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词条 2002 XV93
释义

  1. Orbit and rotation

  2. Physical characteristics

  3. References

  4. External links

{{DISPLAYTITLE:2002 XV93}}{{Infobox planet
| minorplanet = yes
| background = #C2E0FF
| name = {{mp|2002 XV|93}}
| symbol =
| image =
| caption =
| discovery_ref = [1]
| discoverer = M. W. Buie
| discovered = December 10, 2002
| earliest_precovery_date = 16 October 1990
| mpc_name = {{mp|2002 XV|93}}
| mp_category = Plutino[2]
| orbit_ref = [3]
| epoch = 13 January 2016 (JD 2457400.5)
| aphelion = {{Convert|44.427|AU|Tm|abbr=on|lk=on}} (Q)
| perihelion = {{Convert|34.405|AU|Tm|abbr=on}} (q)
| semimajor = {{Convert|39.416|AU|Tm|abbr=on}} (a)
| eccentricity = 0.12713 (e)
| period = 247.47 yr (90387.1 d)
| avg_speed =
| inclination = 13.281° (i)
| asc_node = 19.170° (Ω)
| mean_anomaly = 282.08° (M)
| arg_peri = 163.53° (ω)
| satellites =
| dimensions = 549.2{{±|21.7|23.0}} km[4]
| mass = ≈1.7{{e|20}} kg
| density = 2 g/cm3
| surface_grav = {{Gr|0.17|275|2}} g/cm3
| escape_velocity = {{V2|0.17|275|2}} km/s
| sidereal_day =
| axial_tilt =
| pole_ecliptic_lat =
| pole_ecliptic_lon =
| albedo = 0.040{{±|0.020|0.015}}[4]
| spectral_type = B−V=0.72 ± 0.02
V−R=0.37 ± 0.02[4]
| magnitude = 21.1[4]
| abs_magnitude = 5.42 ± 0.46,[4]
4.73 ± 0.02[5] 5.0[3]
| mean_motion = {{Deg2DMS|0.0039829|sup=ms}} /day (n)
| observation_arc = 6582 days (18.02 yr)
| uncertainty = 3
| moid = {{Convert|33.4096|AU|Tm|abbr=on}}
| jupiter_moid = {{Convert|28.9574|AU|Tm|abbr=on}}
}}{{mp|2002 XV|93}}, also written as 2002 XV93, is a trans-Neptunian object (TNO) with an absolute magnitude of 5.4.[4] A 2:3 orbital resonance with Neptune makes it a plutino.[2]

It has been observed with precovery images back to 1990.[3]

Orbit and rotation

{{mp|2002 XV|93}} is locked in 2:3 resonance with Neptune, which means that when it makes two revolutions around the Sun, Neptune makes exactly three.[2]

The rotation period of this object is not known.

Physical characteristics

The size of {{mp|2002 XV|93}} has been measured by the Herschel Space Telescope to be 549.2{{±|21.7|23.0}} km.[6]

It is likely a dwarf planet.[7]

References

1. ^{{Cite web|url=http://www.minorplanetcenter.org/iau/lists/TNOs.html|title=List Of Transneptunian Objects|accessdate=2010-10-27|publisher=IAU Minor Planet Center| archiveurl= https://archive.is/20101027133511/http://www.minorplanetcenter.org/iau/lists/TNOs.html| archivedate= 27 October 2010 | deadurl= no}}
2. ^{{Cite web |date=2010-07-27 |title=MPEC 2010-O39 :Distant Minor Planets (12 August 2010.0 TT) |publisher=Minor Planet Center & Tamkin Foundation Computer Network |url=http://www.minorplanetcenter.org/mpec/K10/K10O39.html |accessdate=2010-08-07| archiveurl= https://www.webcitation.org/67niL9ZA8?url=http://www.minorplanetcenter.org/mpec/K10/K10O39.html| archivedate= 20 May 2012 | deadurl= no}}
3. ^{{Cite web |type=2008-10-23 last obs |title=JPL Small-Body Database Browser: 2002 XV93 |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002XV93 |accessdate=30 March 2016}}
4. ^{{Cite web |title=AstDys 2002XV93 Ephemerides |publisher=Department of Mathematics, University of Pisa, Italy |url=http://hamilton.dm.unipi.it/astdys/index.php?pc=1.1.0&n=2002XV93 |accessdate=2010-08-07}}
5. ^{{Cite web |url=http://www.physics.nau.edu/~tegler/research/survey.htm |title=Kuiper Belt Object Magnitudes and Surface Colors |accessdate=2009-12-30 |last=Tegler |first=Stephen C. |date=2007-02-01 |archive-url=https://web.archive.org/web/20060901063349/http://www.physics.nau.edu/~tegler/research/survey.htm |archive-date=1 September 2006 |dead-url=yes |df=dmy-all }}
6. ^{{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 }}
7. ^{{cite web|url=http://web.gps.caltech.edu/~mbrown/dps.html |title=How many dwarf planets are there in the outer solar system? |publisher=Gps.caltech.edu|date=2015-07-21|accessdate=16 September 2016}}

External links

  • {{AstDys|2002XV93}}
  • {{JPL small body}}
{{Use dmy dates|date=October 2018}}{{Trans-Neptunian objects}}{{Dwarf planets}}{{Small Solar System bodies}}{{DEFAULTSORT:2002 XV93}}

5 : Plutinos|Minor planet object articles (unnumbered)|Discoveries by Marc W. Buie|Possible dwarf planets|Astronomical objects discovered in 2002

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