1035 Amata

Main-belt asteroid October 2019 yes 1035 Amata #D6D6D6 001035-asteroid shape model (1035) Amata.png Modelled shape of Amata from its lightcurve 29 September 1924 K. Reinmuth Heidelberg Obs. (1035) Amata @ ' m ei t @Noah Webster (1884) A Practical Dictionary of the English Language 1924 SW1935 SU1969 TJ 4A913 UC Amata (Roman mythology) main-belt(outer) 16 February 2017 (JD 2457800.5) 0 102.63 yr (37,484 days) 3.7582 AU 2.5551 AU 3.1566 AU 0.1906 5.61 yr (2,049 days) 242.46° 0.1757 ms / day 18.030° 1.9593° 323.98° 50.69 2.9 km (IRAS:5)50.74 km (derived)56.063 0.40459.28 0.79 km59.838 0.563 km60 6 km62.22 1.11 km 9.05 0.01 h9.081 0.001 h9.08215 0.00001 h9.7 0.07 h 0.0374 0.00790.038 0.0030.039 0.0010.04 0.010.0522 0.006 (IRAS:5)0.0571 (derived) C 10.210.3 1035 Amata @ ' m ei t @ is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 57 kilometers in diameter. It was discovered by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany on 29 September 1924 and assigned the provisional designation 1924 SW. It was probably named after Amata from Roman mythology. Classification and orbit The C-type asteroid orbits the Sun at a distance of 2.6–3.8 AU once every 5 years and 7 months (2,049 days). Its orbit has an eccentricity of 0.19 and an inclination of 18° with respect to the ecliptic. The first used observation was taken at the discovering observatory in 1913, extending the body's observation arc by 11 years prior to its discovery. Naming Amatas name is of uncertain origin. It is thought to have been named after Amata, wife of King Latinus in Roman mythology and a character in Virgil's Aeneid. She is also the mother of Lavinia, the wife of Aeneas, after whom 1172 Äneas, one of the largest Jupiter trojans, is named. Unknown meaning Among the many thousands of named minor planets, Amata is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 164 Eva and 1514 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth. Physical characteristics In October 2002, a rotational light-curve of Amata was obtained from photometric observations by American amateur astronomer Robert Stevens at the Santana Observatory (646) in California. It gave a rotation period of 9.081 0.001 hours with a brightness variation of 0.44 in magnitude (U=3). In the same month, another observation was made at the Oakley Observatory in the U.S. state of Indiana and gave a very similar period of 9.05 0.01 hours and a variation in brightness of 0.32 in magnitude (U=2). According to the space-based surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Amata measures between 50.7 and 62.2 kilometers in diameter, and its surface has a low albedo between 0.038 and 0.052. The Collaborative Asteroid Lightcurve Link derived a diameter of 50.7 kilometers and an albedo of 0.057. References 2016-06-16 last obs. JPL Small-Body Database Browser: 1035 Amata (1924 SW) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001035 Jet Propulsion Laboratory 9 December 2016 Dictionary of Minor Planet Names https://archive.org/details/dictionaryminorp00schm limited Schmadel Lutz D. Springer Berlin Heidelberg (1035) Amata 89 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_1036 Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision Appendix 11 – Minor Planet Names with Unknown Meaning Schmadel Lutz D. Springer Berlin Heidelberg 927–929 2007 978-3-540-00238-3 Lutz D. Schmadel 1035 Amata (1924 SW) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=1035 7 June 2016 Asteroids and comets rotation curves – (1035) Amata Behrend Raoul Geneva Observatory https://obswww.unige.ch/~behrend/page3cou.html#001035 7 June 2016 https://web.archive.org/web/20200123022615/https://obswww.unige.ch/~behrend/page3cou.html#001035 23 January 2020 dead 1035 7 June 2016 E. F. Tedesco P. V. Noah M. Noah S. D. Price October 2004 IRAS Minor Planet Survey V6.0 https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab NASA Planetary Data System 12 IRAS-A-FPA-3-RDR-IMPS-V6.0 2004PDSS...12.....T 22 October 2019 6 Fumihiko Usui Daisuke Kuroda Thomas G. Müller Sunao Hasegawa Masateru Ishiguro Takafumi Ootsubo Daisuke Ishihara Hirokazu Kataza Satoshi Takita Shinki Oyabu Munetaka Ueno Hideo Matsuhara Takashi Onaka October 2011 Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey Publications of the Astronomical Society of Japan 63 5 1117–1138 2011PASJ...63.1117U 10.1093/pasj/63.5.1117 (online, AcuA catalog p. 153) 6 A. Mainzer T. Grav J. Masiero E. Hand J. Bauer D. Tholen R. S. McMillan T. Spahr R. M. Cutri E. Wright J. Watkins W. Mo C. Maleszewski November 2011 NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M The Astrophysical Journal 741 2 25 2011ApJ...741...90M 10.1088/0004-637X/741/2/90 1109.6407 35447010 7 June 2016 6 Joseph R. Masiero A. K. Mainzer T. Grav J. M. Bauer R. M. Cutri C. Nugent M. S. Cabrera November 2012 Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M The Astrophysical Journal Letters 759 1 5 2012ApJ...759L...8M 10.1088/2041-8205/759/1/L8 1209.5794 46350317 7 June 2016 6 V. Alí-Lagoa J. de León J. Licandro M. Delbó H. Campins N. Pinilla-Alonso M. S. Kelley June 2013 Physical properties of B-type asteroids from WISE data http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013A&A...554A..71A Astronomy and Astrophysics 554 16 2013A&A...554A..71A 10.1051/0004-6361/201220680 1303.5487 119214002 7 June 2016 6 Elaine Kirkpatrick Brian Hirsch Crystal Lecrone Dustin Schwoenk Michael Shiery Eric Tollefson Andrew Twarek Sarah White Chris Wolfe September 2003 Oakley Observatory lightcurves of asteroids 670 Ottegebe and 1035 Amata https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2003MPBu...30...41K The Minor Planet Bulletin 30 3 41 1052-8091 2003MPBu...30...41K 7 June 2016 Stephens, Robert D. December 2002 Photometry of 1035 Amata and 1829 Dawson https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2003MPBu...30...31S The Minor Planet Bulletin 30 2 31 1052-8091 2003MPBu...30...31S 7 June 2016 J. Durech J. Hanus D. Oszkiewicz R. Vanco March 2016 Asteroid models from the Lowell photometric database http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016A&A...587A..48D Astronomy and Astrophysics 587 6 2016A&A...587A..48D 10.1051/0004-6361/201527573 1601.02909 118427201 7 June 2016 6 Joseph R. Masiero T. Grav A. K. Mainzer C. R. Nugent J. M. Bauer R. Stevenson S. Sonnett August 2014 Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M The Astrophysical Journal 791 2 11 2014ApJ...791..121M 10.1088/0004-637X/791/2/121 1406.6645 119293330 9 December 2016 External links Lightcurve Database Query (LCDB), at www.minorplanet.info Dictionary of Minor Planet Names, Google books Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center 1035 1034 Mozartia 1035 1036 Ganymed 001035 Category:Discoveries by Karl Wilhelm Reinmuth Category:Named minor planets 19240929