| 词条 | (307463) 2002 VU130 |
| 释义 |
| minorplanet=yes | background=#C2E0FF | name=(307463) 2002 VU130 | discoverer=Marc W. Buie | discovered=7 November 2002 | discovery_ref=[1][1] | alt_names=none | mp_category=TNO (plutino) | epoch=13 January 2016 (JD 2457400.5) | semimajor={{Convert|39.212|AU|Tm|abbr=on}} | perihelion={{Convert|30.920|AU|Tm|abbr=on}} | aphelion={{Convert|47.503|AU|Tm|abbr=on|lk=on}} | eccentricity=0.21145 | period=245.55 yr (89685.6 d) | inclination=1.3688° | asc_node=267.92° | arg_peri=280.32° | mean_anomaly=272.58° | avg_speed= | orbit_ref=[2] | dimensions={{val|252.9|+33.6|-31.3|u=km}}[4] | mass= | density= | surface_grav= | escape_velocity= | rotation= | spectral_type= | abs_magnitude={{val|5.47|0.83}},[4] 6.0[2] | albedo={{val|0.179|+0.202|-0.103}}[4] | single_temperature=~44 K | mean_motion={{Deg2DMS|0.0040140|sup=ms}} / day | observation_arc=4780 days (13.09 yr) | uncertainty=3 | moid={{Convert|29.9218|AU|Tm|abbr=on}} | jupiter_moid={{Convert|25.4717|AU|Tm|abbr=on}} | tisserand=5.497 }}{{mp|(307463) 2002 VU|130}} (also written (307463) 2002 VU130) is a trans-Neptunian object (TNO). It was discovered in 2002 by Marc W. Buie at Kitt Peak Observatory.[1] The object is classified as a plutino (in 2:3 resonance with Neptune).[4] Physical propertiesThe size of {{mp|(307463) 2002 VU|130}} was measured by the Herschel Space Telescope to be {{val|252.9|+33.6|-31.3|u=km}}.[3] References1. ^1 {{cite web |date=2002-12-03 |title=MPEC 2002-X10: 2002 VR130, 2002 VS130, 2002 VT130, 2002 VU130 |first=Brian G. |last=Marsden |work=IAU Minor Planet Center |publisher=Harvard-Smithsonian Center for Astrophysics |url=http://www.minorplanetcenter.net/mpec/K02/K02X10.html |accessdate=2012-05-14}} 2. ^1 2 {{cite web |type=2008-10-22 last obs |title=JPL Small-Body Database Browser: 307463 (2002 VU130) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2307463 |accessdate=7 April 2016}} 3. ^1 2 3 4 {{Cite journal | last1 = Mommert | first1 = Michael| last2 = Harris | first2 = A. W. | last3 = Kiss | first3 = C. | last4 = Pál | first4 = A. | last5 = Santos-Sanz | first5 = P. | last6 = Stansberry | first6 = J. | last7 = Delsanti | first7 = A. | last8 = Vilenius | first8 = E. | last9 = Müller | first9 = T. G. | first10 = N. | last10 = Peixinho| first11 = E. | last11 = Lellouch| first12 = N. | last12 = Szalai| first13 = F. | last13 = Henry| first14 = R. | last14 = Duffard| first15 = S. | last15 = Fornasier| first16 = P. | last16 = Hartogh| first17 = M. | last17 = Mueller| first18 = J. L. | last18 = Ortiz| first19 = S. | last19 = Protopapa| first20 = M. | last20 = Rengel| first21 = A. | last21 = Thirouin| title = TNOs are cool: A survey of the trans-Neptunian region—V. Physical characterization of 18 Plutinos using Herschel-PACS observations| doi = 10.1051/0004-6361/201118562 | journal = Astronomy & Astrophysics | volume = 541 | pages = A93 | date = May 2012| pmid = | pmc = | bibcode = 2012A&A...541A..93M | arxiv = 1202.3657 }} External links
3 : Discoveries by Marc W. Buie|Plutinos|Astronomical objects discovered in 2002 |
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