(175113) 2004 PF115

(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 cubewano.[3][4] It is near a 2:3 resonance with Neptune.[6]

(175113) 2004 PF115
Discovery[1][2]
Discovered byM. Brown, C. A. Trujillo, D. Rabinowitz
Discovery date7 August 2004
Designations
TNO (cubewano)[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
Aphelion41.619 AU (6.2261 Tm)
Perihelion36.519 AU (5.4632 Tm)
39.069 AU (5.8446 Tm)
Eccentricity0.06527
244.20 yr (89195.8 d)
167.19°
0° 0m 14.665s / day
Inclination13.346°
84.441°
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]
0.113+0.082
−0.042
[6]
Temperature~ 44 K
4.54±0.25,[6] 4.3[5]

Physical propertiesEdit

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

ReferencesEdit

  1. ^ a b 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. Retrieved 2012-05-14.
  2. ^ "List Of Transneptunian Objects". IAU Minor Planet Center. Retrieved 7 June 2012.
  3. ^ a b Johnston, W. R. (13 July 2019). "List of Known Trans-Neptunian Objects". Retrieved 3 November 2019.
  4. ^ a b Buie, M. (3 November 2019). "Orbit Fit and Astrometric record for 175113". SwRI (Space Science Department). Archived from the original on 3 November 2019. Retrieved 3 November 2019.
  5. ^ a b "JPL Small-Body Database Browser: 175113 (2004 PF115)". 14 July 2019. Retrieved 3 November 2019.
  6. ^ a b c d e Mommert, Michael; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; Delsanti, A.; Vilenius, E.; Müller, T. G.; Peixinho, N.; Lellouch, E.; Szalai, N.; Henry, F.; Duffard, R.; Fornasier, S.; Hartogh, P.; Mueller, M.; Ortiz, J. L.; Protopapa, S.; Rengel, M.; Thirouin, A. (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. arXiv:1202.3657. Bibcode:2012A&A...541A..93M. doi:10.1051/0004-6361/201118562.

External linksEdit