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1788 Kiess

From Wikipedia, the free encyclopedia
Carbonaceous main-belt asteroid

1788 Kiess
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date25 July 1952
Designations
(1788) Kiess
Named after
Carl C. Kiess(astronomer)[2]
1952 OZ · 1935 NE
1964 WP
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.78 yr (23,660 days)
Aphelion3.5961AU
Perihelion2.6381 AU
3.1171 AU
Eccentricity0.1537
5.50yr (2,010 days)
323.37°
0° 10m 44.76s / day
Inclination0.6816°
161.91°
143.60°
Physical characteristics
Dimensions19.59 km(calculated)[3]
20.993±0.271 km[4][5]
11.0335±0.0071h[6]
12±2 h[7]
0.070±0.014[4][5]
0.08(assumed)[3]
C[3]
11.801±0.002(R)[6] · 11.9[1][3][4] · 11.93±0.26[8]

1788 Kiess, provisional designation1952 OZ, is a carbonaceous Themistianasteroid from the outer region of theasteroid belt, approximately 20 kilometers in diameter. It was discovered on 25 July 1952, by theIndiana Asteroid Program at the U.S.Goethe Link Observatory near Brooklyn, Indiana, United States, and later named after astronomerCarl Kiess.[2][9]

Orbit and classification

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TheC-type asteroid is a member of theThemis family, a dynamical family of outer-belt asteroids with nearly coplanarecliptical orbits. The asteroid orbits the Sun in theouter main-belt at a distance of 2.6–3.6 AU once every 5 years and 6 months (2,010 days). Its orbit has aneccentricity of 0.15 and aninclination of 1° with respect to the ecliptic.[1]Kiess was first identified as1935 NE atAlgiers Observatory in 1935. Itsobservation arc begins with its official discovery observation.[9]

Physical characteristics

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Rotation period

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In 2010, two rotationallightcurves were obtained from photometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 12 and 11.0335 hours with a brightness variation of 0.25 and 0.30magnitude, respectively (U=2-/2).[7][6]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Kiess measures 20.99 kilometers in diameter, and its surface has analbedo of 0.07.[4] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 19.59 kilometers with anabsolute magnitude of 11.9.[3]

Naming

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Thisminor planet was named for American astronomerCarl C. Kiess (1887–1967), a graduate ofIndiana University, who made distinguished contributions both in astronomy andspectroscopy at theU.S. National Bureau of Standards where he worked for over 40 years.[2] The officialnaming citation was published by theMinor Planet Center on 15 June 1973 (M.P.C. 3508).[10] Kiess was also a member of severaleclipse expeditions. The lunar craterKiess was named in his honour.[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1788 Kiess (1952 OZ)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1788) Kiess".Dictionary of Minor Planet Names – (1788) Kiess.Springer Berlin Heidelberg. p. 143.doi:10.1007/978-3-540-29925-7_1789.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1788) Kiess". Asteroid Lightcurve Database (LCDB). Retrieved19 December 2016.
  4. ^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.
  5. ^abMasiero, 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. Retrieved19 December 2016.
  6. ^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. Retrieved19 December 2016.
  7. ^abPolishook, D.; Ofek, E. O.; Waszczak, A.; Kulkarni, S. R.; Gal-Yam, A.; Aharonson, O.; et al. (April 2012)."Asteroid rotation periods from the Palomar Transient Factory survey".Monthly Notices of the Royal Astronomical Society.421 (3):2094–2108.arXiv:1201.1930.Bibcode:2012MNRAS.421.2094P.doi:10.1111/j.1365-2966.2012.20462.x.
  8. ^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. Retrieved19 December 2016.
  9. ^ab"1788 Kiess (1952 OZ)".Minor Planet Center. Retrieved19 December 2016.
  10. ^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

[edit]
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