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1304 Arosa

From Wikipedia, the free encyclopedia
Main-belt asteroid

1304 Arosa
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date21 May 1928
Designations
(1304) Arosa
Named after
Arosa(Swiss village)[2]
1928 KC · 1929 RY
1934 JL · 1934 LE
1974 OW · A908 YC
main-belt · (outer)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc108.22 yr (39,526 days)
Aphelion3.5731AU
Perihelion2.8226 AU
3.1978 AU
Eccentricity0.1173
5.72yr (2,089 days)
207.15°
0° 10m 20.64s / day
Inclination18.991°
86.580°
148.26°
Physical characteristics
Dimensions31.47±3.06 km[5]
41.67 km(derived)[3]
42.94±1.9 km[6]
43.613±0.241 km[7]
48.35±0.81 km[8]
57.443±1.462 km[9]
7.74 h[10]
7.7478±0.0001 h[11][12]
7.77±0.04h[11]
0.1961±0.0279[9]
0.2125(derived)[3]
0.279±0.011[8]
0.337±0.031[7]
0.3480±0.033[6]
0.409±0.084[5]
SMASS =X[1][3] · M[9]
8.6[6][8][9][13] · 9.03±0.27[14] · 9.10[5] · 9.2[1][3]

1304 Arosa, provisional designation1928 KC, is a metallicasteroid from the outer region of theasteroid belt, approximately 40 kilometers in diameter. It was discovered on 21 May 1928, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[15] It was named after the Swiss mountain village ofArosa.[2]

Orbit and classification

[edit]

Arosa is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in theouter asteroid belt at a distance of 2.8–3.6 AU once every 5 years and 9 months (2,089 days;semi-major axis of 3.20 AU). Its orbit has aneccentricity of 0.12 and aninclination of 19° with respect to theecliptic.[1] It was first identified asA908 YC at the discovering observatory in 1908, extending the body'sobservation arc by 20 years prior to its official discovery.[15]

Physical characteristics

[edit]

In theSMASS taxonomy,Arosa is classified as a genericX-type asteroid. TheWide-field Infrared Survey Explorer (WISE) groups it into the metallicM-type asteroid subcategory.[1][9]

Rotation period

[edit]

Several rotationallightcurves were obtained from photometric observations between 2002 and 2006. Lightcurve analysis gave a well-definedrotation period of 7.74 hours with a brightness amplitude between 0.32 and 0.38magnitude (U=3/3/3/2).[10][11][12]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA's WISE space telescope with itsNEOWISE mission,Arosa measures between 31.47 and 57.443 kilometers in diameter, and its surface has analbedo between 0.1961 and 0.409.[5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.2125 and a diameter of 41.67 kilometers, using anabsolute magnitude of 9.2.[3]

Naming

[edit]

Thisminor planet was named for the Swiss mountain village ofArosa, a summer and a winter tourist resort in theSwiss Alps. The official naming citation was also mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 119).[2]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1304 Arosa (1928 KC)" (2017-03-05 last obs.).Jet Propulsion Laboratory. Retrieved25 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1304) Arosa".Dictionary of Minor Planet Names – (1304) Arosa.Springer Berlin Heidelberg. p. 107.doi:10.1007/978-3-540-29925-7_1305.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1304) Arosa". Asteroid Lightcurve Database (LCDB). Retrieved14 March 2017.
  4. ^ab"Asteroid 1304 Arosa – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  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. Retrieved14 March 2017.
  6. ^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.
  7. ^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. Retrieved14 March 2017.
  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. ^abcdefMainzer, 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.
  10. ^abLicchelli, Domenico (December 2006)."Lightcurve analysis of asteroids 453 Tea and 454 Mathesis".The Minor Planet Bulletin.33 (4):105–106.Bibcode:2006MPBu...33..105L.ISSN 1052-8091. Retrieved14 March 2017.
  11. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1304) Arosa".Geneva Observatory. Retrieved14 March 2017.
  12. ^abFauerbach, Michael; Bennett, Thomas; Behrend, Raoul; Bernasconi, Laurent; Casulli, Silvano (December 2006)."Lightcurve analysis of 1304 Arosa".The Minor Planet Bulletin.33 (4): 103.Bibcode:2006MPBu...33..103F.ISSN 1052-8091. Retrieved14 March 2017.
  13. ^Tholen (2007)."Asteroid Absolute Magnitudes".EAR-A-5-DDR-ASTERMAG-V11.0.Planetary Data System. Retrieved14 March 2017.{{cite web}}:|archive-url= is malformed: timestamp (help)CS1 maint: url-status (link)
  14. ^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. Retrieved14 March 2017.
  15. ^ab"1304 Arosa (1928 KC)".Minor Planet Center. Retrieved14 March 2017.

External links

[edit]
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