Astronomy:2002 XV93

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2002 XV93
2002xv93.jpg
2002 XV93 imaged by the Hubble Space Telescope in 2005
Discovery[1]
Discovered byM. W. Buie
Discovery date10 December 2002
Designations
2002 XV93
Minor planet categoryplutino[2]
Orbital characteristics[4]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc6582 days (18.02 yr)
Earliest precovery date16 October 1990
|{{{apsis}}}|helion}}44.427 astronomical unit|AU (6.6462 Tm) (Q)
|{{{apsis}}}|helion}}34.405 AU (5.1469 Tm) (q)
39.416 AU (5.8965 Tm) (a)
Eccentricity0.12713 (e)
Orbital period247.47 yr (90387.1 d)
Mean anomaly282.08° (M)
Mean motion0° 0m 14.338s / day (n)
Inclination13.281° (i)
Longitude of ascending node19.170° (Ω)
|{{{apsis}}}|helion}}≈ 20 March 2070[3]
±5 days
163.53° (ω)
Earth MOID33.4096 AU (4.99801 Tm)
Jupiter MOID28.9574 AU (4.33197 Tm)
Physical characteristics
Dimensions549.2+21.7
−23.0
 km
[5]
Geometric albedo0.040+0.020
−0.015
[5]
  • B−V = 0.72±0.02
  • V−R = 0.37±0.02[5]
Apparent magnitude21.1[6]
Absolute magnitude (H)


2002 XV93, also written as 2002 XV93, is a trans-Neptunian object (TNO) with an absolute magnitude of 5.4.[5] A 2:3 orbital resonance with Neptune makes it a plutino.[2]

It has been observed with precovery images back to 1990.[4]

Orbit and rotation

Precovery image of 2003 XV93 taken by the Palomar Observatory in 1992[8]

2002 XV93 is locked in 2:3 resonance with Neptune, which means that when it makes two revolutions around the Sun, Neptune makes exactly three.[2]

The rotation period of this object is not known.

Physical characteristics

The size of 2002 XV93 has been measured by the Herschel Space Telescope to be 549.2+21.7
−23.0
 km
.[5]

References

  1. "List of Transneptunian Objects". IAU Minor Planet Center. http://www.minorplanetcenter.org/iau/lists/TNOs.html. 
  2. 2.0 2.1 2.2 "MPEC 2010-O39 :Distant Minor Planets (12 August 2010.0 TT)". Minor Planet Center & Tamkin Foundation Computer Network. 27 July 2010. http://www.minorplanetcenter.org/mpec/K10/K10O39.html. 
  3. JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.)
  4. 4.0 4.1 4.2 "JPL Small-Body Database Browser: 2002 XV93". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002XV93. 
  5. 5.0 5.1 5.2 5.3 5.4 5.5 Mommert, Michael; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; Delsanti, A.; Vilenius, E. et al. (May 2012). "TNOs are cool: A survey of the trans-Neptunian region—V. Physical characterization of 18 Plutinos using Herschel-PACS observations". Astronomy & Astrophysics 541: A93. doi:10.1051/0004-6361/201118562. Bibcode2012A&A...541A..93M. 
  6. "AstDys 2002XV93 Ephemerides". Department of Mathematics, University of Pisa, Italy. https://newton.spacedys.com/astdys/index.php?pc=1.1.0&n=2002XV93. 
  7. Tegler, Stephen C. (1 February 2007). "Kuiper Belt Object Magnitudes and Surface Colors". http://www.physics.nau.edu/~tegler/research/survey.htm. 
  8. Lowe, Andrew. "2002 XV93 Precovery Images". http://andrew-lowe.ca/2002xv93.htm. 

External links