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2013 VZ70

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2013 VZ70
Discovery
Discovered byOSSOS
Discovery siteMauna Kea Obs.
Discovery date17 September 2017
(first observed only)
Designations
MPC designation2013 VZ70
Minor planet categorycentaur · horseshoe
Orbital characteristics
Epoch 1 July 2021 (JD 2459396.5)
Uncertainty parameter· 4
Observation arc2.59 yr (946 d)
Earliest precovery date9 August 2013
Aphelion10.010 AU
Perihelion8.2816 AU
Semi-major axis9.1457 AU
Eccentricity0.0945
Orbital period (sidereal)27.66 yr (10,102 d)
Mean anomaly34.155°
Mean motion0° 2 8.16 / day
Inclination12.053°
Longitude of ascending node215.18°
Argument of perihelion245.30°
Saturn MOID0.33076 AU
TJupiter3.150
Physical characteristics
Mean diameter7.9 km (est. 0.09)
Absolute magnitude (H)13.74±0.330

2013 VZ70 is a centaur on a horseshoe co-orbital configuration with Saturn. It was first observed on 1 November 2013 by the Outer Solar System Origins Survey at Mauna Kea Observatory in Hawaii, United States. The discovery was announced on 23 August 2021.

2013 VZ70 is the first minor planet ever discovered in a horseshoe orbit with respect to Saturn. It orbits the Sun at a distance of 8.3–10.0 AU once every 27 years and 8 months (10,102 days; semi-major axis of 9.15 AU). Its orbit has an eccentricity of 0.09 and an inclination of 12° with respect to the ecliptic. Based on a generic magnitude-to-diameter conversion, assuming an albedo of 0.09, 2013 VZ70 measures approximately 7.9 kilometers (4.9 miles) in diameter for an absolute magnitude of 13.74.

The object may have an origin among the trans-Neptunian population. However, an analysis of its orbit within the context of those of the known satellites of Saturn suggests that 2013 VZ70 could be related to the Inuit group; on the other hand, the mutual nodal distances of 2013 VZ70 and the moons Fornjot and Thrymr are below the first percentile of the distribution.

References

  1. ^ "2013 VZ70". Minor Planet Center. International Astronomical Union. Retrieved 24 August 2021.
  2. ^ "MPEC 2021-Q55 : 2013 VZ70". Minor Planet Electronic Circular. Minor Planet Center. 23 August 2021. Retrieved 24 August 2021.
  3. ^ Alexandersen, M.; Greenstreet, S.; Gladman, B.; Bannister, M.; Chen, Y.; Gwyn, S.; et al. (October 2020). The first known Saturnian Horseshoe Coorbital and the distribution of Temporary Coorbitals of the Giant Planets. Division of Planetary Science meeting #52. Bulletin of the American Astronomical Society. Bibcode:2020DPS....5220606A. 206.06. Retrieved 24 August 2021.
  4. ^ "JPL Small-Body Database Browser: (2013 VZ70)" (2016-03-12 last obs.). Jet Propulsion Laboratory. Retrieved 24 August 2021.
  5. ^ "Asteroid Size Estimator". CNEOS NASA/JPL. Retrieved 1 September 2021.
  6. ^ Alexandersen, Mike; Greenstreet, Sarah; Gladman, Brett J.; Bannister, Michele T.; Chen, Ying-Tung; Gwyn, Stephen D. J.; Kavelaars, J.J.; Petit, Jean-Marc; Volk, Kathryn; Lehner, Matthew J.; Wang, Shiang-Yu (2021). "OSSOS. XXIII. 2013 VZ70 and the Temporary Coorbitals of the Giant Planets". The Planetary Science Journal. 2 (1): 212. arXiv:2110.09627. Bibcode:2021PSJ.....2..212A. doi:10.3847/PSJ/ac1c6b. S2CID 238755438.
  7. ^ de la Fuente Marcos, C.; de la Fuente Marcos, R. (10 January 2022). "Centaur 2013 VZ70: Debris from Saturn's irregular moon population?". Astronomy & Astrophysics. 657 (1): A59 (10 pp). arXiv:2110.04264. Bibcode:2022A&A...657A..59D. doi:10.1051/0004-6361/202142166. S2CID 238856647.

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