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2005 VX3

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Trans-Neptunian object and retrograde damocloid on a highly eccentric, cometary-like orbit

2005 VX3
Discovery
Discovered byMount Lemmon Srvy.
Discovery siteMount Lemmon Obs.
(first observed only)
Discovery date1 November 2005
Designations
MPC designation2005 VX3
Minor planet categoryTNO · damocloid
unusual · distant
Orbital characteristics
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 4
Observation arc81 days
Aphelion1825.61 AU
Perihelion4.1058 AU
Semi-major axis914.86 AU
Eccentricity0.9955
Orbital period (sidereal)27,672 yr
Mean anomaly0.1730°
Mean motion0° 0 0 / day
Inclination112.22°
Longitude of ascending node255.35°
Argument of perihelion196.37°
Jupiter MOID0.8884 AU
TJupiter−0.9430
Physical characteristics
Mean diameter7 km (est.)
Geometric albedo0.09 (assumed)
Absolute magnitude (H)14.1

2005 VX3 is trans-Neptunian object and retrograde damocloid on a highly eccentric, cometary-like orbit. It was first observed on 1 November 2005, by astronomers with the Mount Lemmon Survey at the Mount Lemmon Observatory in Arizona, United States. The unusual object measures approximately 7 kilometers (4 miles) in diameter. It has the 3rd largest known heliocentric semi-major axis and aphelion. Additionally its perihelion lies within the orbit of Jupiter, which means it also has the largest orbital eccentricity of any known minor planet.

Description

2005 VX3 orbits the Sun at a distance of 4.1–1,826 AU once every 27,672 years (semi-major axis of 915 AU). Its orbit has an eccentricity of 0.9955 and an inclination of 112° with respect to the ecliptic. It belongs to the dynamical group of damocloids due to its retrograde orbit and its low Tisserand parameter (TJupiter of −0.9430). It is a Jupiter-, Saturn-, Uranus-, and Neptune-crosser. The body's observation arc begins with its first observation by the Mount Lemmon Survey on 1 November 2005.

Orbital evolution — Barycentric elements
Year
(epoch)		 Aphelion Semimajor-axis Ref
1950 2710 AU n.a.
2012 1914 AU n.a.
2015 2563 AU n.a.
2016 3235 AU n.a.
2050 2049 AU 1026 AU

2005 VX3 has a barycentric semi-major axis of ~1026 AU. 2014 FE72 and 2012 DR30 have a larger barycentric semi-major axis. The epoch of January 2016 was when 2005 VX3 had its largest heliocentric semi-major axis.

The object has a short observation arc of 81 days and does not have a well constrained orbit. It has not been observed since January 2006, when it came to perihelion, 4.1 AU from the Sun. It may be a dormant comet that has not been seen outgassing. In the past it may have made closer approaches to the Sun that could have removed most near-surface volatiles. The current orbit crosses the ecliptic just inside Jupiter's orbit and has a Jupiter-MOID of 0.8 AU.

In 2017, it had an apparent magnitude of ~28 and was 24 AU from the Sun. It comes to opposition in mid-June. It would require one of the largest telescopes in the world for any more follow-up observations.

Comparison

The orbits of Sedna, 2012 VP113, Leleākūhonua, and other very distant objects along with the predicted orbit of Planet Nine. The three sednoids (pink) along with the red-colored extreme trans-Neptunian object (eTNO) orbits are suspected to be aligned against the hypothetical Planet Nine while the blue-colored eTNO orbits are aligned. The highly elongated orbits colored brown include centaurs and damocloids with large aphelion distances over 200 AU.

See also

Notes

  1. ^ Given the orbital eccentricity of this object, different epochs can generate quite different heliocentric unperturbed two-body best-fit solutions to the semi-major axis and orbital period. For objects at such high eccentricity, the Sun's barycentric coordinates are more stable than heliocentric coordinates. Using JPL Horizons, the barycentric semi-major axis is approximately 1026 AU.
  2. ^ Archived JPL Small-Body Database Browser: (2005 VX3) from 13 December 2012. JPL Epoch 2012 orbital solution that has aphelion (Q)=1914 AU.
  3. ^ Archived MPC object data for (2005 VX3) from Minor Planet Center archive of Epoch 2015-06-27 with aphelion (Q) of 2563 AU.
  4. ^ Archived MPC object data for (2005 VX3) from JPL Webcite archive of Epoch 2016-Jan-13 with aphelion (Q) of 3235AU.
  5. Archived MPC object data for (2005 VX3) from 8 March 2014.

References

  1. ^ "2005 VX3". Minor Planet Center. Retrieved 20 November 2018.
  2. "MPEC 2005-V58 : 2005 VX3". IAU Minor Planet Center. 8 November 2005. Retrieved 20 November 2018. (K05V03X)
  3. ^ "JPL Small-Body Database Browser: (2005 VX3)" (2006-01-21 last obs.). Jet Propulsion Laboratory. Retrieved 20 November 2018.
  4. ^ Johnston, Wm. Robert (7 October 2018). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 19 November 2018.
  5. "List Of Other Unusual Objects". Minor Planet Center. 14 November 2018. Retrieved 19 November 2018.
  6. "JPL Small-Body Database Search Engine: Asteroids and a > 100 (AU)". JPL Solar System Dynamics. Retrieved 6 March 2014. (Epoch defined at will change every 6 months or so)
  7. ^ Horizons output. "Barycentric Osculating Orbital Elements for 2005 VX3". Retrieved 6 March 2014. (Solution using the Solar System Barycenter and barycentric coordinates. Select Ephemeris Type:Elements and Center:@0)
  8. Kaib, Nathan A.; Becker, Andrew C.; Jones, R. Lynne; Puckett, Andrew W.; Bizyaev, Dmitry; Dilday, Benjamin; et al. (April 2009). "2006 SQ372: A Likely Long-Period Comet from the Inner Oort Cloud". The Astrophysical Journal. 695 (1): 268–275. arXiv:0901.1690. Bibcode:2009ApJ...695..268K. doi:10.1088/0004-637X/695/1/268. S2CID 16987581.

External links

Trans-Neptunian objects
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Dwarf planets (moons)
Sednoids
Small Solar System bodies
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Asteroid
Distant minor planet
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