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1470 Carla

From Wikipedia, the free encyclopedia
Main-belt asteroid

1470 Carla
Discovery[1]
Discovered byA. Bohrmann
Discovery siteHeidelberg Obs.
Discovery date17 September 1938
Designations
(1470) Carla
Named after
Carla Ziegler
(discoverer's friend)[2]
1938 SD · 1930 DE
1955 UN
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc78.15 yr (28,546 days)
Aphelion3.3771AU
Perihelion2.9416 AU
3.1594 AU
Eccentricity0.0689
5.62yr (2,051 days)
1.2909°
0° 10m 31.8s / day
Inclination3.2126°
358.43°
341.84°
Physical characteristics
Dimensions31.66±10.19 km[4]
34.092±5.538 km[5]
34.28±0.84 km[6]
36.94 km(derived)[3]
36.97±1.1 km(IRAS:22)[7]
6.15±0.040 h[8]
6.1514±0.0002h[9]
6.154±0.0028 h[10]
0.0470(derived)[3]
0.0515±0.003(IRAS:22)[7]
0.06±0.09[4]
0.0605±0.0181[5]
0.062±0.003[6]
C[3]
10.800±0.120(R)[8] · 10.947±0.001(R)[10] · 11.0[5][6] · 11.1[1][3] · 11.18[4] · 11.43±0.35[11]

1470 Carla, provisional designation1938 SD, is a carbonaceousasteroid from the outer regions of theasteroid belt, approximately 35 kilometers in diameter.

It was discovered on 17 September 1938, by German astronomerAlfred Bohrmann atHeidelberg Observatory in southwest Germany.[12] It was named after a friend of the discoverer's family, Carla Ziegler.[2]

Description

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Carla orbits the Sun at a distance of 2.9–3.4 AU once every 5 years and 7 months (2,051 days). Its orbit has aneccentricity of 0.07 and aninclination of 3° with respect to theecliptic.[1] It was first identified as1930 DE at Heidelberg 1930. The body'sobservation arc, however, begins the night prior to its official discovery observation in 1938.[12]

Physical characteristics

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Rotation period

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In September 2011, a rotationallightcurve ofCarla was obtained from photometric observations by astronomerFrederick Pilcher at Organ Mesa Observatory (G50) near Las Cruces, New Mexico. Lightcurve analysis gave arotation period of 6.1514 hours with a brightness amplitude of 0.25magnitude (U=3).[9] in 2014, two additional lightcurves in the R-band, obtained at thePalomar Transient Factory, California, gave a period of 6.15 and 6.154 hours with an amplitude of 0.24 and 0.25, respectively (U=2/2).[8][10]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Carla measures between 31.66 and 36.97 kilometers in diameter and its surface has analbedo of 0.051 and 0.062.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link classifies the body as a carbonaceousC-type asteroid, derives an albedo of 0.047 with a diameter of 36.94 kilometers and anabsolute magnitude of 11.1.[3]

Naming

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Thisminor planet was named in honor of Carla Ziegler, a friend of the Bohrmann family at Heidelberg.[2] The officialnaming citation was published by theMinor Planet Center in October 1954 (M.P.C. 1129).[13]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1470 Carla (1938 SD)" (2016-11-11 last obs.).Jet Propulsion Laboratory. Retrieved3 April 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1470) Carla".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. pp. 117–118.doi:10.1007/978-3-540-29925-7_1471.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1470) Carla". Asteroid Lightcurve Database (LCDB). Retrieved3 April 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. ^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.
  6. ^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)
  7. ^abcTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved15 June 2018.
  8. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27.S2CID 17093124. Retrieved3 April 2017.
  9. ^abPilcher, Frederick (April 2012)."Rotation Period Determinations for 31 Euphrosyne, 65 Cybele, 154 Bertha 177 Irma, 200 Dynamene, 724 Hapag, 880 Herba, and 1470 Carla".The Minor Planet Bulletin.39 (2):57–60.Bibcode:2012MPBu...39...57P.ISSN 1052-8091. Retrieved3 April 2017.
  10. ^abcWaszczak, 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 April 2017.
  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 April 2017.
  12. ^ab"1470 Carla (1938 SD)".Minor Planet Center. Retrieved3 April 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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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