| 词条 | (496315) 2013 GP136 |
| 释义 |
| minorplanet = yes | name = {{mp|(496315) 2013 GP|136}} | background = #C2E0FF | image = | image_size = | caption = | discovery_ref = [2] | discovered = 8 February 2013 | discoverer = OSSOS | discovery_site = Mauna Kea Obs. | mpc_name = (496315) {{mp|2013 GP|136}} | alt_names = {{mp|2013 GP|136}} | pronounced = | named_after = | mp_category = TNO {{·}}SDO [4] | orbit_ref = | epoch = 4 September 2017 (JD 2458000.5) | uncertainty = 3 | observation_arc = 4.29 yr (1,566 days) | aphelion = 268.46 AU | perihelion = 41.073 AU | semimajor = 154.76 AU 149.8 AU[6] | eccentricity = 0.7346 | period = {{nowrap|1925 yr (703,239 days)}} | mean_anomaly = 356.44° | mean_motion = {{Deg2DMS|0.0005|sup=ms}} / day | inclination = 33.467° | asc_node = 210.71° | arg_peri = 42.316° | dimensions = 212 km[4] | rotation = | albedo = | spectral_type = | abs_magnitude = 6.6 }}{{mp|2013 GP|136}} is a trans-Neptunian object from the scattered disc in the outermost reaches of the Solar System, approximately 212 kilometers in diameter. It was discovered on 8 February 2013, by the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States.[2] Orbit and classification{{mp|2013 GP|136}} orbits the Sun at a distance of 41.1–268.5 AU once every 1925 years and 4 months (703,239 days). Its orbit has an eccentricity of 0.73 and an inclination of 33° with respect to the ecliptic.It was mentioned in a 2016 paper by Malhotra of the Lunar and Planetary Laboratory, at The University of Arizona, Tucson, AZ as a detached object with a perihelion greater than 40 AUs, a 6:1 orbital period ratio with 90377 Sedna, and in a possible 9:1 mean-motion resonance with a hypothetical large Planet Nine.[6] See also
References1. ^1 2 {{cite web |title = 496315 (2013 GP136) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=496315 |accessdate = 30 July 2017}} [1][2][3]2. ^1 2 {{cite journal |last1=Malhotra |first1=Renu |last2=Volk |first2=Kathryn |last3=Wang |first3=Xianyu |date=2016 |title=Corralling a distant planet with extreme resonant Kuiper belt objects |journal=The Astrophysical Journal Letters |volume=824 |issue=2 |pages=L22 |arxiv=1603.02196 |bibcode=2016ApJ...824L..22M |doi=10.3847/2041-8205/824/2/L22}} 3. ^1 2 {{cite web |title = List of Known Trans-Neptunian Objects |work = Johnston's Archive |url = http://www.johnstonsarchive.net/astro/tnoslist.html |date = 22 July 2017 |accessdate = 30 July 2017}} }}
|title=MPEC 2015-R47 : 2013 GP136 |publisher=IAU Minor Planet Center |date=2016-03-19 |url=http://www.minorplanetcenter.net/mpec/K15/K15R47.html |accessdate=2016-03-19 }} External links
5 : Scattered disc and detached objects|Extreme trans-Neptunian objects|Discoveries by OSSOS|Possible dwarf planets|Astronomical objects discovered in 2013 |
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