Dark background asteroid
1072 Malva , provisional designation1926 TA , is a dark backgroundasteroid from the outer regions of theasteroid belt , approximately 48 kilometers in diameter. It was discovered on 4 October 1926, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in Germany.[ 12] The asteroid was named after the flowering plantMalva (mallow).[ 3]
Orbit and classification [ edit ] Malva is a non-family asteroid from the main belt'sbackground population .[ 5] It orbits the Sun in theouter asteroid belt at a distance of 2.4–3.9 AU once every 5 years and 8 months (2,057 days;semi-major axis of 3.17 AU). Its orbit has aneccentricity of 0.24 and aninclination of 8° with respect to theecliptic .[ 1] The body'sobservation arc begins with its official discovery observation at Heidelberg in October 1926.[ 12]
Physical characteristics [ edit ] Malva is an assumedC-type asteroid .[ 4]
Observations performed byBrian Warner at thePalmer Divide Observatory in Colorado Springs, Colorado, during 2007 produced alightcurve with a period of 10.080 ± 0.005 hours and a brightness range of 0.17 ± 0.02 inmagnitude (U=3 ).[ 11] [ a] Another lightcurve obtained by Italian amateur astronomers Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station (A12 ) gave aperiod of 9.0127 hours with an amplitude of 0.17 magnitude (U=2 ).[ 10]
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 ,Malva measures between 45.05 and 53.675 kilometers in diameter and its surface has analbedo between 0.032 and 0.0549.[ 6] [ 7] [ 8] [ 9]
TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0458 and a diameter of 44.97 kilometers based on anabsolute magnitude of 10.7.[ 4]
Thisminor planet was named after the genus of flowering plants,Malva , also known as mallow. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 101 ).[ 3]
Due to his many discoveries,Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between(1009) and(1200) , and also contained a sequence of 28 asteroids, starting with1054 Forsytia , that were all named after plants, in particularflowering plants (also see list of minor planets named after animals and plants) .[ 13]
^a b c d "JPL Small-Body Database Browser: 1072 Malva (1926 TA)" (2017-11-02 last obs.).Jet Propulsion Laboratory . Retrieved7 December 2017 .^ "malva" .Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.) ^a b c Schmadel, Lutz D. (2007). "(1072) Malva".Dictionary of Minor Planet Names – (1072) Malva .Springer Berlin Heidelberg . p. 92.doi :10.1007/978-3-540-29925-7_1073 .ISBN 978-3-540-00238-3 . ^a b c d e f g "LCDB Data for (1072) Malva" . Asteroid Lightcurve Database (LCDB). Retrieved7 December 2017 .^a b "Asteroid 1072 Malva – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved28 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 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 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 . Retrieved7 December 2017 . ^a b Behrend, Raoul."Asteroids and comets rotation curves – (1072) Malva" . Geneva Observatory. Retrieved7 December 2017 . ^a b Warner, Brian D. (September 2007)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory - December 2006 - March 2007" .The Minor Planet Bulletin .34 (3):72– 77.Bibcode :2007MPBu...34...72W .ISSN 1052-8091 . Retrieved7 December 2017 . ^a b "1072 Malva (1926 TA)" .Minor Planet Center . Retrieved7 December 2017 .^ Schmadel, Lutz D. (2007). "(1054) Forsytia".Dictionary of Minor Planet Names – (1054) Forsytia . Springer Berlin Heidelberg. p. 90.doi :10.1007/978-3-540-29925-7_1055 .ISBN 978-3-540-00238-3 .