Main-belt asteroid
333 Badenia (/b ə ˈ d iː n i ə / bə-DEE -nee-ə ;prov. designation :A892 QA or 1892 A ) is a largebackground asteroid , approximately 72 kilometers (45 miles) in diameter, located the outer region of theasteroid belt . It was discovered on 22 August 1892, by astronomerMax Wolf at theHeidelberg-Königstuhl State Observatory in southwest Germany.[ 1] The carbonaceousC-type asteroid has arotation period of 9.9 hours. It was named after the historicalGrand Duchy of Baden that existed until 1918, and where the discovering observatory is located.[ 2] Badenia was the first asteroid to receive a provisional designation.
Orbit and classification [ edit ] Badenia is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements .[ 4] [ 5] It orbits the Sun in theouter main-belt at a distance of 2.6–3.6 AU once every 5 years and 6 months (2,023 days;semi-major axis of 3.13 AU). Its orbit has aneccentricity of 0.16 and aninclination of 4° with respect to theecliptic .[ 3]
Physical characteristics [ edit ] In theTholen classification ,Badenia is a common carbonaceousC-type asteroid , though with a nosy spectrum (:).[ 3]
In April 2017, a rotationallightcurve ofBadenia was obtained fromphotometric observations byFrederick Pilcher . Lightcurve analysis gave arotation period of 9.862± 0.001 hours with a brightness variation of 0.24± 0.02magnitude (U=3 ).[ 10] [ 11]
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 ,Badenia measures between 64.01 and 78.51 kilometers in diameter and its surface has analbedo between 0.047 and 0.061.[ 5] [ 6] [ 7] [ 8] TheCollaborative Asteroid Lightcurve Link adopts the results from IRAS, that is, an albedo of 0.0475 and a diameter of 78.17 kilometers based on anabsolute magnitude of 9.46.[ 11]
^a b c d "333 Badenia (A892 QA)" .Minor Planet Center . Retrieved11 March 2020 .^a b Schmadel, Lutz D. (2007). "(333) Badenia".Dictionary of Minor Planet Names . Springer Berlin Heidelberg. p. 43 .doi :10.1007/978-3-540-29925-7_334 .ISBN 978-3-540-00238-3 . ^a b c d e f g h "JPL Small-Body Database Browser: 333 Badenia (A892 QA)" (2020-02-04 last obs.).Jet Propulsion Laboratory . Retrieved11 March 2020 .^a b "Asteroid 333 Badenia – Proper Elements" . AstDyS-2, Asteroids – Dynamic Site. Retrieved11 March 2020 .^a b c "Asteroid 333 Badenia" .Small Bodies Data Ferret . Retrieved11 March 2020 .^a b c 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 Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0" .NASA Planetary Data System .Bibcode :2016PDSS..247.....M . Retrieved11 March 2020 . ^a b c 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 . Retrieved11 March 2020 . ^ Krasinsky, G. A.; Pitjeva, E. V.; Vasilyev, M. V.; Yagudina, E. I. (July 2002). "Hidden Mass in the Asteroid Belt".Icarus .158 (1):98– 105.Bibcode :2002Icar..158...98K .doi :10.1006/icar.2002.6837 .ISSN 0019-1035 . ^a b Pilcher, Frederick (October 2017)."Rotation Period Determination for 46 Hestia, 118 Peitho, 333 Badenia, 356 Liguria, and 431 Nephele" (PDF) .Minor Planet Bulletin .44 (4):294– 297.Bibcode :2017MPBu...44..294P .ISSN 1052-8091 . ^a b c "LCDB Data for (333) Badenia" . Asteroid Lightcurve Database (LCDB). Retrieved11 March 2020 .