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2016 Heinemann

From Wikipedia, the free encyclopedia
Themistian asteroid

2016 Heinemann
Discovery[1]
Discovered byA. Bohrmann
Discovery siteHeidelberg Obs.
Discovery date18 September 1938
Designations
(2016) Heinemann
Named after
Karl Heinemann(1898–1970)
(German astronomer)
[2]
1938 SE · 1927 SM
1930 DF · 1949 SB1
1971 OB1 · 1971 QP2
1972 VY · 1977 RZ7
A905 UF
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc111.34 yr (40,667 days)
Aphelion3.7291AU
Perihelion2.5295 AU
3.1293 AU
Eccentricity0.1917
5.54yr (2,022 days)
72.570°
0° 10m 40.8s / day
Inclination0.9191°
16.986°
340.99°
Physical characteristics
Dimensions21.68 km(derived)[3]
22.435±0.142 km[4]
22.718±0.080 km[5]
24.18±0.23 km[6]
25.52±1.41 km[7]
22.96±0.01h[8]
0.058±0.010[6]
0.0653(derived)[3]
0.075±0.009[7]
0.0944±0.0179[5]
C[3]
11.4[5][7] · 11.80[6] · 11.9[1][3] · 12.01±0.33[9]

2016 Heinemann, provisional designation1938 SE, is a carbonaceous Themistianasteroid from the outer regions of theasteroid belt, approximately 22 kilometers in diameter. It was discovered on 18 September 1938, by German astronomerAlfred Bohrmann atHeidelberg Observatory in southwest Germany, and later named afterARI-astronomer Karl Heinemann (1898–1970).[2][10]

Orbit and classification

[edit]

Heinemann is a member of theThemis family, a dynamical family ofcarbonaceous asteroids with nearly coplanarecliptical orbits, located in theouter-belt main. It orbits the Sun at a distance of 2.5–3.7 AU once every 5 years and 6 months (2,022 days). Its orbit has aneccentricity of 0.19 and aninclination of 1° with respect to the ecliptic.[1]

The body'sobservation arc begins 33 year prior to its official discovery observation, with its first identification asA905 UF at Heidelberg in October 1905.[10]

Physical characteristics

[edit]

Rotation period

[edit]

In October 2016, a rotationallightcurve ofHeinemann was obtained from photometric observations by French astronomer Matthieu Conjat. Lightcurve analysis gave arotation period of 22.96 hours with a brightness variation of 0.36magnitude (U=2+).[8]

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,Heinemann measures between 22.435 and 25.52 kilometers in diameter and its surface has analbedo between 0.058 and 0.0944.[4][5][6][7]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0653 and a diameter of 21.68 kilometers based on anabsolute magnitude of 11.9.[3]

Naming

[edit]

Thisminor planet was named after Karl Heinemann (1898–1970), German astronomer and long-time staff member at theAstronomisches Rechen-Institut. His activities includedspherical astronomy and the editing of the "Astronomischer Jahresbericht" during 1934–1958.[2]

The officialnaming citation was published by theMinor Planet Center on 15 October 1977 (M.P.C. 4238).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2016 Heinemann (1938 SE)" (2017-02-26 last obs.).Jet Propulsion Laboratory. Retrieved29 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2016) Heinemann".Dictionary of Minor Planet Names – (2016) Heinemann.Springer Berlin Heidelberg. p. 163.doi:10.1007/978-3-540-29925-7_2017.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2016) Heinemann". Asteroid Lightcurve Database (LCDB). Retrieved29 June 2017.
  4. ^abMasiero, 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. Retrieved29 June 2017.
  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.
  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. Retrieved29 June 2017.
  7. ^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)
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2016) Heinemann".Geneva Observatory. Retrieved29 June 2017.
  9. ^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. Retrieved29 June 2017.
  10. ^ab"2016 Heinemann (1938 SE)".Minor Planet Center. Retrieved29 June 2017.
  11. ^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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