(202421)_2005_UQ513 Knowpia

(202421) 2005 UQ₅₁₃
	Precovery image of 2005 UQ513, taken by the Palomar Observatory in 22 August 2002.
Discovery
Discovered by	M. E. Brown; D. L. Rabinowitz; C. A. Trujillo
Discovery date	21 October 2005
Designations
MPC designation	(202421) 2005 UQ513
Minor planet category	Cubewano (MPC); ScatExt (DES)
Orbital characteristics
	Epoch 13 January 2016 (JD 2457400.5)
	Uncertainty parameter 3
Observation arc	8474 days (23.20 yr)
Earliest precovery date	15 September 1990
Aphelion	49.689 AU (7.4334 Tm) (Q)
Perihelion	36.713 AU (5.4922 Tm) (q)
Semi-major axis	43.201 AU (6.4628 Tm) (a)
Eccentricity	0.15018 (e)
Orbital period (sidereal)	283.95 yr (103713 d)
Mean anomaly	223.93° (M)
Mean motion	0° 0m 12.496s / day (n)
Inclination	25.7315° (i)
Longitude of ascending node	307.8679° (Ω)
Time of perihelion	≈ 30 July 2123; ±3 days
Argument of perihelion	221.89° (ω)
Earth MOID	35.763 AU (5.3501 Tm)
Jupiter MOID	31.568 AU (4.7225 Tm)
TJupiter	5.253
Physical characteristics
Dimensions	498+63; −75 km
Synodic rotation period	7.03 h (0.293 d)
Sidereal rotation period	7.03 hr?
Geometric albedo	0.31+0.12; −0.065
Apparent magnitude	20.8
Absolute magnitude (H)	3.97

(202421) 2005 UQ₅₁₃ (provisional designation 2005 UQ₅₁₃) is a cubewano with an absolute magnitude of 3.97.^[3] Its spectrum has a weak signature of absorption by water ice.^[10]^[11] Like Quaoar, it has a very red spectrum,^[12]^[13] which indicates that its surface probably contains many complex, processed organic molecules.^[12] Its light curve shows variations of Δm=0.3 mag, but no period has been determined.^[13]

Classification edit

2005 UQ₅₁₃ has a perihelion of 37.3 AU.^[3] The Minor Planet Center (MPC) classifies it as a cubewano^[4] while the Deep Ecliptic Survey (DES) classifies it as ScatExt (scattered-extended).^[5] Although dynamically it would have been a good candidate to be a member of the Haumea collisional family, given its red spectrum, it is not.^[12]^[13]

Distance edit

As of December 2018, it is currently 48.0 AU from the Sun.^[9] It will come to perihelion in 2123.^[7]

It has been observed 194 times over 14 oppositions with precovery images back to 1990.^[3]

References edit

^ Lowe, Andrew. "(202421) 2005 UQ513 Precovery Images". andrew-lowe.ca.
^ Brown, M.; Trujillo, C.; Rabinowitz, D.; Marsden, B. G. (2007). "2003 UY413, 2003 UZ413, 2004 NT33, 2005 CA79, 2005 CB79, 2005 UQ513". Minor Planet Electronic Circulars. 2007-R02: R02. Bibcode:2007MPEC....R...02B.
^ ^a ^b ^c ^d ^e ^f ^g "JPL Small-Body Database Browser: (2005 UQ513)" (2011-12-26 last obs., 12 opp). Retrieved 7 April 2016.
^ ^a ^b "MPEC 2010-S44 : DISTANT MINOR PLANETS (2010 OCT. 11.0 TT)". IAU Minor Planet Center. 2010-09-25. Retrieved 2011-01-26.
^ ^a ^b Marc W. Buie. "Orbit Fit and Astrometric record for 202421" (2012/05/06 using 59 observations). SwRI (Space Science Department). Retrieved 2012-05-05.
^ "AstDyS (202421) 2005UQ513 Orbital information". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.
^ ^a ^b JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.)
^ ^a ^b TNOs are Cool: A survey of the trans-Neptunian region. X. Analysis of classical Kuiper belt objects from Herschel* and Spitzer observations p. 18 arXiv:1403.6309
^ ^a ^b "AstDyS (202421) 2005UQ513 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.
^ Ragozzine, D. & Brown, M. E. (2007). "Candidate Members and Age Estimate of the Family of Kuiper Belt Object 2003 EL₆₁". The Astronomical Journal. 134 (6): 2160–2167. arXiv:0709.0328. Bibcode:2007AJ....134.2160R. doi:10.1086/522334. S2CID 8387493. Retrieved 2009-12-05.
^ Trujillo, C. A., Sheppard, S. S., & Schaller E. L. (2011). A Photometric System for Detection of Water and Methane Ices on Kuiper Belt Objects arXiv:1102.1971
^ ^a ^b ^c Pinilla-Alonso, N., Licandro, J., & Lorenzi, V. (2008). Visible spectroscopy in the neighborhood of 2003 EL₆₁ (Haumea) arXiv:0807.2670
^ ^a ^b ^c Snodgrass, C., Carry, B., Dumas, C., & Hainaut, O. (2009). Characterisation of candidate members of (136108) Haumea’s family arXiv:0912.3171

External links edit

(202421) 2005 UQ513 Precovery Images
(202421) 2005 UQ513 at the JPL Small-Body Database
- Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

[andrew-lowe-1] Lowe, Andrew. "(202421) 2005 UQ513 Precovery Images". andrew-lowe.ca.

[MPEC2007-R02-2] Brown, M.; Trujillo, C.; Rabinowitz, D.; Marsden, B. G. (2007). "2003 UY413, 2003 UZ413, 2004 NT33, 2005 CA79, 2005 CB79, 2005 UQ513". Minor Planet Electronic Circulars. 2007-R02: R02. Bibcode:2007MPEC....R...02B.

[jpldata-3] ^ ^a ^b ^c ^d ^e ^f ^g "JPL Small-Body Database Browser: (2005 UQ513)" (2011-12-26 last obs., 12 opp). Retrieved 7 April 2016.

[MPEC2010-S44-4] "MPEC 2010-S44 : DISTANT MINOR PLANETS (2010 OCT. 11.0 TT)". IAU Minor Planet Center. 2010-09-25. Retrieved 2011-01-26.

[Buie-5] Marc W. Buie. "Orbit Fit and Astrometric record for 202421" (2012/05/06 using 59 observations). SwRI (Space Science Department). Retrieved 2012-05-05.

[AstDySOrb-6] "AstDyS (202421) 2005UQ513 Orbital information". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.

[perihelion-7] JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.)

[TNOsCool8-8] TNOs are Cool: A survey of the trans-Neptunian region. X. Analysis of classical Kuiper belt objects from Herschel* and Spitzer observations p. 18 arXiv:1403.6309

[AstDySEph-9] "AstDyS (202421) 2005UQ513 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.

[10] Ragozzine, D. & Brown, M. E. (2007). "Candidate Members and Age Estimate of the Family of Kuiper Belt Object 2003 EL₆₁". The Astronomical Journal. 134 (6): 2160–2167. arXiv:0709.0328. Bibcode:2007AJ....134.2160R. doi:10.1086/522334. S2CID 8387493. Retrieved 2009-12-05.

[photometricKBO-11] Trujillo, C. A., Sheppard, S. S., & Schaller E. L. (2011). A Photometric System for Detection of Water and Methane Ices on Kuiper Belt Objects arXiv:1102.1971

[specHaumea-12] Pinilla-Alonso, N., Licandro, J., & Lorenzi, V. (2008). Visible spectroscopy in the neighborhood of 2003 EL₆₁ (Haumea) arXiv:0807.2670

[Haumeafcand-13] Snodgrass, C., Carry, B., Dumas, C., & Hainaut, O. (2009). Characterisation of candidate members of (136108) Haumea’s family arXiv:0912.3171

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Summary

Classification edit

Distance edit

See also edit

References edit

External links edit

Discovery^[2]
Precovery image of 2005 UQ₅₁₃, taken by the Palomar Observatory in 22 August 2002.^[1]
Discovered by	M. E. Brown D. L. Rabinowitz C. A. Trujillo
Discovery date	21 October 2005^[3]
Designations
MPC designation	(202421) 2005 UQ₅₁₃
Minor planet category	Cubewano (MPC)^[4] ScatExt (DES)^[5]
Orbital characteristics^[3]^[6]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc	8474 days (23.20 yr)
Earliest precovery date	15 September 1990
Aphelion	49.689 AU (7.4334 Tm) (Q)
Perihelion	36.713 AU (5.4922 Tm) (q)
Semi-major axis	43.201 AU (6.4628 Tm) (a)
Eccentricity	0.15018 (e)
Orbital period (sidereal)	283.95 yr (103713 d)
Mean anomaly	223.93° (M)
Mean motion	0° 0^m 12.496^s / day (n)
Inclination	25.7315° (i)
Longitude of ascending node	307.8679° (Ω)
Time of perihelion	≈ 30 July 2123^[7] ±3 days
Argument of perihelion	221.89° (ω)
Earth MOID	35.763 AU (5.3501 Tm)
Jupiter MOID	31.568 AU (4.7225 Tm)
T_Jupiter	5.253
Physical characteristics
Dimensions	498+63 −75 km^[8]
Synodic rotation period	7.03 h (0.293 d)
Sidereal rotation period	7.03 hr?^[3]
Geometric albedo	0.31+0.12 −0.065^[8]
Apparent magnitude	20.8 ^[9]
Absolute magnitude (H)	3.97 ^[3]