Background asteroid
1069 Planckia , provisional designation1927 BC , is abackground asteroid from the outer regions of theasteroid belt , approximately 39 kilometers (24 miles) in diameter. It was discovered on 28 January 1927, by astronomerMax Wolf at theHeidelberg-Königstuhl State Observatory in Germany.[ 14] The asteroid was named after German physicistMax Planck .[ 2]
Orbit and classification [ edit ] Planckia is a non-family asteroid from the main belt'sbackground population .[ 4] It orbits the Sun in theouter main-belt at a distance of 2.8–3.5 AU once every 5 years and 6 months (2,019 days;semi-major axis of 3.13 AU). Its orbit has aneccentricity of 0.11 and aninclination of 14° with respect to theecliptic .[ 1] The body'sobservation arc begins at Heidelberg in February 1927, or 10 days after its official discovery observation.[ 14]
Thisminor planet was named after noted German physicistMax Planck (1858–1947), on the commemoration of his 80th birthday. He was a professor of physics at Berlin University and the founder ofquantum mechanics . In 1918, he received theNobel prize in Physics . The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 101 ). He is also honored by a lunar craterPlanck .[ 2]
Physical characteristics [ edit ] In theSMASS classification ,Planckia is a common, stonyS-type asteroid .[ 1] [ 3]
Between 2000 and 2010, several rotationallightcurves ofPlanckia were obtained from photometric observations byBrian Warner , Jérôme Caron andRené Roy (U=2/3/3/2/2- ).[ 10] [ 11] [ 12] [ 13] Lightcurve analysis gave a consolidatedrotation period of 8.665 hours with a brightness amplitude between 0.14 and 0.42magnitude .[ 3] [ a]
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 ,Planckia measures between 35.657 and 44.34 kilometers in diameter and its surface has analbedo between 0.1771 and 0.219.[ 5] [ 6] [ 7] [ 8] [ 9]
TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1982 and a diameter of 39.35 kilometers based on anabsolute magnitude of 9.4.[ 3]
^a b c d e f "JPL Small-Body Database Browser: 1069 Planckia (1927 BC)" (2017-10-29 last obs.).Jet Propulsion Laboratory . Retrieved7 December 2017 .^a b c Schmadel, Lutz D. (2007). "(1069) Planckia".Dictionary of Minor Planet Names .Springer Berlin Heidelberg . p. 91 .doi :10.1007/978-3-540-29925-7_1070 .ISBN 978-3-540-00238-3 . ^a b c d e f g h "LCDB Data for (1069) Planckia" . Asteroid Lightcurve Database (LCDB). Retrieved7 December 2017 .^a b "Asteroid 1069 Planckia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019 .^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 . ^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 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 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 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 Warner, B. D.; Malcolm, G.; Stephens, R. D. (December 2001)."The Lightcurve of 1069 Planckia Revisited" (PDF) .Minor Planet Bulletin .28 (1):71– 72.Bibcode :2001MPBu...28...71W . Archived fromthe original (PDF) on 13 February 2020. Retrieved12 March 2020 . ^a b c Behrend, Raoul."Asteroids and comets rotation curves – (1069) Planckia" .Geneva Observatory . Retrieved7 December 2017 . ^a b Warner, Brian D. (July 2010)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 December - 2010 March" (PDF) .Minor Planet Bulletin .37 (3):112– 118.Bibcode :2010MPBu...37..112W .ISSN 1052-8091 . Archived fromthe original (PDF) on 13 February 2020. Retrieved12 March 2020 . ^a b Warner, B. (September 2001)."Asteroid Photometry at the Palmer Divide Observatory" (PDF) .Minor Planet Bulletin .28 (1):40– 41.Bibcode :2001MPBu...28...40W . Archived fromthe original (PDF) on 13 February 2020. Retrieved12 March 2020 . ^a b "1069 Planckia (1927 BC)" .Minor Planet Center . Retrieved7 December 2017 .