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7846 Setvák

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7846 Setvák
Discovery [1]
Discovered byM. Tichý
Discovery siteKleť Obs.
Discovery date16 January 1996
Designations
(7846) Setvák
Named after
Stáňa and Martin Setvák
(Czech meteorologist)[2]
1996 BJ · 1979 OZ2
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc37.53 yr (13,707 days)
Aphelion2.7686AU
Perihelion1.9306 AU
2.3496 AU
Eccentricity0.1783
3.60yr (1,315 days)
337.86°
Inclination3.4546°
291.31°
224.12°
Physical characteristics
Dimensions2.69 km(calculated)[3]
2.964±0.127 km[4][5]
2.613±0.0006h[6]
2.620±0.010 h[7]
0.24(assumed)[3]
0.349±0.036[4][5]
S[3] · LS [8]
14.4[4] · 14.490±0.050(R)[7] · 14.565±0.001(R)[6] · 14.6[1] · 14.97±0.27[8] · 15.01[3]

7846 Setvák, provisional designation1996 BJ, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 3 kilometers in diameter. It was discovered on 16 January 1996, by Czech astronomerMiloš Tichý atKleť Observatory in South Bohemia.[9] The asteroid was named for Czech coupleStáňa andMartin Setvák.[2]

Orbit and classification

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Setvák is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.8 AU once every 3 years and 7 months (1,315 days). Its orbit has aneccentricity of 0.18 and aninclination of 3° with respect to theecliptic.[1] Itsobservation arc dates back to 1979, due toprecoveries obtained at the U.S.Palomar Observatory and theSiding Spring Observatory in Australia.[9]

Physical characteristics

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Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures 3.0 kilometers in diameter and its surface has a highalbedo of 0.35,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 (in accordance with the family's largest member and namesake,8 Flora) and calculates a diameter of 2.7 kilometers.[3] A large-scale survey byPan-STARRS (PS1) assigns an LS-type, presumably an intermediaryspectral type between the common stony S-types and the rather rare and reddishL-type asteroids.[8]

Rotation period

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Two rotationallightcurves were obtained fromphotometric observations taken in the R-band at the U.S.Palomar Transient Factory in January 2014. The lightcurves gave arotation period of 2.613 and 2.610 hours with a brightness amplitude of 0.11 and 0.14 inmagnitude, respectively (U=2/2).[6][7]

Naming

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Thisminor planet was named for Czech meteorologist Martin Setvák (born 1958), amateurastrophotographer and head of the Satellite Department of theCzech Hydrometeorological Institute, to honor his 40th birthday, as well as for his wife Stáňa Setváková (born 1967), a staff member of the Prague Planetarium.[2] The official naming citation was published by theMinor Planet Center on 11 February 1998 (M.P.C. 31298).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 7846 Setvak (1996 BJ)" (2017-02-01 last obs.).Jet Propulsion Laboratory. Retrieved22 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(7846) Setvák".Dictionary of Minor Planet Names – (7846) Setvák.Springer Berlin Heidelberg. p. 618.doi:10.1007/978-3-540-29925-7_6702.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (7846) Setvák". Asteroid Lightcurve Database (LCDB). Retrieved11 March 2017.
  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. ^abcMasiero, 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. Retrieved11 March 2017.
  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. Retrieved11 March 2017.
  7. ^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. Retrieved11 March 2017.
  8. ^abcVeres, 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. Retrieved11 March 2017.
  9. ^ab"7846 Setvak (1996 BJ)".Minor Planet Center. Retrieved11 March 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved11 March 2017.

External links

[edit]
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