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1308 Halleria

From Wikipedia, the free encyclopedia
Main-belt asteroid

1308 Halleria
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date12 March 1931
Designations
(1308) Halleria
Named after
Albrecht von Haller[2]
(Swiss physiologist)
1931 EB · 1933 SP
1936 FU1 · 1938 SO1
1938 SP1 · 1953 TT
1963 VA · A901 DB
main-belt · (outer)[3]
Charis[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc116.76 yr (42,645 days)
Aphelion2.9438AU
Perihelion2.8738 AU
2.9088 AU
Eccentricity0.0120
4.96yr (1,812 days)
173.29°
0° 11m 55.32s / day
Inclination5.5766°
354.14°
164.00°
Physical characteristics
Dimensions39.33±12.48 km[5]
41.87±10.07 km[6]
43.13 km(derived)[3]
43.16±1.4 km[7]
45.05±0.57 km[8]
46.951±0.275 km[9]
50.046±0.301 km[10]
6.013h[a]
6.026±0.002 h[11]
6.028±0.004 h[11]
0.0338±0.0116[10]
0.038±0.009[9]
0.0415(derived)[3]
0.042±0.001[8]
0.0454±0.003[7]
0.05±0.06[6]
0.05±0.07[5]
C(assumed)[3]
10.80[5][7][8][10] · 10.9[1][3] · 10.95[6] · 10.97±0.28[12]

1308 Halleria, provisional designation1931 EB, is a carbonaceous Charisasteroid from the outer regions of theasteroid belt, approximately 43 kilometers in diameter. It was discovered on 12 March 1931, by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory.[13] The asteroid was named afterAlbrecht von Haller a Swiss physician, botanist and poet.[2]

Orbit and classification

[edit]

Halleria belongs to the carbonaceousCharis family (616),[4] afamily of more than 800 members, named after its parent body627 Charis.[14]: 23  It orbits the Sun in theouter main-belt at a distance of 2.87–2.94 AU once every 4 years and 12 months (1,812 days;semi-major axis 2.91 AU). Its orbit has aneccentricity of 0.01 and aninclination of 6° with respect to theecliptic.[1]

The asteroid was first observed asA901 DB at Heidelberg Observatory in February 1901. The body'sobservation arc begins with its official discovery observation in March 1931.[13]

Physical characteristics

[edit]

Halleria is an assumed carbonaceousC-type asteroid,[3] which agrees with the overallspectral type for members of theCharis family.[14]: 23 

Rotation period

[edit]

Between 2005 and 2011, three rotationallightcurves ofHalleria were obtained from photometric observations byDonald Pray,René Roy, andPierre Antonini (U=3/3-/3).[11][a] Lightcurve analysis gave a consolidatedrotation period of 6.028 hours with a brightness amplitude between 0.14 and 0.17magnitude.[3]

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,Halleria measures between 39.33 and 50.046 kilometers in diameter and its surface has analbedo between 0.0338 and 0.05.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0415 and a diameter of 43.13 kilometers based on anabsolute magnitude of 10.9.[3]

Naming

[edit]

Thisminor planet was named forAlbrecht von Haller (1708–1777) a Swiss physician, botanist and poet. The naming took place during the 1935 meeting of theAstronomische Gesellschaft in Bern, Switzerland. The author of theDictionary of Minor Planet Names learned about the naming circumstances from Dutch astronomerIngrid van Houten-Groeneveld.[2]

Notes

[edit]
  1. ^abPray (2011): rotation period6.013 hours with a brightness amplitude of0.14 mag. Quality code of 3. Summary figures for (1308) Halleria at theLCDB

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1308 Halleria (1931 EB)" (2017-11-25 last obs.). Jet Propulsion Laboratory. Retrieved20 December 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1308) Halleria".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 107.doi:10.1007/978-3-540-29925-7_1309.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1308) Halleria". Asteroid Lightcurve Database (LCDB). Retrieved20 December 2017.
  4. ^ab"Asteroid 1308 Halleria – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdNugent, 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. Retrieved20 December 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. ^abcdTedesco, 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.
  8. ^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)
  9. ^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.
  10. ^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.
  11. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1308) Halleria". Geneva Observatory. Retrieved20 December 2017.
  12. ^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. Retrieved20 December 2017.
  13. ^ab"1308 Halleria (1931 EB)".Minor Planet Center. Retrieved20 December 2017.
  14. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

[edit]
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