Main-belt asteroid
456 Abnoba , provisional designation1900 FH , is a stony backgroundasteroid from the central regions of theasteroid belt , approximately 40 kilometers in diameter. It was discovered on 4 June 1900, by astronomersMax Wolf andArnold Schwassmann at theHeidelberg-Königstuhl State Observatory in southwest Germany.[ 16] The asteroid was named after the Celtic deityAbnoba .[ 4]
Orbit and classification [ edit ] Abnoba is a non-family asteroid from the main belt'sbackground population .[ 5] It orbits the Sun in thecentral main-belt at a distance of 2.3–3.3 AU once every 4 years and 8 months (1,701 days). Its orbit has aneccentricity of 0.18 and aninclination of 14° with respect to theecliptic .[ 1]
The body'sobservation arc begins atBordeaux Observatory , eleven days after its official discovery observation at Heidelberg.[ 16]
Physical characteristics [ edit ] In theSMASS classification ,Abnoba is a stonyS-type asteroid .[ 1] Its stony composition was also confirmed by polarimetric observations in 2017.[ 15]
Several rotationallightcurves ofAbnoba have been obtained from photometric observations since 2004.[ 12] [ 13] [ a] Analysis of the best-rated lightcurve from the Bigmuskie Observatory (B88 ) in Italy, gave arotation period of 18.281 hours with a brightness amplitude of 0.32magnitude (U=3 ).[ 14]
Diameter and albedo [ edit ] According to the surveys carried out by the Infrared Astronomical SatelliteIRAS , the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer ,Abnoba measures between 37.64 and 50.495 kilometers in diameter and its surface has analbedo between 0.1467 and 0.286.[ 6] [ 7] [ 8] [ 10] [ 11]
TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2537 and a diameter of 39.94 kilometers based on anabsolute magnitude of 9.1.[ 9]
456 Abnoba has been observed tooccult 6 stars between 2006 and 2023.
Thisminor planet was named after the Gaulish goddessAbnoba from Celtic mythology. The goddess was worshipped in the Black Forest of southern Germany, and known as "Diana Abnoba" to the Roman troops stationed in this region. The official naming citation was authored byLutz D. Schmadel based on his own research.[ 4]
^a b c d e f "JPL Small-Body Database Browser: 456 Abnoba (1900 FH)" (2017-07-02 last obs.).Jet Propulsion Laboratory . Archived fromthe original on 16 September 2020. Retrieved27 September 2017 .^ Walker (1830)A Key to the Classical Pronunciation of Greek, Latin, and Scripture Proper Names ^ Noah Webster (1884)A Practical Dictionary of the English Language ^a b c Schmadel, Lutz D. (2007). "(456) Abnoba".Dictionary of Minor Planet Names – (456) Abnoba .Springer Berlin Heidelberg . p. 51.doi :10.1007/978-3-540-29925-7_457 .ISBN 978-3-540-00238-3 . ^a b "Asteroid 456 Abnoba – Nesvorny HCM Asteroid Families V3.0" .Small Bodies Data Ferret . Retrieved24 October 2019 .^a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids" .The Astrophysical Journal Letters .759 (1): 5.arXiv :1209.5794 .Bibcode :2012ApJ...759L...8M .doi :10.1088/2041-8205/759/1/L8 . Retrieved27 September 2017 . ^a b 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 . Retrieved27 September 2017 . ^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 d e "LCDB Data for (456) Abnoba" . Asteroid Lightcurve Database (LCDB). Retrieved27 September 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 . (online ,AcuA catalog p. 153 )^a b c d 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 . ^a b c Behrend, Raoul."Asteroids and comets rotation curves – (456) Abnoba" .Geneva Observatory . Retrieved27 September 2017 . ^a b Warner, Brian D. (July 2010)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 December - 2010 March" .The Minor Planet Bulletin .37 (3):112– 118.Bibcode :2010MPBu...37..112W .ISSN 1052-8091 . Retrieved27 September 2017 . ^a b Ferrero, Andrea (January 2013)."Rotational Period of Five Asteroids" .The Minor Planet Bulletin .40 (1):31– 32.Bibcode :2013MPBu...40...31F .ISSN 1052-8091 . Retrieved27 September 2017 . ^a b Belskaya, I. N.; Fornasier, S.; Tozzi, G. P.; Gil-Hutton, R.; Cellino, A.; Antonyuk, K.; et al. (March 2017)."Refining the asteroid taxonomy by polarimetric observations" .Icarus .284 :30– 42.Bibcode :2017Icar..284...30B .doi :10.1016/j.icarus.2016.11.003 .hdl :11336/63617 . Retrieved27 September 2017 . ^a b "456 Abnoba (1900 FH)" .Minor Planet Center . Retrieved27 September 2017 .