1124 Stroobantia

Metallic asteroid yes 1124 Stroobantia #D6D6D6 6 October 1928 E. Delporte Uccle Obs. (1124) Stroobantia 1928 TB1926 FC1930 BK1951 DJ Paul Stroobant(Belgian astronomer) main-belt(outer) 16 February 2017 (JD 2457800.5) 0 86.39 yr (31,554 days) 3.0157 AU 2.8384 AU 2.9271 AU 0.0303 5.01 yr (1,829 days) 309.88° 0.1968 ms / day 7.7935° 22.248° 264.49° 24.450 0.140 km24.65 1.1 km (IRAS:9)25.823 0.121 km27.03 0.70 km29.68 0.57 km 16.39 h17.0 0.2 h 0.108 0.0140.135 0.0080.1454 0.01650.1569 0.015 (IRAS:9) B–V = 0.702U–B = 0.223Tholen = XMX 10.6710.67 0.22 1124 Stroobantia, provisional designation 1928 TB, is a metallic asteroid from the outer region of the asteroid belt, approximately 25 kilometers in diameter. It was discovered on 6 October 1928, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium. It is named for astronomer Paul Stroobant. Description Stroobantia orbits the Sun at a distance of 2.8–3.0 AU once every 5.01 years (1,829 days). Its orbit has an eccentricity of 0.03 and an inclination of 8° with respect to the ecliptic. First identified as 1926 FC at Heidelberg in 1926, the asteroid's observation arc begins at Algiers Observatory in 1931, or three years after its official discovery observation at Uccle. Physical characteristics In the Tholen taxonomy, Stroobantia is classified as a generic X-type asteroid. It was grouped it into the metallic subcategory of M-type asteroid by a spectroscopic survey of X-type asteroids using the TNG, NTT and IRTF telescopes. Rotation period Two fragmentary rotational lightcurves of Stroobantia were obtained from photometric observations by Ricardo Gil-Hutton at the Félix Aguilar Observatory in Argentina, and by French amateur astronomers Laurent Bernasconi. Lightcuve analysis gave a rotation period of 16.39 and 17.0 hours with a brightness amplitude of 0.15 and 0.06 magnitude, respectively (U=1/1). Diameter and albedo According to the 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, Stroobantia measures between 24.45 and 29.68 kilometers in diameter, and its surface has an albedo between 0.108 and 0.1569. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.1569 and a diameter of 24.65 kilometers with an absolute magnitude of 10.67. Naming This minor planet was named for Paul Stroobant (1868–1936), a Belgian astronomer and director of the Uccle Observatory, where this asteroid was discovered. Stroobant's research included the number, mass and distribution of the minor planets. Naming citation was first mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 105). References 30em 2016-06-08 last obs. JPL Small-Body Database Browser: 1124 Stroobantia (1928 TB) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001124 Jet Propulsion Laboratory 14 March 2017 Dictionary of Minor Planet Names – (1124) Stroobantia Schmadel Lutz D. Springer Berlin Heidelberg 95 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_1125 (1124) Stroobantia 1124 Stroobantia (1928 TB) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=1124 14 March 2017 Asteroids and comets rotation curves – (1124) Stroobantia Behrend Raoul Geneva Observatory http://obswww.unige.ch/~behrend/page3cou.html#001124 14 March 2017 3 December 2002 https://web.archive.org/web/20021203214643/http://obswww.unige.ch/~behrend/page3cou.html#001124 dead 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 14 March 2017 1124 14 March 2017 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 free (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 The Astrophysical Journal 741 2 25 2011ApJ...741...90M 10.1088/0004-637X/741/2/90 1109.6407 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 14 March 2017 Gil-Hutton, Ricardo April 1998 Photometry of Asteroids 558 Carmen, 613 Ginevra, and 1124 Stroobantia http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1998RMxAA..34....9G Revista Mexicana de Astronomía y Astrofísica 34 9(RMxAAHomepage) 1998RMxAA..34....9G 14 March 2017 S. Fornasier B. E. Clark E. Dotto July 2011 Spectroscopic survey of X-type asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011Icar..214..131F Icarus 214 1 131–146 2011Icar..214..131F 10.1016/j.icarus.2011.04.022 1105.3380 14 March 2017 6 Peter Veres Robert Jedicke Alan Fitzsimmons Larry Denneau Mikael Granvik Bryce Bolin Serge Chastel Richard J. Wainscoat William S. Burgett Kenneth C. Chambers Heather Flewelling Nick Kaiser Eugen A. Magnier Jeff S. Morgan Paul A. Price John L. Tonry Christopher Waters November 2015 Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V Icarus 261 34–47 2015Icar..261...34V 10.1016/j.icarus.2015.08.007 1506.00762 14 March 2017 External links Obituary: Paul Stroobant, The Observatory, Vol. 59, p. 349-352 (1936) 1936Obs....59..349. Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 2017-12-16 ) Dictionary of Minor Planet Names, Google books Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 2016-07-29 – Observatoire de Genève, Raoul Behrend Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center 1124 1124 Stroobantia (1928 TB) 2001124 1123 Shapleya 1124 1125 China 001124 Category:Discoveries by Eugène Joseph Delporte Category:Named minor planets 001124 19281006