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2026 Cottrell

From Wikipedia, the free encyclopedia
Main-belt asteroid

2026 Cottrell
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date30 March 1955
Designations
(2026) Cottrell
Named after
Frederick Gardner Cottrell
(American chemist)[2]
1955 FF · 1951 EL1
1972 TE1
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.15 yr (24,163 days)
Aphelion2.7290AU
Perihelion2.1638 AU
2.4464 AU
Eccentricity0.1155
3.83yr (1,398 days)
135.21°
0° 15m 27.36s / day
Inclination2.4510°
311.10°
211.67°
Physical characteristics
Dimensions7.46 km(calculated)[3]
11.43±2.35 km[4]
13.19±0.55 km[5]
13.97±7.02 km[6]
14.279±0.071 km[7][8]
4.499±0.0014h[9]
4.499±0.0010 h[9]
4.4994±0.0004 h[10]
0.050±0.005[7][8]
0.063±0.053[6]
0.07±0.10[4]
0.088±0.009[5]
0.20(assumed)[3]
S[3]
12.8[5][7] · 12.90[6] · 12.964±0.002(R)[9] · 13.0[1][3] · 13.15±0.90[11] · 13.18[4]

2026 Cottrell, provisional designation1955 FF, is a darkasteroid from the inner regions of theasteroid belt, approximately 12 kilometers in diameter.

The asteroid was discovered on 30 March 1955, byIU'sIndiana Asteroid Program atGoethe Link Observatory near Brooklyn, Indiana, United States.[12] It was named after American chemistFrederick Gardner Cottrell.[2]

Orbit and classification

[edit]

Cottrell orbits the Sun in theinner main-belt at a distance of 2.2–2.7 AU once every 3 years and 10 months (1,398 days). Its orbit has aneccentricity of 0.12 and aninclination of 2° with respect to theecliptic.[1]

In March 1951, the asteroid was identified as1951 EL1 atNice Observatory and two days later atMcDonald Observatory, extending the body'sobservation arc by four years prior to its official discovery observation at Goethe Link.[12]

Physical characteristics

[edit]

Lightcurves

[edit]

Two rotationallightcurve ofCottrell were obtained from photometric observations by astronomers at thePalomar Transient Factory in California. Analysis gave an identicalrotation period of 4.499 hours for both lightcurves and a brightness variation of 0.42 and 0.44magnitude, respectively (U=2/2).[9]

In February 2012, photometry at the Etscorn Campus Observatory (719), New Mexico, gave a well-defined period of 4.4994 hours with an amplitude of 0.77 magnitude, which indicates that the body has a non-spheroidal shape (U=3).[10]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Cottrell measures between 11.43 and 14.279 kilometers in diameter and its surface has analbedo between 0.050 and 0.088.[4][5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forstony asteroids of 0.20 and consequently calculates a much smaller diameter of 7.46 kilometers based on anabsolute magnitude of 13.0.[3]

Naming

[edit]

Thisminor planet was named after American chemistFrederick Gardner Cottrell (1877–1948), who was a benefactor of the minor planet program at the discovering Goethe Link Observatory.[2] The officialnaming citation was published by theMinor Planet Center on 1 November 1978 (M.P.C. 4547).[13]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2026 Cottrell (1955 FF)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2026) Cottrell".Dictionary of Minor Planet Names – (2026) Cottrell.Springer Berlin Heidelberg. p. 164.doi:10.1007/978-3-540-29925-7_2027.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2026) Cottrell". Asteroid Lightcurve Database (LCDB). Retrieved3 July 2017.
  4. ^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.
  5. ^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)
  6. ^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. Retrieved3 July 2017.
  7. ^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.
  8. ^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.S2CID 118745497. Retrieved3 July 2017.
  9. ^abcdWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929. Retrieved3 July 2017.
  10. ^abKlinglesmith, Daniel A., III (July 2012)."Asteroid Lightcurve Analysis at the Etscorn Campus Observatory for January and February 2012".The Minor Planet Bulletin.39 (3):109–110.Bibcode:2012MPBu...39..109K.ISSN 1052-8091. Retrieved3 July 2017.{{cite journal}}: CS1 maint: numeric names: authors list (link)
  11. ^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. Retrieved3 July 2017.
  12. ^ab"2026 Cottrell (1955 FF)".Minor Planet Center. Retrieved3 July 2017.
  13. ^Schmadel, Lutz D. (2009). "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.


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