(24835) 1995 SM55 (provisional designation 1995 SM55 ) is a trans-Neptunian object and member of the Haumea family that resides in the Kuiper belt , located in the outermost region of the Solar System . It was discovered on 19 September 1995, by American astronomer Nichole Danzl of the Spacewatch program at Kitt Peak National Observatory near Tucson, Arizona, in the United States.[ 2] It measures approximately 200 kilometers in diameter and was the second-brightest known object in the Kuiper belt, after Pluto, until 1996 TO66 was discovered.
Origin
1995 SM55 is a member of the Haumea family .[ 3] It has the highest collisional velocity, a δv of 123.3 m/s, of all confirmed members.[ 19] Based on their common pattern of IR water-ice absorptions, neutral visible spectrum [ 20] and the clustering of their orbital elements, the other KBOs 1996 TO66 , 2002 TX300 , 2003 OP32 and 2005 RR43 all appear to be collisional fragments broken off of the dwarf planet Haumea .
Naming
As of January 2025, this minor planet has not been named by the Minor Planet Center .[ 2]
Orbital diagram
1995 SM55 among other members of the Haumea family
References
^ a b c d "JPL Small-Body Database Browser: 24835 (1995 SM55)" (2016-12-29 last obs.). Jet Propulsion Laboratory . Retrieved 8 February 2018 .
^ a b c d "24835 (1995 SM55)" . Minor Planet Center . Retrieved 8 February 2018 .
^ a b c d e Michael E. Brown. "How many dwarf planets are there in the outer solar system?" . California Institute of Technology . Retrieved 8 February 2018 .
^ a b c Johnston, Wm. Robert (15 October 2017). "List of Known Trans-Neptunian Objects" . Johnston's Archive . Retrieved 8 February 2018 .
^ "MPEC 2009-R09 :Distant Minor Planets (2009 SEPT. 16.0 TT)" . IAU Minor Planet Center . 4 September 2009. Retrieved 4 October 2009 .
^ Marc W. Buie . "Orbit Fit and Astrometric record for 24835" (2004-11-02 using 119 of 123 observations). SwRI (Space Science Department). Retrieved 4 October 2009 .
^ JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma .)
^ a b c d e f g "LCDB Data for (24835)" . Asteroid Lightcurve Database (LCDB). Retrieved 8 February 2018 .
^ "Asteroid Size Estimator" . CNEOS NASA/JPL. Retrieved 8 February 2018 .
^ a b Grundy, W. M.; Noll, K. S.; Stephens, D. C. (July 2005). "Diverse albedos of small trans-neptunian objects". Icarus . 176 (1): 184– 191. arXiv :astro-ph/0502229 . Bibcode :2005Icar..176..184G . doi :10.1016/j.icarus.2005.01.007 . S2CID 118866288 .
^
John Stansberry; Will Grundy; Mike Brown; Dale Cruikshank; John Spencer; David Trilling; et al. (2007). Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope . arXiv :astro-ph/0702538 . Bibcode :2008ssbn.book..161S .
^ Thirouin, Audrey; Sheppard, Scott S.; Noll, Keith S.; Moskovitz, Nicholas A.; Ortiz, Jose Luis; Doressoundiram, Alain (June 2016). "Rotational Properties of the Haumea Family Members and Candidates: Short-term Variability" . The Astronomical Journal . 151 (6): 20. arXiv :1603.04406 . Bibcode :2016AJ....151..148T . doi :10.3847/0004-6256/151/6/148 . S2CID 118510175 .
^ Sheppard, Scott S.; Jewitt, David C. (June 2003). "Hawaii Kuiper Belt Variability Project: An Update". Earth, Moon, and Planets . 92 (1): 207– 219. Bibcode :2003EM&P...92..207S . doi :10.1023/B:MOON.0000031943.12968.46 . S2CID 189905992 .
^ Belskaya, Irina N.; Barucci, Maria A.; Fulchignoni, Marcello; Dovgopol, Anatolij N. (April 2015). "Updated taxonomy of trans-neptunian objects and centaurs: Influence of albedo". Icarus . 250 : 482– 491. Bibcode :2015Icar..250..482B . doi :10.1016/j.icarus.2014.12.004 .
^ Jewitt, David; Peixinho, Nuno; Hsieh, Henry H. (November 2007). "U-Band Photometry of Kuiper Belt Objects" . The Astronomical Journal . 134 (5): 2046– 2053. Bibcode :2007AJ....134.2046J . doi :10.1086/522787 .
^ Peixinho, N.; Delsanti, A.; Guilbert-Lepoutre, A.; Gafeira, R.; Lacerda, P. (October 2012). "The bimodal colors of Centaurs and small Kuiper belt objects". Astronomy and Astrophysics . 546 : 12. arXiv :1206.3153 . Bibcode :2012A&A...546A..86P . doi :10.1051/0004-6361/201219057 . S2CID 55876118 .
^ Rabinowitz, David L.; Schaefer, Bradley E.; Schaefer, Martha; Tourtellotte, Suzanne W. (October 2008). "The Youthful Appearance of the 2003 EL61 Collisional Family". The Astronomical Journal . 136 (4): 1502– 1509. arXiv :0804.2864 . Bibcode :2008AJ....136.1502R . doi :10.1088/0004-6256/136/4/1502 . S2CID 117167835 .
^ Romanishin, W.; Tegler, S. C. (December 2005). "Accurate absolute magnitudes for Kuiper belt objects and Centaurs". Icarus . 179 (2): 523– 526. Bibcode :2005Icar..179..523R . doi :10.1016/j.icarus.2005.06.016 .
^ Snodgrass, C.; Carry, B.; Dumas, C.; Hainaut, O. (February 2010). "Characterisation of candidate members of (136108) Haumea's family". Astronomy and Astrophysics . 511 : 9. arXiv :0912.3171 . Bibcode :2010A&A...511A..72S . doi :10.1051/0004-6361/200913031 . S2CID 62880843 .
^ Pinilla-Alonso, N.; Licandro, J.; Gil-Hutton, R.; Brunetto, R. (June 2007). "The water ice rich surface of (145453) 2005 RR43: a case for a carbon-depleted population of TNOs?". Astronomy and Astrophysics . 468 (1): L25. arXiv :astro-ph/0703098 . Bibcode :2007A&A...468L..25P . doi :10.1051/0004-6361:20077294 . S2CID 18546361 .
External links
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