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333 Badenia

From Wikipedia, the free encyclopedia
Main-belt asteroid

333 Badenia
Modelled shape ofBadenia from itslightcurve
Discovery[1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date22 August 1892
Designations
(333) Badenia
Pronunciation/bəˈdniə/
Named after
Grand Duchy of Baden
(Großherzogtum Baden)[2]
A892 QA · 1930 JD
1932 TC · 1936 QQ
1937 VB · 1950 BP1
A895 DC · A911 CA
1892 A
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc127.45yr (46,551 d)
Aphelion3.6300AU
Perihelion2.6314 AU
3.1307 AU
Eccentricity0.1595
5.54 yr (2,023 d)
20.070°
0° 10m 40.44s / day
Inclination3.7393°
353.16°
22.785°
Physical characteristics
  • 69.73±2.80 km[6]
  • 72.199±0.259 km[7]
  • 78.17±1.9 km[8]
~1.4 g/cm3[9]
9.862±0.001 h[10][11]
9.4[1][3]

333 Badenia (/bəˈdniə/bə-DEE-nee-ə;prov. designation:A892 QAor1892 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]

Rotation period

[edit]

In April 2017, a rotationallightcurve ofBadenia was obtained fromphotometric observations byFrederick Pilcher. Lightcurve analysis gave arotation period of9.862±0.001 hours with a brightness variation of0.24±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]

References

[edit]
  1. ^abcd"333 Badenia (A892 QA)".Minor Planet Center. Retrieved11 March 2020.
  2. ^abSchmadel, 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.
  3. ^abcdefgh"JPL Small-Body Database Browser: 333 Badenia (A892 QA)" (2020-02-04 last obs.).Jet Propulsion Laboratory. Retrieved11 March 2020.
  4. ^ab"Asteroid 333 Badenia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved11 March 2020.
  5. ^abc"Asteroid 333 Badenia".Small Bodies Data Ferret. Retrieved11 March 2020.
  6. ^abcUsui, 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)
  7. ^abcMainzer, 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.
  8. ^abcTedesco, 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.
  9. ^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.
  10. ^abPilcher, 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.
  11. ^abc"LCDB Data for (333) Badenia". Asteroid Lightcurve Database (LCDB). Retrieved11 March 2020.

External links

[edit]
Minor planets
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Distant minor planet
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