Astronomy:(148975) 2001 XA255
Discovery | |
---|---|
Discovered by | David C. Jewitt, Scott S. Sheppard and Jan Kleyna |
Discovery date | 9 December 2001 |
Designations | |
(148975) 2001 XA255 | |
Minor planet category | Centaur |
Orbital characteristics[1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 2 | |
Observation arc | 3812 days (10.44 yr) |
|{{{apsis}}}|helion}} | 48.731 astronomical unit|AU (7.2901 Tm) |
|{{{apsis}}}|helion}} | 9.3364 AU (1.39671 Tm) |
29.034 AU (4.3434 Tm) | |
Eccentricity | 0.67843 |
Orbital period | 156.44 yr (57141.1 d) |
Mean anomaly | 12.809° |
Mean motion | 0° 0m 22.681s / day |
Inclination | 12.628° |
Longitude of ascending node | 105.89° |
90.452° | |
Jupiter MOID | 4.12722 AU (617.423 Gm) |
Physical characteristics | |
Mean diameter | 12.5 km[2] 38 km[1][3] |
Geometric albedo | 0.041[1][3] |
Absolute magnitude (H) | 11.1[1] |
(148975) 2001 XA255, provisional designation: 2001 XA255, is a dark minor planet in the outer Solar System, classified as centaur, approximately 38 kilometers (24 miles) in diameter.[1] It was discovered on 9 December 2001, by David C. Jewitt, Scott S. Sheppard, and Jan Kleyna observing from the Mauna Kea Observatory.[4] The object is currently trapped in a 1:1 mean-motion resonance with Neptune following a path of the horseshoe type.[5]
Orbit and classification
2001 XA255 follows a very eccentric orbit (0.68) with perihelion just inside the orbit of Saturn, aphelion in the trans-Neptunian belt and a semi-major axis of 28.9 AU. The orbital inclination of this object is moderate at 12.6º.[1]
Resonance with Neptune
2001 XA255 was identified as trapped in a 1:1 mean-motion resonance with Neptune and 1:2 with Uranus by T. Gallardo in 2006.[6] The object is dynamically unstable and it entered the region of the giant planets relatively recently, perhaps 50,000 years ago, from the scattered disk. It follows a short-lived horseshoe orbit around Neptune.[5]
Physical characteristics
The object has an estimated diameter of 12.5 km and it was classified as an inactive centaur by David Jewitt.[2] Observations by the NEOWISE mission gave a larger diameter of 37.7 kilometers and an albedo of 0.041.[3] It has an absolute magnitude is 11.1.[1]
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "148975 (2001 XA255)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=148975;cad=1.
- ↑ 2.0 2.1 Jewitt, David C. (2009). "The Active Centaurs". The Astronomical Journal 137 (5): 4296–4312. doi:10.1088/0004-6256/137/5/4296. Bibcode: 2009AJ....137.4296J.
- ↑ 3.0 3.1 3.2 Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. http://www.johnstonsarchive.net/astro/tnoslist.html. Retrieved 12 August 2021.
- ↑ Jewitt, David C.; Sheppard, S. S.; Kleyna, J.; Marsden, B. G.. "2001 XA255". Minor Planet Electronic Circular.
- ↑ 5.0 5.1 de la Fuente Marcos, C.; de la Fuente Marcos, R. (2012). "Four temporary Neptune co-orbitals: (148975) 2001 XA255, (310071) 2010 KR59, (316179) 2010 EN65, and 2012 GX17". Astronomy and Astrophysics 547: L2. doi:10.1051/0004-6361/201220377. Bibcode: 2012A&A...547L...2D.
- ↑ ADS link Gallardo, T. (2006) Atlas of the mean-motion resonances in the Solar System
External links
- 2001 XA255, Jewitt, D. C., Sheppard, S. S., Kleyna, J., & Marsden, B. G. 2002, Minor Planet Electronic Circular, 2002-A85.
- The Active Centaurs, Jewitt, D. C. 2009, Astronomical Journal, Volume 137, Number 5, pp. 4296–4312.
- (148975) 2001 XA255 data at MPC
- Atlas of the mean motion resonances in the Solar System Gallardo, T. 2006, Icarus, Volume 184, Issue 1, pp. 29–38.
- Four temporary Neptune co-orbitals: (148975) 2001 XA255, (310071) 2010 KR59, (316179) 2010 EN65, and 2012 GX17 de la Fuente Marcos, C., & de la Fuente Marcos, R. 2012, Astronomy and Astrophysics, Volume 547, id.L2, 7 pp.
- IAU list of centaurs and scattered-disk objects
- IAU list of trans-neptunian objects
- Another list of TNOs
- (148975) 2001 XA255 at the JPL Small-Body Database