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1768 Appenzella

From Wikipedia, the free encyclopedia
Main-belt asteroid

1768 Appenzella
Shape model ofAppenzella from itslightcurve
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date23 September 1965
Designations
(1768) Appenzella
Named after
Appenzell(canton)[2]
1965 SA · 1934 PM
1942 TH
main-belt · Nysa[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc74.56 yr (27,232 days)
Aphelion2.8899AU
Perihelion2.0141 AU
2.4520 AU
Eccentricity0.1786
3.84yr (1,402 days)
175.69°
0° 15m 24.12s / day
Inclination3.2582°
12.423°
19.718°
Physical characteristics
Dimensions19.0±1.9 km[4]
19.30±0.17 km[5]
20.221±0.129 km[6][7]
20.86±2.3 km(IRAS:2)[8]
21±2 km[9]
5.18335±0.00001h[10]
5.1839±0.0001 h[11]
0.03±0.01[9]
0.032±0.007[6][7]
0.0338±0.009(IRAS:2)[8]
0.039±0.008[5]
0.04±0.01[4]
F(Tholen)[1]
C(SMASS)[1]
B–V = 0.615[1]
U–B = 0.230[1]
12.70[1][3][4][5][6][9]

1768 Appenzella (prov. designation:1965 SA) is a rare-typeNysian asteroid from the inner regions of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 23 September 1965, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland.[12] It was later named after the Swiss canton ofAppenzell.[2]

Classification and orbit

[edit]

Appenzella is a darkcarbonaceous asteroid and a member of the Polanian subgroup of theNysa family. On theTholen taxonomic scheme, it belongs to the small group of 28 bodies known to have aF-type spectrum.[13]

It orbits the Sun in theinner main-belt at a distance of 2.0–2.9 AU once every 3 years and 10 months (1,402 days). Its orbit has aneccentricity of 0.18 and aninclination of 3° with respect to theecliptic.[1] The first used[clarification needed] observation was made at the FinnishTurku Observatory in 1942, extending the asteroid'sobservation arc by 23 years prior to its discovery.[12]

Lightcurve

[edit]

In November 2011, a rotationallightcurve ofAppenzella was obtained by French astronomerRené Roy at his Blauvac Observatory (627) in southeastern France. Lightcurve analysis gave a well-definedrotation period of5.1839 hours with a brightness variation of 0.53magnitude (U=3).[11] In 2016, remodeled photometric data from the Lowell database gave in a very similar period of 5.18335 hours.[10]

Diameter and albedo

[edit]

Based on the surveys carried out by NASA'sWide-field Infrared Survey Explorer and its subsequentNEOWISE mission, the asteroid measures between 19.0 and 21 kilometers in diameter and its surface has a lowalbedo between 0.03 and 0.04.[4][5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by the Infrared Astronomical Satellite,IRAS, which found an albedo of 0.034 and a mean diameter of 20.9 kilometers, with anabsolute magnitude of 12.7.[1][3]

Naming

[edit]

In 1971,Appenzella was named by the discoverer in honor of the ruralSwiss canton ofAppenzell, during the celebration of the 150th anniversary of the public middle school "Kantonsschule Trogen",Appenzell Ausserrhoden, founded in 1821.[2][14] The officialnaming citation was published by theMinor Planet Center on 1 July 1972 (M.P.C. 3297).[15]

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 1768 Appenzella (1965 SA)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1768) Appenzella".Dictionary of Minor Planet Names – (1768) Appenzella.Springer Berlin Heidelberg. p. 141.doi:10.1007/978-3-540-29925-7_1769.ISBN 978-3-540-00238-3.
  3. ^abc"LCDB Data for (1768) Appenzella". Asteroid Lightcurve Database (LCDB). Retrieved10 August 2016.
  4. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614. Retrieved10 August 2016.
  5. ^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. Retrieved10 August 2016.
  6. ^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.
  7. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved8 December 2016.
  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. Retrieved22 October 2019.
  9. ^abcdAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680. Retrieved10 August 2016.
  10. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved10 August 2016.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1768) Appenzella".Geneva Observatory. Retrieved10 August 2016.
  12. ^ab"1768 Appenzella (1965 SA)".Minor Planet Center. Retrieved10 August 2016.
  13. ^"JPL Small-Body Database Search Engine: [ spec. type = F (Tholen)]".JPL Solar System Dynamics. Retrieved10 August 2016.
  14. ^"Kanstonsschule Trogen".Kantonsschule Trogen (in German). 2014. Archived fromthe original on 25 May 2015. Retrieved14 January 2016.
  15. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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