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1682 Karel

From Wikipedia, the free encyclopedia
Stony asteroid

1682 Karel
Lightcurve-based 3D-model ofKarel
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date2 August 1949
Designations
(1682) Karel
Named after
Karel van Houten
(son of astronomers)
Cornelis andIngrid[2]
1949 PH · 1929 SD
1939 RK · 1946 WC
1949 QQ · 1949 QX1
1949 SL · 1959 PH
1988 CR3
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc87.39 yr (31,918 days)
Aphelion2.6685AU
Perihelion1.8085 AU
2.2385 AU
Eccentricity0.1921
3.35yr (1,223 days)
106.49°
0° 17m 39.48s / day
Inclination4.0276°
325.78°
9.9066°
Physical characteristics
Dimensions4.80±0.55 km[4]
7.267±0.195 km[5]
7.47 km(calculated)[3]
3.37485±0.00003h[6]
3.37485±0.00005 h[7]
0.24(assumed)[3]
0.278±0.027[5]
0.531±0.124[4]
S[3]
12.70[5] · 12.8[1][3] · 12.82±0.32[8] · 12.90[4]

1682 Karel, provisional designation1949 PH, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 7.5 kilometers in diameter.

It was discovered on 2 August 1949, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany, and later named after the son of Dutch astronomer coupleIngrid andCornelis van Houten.[2][9]

Orbit and classification

[edit]

Karel is a member of theFlora family, one of the largest collisional populations ofstony asteroids in theinner main-belt. It orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,223 days). Its orbit has aneccentricity of 0.19 and aninclination of 4° with respect to theecliptic.[1] In 1929,Karel was first identified as1929 SD at Heidelberg, extending the body'sobservation arc by 20 years prior to its official discovery observation.[9]

Physical characteristics

[edit]

Rotation period

[edit]

AstronomersFrançois Colas, Jean Lecacheux, Federico Manzini andRaoul Behrend obtained a rotationallightcurve ofKarel from photometric observations in January 2008. It gave a well-definedrotation period of 3.37485 hours with a brightness variation of 0.47 inmagnitude (U=3).[6] An identical period was modeled from the Lowell Photometric Database (U=n.a.).[7]

Diameter and albedo

[edit]

According to the survey carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Karel measures 4.80 and 7.27 kilometers in diameter, and its surface has analbedo of 0.278 and 0.531, respectively.[4][5] TheCollaborative Asteroid Lightcurve Link assumes analbedo of 0.24 – derived from8 Flora, the largest member and namesake of this family – and calculates a diameter of 7.47 kilometers based on an absolute magnitude of 12.8.[3]

Naming

[edit]

Thisminor planet was named after Karel van Houten, son of Dutch astronomersIngrid andCornelis van Houten of theLeiden Observatory.[2] Together with Ingrid, Reinmuth discovered the minor planet1691 Oort in 1956. Reinmuth also named his two discoveries,1673 van Houten and1674 Groeneveld, after the prolific couple of Dutch astronomers.[10][11] The officialnaming citation was published by theMinor Planet Center on 15 December 1968 (M.P.C. 2901).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1682 Karel (1949 PH)" (2017-02-15 last obs.).Jet Propulsion Laboratory. Retrieved6 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1682) Karel".Dictionary of Minor Planet Names – (1682) Karel.Springer Berlin Heidelberg. p. 134.doi:10.1007/978-3-540-29925-7_1683.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1682) Karel". Asteroid Lightcurve Database (LCDB). Retrieved22 December 2016.
  4. ^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)
  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. Retrieved22 December 2016.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1682) Karel".Geneva Observatory. Retrieved22 December 2016.
  7. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved22 December 2016.
  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. Retrieved22 December 2016.
  9. ^ab"1682 Karel (1949 PH)".Minor Planet Center. Retrieved22 December 2016.
  10. ^Schmadel, Lutz D. (2007). "(1673) van Houten".Dictionary of Minor Planet Names – (1673) van Houten. Springer Berlin Heidelberg. p. 133.doi:10.1007/978-3-540-29925-7_1674.ISBN 978-3-540-00238-3.
  11. ^Schmadel, Lutz D. (2007). "(1674) Groeneveld".Dictionary of Minor Planet Names – (1674) Groeneveld. Springer Berlin Heidelberg. p. 133.doi:10.1007/978-3-540-29925-7_1675.ISBN 978-3-540-00238-3.
  12. ^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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Asteroid
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Comets
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