Ref: 
Epoch:17 December 2020 (JD 2459200.5)
Observation Arc:15.19 yr (5,545 d)
Eccentricity:0.1701900
Period:2.10 yr (767.60 d)
Mean Anomaly:109.89836°
Mean Motion: / day
Inclination:166.33403°
13.66597°
Asc Node:130.59522°
Arg Peri:45.62861°
Satellite Of:Jupiter
Group:Carme group
Mean Diameter:
Albedo:0.04
Magnitude:23.7
Abs Magnitude:16.9

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 2003.

is about 1 kilometre in diameter, and orbits Jupiter at an average distance of in 767.60 days, at an inclination of 166.3° to the ecliptic (166° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.17.

It belongs to the Carme group, made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°.

This moon was once considered lost[1] [2] [3] [4] until November 2020, when the Minor Planet Center announced the recovery of S/2003 J 9 by Scott Sheppard in observations from September 2011 to April 2018.

Notes and References

  1. Web site: Outer-Planet Moons Found — and Lost . Beatty . Kelly . 4 April 2012 . www.skyandtelescope.com . Sky & Telescope . 27 June 2017.
  2. Brozović . Marina . Jacobson . Robert A. . 9 March 2017 . The Orbits of Jupiter's Irregular Satellites . The Astronomical Journal . 153 . 4 . 147 . 10.3847/1538-3881/aa5e4d. 2017AJ....153..147B . free .
  3. Jacobson . B. . Brozović . M. . B. . Gladman . M. . Alexandersen . P. D. . Nicholson . C. . Veillet . 28 September 2012 . Irregular Satellites of the Outer Planets: Orbital Uncertainties and Astrometric Recoveries in 2009–2011 . The Astronomical Journal . 144 . 5 . 132 . 10.1088/0004-6256/144/5/132 . 2012AJ....144..132J . 123117568 . free .
  4. Web site: New Moons of Jupiter Announced in 2017 . Sheppard . Scott S. . 2017 . home.dtm.ciw.edu . 27 June 2017 . We likely have all of the lost moons in our new observations from 2017, but to link them back to the remaining lost 2003 objects requires more observations a year later to confirm the linkages, which will not happen until early 2018. ... There are likely a few more new moons as well in our 2017 observations, but we need to reobserve them in 2018 to determine which of the discoveries are new and which are lost 2003 moons..