Dark background asteroid from the inner regions of the asteroid belt
220 Stephania is a dark backgroundasteroid from the inner regions of theasteroid belt , approximately 32 km (20 mi) in diameter. It was discovered on 19 May 1881, by Austrian astronomerJohann Palisa at theVienna Observatory .[ 15] TheC-type asteroid has arotation period of 18.2 hours.[ 4] It was named afterPrincess Stéphanie of Belgium .[ 3]
Classification and orbit [ edit ] Stephania is a non-family asteroid of the main belt'sbackground population , when applying theHierarchical Clustering Method to itsproper orbital elements .[ 5] It orbits the Sun in theinner asteroid belt at a distance of 1.7–3.0 AU once every 3 years and 7 months (1,315 days). Its orbit has aneccentricity of 0.26 and aninclination of 8° with respect to theecliptic .[ 1]
Discovery and naming [ edit ] Stephania was discovered byJohann Palisa on May 19, 1881, inVienna .[ 15] It was the first discovery he made after transferring to the observatory from Pola.[ 3]
The name honoursCrown Princess Stéphanie (1864–1945), wife of theheir-apparent Crown Prince Rudolf of Austria . The couple was married the year the asteroid was discovered. It was the first time that a naming commemorated a wedding and was given as a wedding gift.[ 3] The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 27 ).[ 3]
Physical characteristics [ edit ] In theTholen classification , this asteroid's spectrum is ambiguous, close to anX-type and somewhat similar to that of a carbonaceousC-type asteroid (CX).[ 4] A French spectroscopic survey that observed two dozens of these X-types classified by Tholen, determined thatStephania is in fact a carbonaceousC-type asteroid (rather than an X-type).[ 14] TheWide-field Infrared Survey Explorer (WISE) has also characterized it as a primitiveP-type asteroid .[ 4] [ 11]
Lightcurve data has also been recorded by observers at the Antelope Hill Observatory (H09 ), which has been designated as an official observatory by theMinor Planet Center .[ b]
Diameter and albedo [ edit ] According to the surveys carried out by the Infrared Astronomical SatelliteIRAS , the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Stephania measures between 31.12 and 38.46 kilometers in diameter and its surface has a lowalbedo between 0.03 and 0.075.[ 6] [ 7] [ 8] [ 9] [ 10] [ 11] [ 12] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0607 and a diameter of 31.04 kilometers based on anabsolute magnitude of 11.2.[ 4]
^ Anonymous lightcurve –CALL-2011 (web): rotation period 18.19 hours with a brightness amplitude of 0.25 mag. Quality code of 2. Summary figures for (220) Stephania at theLCDB ^a b Lightcurve plot of (220) Stephania by Robert A. Koff (a.k.a. William Koff) Antelope Hills Observatory, Colorado (H09 ); Rotation period 18.21 hours with a brightness amplitude of 0.21 mag. Quality code of 2. Summary figures at theLCDB ^a b c d e "JPL Small-Body Database Browser: 220 Stephania" (2017-07-01 last obs.).Jet Propulsion Laboratory . Retrieved28 October 2017 .^ "Stephanian" .Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.) ^a b c d e Schmadel, Lutz D. (2007). "(220) Stephania".Dictionary of Minor Planet Names – (220) Stephania .Springer Berlin Heidelberg . p. 35.doi :10.1007/978-3-540-29925-7_221 .ISBN 978-3-540-00238-3 . ^a b c d e f g h i "LCDB Data for (220) Stephania" . Asteroid Lightcurve Database (LCDB). Retrieved28 October 2017 .^a b "Asteroid 220 Stephania" .Small Bodies Data Ferret . Retrieved24 October 2019 .^a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0" .NASA Planetary Data System .12 : IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode :2004PDSS...12.....T . Retrieved22 October 2019 . ^a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos" .The Astrophysical Journal .791 (2): 11.arXiv :1406.6645 .Bibcode :2014ApJ...791..121M .doi :10.1088/0004-637X/791/2/121 .S2CID 119293330 . Retrieved28 October 2017 . ^a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos" .The Astrophysical Journal .814 (2): 13.arXiv :1509.02522 .Bibcode :2015ApJ...814..117N .doi :10.1088/0004-637X/814/2/117 .S2CID 9341381 . Retrieved28 October 2017 . ^a b c d Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey" .Publications of the Astronomical Society of Japan .63 (5):1117– 1138.Bibcode :2011PASJ...63.1117U .doi :10.1093/pasj/63.5.1117 . ^a b c d Durech, J.; Delbo', M.; Carry, B.; Hanus, J.; Alí-Lagoa, V. (July 2017)."Asteroid shapes and thermal properties from combined optical and mid-infrared photometry inversion" .Astronomy and Astrophysics .604 : 8.arXiv :1706.01232 .Bibcode :2017A&A...604A..27D .doi :10.1051/0004-6361/201730868 .S2CID 54934721 . Retrieved28 October 2017 . ^a b c d e f Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal .741 (2): 25.arXiv :1109.6407 .Bibcode :2011ApJ...741...90M .doi :10.1088/0004-637X/741/2/90 .S2CID 35447010 . ^a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos" .The Astronomical Journal .152 (3): 12.arXiv :1606.08923 .Bibcode :2016AJ....152...63N .doi :10.3847/0004-6256/152/3/63 . ^ Mohamed, R. A.; Chiorny, V. G.; Dovgopol, A. N.; Shevchenko, V. G. (November 1994)."Photometry of five asteroids: 189 Phthia, 220 Stephania, 289 Nenetta, 312 Pierretta and 626 Notburga" .Astronomy and Astrophysics Supplement .108 :69– 72.Bibcode :1994A&AS..108...69M . Retrieved28 October 2017 . ^a b Fornasier, S.; Clark, B. E.; Dotto, E. (July 2011). "Spectroscopic survey of X-type asteroids".Icarus .214 (1):131– 146.arXiv :1105.3380 .Bibcode :2011Icar..214..131F .doi :10.1016/j.icarus.2011.04.022 .S2CID 118549118 . ^a b "220 Stephania" .Minor Planet Center . Retrieved28 October 2017 .