Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

9931 Herbhauptman

From Wikipedia, the free encyclopedia
Asteroid

9931 Herbhauptman
Discovery[1]
Discovered byA. Mrkos
Discovery siteKleť Obs.
Discovery date18 April 1985
Designations
(9931) Herbhauptman
Named after
Herbert A. Hauptman[1]
(American mathematician)
1985 HH · 1982 QJ1
1996 HA1
main-belt[1][2] · (inner)[3]
Nysa[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc35.60yr (13,004 d)
Aphelion2.7991AU
Perihelion1.9573 AU
2.3782 AU
Eccentricity0.1770
3.67 yr (1,340 d)
329.47°
0° 16m 7.32s / day
Inclination2.4717°
157.21°
80.707°
Physical characteristics
4.54 km(calculated)[3]
5.179±0.368 km[5][6]
4.438±0.0091 h[7]
4.44±0.020 h[8]
0.20(assumed)[3]
0.239±0.042[5][6]
S[3][9]
13.6[6]
13.629±0.001(R)[7]
13.660±0.090(R)[8]
13.7[2]
14.06±0.32[9]
14.08[3]

9931 Herbhauptman, provisional designation1985 HH, is a stony Nysianasteroid from the inner regions of theasteroid belt, approximately 5 kilometers (3 miles) in diameter. It was discovered on 18 April 1985, by Czech astronomerAntonín Mrkos at theKleť Observatory in former Czechoslovakia.[1] TheS-type asteroid has arotation period of 4.44 hours.[3] It was named after American mathematician and Nobel laureateHerbert A. Hauptman.[1]

Orbit and classification

[edit]
Orbit ofHerbhauptman (blue) with theinner planets andJupiter in red

Herbhauptman is member of theNysa family (405),[4] one of the largestasteroid families.[10]

It orbits the Sun in theinner main-belt at a distance of 2.0–2.8 AU once every 3 years and 8 months (1,340 days;semi-major axis of 2.38 AU). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[2] The body'sobservation arc begins with its first observations as1982 QJ1 atPalomar Observatory in August 1982.[1]

Physical characteristics

[edit]

Herbhauptman has been characterized as a stonyS-type asteroid byPan-STARRS' survey.[3][9]

Rotation period

[edit]

In 2014, two rotationallightcurves ofHerbhauptman have been obtained fromphotometric observations in the R-band by astronomers at thePalomar Transient Factory in California.[7][8] Lightcurve analysis gave arotation period of 4.438 and 4.44 hours with a brightness amplitude of 0.15 and 0.21magnitude, respectively (U=2/2).[3]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Herbhauptman measures 5.179 kilometers in diameter and its surface has analbedo of 0.239,[5][6] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for astony asteroid of 0.20 and calculates a diameter of 4.54 kilometers based on anabsolute magnitude of 14.08.[3]

Naming

[edit]

Thisminor planet was named after American mathematicianHerbert A. Hauptman (1917–2011), who was awarded with theNobel Prize in Chemistry fordevelopingdirect methods for the determination ofcrystal structures in 1985.[1] The official naming citation was published by theMinor Planet Center on 28 September 2004 (M.P.C. 52767).[11]

References

[edit]
  1. ^abcdefg"9931 Herbhauptman (1985 HH)".Minor Planet Center. Retrieved2 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 9931 Herbhauptman (1985 HH)" (2018-03-27 last obs.).Jet Propulsion Laboratory. Retrieved2 May 2018.
  3. ^abcdefghi"LCDB Data for (9931) Herbhauptman". Asteroid Lightcurve Database (LCDB). Retrieved2 May 2018.
  4. ^ab"Asteroid 9931 Herbhauptman – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  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.S2CID 118745497.
  6. ^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 118700974. (catalog)
  7. ^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.S2CID 8342929.
  8. ^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.S2CID 17093124.
  9. ^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.S2CID 53493339.
  10. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.S2CID 119280014.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved2 May 2018.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=9931_Herbhauptman&oldid=1294083207"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp