Main-belt asteroid
1010 Marlene (prov. designation :A923 VH or 1923 PF ) is a carbonaceous backgroundasteroid from the outer regions of theasteroid belt , approximately 47 kilometers in diameter. It was discovered on 12 November 1923, by astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory in southwest Germany.[ 14] The asteroid was named after German actress and singerMarlene Dietrich .[ 2]
Classification and orbit [ edit ] Marlene is not a member of any knownasteroid family . It orbits the Sun in theouter main-belt at a distance of 2.6–3.2 AU once every 5.02 years (1,832 days). Its orbit has aneccentricity of 0.10 and aninclination of 4° with respect to theecliptic .[ 1]
The asteroid was first identified asA903 UD at the discovering observatory in October 1903. The body'sobservation arc begins at Heidelberg in January 1924, more than two months after its official discovery observation.[ 14]
Thisminor planet was named after German-bornMarlene Dietrich (1901–1992), actor, singer and high-profile entertainer duringWorld War II . The name was proposed by astronomer Gustav Stracke. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 97 ).[ 2]
Physical characteristics [ edit ] Marlene is an assumed carbonaceousC-type asteroid .[ 3]
Photometric measurements ofMarlene – made by American astronomerBrian Warner at the Palmer Divide Observatory (716 ), Colorado, in February 2005 – showed alightcurve with a longer-than averagerotation period of 31.06± 0.02 hours and a brightness variation of 0.32± 0.02 inmagnitude (U=2+ ).[ 11] [ a] Most asteroids have periodsshorter than 20 hours .
Another lightcurve, obtained by French amateur astronomerRené Roy , gave a period of 29.0 hours and an amplitude of 0.17 magnitude (U=2 ).[ 10]
In 2013 and 2016, an international study modeled a lightcurve with a concurring period of 31.0651 and 31.066 hours, respectively. The study also determined twospin axis of (299.0°, 42.0°) and (106.0°, 47.0°) inecliptic coordinates (λ, β) (U=n.a. ).[ 12] [ 13]
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 ,Marlene measures between 43.47 and 51.085 kilometers in diameter and its surface has analbedo between 0.03 and 0.0647.[ 4] [ 5] [ 6] [ 7] [ 8] [ 9]
TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.054 and a diameter of 43.38 kilometers based on anabsolute magnitude of 10.6.[ 3]
^a b c d "JPL Small-Body Database Browser: 1010 Marlene (1923 PF)" (2017-06-05 last obs.).Jet Propulsion Laboratory . Archived fromthe original on 16 December 2019. Retrieved30 August 2017 .^a b c Schmadel, Lutz D. (2007). "(1010) Marlene".Dictionary of Minor Planet Names – (1010) Marlene .Springer Berlin Heidelberg . p. 87.doi :10.1007/978-3-540-29925-7_1011 .ISBN 978-3-540-00238-3 . ^a b c d e f g "LCDB Data for (1010) Marlene" . Asteroid Lightcurve Database (LCDB). Retrieved30 August 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 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 . Retrieved30 August 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 . Retrieved30 August 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 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 . Retrieved30 August 2017 . ^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 Behrend, Raoul."Asteroids and comets rotation curves – (1010) Marlene" .Geneva Observatory . Retrieved30 August 2017 . ^a b Warner, Brian D. (September 2005)."Asteroid lightcurve analysis at the Palmer Divide Observatory – winter 2004-2005" .The Minor Planet Bulletin .32 (3):54– 58.Bibcode :2005MPBu...32...54W .ISSN 1052-8091 . Retrieved30 August 2017 . ^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 . ^a b Hanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method" .Astronomy & Astrophysics .530 : 16.arXiv :1104.4114 .Bibcode :2011A&A...530A.134H .doi :10.1051/0004-6361/201116738 . Retrieved30 August 2017 . ^a b "1010 Marlene (1923 PF)" .Minor Planet Center . Retrieved30 August 2017 .