(175113) 2004 PF115

Last updated
(175113) 2004 PF115
Discovery [1] [2]
Discovered by M. Brown, C. A. Trujillo, D. Rabinowitz
Discovery date7 August 2004
Designations
TNO (plutino?) [3] [4]
Orbital characteristics [5]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 3
Observation arc 9593 days (26.26 yr)
Earliest precovery date4 June 1992
Aphelion 41.619  AU (6.2261  Tm)
Perihelion 36.519 AU (5.4632 Tm)
39.069 AU (5.8446 Tm)
Eccentricity 0.06527
244.20 yr (89195.8 d)
167.19°
0° 0m 14.665s / day
Inclination 13.346°
84.441°
87.197°
Earth  MOID 35.5528 AU (5.31862 Tm)
Jupiter  MOID 31.2172 AU (4.67003 Tm)
Physical characteristics
Dimensions 406.3+97.6
−75.3 km [6]
0.113+0.082
−0.042 [6]
Temperature ~ 44 K
4.54±0.25, [6] 4.3 [5]

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

    Contents

    Physical properties

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

    References

    1. 1 2 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. 1 2 Johnston, W. R. (27 December 2020). "List of Known Trans-Neptunian Objects" . Retrieved 22 February 2020.
    4. 1 2 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. 1 2 "JPL Small-Body Database Browser: 175113 (2004 PF115)". 14 July 2019. Retrieved 3 November 2019.
    6. 1 2 3 4 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. S2CID   119253817.


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