(120348) 2004 TY364

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(120348) 2004 TY364
Discovery
Synodic rotation period
11.70 h (0.488 d)[1]
0.107+0.020
−0.015[6]
20.4[7]
4.520±0.070,[6] 4.8[1]

(120348) 2004 TY364, provisionally known as 2004 TY364, is a

Marc Buie's definition[specify].[3] It is also not listed as a scattered disc object by the Minor Planet Center.[8] It was discovered by Michael E. Brown, Chad Trujillo and David L. Rabinowitz on October 3, 2004 at the Palomar Observatory
.

Light-curve analysis suggests it is not a dwarf planet.[9]

As of 2014, it is 39.2 AU from the Sun.[7]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 120348 (2004 TY364)" (2005-09-01 last obs; arc: 22.13 years). Retrieved 7 April 2016.
  2. ^ a b Nomenclature in the outer Solar System
  3. ^
    Marc W. Buie. "Orbit Fit and Astrometric record for 120348"
    (last observation: 2005-08-31 using 20 of 21 observations over 22 years). SwRI (Space Science Department). Retrieved 2014-11-13.
  4. IAU Minor Planet Center
    . 2010-09-25. Retrieved 2014-11-16.
  5. 3-sigma
    .)
  6. ^ a b c Lellouch, E.; Santos-Sanz, P.; Lacerda, P.; Mommert, M.; Duffard, R.; Ortiz, J. L.; Müller, T. G.; Fornasier, S.; Stansberry, J.; Kiss, Cs.; Vilenius, E.; Mueller, M.; Peixinho, N.; Moreno, R.; Groussin, O.; Delsanti, A.; Harris, A. W. (September 2013). ""TNOs are Cool": A survey of the trans-Neptunian region. IX. Thermal properties of Kuiper belt objects and Centaurs from combined Herschel and Spitzer observations" (PDF). Astronomy & Astrophysics. 557: A60.
    doi:10.1051/0004-6361/201322047
    . Retrieved 7 November 2014.
  7. ^ a b "AstDys (120348) 2004TY364 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2009-12-10.
  8. ^ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2014-11-13.
  9. ^ Gonzalo Tancredi & Sofía Favre (13 October 2008). "Dwarf Planet & Plutoid Headquarters". Portal Uruguayo de Astronomía. Retrieved 2010-09-22. (Which are the dwarfs in the Solar System?)

External links


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