(612533) 2002 XV93: Difference between revisions

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	The size of {{mp\|2002 XV\|93}} has been measured by the ] to be 549.2{{±\|21.7\|23.0}} km.<ref name=Herschel>{{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 = ] \| volume = 541 \| pages = A93 \| date = May 2012\| pmid = \| pmc = \| bibcode = 2012A&A...541A..93M \| arxiv = 1202.3657 }}</ref>		The size of {{mp\|2002 XV\|93}} has been measured by the ] to be 549.2{{±\|21.7\|23.0}} km.<ref name=Herschel>{{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 = ] \| volume = 541 \| pages = A93 \| date = May 2012\| pmid = \| pmc = \| bibcode = 2012A&A...541A..93M \| arxiv = 1202.3657 }}</ref>

	It is ].<ref name=brown>{{cite web\|url=http://www.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=2015-07-22}}</ref>		It is ].<ref name=brown>{{cite web\|url=http://www.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=2015-07-22 \|deadurl=yes \|archiveurl=https://web.archive.org/web/20111018154917/http://www.gps.caltech.edu/~mbrown/dps.html \|archivedate=2011-10-18 \|df= }}</ref>

	==References==		==References==

Revision as of 17:09, 17 September 2016

2002 XV₉₃
Discovery
Discovered by	M. W. Buie
Discovery date	December 10, 2002
Designations
MPC designation	2002 XV₉₃
Minor planet category	Plutino
Orbital characteristics
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc	6582 days (18.02 yr)
Aphelion	44.427 AU (6.6462 Tm) (Q)
Perihelion	34.405 AU (5.1469 Tm) (q)
Semi-major axis	39.416 AU (5.8965 Tm) (a)
Eccentricity	0.12713 (e)
Orbital period (sidereal)	247.47 yr (90387.1 d)
Mean anomaly	282.08° (M)
Mean motion	0° 0 14.338 /day (n)
Inclination	13.281° (i)
Longitude of ascending node	19.170° (Ω)
Argument of perihelion	163.53° (ω)
Earth MOID	33.4096 AU (4.99801 Tm)
Jupiter MOID	28.9574 AU (4.33197 Tm)
Physical characteristics
Dimensions	549.2 _−23.0 km
Mass	≈1.7×10 kg
Mean density	2 g/cm
Equatorial surface gravity	0.15 g/cm
Equatorial escape velocity	0.29 km/s
Geometric albedo	0.040 _−0.015
Spectral type	B−V=0.72 ± 0.02 V−R=0.37 ± 0.02
Apparent magnitude	21.1
Absolute magnitude (H)	5.42 ± 0.46, 4.73 ± 0.02 5.0

2002 XV₉₃, also written as 2002 XV93, is a trans-Neptunian object (TNO) with an absolute magnitude of 5.4. A 2:3 orbital resonance with Neptune makes it a plutino.

It has been observed with precovery images back to 1990.

Orbit and rotation

2002 XV₉₃ is locked in 2:3 resonance with Neptune, which means that when it makes two revolutions around the Sun, Neptune makes exactly three.

The rotation period of this object is not known.

Physical characteristics

The size of 2002 XV₉₃ has been measured by the Herschel Space Telescope to be 549.2
_−23.0 km.

It is likely a dwarf planet.

References

"List Of Transneptunian Objects". IAU Minor Planet Center. Archived from the original on 27 October 2010. Retrieved 2010-10-27. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
^ "MPEC 2010-O39 :Distant Minor Planets (12 August 2010.0 TT)". Minor Planet Center & Tamkin Foundation Computer Network. 2010-07-27. Archived from the original on 2 August 2010. Retrieved 2010-08-07. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
^ "JPL Small-Body Database Browser: 2002 XV93" (2008-10-23 last obs). Retrieved 30 March 2016.
^ 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.
"AstDys 2002XV93 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2010-08-07. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
Tegler, Stephen C. (2007-02-01). "Kuiper Belt Object Magnitudes and Surface Colors". Retrieved 2009-12-30.
"How many dwarf planets are there in the outer solar system?". Gps.caltech.edu. 2015-07-21. Archived from the original on 2011-10-18. Retrieved 2015-07-22. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)

External links

Orbital simulation from JPL (Java) / Horizons Ephemeris
(612533) 2002 XV93 at the JPL Small-Body Database
- Close approach · Discovery · Ephemeris · Orbit viewer · Orbit parameters · Physical parameters

Small Solar System bodies

Minor planets

Designation Groups List Moon Meanings of names
Asteroid	Active Aten asteroid Asteroid belt Family Jupiter trojan Near-Earth Spectral types
Distant minor planet	Centaur Neptune trojan Damocloid Trans-Neptunian object Detached Kuiper belt Oort cloud Scattered disc

Comets

Other

v t e Trans-Neptunian objects
TNO classes	Cubewanos Scattered-disc objects Detached objects Resonant objects Neptune trojans Plutinos Twotinos TNO moons
Dwarf planets (moons)	Orcus Vanth Pluto Charon Styx Nix Kerberos Hydra Haumea Namaka Hiʻiaka Ring Quaoar Weywot Rings Makemake MK2 Gonggong Xiangliu Eris Dysnomia Sedna
Sednoids	90377 Sedna 2012 VP113 541132 Leleākūhonua

Dwarf planets

List of possible dwarf planets
Former dwarf planets
- Phoebe
- Triton
- Vesta
- Pallas
Mesoplanet
Planemo

Consensus

Ceres
- Geology
- Atmosphere
Orcus
- Moon
Pluto
- Geology
- Atmosphere
- Moons
Haumea
- Moons
- Ring
Makemake
- Moon
Quaoar
- Moon
- Rings
Eris
- Moon
Gonggong
- Moon
Sedna

Candidate

Asteroids	Hygiea Interamnia
Centaurs	Chariklo Chiron Pholus 1999 OX₃ 2013 TC₁₄₆ 2014 NW₆₅
Plutinos	Huya Ixion 2001 QF₂₉₈ 2002 VR₁₂₈ 2002 XV₉₃ 2003 AZ₈₄ 2003 UZ₄₁₃ 2003 VS₂ 2007 JH₄₃ 2017 OF69
Twotinos	2002 WC₁₉
Cubewanos	Chaos Salacia Varda Varuna 1998 SN₁₆₅ 2002 AW₁₉₇ 2002 CY248 2002 KX₁₄ 2002 MS₄ 2002 UX₂₅ 2003 QW₉₀ 2004 GV₉ 2004 NT₃₃ 2004 PF₁₁₅ 2004 TY₃₆₄ 2004 UX₁₀ 2005 RN₄₃ 2005 UQ₅₁₃ 2010 FX86
Other KBOs	1999 CD₁₅₈ 1999 DE₉ 2000 YW₁₃₄ 2002 XW₉₃ 2010 JO₁₇₉ 2010 VK₂₀₁ 2011 FW62 2011 GM₂₇ 2013 FZ₂₇ 2014 UM₃₃ 2015 AM₂₈₁ 2015 RR₂₄₅
Scattered disc objects	Gǃkúnǁʼhòmdímà Dziewanna 1996 GQ₂₁ 1996 TL₆₆ 2001 UR₁₆₃ 2002 TC₃₀₂ 2004 XA₁₉₂ 2005 QU₁₈₂ 2005 RM₄₃ 2006 QH181 2008 OG₁₉ 2010 KZ39 2010 RE₆₄ 2010 RF₄₃ 2010 JO179 2010 TJ 2010 VZ₉₈ 2013 FY₂₇ 2014 AN₅₅ 2014 EZ₅₁ 2014 UZ224 2014 WK₅₀₉ 2015 KH162 2015 RR245 2017 FO161 2018 AG37 2018 VG18 2021 DR15 2021 LL37
Detached objects	2003 FY₁₂₈ 2003 QX₁₁₃ 2004 XR₁₉₀ 2005 TB₁₉₀ 2007 JJ₄₃ 2008 ST₂₉₁
Sednoids	2012 VP113

Category

Categories:

Revision as of 22:48, 26 July 2016 editTom.Reding (talk \| contribs)Autopatrolled, Extended confirmed users, Page movers, Template editors3,879,760 editsm +Category:Unnumbered minor planets using AWB ← Previous edit		Revision as of 17:09, 17 September 2016 edit undoInternetArchiveBot (talk \| contribs)Bots, Pending changes reviewers5,386,303 edits Rescuing 1 sources and tagging 0 as dead. #IABot (v1.2.4)Next edit →
Line 70:		Line 70:
	The size of {{mp\|2002 XV\|93}} has been measured by the ] to be 549.2{{±\|21.7\|23.0}} km.<ref name=Herschel>{{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 = ] \| volume = 541 \| pages = A93 \| date = May 2012\| pmid = \| pmc = \| bibcode = 2012A&A...541A..93M \| arxiv = 1202.3657 }}</ref>		The size of {{mp\|2002 XV\|93}} has been measured by the ] to be 549.2{{±\|21.7\|23.0}} km.<ref name=Herschel>{{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 = ] \| volume = 541 \| pages = A93 \| date = May 2012\| pmid = \| pmc = \| bibcode = 2012A&A...541A..93M \| arxiv = 1202.3657 }}</ref>

	It is ].<ref name=brown>{{cite web\|url=http://www.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=2015-07-22}}</ref>		It is ].<ref name=brown>{{cite web\|url=http://www.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=2015-07-22 \|deadurl=yes \|archiveurl=https://web.archive.org/web/20111018154917/http://www.gps.caltech.edu/~mbrown/dps.html \|archivedate=2011-10-18 \|df= }}</ref>

	==References==		==References==