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1732 Heike

From Wikipedia, the free encyclopedia
Main-belt asteroid

1732 Heike
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date9 March 1943
Designations
(1732) Heike
Named after
Heike Neckel(granddaughter of astronomer Alfred Bohrmann)[2]
1943 EY · 1934 LC
1935 TD · 1938 FC
1938 GB · 1950 NR1
1951 WW · 1960 ME
1961 TU1 · 1966 QJ
1971 QY1 · A906 FA
A924 PB
main-belt · Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc111.22 yr (40,623 days)
Aphelion3.3482AU
Perihelion2.6793 AU
3.0137 AU
Eccentricity0.1110
5.23yr (1,911 days)
249.18°
0° 11m 18.24s / day
Inclination10.776°
155.63°
211.36°
Physical characteristics
Dimensions20.50±0.79 km[5]
22.378±0.235[6]
23.485±0.161 km[7]
24.06±4.2 km[8]
24.17 km(derived)[3]
24.31±1.45 km[9]
3.90h[4]
4.742±0.013 h[10]
0.1108±0.052[8]
0.114±0.015[9]
0.1169±0.0116[7]
0.128±0.025[6]
0.1320(derived)[3]
0.201±0.040[5]
LS[11] · S[3]
10.80[5] · 10.82±0.19[11] · 10.9[1][3] · 11.1[8][9][7]

1732 Heike, provisional designation1943 EY, is a stony Eoanasteroid from the outer region of theasteroid belt, approximately 24 kilometers in diameter.

It was discovered on 9 March 1943, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany, and named after Heike Neckel, the granddaughter of astronomerAlfred Bohrmann.[2][12]

Classification and orbit

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TheS-type asteroid is a member of theEos family. It orbits the Sun in theouter main-belt at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,911 days). Its orbit has aneccentricity of 0.11 and aninclination of 11° with respect to theecliptic.[1]Heike was first identified asA906 FA at Heidelberg Observatory in 1906. The body's first used observation was also taken at Heidelberg in 1924, when it was identified as1924 PB, extending the body'sobservation arc by 19 years prior to its official discovery observation.[12]

Rotation period

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In October 2010, a rotationallightcurve ofHeike was obtained from photometric observations at the Truman Observatory. It gave a well-definedrotation period of 4.742 hours with a brightness variation of 0.32magnitude (U=3),[10][13] superseding a previous period of 3.90 hours (U=2).[4]

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, the asteroid measures between 20.50 and 24.31 kilometers in diameter, and its surface has analbedo between 0.110 and 0.201.[5][7][8][9] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.132 and a diameter of 24.17 kilometers with anabsolute magnitude of 10.9.[3]

Naming

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Thisminor planet was named after Heike Neckel, granddaughter of German astronomerAlfred Bohrmann (1904–2000), who was a colleague of the discoverer at Heidelberg. The asteroid1635 Bohrmann bears his name.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3933).[14]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1732 Heike (1943 EY)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved1 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1732) Heike".Dictionary of Minor Planet Names – (1732) Heike.Springer Berlin Heidelberg. p. 138.doi:10.1007/978-3-540-29925-7_1733.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1732) Heike". Asteroid Lightcurve Database (LCDB). Retrieved21 December 2016.
  4. ^abcAlvarez-Candal, Alvaro; Duffard, René; Angeli, Cláudia A.; Lazzaro, Daniela; Fernández, Silvia (December 2004)."Rotational lightcurves of asteroids belonging to families".Icarus.172 (2):388–401.Bibcode:2004Icar..172..388A.doi:10.1016/j.icarus.2004.06.008. Retrieved21 December 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. Retrieved21 December 2016.
  6. ^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. Retrieved21 December 2016.
  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.
  8. ^abcdTedesco, 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. Retrieved17 October 2019.
  9. ^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)
  10. ^abKing, J. Ryan; Beaky, Matthew M. (January 2010)."A Revised Period for Asteroid 1732 Heike".The Minor Planet Bulletin.37 (1): 34.Bibcode:2010MPBu...37...34K.ISSN 1052-8091. Retrieved21 December 2016.
  11. ^abVeres, 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. Retrieved21 December 2016.
  12. ^ab"1732 Heike (1943 EY)".Minor Planet Center. Retrieved21 December 2016.
  13. ^Carbo, Landy; Kragh, Katherine; Krotz, Jonathan; Meiers, Andrew; Shaffer, Nelson; Torno, Steven; et al. (July 2009)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory and Oakley Observatory: 2008 September and October".The Minor Planet Bulletin.36 (3):91–94.Bibcode:2009MPBu...36...91C.ISSN 1052-8091. Retrieved21 December 2016.
  14. ^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

[edit]
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