Main-belt asteroid
763 Cupido (prov. designation :A913 SE or 1913 ST ) is aFlora asteroid ,tumbler andslow rotator from the inner regions of theasteroid belt , approximately 7 kilometers (4.3 miles) in diameter. It was discovered on 25 September 1913, by German astronomerFranz Kaiser at theHeidelberg-Königstuhl State Observatory in southwest Germany.[ 1] TheS /L-type asteroid has an exceptionally longrotation period of 151 hours. It was named by its Latin name afterCupid , the Roman god of erotic love, attraction and affection.[ 3]
Orbit and classification [ edit ] When applying the synthetichierarchical clustering method (HCM) byNesvorný ,[ 5] or the 1995 HCM-analysis byZappalà ,[ 6] Cupido is a member of theFlora family (402 ), a giantasteroid family and the largest family of stony asteroids in the main-belt.[ 14] : 23 However, according to another HCM-analysis byMilani andKnežević (AstDys), it is abackground asteroid as this analysis does not recognize the Floraasteroid clan .[ 7] Cupido orbits the Sun in theinner asteroid belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,226 days;semi-major axis of 2.24 AU). Its orbit has aneccentricity of 0.17 and aninclination of 4° with respect to theecliptic .[ 4] The body'sobservation arc begins atYerkes Observatory (754 ) in September 1933, or 20 years after to its official discovery observation byFranz Kaiser atHeidelberg Observatory in 1913.[ 1]
Thisminor planet was named "Cupido", the Latin name ofCupid , god of erotic love, attraction and affection inRoman mythology whose Greek counterpart isEros (also see asteroid433 Eros ) .Cupido was named due to its relative proximity to the Sun probably by Swedish astronomerBror Ansgar Asplind (1890–1954) who was honored by asteroid958 Asplinda . Thenaming was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 76 ).[ 3]
Physical characteristics [ edit ] In theSDSS -based taxonomy,Cupido is an SL-type that transitions from the common, stonyS-type asteroids to the uncommonL-type asteroids .[ 12]
In October 2017, a rotationallightcurve ofCupido was obtained fromphotometric observations by American astronomerFrederick Pilcher in collaboration with Vladimir Benishek atBelgrade Observatory andDaniel A. Klinglesmith at Etscorn Observatory (719 ). Lightcurve analysis gave arotation period of 151.5± 0.1 hours with a brightness variation of 0.45± 0.10magnitude (U=3- ). The observations also showed that it is atumbling asteroid , which wobbles on its non-principal axis rotation.[ 11] During the same opposition,Tom Polakis at the Command Module Observatory (V02 ) also observed the asteroid and measured a period of 151.1± 0.1 hours and an amplitude of 0.24± 0.02 magnitude (U=2+ ).[ 15] The results supersede a tentative period determination of 14.88 hours byRené Roy from 2005.[ 16]
Diameter and albedo [ edit ] According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Cupido measures ( 7.005± 0.115 ) kilometers in diameter and its surface has analbedo of ( 0.373± 0.072 ).[ 9] [ 10] Other publications by the WISE team give amean diameter of ( 7.38± 1.57 km ), ( 7.644± 0.067 km ) and ( 7.76± 0.30 km ) with a corresponding albedo of ( 0.33± 0.14 ), ( 0.3037± 0.0529 ) and ( 0.322± 0.046 ), respectively.[ 17] [ 13] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for aFlora asteroid of 0.20 and calculates a diameter of 8.97 kilometers based on anabsolute magnitude of 12.6.[ 13]
^a b c d e "763 Cupido (A913 SE)" .Minor Planet Center . Retrieved2 June 2020 .^ Noah Webster (1884)A Practical Dictionary of the English Language ^a b c Schmadel, Lutz D. (2007). "(763) Cupido".Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 72.doi :10.1007/978-3-540-29925-7_764 .ISBN 978-3-540-00238-3 . ^a b c d "JPL Small-Body Database Browser: 763 Cupido (A913 SE)" (2020-04-28 last obs.).Jet Propulsion Laboratory . Retrieved2 June 2020 .^a b "Asteroid 763 Cupido – Nesvorny HCM Asteroid Families V3.0" .Small Bodies Data Ferret . Retrieved2 June 2020 .^a b Zappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997)."Asteroid Dynamical Families" .NASA Planetary Data System : EAR-A-5-DDR-FAMILY-V4.1. Retrieved2 June 2020 . (PDS main page )^a b "Asteroid 763 Cupido – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved2 June 2020 .^ Gifford & Dyce (1833)Some account of Shirley and his writings , p. 46 ^a b c d Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0" .NASA Planetary Data System .Bibcode :2016PDSS..247.....M . Retrieved2 June 2020 . ^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 . ^a b Pilcher, Frederick; Benishek, Vladimir; Klinglesmith, Daniel A. III; Odden, Caroline E.; Pennington, Olin O. (April 2018)."763 Cupido: A Tumbling Asteroid" (PDF) .Minor Planet Bulletin .45 (2):111– 112.Bibcode :2018MPBu...45..111P .ISSN 1052-8091 . Archived fromthe original (PDF) on 12 February 2020. Retrieved1 June 2020 . ^a b Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids" .Astronomy and Astrophysics .510 : 12.Bibcode :2010A&A...510A..43C .doi :10.1051/0004-6361/200913322 . Retrieved2 June 2020 . (PDS data set) ^a b c "LCDB Data for (763) Cupido" . Asteroid Lightcurve Database (LCDB). Retrieved2 June 2020 .^ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV . pp. 297– 321.arXiv :1502.01628 .Bibcode :2015aste.book..297N .doi :10.2458/azu_uapress_9780816532131-ch016 .ISBN 978-0-8165-3213-1 .S2CID 119280014 . ^ Polakis, Tom (April 2018)."Lightcurve Analysis for Seven Main-belt Asteroids" (PDF) .Minor Planet Bulletin .45 (2):112– 115.Bibcode :2018MPBu...45..112P .ISSN 1052-8091 . Archived fromthe original (PDF) on 12 February 2020. Retrieved1 June 2020 . ^ Behrend, Raoul."Asteroids and comets rotation curves – (763) Cupido" . Geneva Observatory. Retrieved2 June 2020 . ^ "Asteroid 763 Cupido" .Small Bodies Data Ferret . Retrieved2 June 2020 .