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971 Alsatia

From Wikipedia, the free encyclopedia
Main-belt asteroid

971 Alsatia
Discovery[1]
Discovered byA. Schaumasse
Discovery siteNice Obs.
Discovery date23 November 1921
Designations
(971) Alsatia
Pronunciation/ælˈsʃə/[2]
Named after
Alsace[3](French province)
1921 LF · 1961 AA
A908 UE
main-belt · (middle)
background[4]
EUN(interloper)[5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc108.67 yr (39,693 days)
Aphelion3.0666AU
Perihelion2.2182 AU
2.6424 AU
Eccentricity0.1605
4.30yr (1,569 days)
86.606°
0° 13m 46.2s / day
Inclination13.774°
83.539°
6.2645°
Physical characteristics
Dimensions55.31±13.87 km[6]
60.71±0.88 km[7]
60.867±0.527 km[8]
62.92±0.58 km[9]
63.75±1.7 km[5][10]
64.724±0.657 km[11]
6.81±0.01h[12]
9.600±0.007 h[13]
9.606±0.001 h[14]
9.61±0.02 h[15]
9.614±0.003 h[16][a]
0.0403±0.0078[11]
0.0415±0.002[5][10]
0.043±0.006[9]
0.046±0.002[7]
0.046±0.005[8]
0.05±0.02[6]
SMASS =C[1][5]
B–V = 0.669[1]
U–B = 0.298[1]
10.05[1][5][7][9][10][11] · 10.11±0.10[17] · 10.21[6]

971 Alsatia, provisional designation1921 LF, is a carbonaceous backgroundasteroid from the central region of theasteroid belt, approximately 60 kilometers (37 miles) in diameter. It was discovered on 23 November 1921, by French astronomerAlexandre Schaumasse atNice Observatory in southeastern France.[18] The asteroid was named after the French provinceAlsace.[3]

Orbit and classification

[edit]

Alsatia is a non-family asteroid of the main belt'sbackground population when applying theHierarchical Clustering Method to itsproper orbital elements.[4] It has also been dynamically classified as a member of theEunomia family (502), which has a different spectral type though. This suggests thatAlsatia may be aninterloper to that family.[5]

It orbits the Sun in thecentral main-belt at a distance of 2.2–3.1 AU once every 4 years and 4 months (1,569 days). Its orbit has aneccentricity of 0.16 and aninclination of 14° with respect to theecliptic.[1]

The body'sobservation arc begins with its first identification asA908 UE atHeidelberg Observatory in October 1908, more than 13 years prior to its official discovery observation at Nice.[18]

Physical characteristics

[edit]

In theSMASS classification,Alsatia is a carbonaceousC-type asteroid.[1]

Rotation period

[edit]

Several rotationallightcurves ofAlsatia have been obtained from photometric observations byRobert Stephens (2000),[12]Laurent Bernasconi (2005),[13] astronomer at theOakley Southern Sky Observatory (2011),[15]Brian Warner (2011),[16] and Daniel Klinglesmith (2017).[14] Lightcurve analysis gave a consolidatedrotation period of 9.614 hours with a brightness amplitude of 0.17 to 0.29magnitude (U=2/2/2/3/3-).[5][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,Alsatia measures between 55.31 and 64.724 kilometers in diameter and its surface has analbedo between 0.0403 and 0.05.[6][7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0415 and a diameter of 63.75 kilometers based on anabsolute magnitude of 10.05.[5][10]

Naming

[edit]

Thisminor planet was named after the French provinceAlsace (regained from Germany after theWWI) in northeast France between the Rhine river and the Vosges mountains. In 1922, the discoverer proposed the name Alsace. However, theAstronomical Calculation Institute, then responsible for the naming of minor planets, changed the name in Alsatia.[3] The political status of Alsace has been heavily influenced by historical decisions, wars, and strategic politics.

Notes

[edit]
  1. ^abLightcurve plot of 971 Alsatia, Palmer Divide Observatory, Brian D. Warner (2011). Quality code of 3. Summary figures at theLCDB

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 971 Alsatia (1921 LF)" (2017-07-02 last obs.). Jet Propulsion Laboratory. Retrieved2 November 2017.
  2. ^"Alsatia".Lexico UK English Dictionary.Oxford University Press. Archived fromthe original on 16 September 2020.
  3. ^abcSchmadel, Lutz D. (2007). "(971) Alsatia".Dictionary of Minor Planet Names – (971) Alsatia. Springer Berlin Heidelberg. p. 85.doi:10.1007/978-3-540-29925-7_972.ISBN 978-3-540-00238-3.
  4. ^ab"Asteroid 971 Alsatia – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  5. ^abcdefgh"LCDB Data for (971) Alsatia". Asteroid Lightcurve Database (LCDB). Retrieved2 November 2017.
  6. ^abcdNugent, 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.
  7. ^abcdUsui, 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)
  8. ^abcMasiero, 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. Retrieved2 November 2017.
  9. ^abcdMasiero, 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.S2CID 46350317. Retrieved2 November 2017.
  10. ^abcdeTedesco, 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.
  11. ^abcdMainzer, 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.
  12. ^abStephens, R. D. (September 2000)."Asteroid Photometry at Santana Observatory: Results for 691 Lehigh 762 Pulcova, and 971 Alsatia".The Minor Planet Bulletin.27:27–28.Bibcode:2000MPBu...27...27S. Retrieved21 December 2015.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (971) Alsatia". Geneva Observatory. Retrieved2 November 2017.
  14. ^abKlinglesmith, Daniel A. III; Hendrickx, Sebastian; Kimber, Cameron; Madden, Karl (July 2017)."CCD Asteroid Photometry from Etscorn Observatory".The Minor Planet Bulletin.44 (3):244–246.Bibcode:2017MPBu...44..244K.ISSN 1052-8091. Retrieved2 November 2017.
  15. ^abMelton, Elizabeth; Carver, Spencer; Harris, Andrew; Karnemaat, Ryan; Klaasse, Matthew; Ditteon, Richard (July 2012)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2011 November-December".The Minor Planet Bulletin.39 (3):131–133.Bibcode:2012MPBu...39..131M.ISSN 1052-8091. Retrieved21 December 2015.
  16. ^abWarner, Brian D. (April 2012)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2011 September - December".The Minor Planet Bulletin.39 (2):69–80.Bibcode:2012MPBu...39...69W.ISSN 1052-8091. Retrieved21 December 2015.
  17. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved2 November 2017.
  18. ^ab"971 Alsatia (1921 LF)".Minor Planet Center. Retrieved2 November 2017.

External links

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