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3628 Božněmcová

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Asteroid

3628 Božněmcová
Discovery[1]
Discovered byZ. Vávrová
Discovery siteKleť Obs.
Discovery date25 November 1979
Designations
(3628) Boznemcova
Named after
Božena Němcová
(Czech writer)[2]
1979 WD · 1930 MQ
1962 JP · 1975 XT4
1978 JX · 1979 YB10
1985 CQ2
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.76 yr (31,689 days)
Aphelion3.2963AU
Perihelion1.7799 AU
2.5381 AU
Eccentricity0.2987
4.04yr (1,477 days)
174.61°
0° 14m 37.32s / day
Inclination6.8866°
156.74°
187.79°
Physical characteristics
Dimensions5.40±1.17 km[4]
6.914±0.143 km[5][6]
8.14±0.34 km[7]
8.18 km(calculated)[3]
3.335410±0.000057h[8]
0.20(assumed)[3]
0.256±0.024[7]
0.32±0.13[4]
0.3370±0.0705[5]
0.359±0.029[6]
SMASS = O[1] · O[3][9]
12.60[5][7] · 12.8[1][3] · 13.05±0.34[9] · 13.11[4]

3628 Božněmcová, provisional designation1979 WD, is a rareO-typeasteroid from the middle region of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 25 November 1979, by Czech astronomerZdeňka Vávrová atKleť Observatory in the Czech Republic.[10] It is named for Czech writerBožena Němcová.[2]

Orbit and classification

[edit]

Božněmcová orbits the Sun in thecentral main-belt at a distance of 1.8–3.3 AU once every 4.04 years (1,477 days). Its orbit has aneccentricity of 0.30 and aninclination of 7° with respect to theecliptic.[1] It was first identified as1930 MQ atLowell Observatory in 1930, extending the body'sobservation arc by 49 years prior to its official discovery observation at Klet.[10]

Physical characteristics

[edit]

In theSMASS taxonomy, Božněmcová is a brightO-type asteroid, a rare group with spectra that best fits those of the L6 and LL6 ordinarychondrite-typemeteorites.[11]

Rotation period

[edit]

In September 2007, a rotationallightcurve of Božněmcová was obtained from photometric observations by American astronomerBrian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-definedrotation period of 3.335410 hours with a low brightness amplitude of 0.09magnitude (U=3).[8]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, Božněmcová measures between 5.40 and 8.14 kilometers in diameter, and its surface has analbedo between 0.256 and 0.359.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.18 kilometers at anabsolute magnitude of 12.8, as the lower the albedo (reflectivity), the larger the body's diameter for an unchanged brightness.[3]

Naming

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Thisminor planet was named in memory ofBožena Němcová (1820–1862), a Czech writer, author of the novellaThe Grandmother (Czech:Babička), the most frequently read book in Czech literature.[2] The official naming citation was published by theMinor Planet Center on 4 June 1993 (M.P.C. 22245).[12]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 3628 Boznemcova (1979 WD)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved19 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3628) Božněmcová".Dictionary of Minor Planet Names – (3628) Božněmcová.Springer Berlin Heidelberg. p. 305.doi:10.1007/978-3-540-29925-7_3627.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3628) Božněmcová". Asteroid Lightcurve Database (LCDB). Retrieved13 March 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  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.S2CID 35447010.
  6. ^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.S2CID 118745497. Retrieved14 November 2016.
  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. ^abWarner, Brian D. (June 2008)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory - June - October 2007".The Minor Planet Bulletin.35 (2):56–60.Bibcode:2008MPBu...35...56W.ISSN 1052-8091. Retrieved13 March 2017.
  9. ^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.S2CID 53493339. Retrieved13 March 2017.
  10. ^ab"3628 Boznemcova (1979 WD)".Minor Planet Center. Retrieved13 March 2017.
  11. ^Bus, S. J.; Binzel, R. P. (2002)."Phase II of the Small Main-Belt Asteroid Spectroscopic Survey A Feature-Based Taxonomy"(PDF).Icarus.158 (1):146–177.Bibcode:2002Icar..158..146B.doi:10.1006/icar.2002.6856.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved13 March 2017.

External links

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