1115 Sabauda

Carbonaceous Meliboean asteroid October 2019 yes 1115 Sabauda #D6D6D6 L. Volta Pino Torinese Obs. 13 December 1928 (1115) Sabauda 1928 XCA906 YF s ə ' b ɔː d ə House of Savoy(former rulers of Italy) main-belt(outer)Meliboea 4 September 2017 (JD 2458000.5) 0 88.47 yr (32,314 days) 3.6333 AU 2.5750 AU 3.1041 AU 0.1705 5.47 yr (1,998 days) 58.449° 0.1802 ms / day 15.271° 71.679° 57.292° 67.24 21.50 km68.53 km (derived)68.82 1.8 km70.76 0.90 km75.907 0.656 km75.91 0.66 km 6.7165 0.0007 hlcdb-Polakis-2017b6.718 0.001 h6.72 0.01 hlightcurve-plot6.72 0.05 h6.732 0.005 h 0.04 0.060.044 0.0060.0496 (derived)0.068 0.0020.0711 0.004 C 9.309.609.63 0.629.699.7 1115 Sabauda s ə ' b ɔː d ə is a carbonaceous Meliboean asteroid from the outer region of the asteroid belt, approximately 68 kilometers in diameter. Discovered in 1928 by Italian astronomer Luigi Volta, it was assigned the provisional designation 1928 XC. The asteroid was probably named after the House of Savoy, the former rulers of Italy. Discovery Sabauda was discovered on 13 December 1928, by Italian astronomer Luigi Volta at the Observatory of Turin (Pino Torinese Observatory). Five nights later, it was independently discovered by Catalan astronomer Josep Comas i Solà at the Fabra Observatory in Barcelona, Spain. The asteroid was first identified as A906 YF at Heidelberg Observatory in December 1906, and its observation arc begins at Heidelberg in January 1929, one month after its official discovery observation at Pino Torinese. Orbit and classification Sabauda is a member of the Meliboea family, a smaller asteroid family of carbonaceous outer-belt asteroids with a few hundred members, named after 137 Meliboea.23 It orbits the Sun in the outer main-belt at a distance of 2.6–3.6 AU once every 5 years and 6 months (1,998 days). Its orbit has an eccentricity of 0.17 and an inclination of 15° with respect to the ecliptic. Physical characteristics Sabauda is an assumed carbonaceous C-type asteroid, in line with the Meliboea family's overall spectral type.23 Rotation period Several rotational lightcurves of Sabauda were obtained from photometric observations. Lightcurve analysis gave a rotation period between 6.718 and 6.732 hours with a brightness amplitude of 0.16 to 0.27 magnitude (U=2+/3-/3).lcdb-Polakis-2017blightcurve-plot Diameter and albedo According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Sabauda measures between 67.24 and 75.91 kilometers in diameter and its surface has an albedo between 0.04 and 0.0711. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0496 and a diameter of 68.53 kilometers based on an absolute magnitude of 9.7. Naming This minor planet bears the Latin name of the former rulers of Italy, the House of Savoy (Sabauda, or Sapauda). It is also possible that it was named after the new established town of Sabauda in the Pontine Marshes, central Italy. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 104). Notes lightcurve-plot Lightcurve plot of 1115 Sabauda, Palmer Divide Observatory, Brian D. Warner (2006) lcdb-Polakis-2017b Polakis (2017) publication currently not yet indexed in ADS. Rotation period 6.7165 0.0007 hours. Summary figures for (1115) Sabauda at Collaborative Asteroid Lightcurve Link (CALL) References 30em 2017-07-02 last obs. JPL Small-Body Database Browser: 1115 Sabauda (1928 XC) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001115 Jet Propulsion Laboratory 2 September 2017 Schmadel Lutz D. Dictionary of Minor Planet Names Springer Berlin Heidelberg 95 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_1116 (1115) Sabauda 1115 Sabauda (1928 XC) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=1115 2 September 2017 Asteroids and comets rotation curves – (1115) Sabauda Behrend Raoul Geneva Observatory https://obswww.unige.ch/~behrend/page3cou.html#001115 2 September 2017 https://web.archive.org/web/20200123022615/https://obswww.unige.ch/~behrend/page3cou.html#001115 23 January 2020 dead Asteroid 1115 Sabauda – Nesvorny HCM Asteroid Families V3.0 Small Bodies Data Ferret https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1115+Sabauda#Asteroid%201115%20SabaudaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0 26 October 2019 https://web.archive.org/web/20201004034002/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1115+Sabauda#Asteroid%201115%20SabaudaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0 4 October 2020 dead D. Nesvorný M. Broz V. Carruba December 2014 Identification and Dynamical Properties of Asteroid Families Asteroids IV 297–321 2015aste.book..297N 10.2458/azu_uapress_9780816532131-ch016 1502.01628 9780816532131 1115 2 September 2017 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 2 September 2017 6 C. R. Nugent A. Mainzer J. Bauer R. M. Cutri E. A. Kramer T. Grav J. Masiero S. Sonnett E. L. Wright September 2016 NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos The Astronomical Journal 152 3 12 2016AJ....152...63N 10.3847/0004-6256/152/3/63 1606.08923 free 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) 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 Warner, Brian D. December 2006 Asteroid lightcurve analysis at the Palmer Divide Observatory - March - June 2006 https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006MPBu...33...85W The Minor Planet Bulletin 33 4 85–88 1052-8091 2006MPBu...33...85W 2 September 2017 Ruthroff, John C. April 2013 Lightcurve Analysis of Main Belt Asteroids 1115 Sabauda 1554 Yugoslavia, 1616 Filipoff, 2890 Vilyujsk, (5153) 1940 GO, and (31179) 1997 YR2 https://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2013MPBu...40...90R The Minor Planet Bulletin 40 2 90–91 1052-8091 2013MPBu...40...90R 2 September 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 2 September 2017 External links Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 ) Dictionary of Minor Planet Names, Google books Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center 1115 1114 Lorraine 1115 1116 Catriona 001115 Category:Discoveries by Luigi Volta Category:Named minor planets 19281213