2015 RR245

2015 RR245

Orbit of 2015 RR245
Designations
MPC designation 2015 RR245
Orbital characteristics
Epoch 2016 July 31.0 TT = JDT 2457600.5
Aphelion 128.8650253 AU (Q)
Perihelion 33.7133696 AU (q)
81.2891975 AU (a)
Eccentricity 0.5852663 (e)
733 yr
322.50413° (M)
Inclination 7.57643° (i)
211.67680° (Ω)
261.41753° (ω)
Physical characteristics
Dimensions 670 km (420 mi) diameter
Mass 2,374 km (1,475 mi)
0.12?

    2015 RR245 is a possible dwarf planet in the Kuiper belt. 2015 RR245 is one of the few dwarf planets to survive after the formation of the solar system, along with Pluto and Eris.[1] It was discovered in February 2016[2][3] by the Outer Solar System Origins Survey (OSSOS).[2][3]

    2015 RR245 was discovered by a research team while poring over images that the Canada–France–Hawaii Telescope in Hawaii took in September 2015 as part of the OSSOS (Outer Solar System Origins Survey).[2][3]

    Its exact size is uncertain, but the best estimate is around 670 km (420 mi) in diameter, assuming an albedo of 12%. For comparison, Pluto, the largest object in the Kuiper belt, is about 2,374 km (1,475 mi) in diameter.[2][3]

    Orbit

    As of July 2016, the orbit of 2015 RR245 is approximately, but not precisely known. It has a 700-year orbit. It appears to come as close as 33.7 AU[4] to the Sun (still beyond the orbit of Neptune at 30 AU), and up to 129 AU distant.[5] It will make its closest approach to the Sun in 2096.[2]

    Resonance with Neptune

    2015 RR2015's orbit librating in a 2:9 resonance with Neptune

    Additional precovery astrometry from the Pan-STARRS1 survey shows that 2015 RR245 is securely trapped in a 2:9 mean motion resonance with Neptune, meaning that 2015 RR245 orbits the Sun twice in the same amount of time it takes Neptune to complete 9 orbits.[6]

    See also

    References

    1. "New Distant Dwarf Planet Beyond Neptune". United Press International. 18 July 2016. Retrieved 9 October 2016 via Gale General OneFile.
    2. 1 2 3 4 5 "New Dwarf Planet Discovered Far Beyond Pluto's Orbit". space.com. 11 July 2016.
    3. 1 2 3 4 Chang, Kenneth (13 July 2016). "Astronomers Discover New Likely Dwarf Planet, the Latest of Many". New York Times. Retrieved 14 July 2016.
    4. "New Dwarf Planet".
    5. "Kuiper Belt's Big, New, Far-Out Object - Sky & Telescope". 13 July 2016.
    6. Bannister, Michele T.; Alexandersen, Mike; Benecchi, Susan D.; Chen, Ying-Tung; Delsanti, Audrey; Fraser, Wesley C.; Gladman, Brett J.; Granvik, Mikael; Grundy, Will M.; Guilbert-Lepoutre, Aurelie; Gwyn, Stephen D. J.; Ip, Wing-Huen; Jakubik, Marian; Lynne Jones, R.; Kaib, Nathan; Kavelaars, J. J.; Lacerda, Pedro; Lawler, Samantha; Lehner, Matthew J.; Hsing Wen Lin; Patryk Sofia Lykawka; Marsset, Michael; Murray-Clay, Ruth; Noll, Keith S.; Parker, Alex; Petit, Jean-Marc; Pike, Rosemary E.; Rousselot, Philippe; Schwamb, Megan E.; et al. (2016). "OSSOS: IV. Discovery of a dwarf planet candidate in the 9:2 resonance". arXiv:1607.06970v1Freely accessible [astro-ph.EP].

    External links


    This article is issued from Wikipedia - version of the 11/11/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.