Astronomy:Saturn LXVII

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Saturn LXVII
Discovery[1]
Discovered byScott S. Sheppard et al.
Discovery siteMauna Kea Obs.
Discovery date12 December 2004
Designations
Designation
Saturn LXVII (67)[2]
S/2004 S 7[2]
Orbital characteristics[3]
Epoch 9 August 2022 (JD 2459800.5)
Observation arc15.61 yr (5,703 days)
0.1441103 astronomical unit|AU (21,559,000 km)
Eccentricity0.5743875
Orbital period–3.24 yr (–1181.80 d)
Mean anomaly94.00208°
Mean motion0° 18m 16.63s / day
Inclination165.04992° (to ecliptic)
Longitude of ascending node14.74072°
127.76280°
Satellite ofSaturn
GroupNorse group
Physical characteristics
Mean diameter≈6 km[4]
Albedo0.04 (assumed)[4]
Apparent magnitude24.5[4]
Absolute magnitude (H)15.6[3]


Saturn LXVII, provisionally designated S/2004 S 7, is a natural satellite of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on 4 May 2005 from observations taken between 12 December 2004 and 8 March 2005.

Saturn LXVII is about 6 kilometres in diameter, and orbits Saturn at an average distance of 21,559,000 kilometres in about 1,182 days, at an inclination of 165.0° to the ecliptic, in a retrograde direction and with an eccentricity of 0.574.[3][5] Denk et al. (2018) tentatively assigned this moon to the Mundilfari dynamical family, but it may instead be more closely related to Thrymr.[6]

This moon was considered lost[7] until its recovery was announced on 12 October 2022.[3] On 14 April 2026, the Minor Planet Center gave the moon its Roman numeral designation Saturn LXVII (Saturn 67).[8]

References

  1. ↑ Discovery Circumstances from JPL
  2. ↑ 2.0 2.1 "MPC Explorer - Saturn 67". Minor Planet Center. https://data.minorplanetcenter.net/explorer/?tab=Designated&search=Saturn+67. Retrieved 2026-06-03. 
  3. ↑ 3.0 3.1 3.2 3.3 "MPEC 2022-T127 : S/2004 S 7". Minor Planet Electronic Circular. Minor Planet Center. 12 October 2022. https://minorplanetcenter.net/mpec/K22/K22TC7.html. Retrieved 12 October 2022. 
  4. ↑ 4.0 4.1 4.2 S.S. Sheppard (2019), Moons of Saturn, Carnegie Science, on line
  5. ↑ Jacobson, R.A. (2007) SAT272 (2007-06-28). "Planetary Satellite Mean Orbital Parameters". JPL/NASA. http://ssd.jpl.nasa.gov/?sat_elem#saturn. 
  6. ↑ Denk, T.; Mottola, S.; Bottke, W. F.; Hamilton, D. P. (2018). "The Irregular Satellites of Saturn". Enceladus and the Icy Moons of Saturn. 322. University of Arizona Press. pp. 409–434. doi:10.2458/azu_uapress_9780816537075-ch020. ISBN 9780816537488. Bibcode: 2018eims.book..409D. https://tilmanndenk.de/wp-content/uploads/DenkEtAl2018_IrregularMoons.pdf. 
  7. ↑ Jacobson, B.; Brozović, M.; Gladman, B.; Alexandersen, M.; Nicholson, P. D.; Veillet, C. (28 September 2012). "Irregular Satellites of the Outer Planets: Orbital Uncertainties and Astrometric Recoveries in 2009–2011". The Astronomical Journal 144 (5): 132. doi:10.1088/0004-6256/144/5/132. Bibcode: 2012AJ....144..132J. 
  8. ↑ "M.P.C. 194209". Minor Planet Circulars (Minor Planet Center) (51876): 412. 2026-04-14. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/2026/MPC_20260414.pdf#page=2309. Retrieved 2026-06-03.