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(307261) 2002 MS 4 is a large, the second-largest known object in the Solar System without a name, after. It was discovered in 2002. Brown's website lists it as to be a. The estimated it to have a diameter of 000000000♠726 ±123 km.

First published: 17 January 2002. Cited by: 1285. Figures; Related. 2002 Seattle Mariners Statistics 2001 Season 2003 Season Record: 93-69, Finished 3rd in AL_West ( Schedule and Results ).

The Herschel team estimates it to be 000000000♠934 ±47 km, which would make it one of the 10 largest TNOs currently known and large enough to be considered a dwarf planet under the of the. It is currently 47.2 AU from the Sun and will come to in 2123. It has been observed 55 times, with images back to April 8, 1954. Retrieved 2009-08-26.

IAU Minor Planet Center. Retrieved 2009-08-31. • (2008-05-03). SwRI (Space Science Department). From the original on 4 June 2011.

Retrieved 2009-08-31. • ^ (2009-09-19 last obs.).

Retrieved 7 April 2016. • ^ Vilenius, E.; Kiss, C.; Mommert, M.; et al. ' 'TNOs are Cool': A survey of the trans-Neptunian region VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects'. Astronomy & Astrophysics. 541: A94.:.. • Tegler, Stephen C.

Archived from on November 16, 2007. Retrieved 2006-11-05. Department of Mathematics, University of Pisa, Italy. From the original on 2009-09-04. Retrieved 2009-08-27. Archived from on 2011-10-18.

Retrieved 2011-08-25. • Stansberry, Grundy, Brown, Spencer, Trilling, Cruikshank, Luc Margot Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope (2007) • (2006-08-16). Harvard-Smithsonian Center for Astrophysics and IAU EC Planet Definition Committee chair. Retrieved 2007-03-13. External links [ ] • • at the •.