Astronomy:(230965) 2004 XA192
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Discovery | |
---|---|
Discovered by | Palomar |
Discovery date | 12 December 2004 |
Designations | |
Minor planet category | SDO (near or extended)[2] |
Orbital characteristics[3] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 3 | |
Observation arc | 9268 days (25.37 yr) |
Earliest precovery date | 29 August 1989 |
|{{{apsis}}}|helion}} | 58.967 astronomical unit|AU (8.8213 Tm) |
|{{{apsis}}}|helion}} | 35.465 AU (5.3055 Tm) |
47.216 AU (7.0634 Tm) | |
Eccentricity | 0.24888 |
Orbital period | 324.44 yr (118503 d) |
Mean anomaly | 356.376° |
Mean motion | 0° 0m 10.936s / day |
Inclination | 38.07711° |
Longitude of ascending node | 328.7517° |
132.632° | |
Earth MOID | 34.588 AU (5.1743 Tm) |
Jupiter MOID | 30.7418 AU (4.59891 Tm) |
TJupiter | 4.703 |
Physical characteristics | |
Dimensions | 549 km[4] 339+120 −95 km[5] |
Rotation period | 7.88 h (0.328 d) |
Sidereal rotation period | 7.88[3] |
Geometric albedo | 0.09 (assumed)[4] 0.26+0.34 −0.15[5] |
Apparent magnitude | 19.84[6] |
Absolute magnitude (H) | 4.2[3] 4.42±0.63[5] 4.6[4] |
(230965) 2004 XA192 is a Kuiper-belt object with a diameter of 339+120
−95 km. It has an absolute magnitude of approximately 4.42, and albedo around 26%. It was discovered on 12 December 2004 at Palomar Observatory.
It is currently at 35.8 AU from the Sun, near its perihelion.[7]
References
- ↑ Lowe, Andrew. "(230965) 2004 XA192 Precovery Images". http://andrew-lowe.ca/2004xa192.htm.
- ↑ Marc Buie (2014-08-23). "Orbit Fit and Astrometric record for 230965". SwRI (Space Science Department). http://www.boulder.swri.edu/~buie/kbo/astrom/230965.html. Retrieved 2014-11-14.
- ↑ 3.0 3.1 3.2 "JPL Small-Body Database Browser: 230965 (2004 XA192)". https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=230965. Retrieved 11 April 2016.
- ↑ 4.0 4.1 4.2 Brown, Michael E.. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. http://web.gps.caltech.edu/~mbrown/dps.html. Retrieved 28 April 2019.
- ↑ 5.0 5.1 5.2 TNOs are Cool: A survey of the trans-Neptunian region. X. Analysis of classical Kuiper belt objects from Herschel* and Spitzer observations p. 18
- ↑ 0 & n = 230965 AstDys Summary for (230965) 2004 XA192. Retrieved 31 August 2009
- ↑ AstDys Ephmerides for (230965) 2004 XA192, retrieved 31 August 2009
External links
Original source: https://en.wikipedia.org/wiki/(230965) 2004 XA192.
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