Main-belt asteroid
1135 Colchis (/ˈ k ɒ l k ɪ s / );prov. designation :1929 TA ) is abackground asteroid from the central region of theasteroid belt . It was discovered on 3 October 1929, by Soviet astronomerGrigory Neujmin at theSimeiz Observatory on the Crimean peninsula.[ 4] TheX-type asteroid has arotation period of hours 23.5 and measures approximately 49 kilometers (30 miles) in diameter. It was named for the ancient Kingdom ofColchis .[ 3]
Orbit and classification [ edit ] Colchis is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements .[ 5] [ 6] It orbits the Sun in thecentral main-belt at a distance of 2.4–3.0 AU once every 4 years and 4 months (1,589 days;semi-major axis 2.67 AU). Its orbit has aneccentricity of 0.12 and aninclination of 5° with respect to theecliptic .[ 1] The asteroid was first observed asA911 MJ atJohannesburg Observatory in June 1911. The body'sobservation arc begins atLowell Observatory in September 1929, or four days prior its official discovery observation at Simeiz.[ 4]
Thisminor planet was named after the ancient Kingdom ofColchis , bordering on Black Sea south of the Caucasus mountains, in what is now part ofGeorgia .[ 3] Thenaming was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 106 ).[ 3]
Physical characteristics [ edit ] In theSMASS classification ,Colchis is a Xk-subtype that transitions between theX- andK-type asteroids .[ 1] Conversely, theWide-field Infrared Survey Explorer characterizes it as a primitiveP-type asteroid .[ 11]
In March 2001, a rotationallightcurve ofColchis was obtained from photometric observations byRobert Stephens . Lightcurve analysis gave arotation period of 23.47 hours with a brightness variation of 0.45magnitude (U=2 ).[ 16] In September 2016, French amateur astronomerPatrick Sogorb measured an identical period and an amplitude of 0.46 magnitude (U=2 ).[ 17] A similar period of 23.41 hours with an amplitude of 0.33 magnitude was obtained by astronomers at thePalomar Transient Factory in January 2014.[ 15]
In 2016, two modeled lightcurves using photometric data from the Lowell Photometric Database (LPD) and other sources, gave a concurring period of 23.4827 and 23.4830 hours, respectively. Each modeled lightcurve also determined twospin axis of (139.0°, −58.0°) and (330.0°, −81.0°), as well as (7.0°, −54.0°) and (168.0°, −56.0°) inecliptic coordinates (λ, β), respectively.[ 18] [ 19]
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,Colchis measures between 45.341 and 50.64 kilometers in diameter and its surface has analbedo between 0.05 and 0.068.[ 7] [ 8] [ 9] [ 10] [ 11] [ 13] [ 14]
TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0437 and a diameter of 50.50 kilometers based on anabsolute magnitude of 10.5.[ 12]
^a b c d e f g "JPL Small-Body Database Browser: 1135 Colchis (1929 TA)" (2017-11-24 last obs.).Jet Propulsion Laboratory . Retrieved8 January 2018 .^ "Colchic" .Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.) ^a b c d Schmadel, Lutz D. (2007). "(1135) Colchis".Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 96.doi :10.1007/978-3-540-29925-7_1136 .ISBN 978-3-540-00238-3 . ^a b c "1135 Colchis (1929 TA)" .Minor Planet Center . Retrieved8 January 2018 .^a b "Asteroid 1135 Colchis – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved14 March 2020 .^a b c d "Asteroid 1135 Colchis" .Small Bodies Data Ferret . Retrieved14 March 2020 .^a b c d Masiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos" .The Astronomical Journal .154 (4): 10.arXiv :1708.09504 .Bibcode :2017AJ....154..168M .doi :10.3847/1538-3881/aa89ec . ^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 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 . ^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 . ^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 "LCDB Data for (1135) Colchis" . Asteroid Lightcurve Database (LCDB). Retrieved8 January 2018 .^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 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 Chang, Chan-Kao;Ip, Wing-Huen ; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015). "Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series .219 (2): 19.arXiv :1506.08493 .Bibcode :2015ApJS..219...27C .doi :10.1088/0067-0049/219/2/27 .S2CID 17093124 . ^a b Stephens, R. D.; Malcolm, G. (December 2001)."Collaborative Photometry of 1135 Colchis, March and April 2001" (PDF) .Minor Planet Bulletin .28 (1): 61.Bibcode :2001MPBu...28...61S . Archived fromthe original (PDF) on 13 February 2020. Retrieved14 March 2020 . ^a b Behrend, Raoul."Asteroids and comets rotation curves – (1135) Colchis" .Geneva Observatory . Retrieved6 January 2018 . ^a b Durech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016). "Asteroid models from the Lowell photometric database".Astronomy and Astrophysics .587 : 6.arXiv :1601.02909 .Bibcode :2016A&A...587A..48D .doi :10.1051/0004-6361/201527573 .S2CID 118427201 . ^a b Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics .586 : 24.arXiv :1510.07422 .Bibcode :2016A&A...586A.108H .doi :10.1051/0004-6361/201527441 .S2CID 119112278 .