Astronomy:(175113) 2004 PF115

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(175113) 2004 PF115
Discovery[1][2]
Discovered byM. Brown, C. A. Trujillo, D. Rabinowitz
Discovery date7 August 2004
Designations
Minor planet categoryTNO (plutino?)[3][4]
Orbital characteristics[5]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 3
Observation arc9593 days (26.26 yr)
Earliest precovery date4 June 1992
|{{{apsis}}}|helion}}41.619 astronomical unit|AU (6.2261 Tm)
|{{{apsis}}}|helion}}36.519 AU (5.4632 Tm)
39.069 AU (5.8446 Tm)
Eccentricity0.06527
Orbital period244.20 yr (89195.8 d)
Mean anomaly167.19°
Mean motion0° 0m 14.665s / day
Inclination13.346°
Longitude of ascending node84.441°
87.197°
Earth MOID35.5528 AU (5.31862 Tm)
Jupiter MOID31.2172 AU (4.67003 Tm)
Physical characteristics
Dimensions406.3+97.6
−75.3
 km
[6]
Geometric albedo0.113+0.082
−0.042
[6]
Physics~ 44 K
Absolute magnitude (H)4.54±0.25,[6] 4.3[5]


(175113) 2004 PF115 (also written 2004 PF115) is a trans-Neptunian object (TNO). It was discovered in 2006 by M. Brown, C. Trujillo, D. Rabinowitz.[1] The object is classified as a possible plutino.[3][4]

Physical properties

The size of (175113) 2004 PF115 was measured by the Herschel Space Telescope to be 406.3+97.6
−75.3
 km
.[6]

References

  1. 1.0 1.1 Marsden, Brian G. (1 September 2007). "MPEC 2007-R03 : 2004 PF115, 2004 PG115, 2004 XA192, 2005 QU182". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. https://www.minorplanetcenter.net/mpec/K07/K07R03.html. Retrieved 2012-05-14. 
  2. "List Of Transneptunian Objects". IAU Minor Planet Center. http://www.minorplanetcenter.org/iau/lists/TNOs.html. Retrieved 7 June 2012. 
  3. 3.0 3.1 Johnston, W. R. (27 December 2020). "List of Known Trans-Neptunian Objects". http://www.johnstonsarchive.net/astro/tnoslist.html. 
  4. 4.0 4.1 Buie, M. (3 November 2019). "Orbit Fit and Astrometric record for 175113". SwRI (Space Science Department). https://www.boulder.swri.edu/~buie/kbo/astrom/175113.html. Retrieved 3 November 2019. 
  5. 5.0 5.1 "JPL Small-Body Database Browser: 175113 (2004 PF115)". 14 July 2019. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2175113. Retrieved 3 November 2019. 
  6. 6.0 6.1 6.2 6.3 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. 

External links