Astronomy:(148975) 2001 XA255

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(148975) 2001 XA255
Discovery
Discovered byDavid C. Jewitt, Scott S. Sheppard and Jan Kleyna
Discovery date9 December 2001
Designations
(148975) 2001 XA255
Minor planet categoryCentaur
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 2
Observation arc3812 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)
Eccentricity0.67843
Orbital period156.44 yr (57141.1 d)
Mean anomaly12.809°
Mean motion0° 0m 22.681s / day
Inclination12.628°
Longitude of ascending node105.89°
90.452°
Jupiter MOID4.12722 AU (617.423 Gm)
Physical characteristics
Mean diameter12.5 km[2]
38 km[1][3]
Geometric albedo0.041[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. 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. 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. Bibcode2009AJ....137.4296J. 
  3. 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. 
  4. Jewitt, David C.; Sheppard, S. S.; Kleyna, J.; Marsden, B. G.. "2001 XA255". Minor Planet Electronic Circular. 
  5. 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. Bibcode2012A&A...547L...2D. 
  6. ADS link Gallardo, T. (2006) Atlas of the mean-motion resonances in the Solar System

External links