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4435 Holt

From Wikipedia, the free encyclopedia
Asteroid

4435 Holt
Discovery[1]
Discovered byC. Shoemaker
Discovery sitePalomar Obs.
Discovery date13 January 1983
Designations
(4435) Holt
Pronunciation/ˈhlt/
Named after
Henry E. Holt
(American astronomer)[2]
1983 AG2 · 1978 PZ2
Mars-crosser[1][3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc37.89 yr (13,840 days)
Aphelion3.0939AU
Perihelion1.5405 AU
2.3172 AU
Eccentricity0.3352
3.53yr (1,288 days)
319.21°
0° 16m 45.84s / day
Inclination21.905°
330.93°
110.08°
Knownsatellites1
Physical characteristics
5.03±1.17 km[5]
6.44 km(derived)[4]
2.8670±0.0002 h[4]
0.20(assumed)[4]
0.28±0.15 km[5]
SMASS =S[1][4]
13.1[1] · 13.32±0.11[6][7]

4435 Holt, provisional designation1983 AG2, is a stonyasteroid, sizableMars-crosser andbinary system from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. It was discovered on 13 January 1983, by American astronomerCarolyn Shoemaker at thePalomar Observatory in California, United States.[3] It was later named after American astronomerHenry E. Holt.[2] The discovery of itscompanion was announced in January 2018.

Orbit and classification

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Holt orbits the Sun in theinner main-belt at a distance of 1.5–3.1 AU once every 3 years and 6 months (1,288 days). Its orbit has aneccentricity of 0.34 and aninclination of 22° with respect to theecliptic.[1] The firstprecovery was taken atCrimea-Nauchnij in 1978, extending the asteroid'sobservation arc by 5 years prior to its discovery.[3]

Naming

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Thisminor planet was named for Americanplanetary geologist and astronomerHenry E. Holt (born 1929), atNAU andUSGS, who has explored thesurface of the Moon, its geology andphotometric properties during theApollo andSurveyor programs.[2]

After his retirement, Holt was a principal participant in thePalomar Asteroid and Comet Survey (PACS) from 1983 to 1993.[8] Holt has discovered and co-discovered six comets and 683 minor planets between 1989 and 1993,[9] including4581 Asclepius,[10] a potentially hazardous asteroid that has made the closest approach to Earth of all numbered asteroids.[2] The official naming citation was published by theMinor Planet Center on 30 January 1991 (M.P.C. 17656).[11]

Physical characteristics

[edit]

In theSMASS classification,Holt is a commonS-type asteroid.[1]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Holt measures 5.03 kilometers in diameter and its surface has analbedo of 0.28,[5] while theCollaborative Asteroid Lightcurve Linkassumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 6.44 kilometer with anabsolute magnitude of 13.32.[4][6][7]

Satellite and rotation

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In November 2017, a rotationallightcurve ofHolt was obtained fromphotometric observation byRobert Stephens and collaborators. Lightcurve analysis gave arotation period of2.8670±0.0002 hours with a brightness variation of 0.15 magnitude.[4] During the observations, the presence of an approximately 2-kilometer sizedminor-planet moon was detected. The satellite orbits its primary every 42.6 hours (1.777 d).

References

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  1. ^abcdefg"JPL Small-Body Database Browser: 4435 Holt (1983 AG2)" (2016-06-29 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(4435) Holt".Dictionary of Minor Planet Names – (4435) Holt.Springer Berlin Heidelberg. p. 381.doi:10.1007/978-3-540-29925-7_4384.ISBN 978-3-540-00238-3.
  3. ^abc"4435 Holt (1983 AG2)".Minor Planet Center. Retrieved25 January 2016.
  4. ^abcdefg"LCDB Data for (4435) Holt". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  5. ^abcNugent, 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.
  6. ^abWisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995)."Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W. Retrieved17 May 2016.
  7. ^abPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved17 May 2016.
  8. ^Shoemaker, C. S.; Holt, H. E.; Shoemaker, E. M.; Bowell, E.; Levy, D. H. (December 1992)."The Palomar Asteroid and Comet Survey (PACS), 1983-1993".Abstracts for the IAU Symposium 160: Asteroids.810: 269.Bibcode:1993LPICo.810..269S. Retrieved25 January 2016.
  9. ^"Minor Planet Discoverers (by number)".Minor Planet Center. 22 March 2016. Retrieved26 April 2016.
  10. ^"4581 Asclepius (1989 FC)".Minor Planet Center. Retrieved26 April 2016.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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