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1831 Nicholson

From Wikipedia, the free encyclopedia
Main-belt asteroid

1831 Nicholson
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date17 April 1968
Designations
(1831) Nicholson
Named after
Seth B. Nicholson[2]
(American astronomer)
1968 HC · 1948 GF
1955 ML
main-belt[1][3] · (inner)
Baptistina[4] · Flora[4][5]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc62.92yr (22,982 d)
Aphelion2.5257AU
Perihelion1.9527 AU
2.2392 AU
Eccentricity0.1279
3.35 yr (1,224 d)
36.790°
0° 17m 38.76s / day
Inclination5.6335°
72.604°
183.46°
Physical characteristics
7.10±1.29 km[6]
8.08±0.47 km[7][8]
3.228±0.001 h[9]
0.296[8][7]
0.39[6]
SMASS =S[3][5]
12.40[7][8]
12.5[1][3][5]
12.70[6]

1831 Nicholson, provisional designation1968 HC, is a stonyasteroid of theBaptistina family from the inner regions of theasteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 17 April 1968, by Swiss astronomerPaul Wild at theZimmerwald Observatory near Bern, Switzerland.[1] TheS-type asteroid has arotation period of 3.2 hours. It was named for American astronomerSeth B. Nicholson.[2]

Orbit and classification

[edit]

According to aHCM-analysis byDavid Nesvorný,Nicholson is a member of theBaptistina family (403),[4] located within the greaterFlora family a giantasteroid clan and the largestfamily of stony asteroids in the asteroid belt.[5][4][10] Conversely, and since the existence of a proper Flora family has been ruled out by other astronomers,Nicholson has also been classified as abackground asteroid.[11]

It orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,224 days;semi-major axis of 2.24 AU). Its orbit has aneccentricity of 0.13 and aninclination of 6° with respect to theecliptic.[3] The asteroid was first observed as1948 GF at theNice Observatory in April 1948. The body'sobservation arc begins with its observation as1955 ML at theGoethe Link Observatory in June 1955, almost 13 years prior to its official discovery observation atZimmerwald.[1]

Naming

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Thisminor planet was named by the discoverer in memory of American astronomerSeth B. Nicholson (1891–1963), who pioneered in several branches of planetary research atMount Wilson Observatory and who discovered four ofJupiter's numerous moons – namely,Sinope,Lysithea,Carme, andAnanke. The lunar craterNicholson and the dark terrain ofNicholson Regio on Jupiter's moonGanymede, as well as the impact craterNicholson on Mars have also been named after him.[2] The officialnaming citation was published by theMinor Planet Center on 15 October 1977 (M.P.C. 4236).[12]

Physical characteristics

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In theSMASS classification,Nicholson is a common stonyS-type asteroid.[3][5]

Rotation period

[edit]

In April 2015, a rotationallightcurve ofNicholson was obtained fromphotometric observations by a group of Spanish astronomers from Valencia and Alicante at various observatories: (J08), (Z95), (J67), (Z98) and (I57). Lightcurve analysis gave a well-definedrotation period of3.228±0.001 hours and a brightness variation of 0.24magnitude (U=3).[9] At the same time, Serbian astronomer Vladimir Benishek at theBelgrade Observatory determined a concurring period of3.25510±0.00003 hours with an amplitude of 0.29 magnitude (U=3).[13]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Nicholson measures 7.1 and 8.1 kilometers in diameter and its surface has analbedo of 0.39 and 0.296, respectively.[6][7][8] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the namesake of the Flora family – and calculates a diameter of 8.58 kilometers based on anabsolute magnitude of 12.5.[5]

References

[edit]
  1. ^abcde"1831 Nicholson (1968 HC)".Minor Planet Center. Retrieved7 December 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(1831) Nicholson".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 147.doi:10.1007/978-3-540-29925-7_1832.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 1831 Nicholson (1968 HC)" (2018-05-25 last obs.).Jet Propulsion Laboratory. Retrieved7 December 2018.
  4. ^abcd"Asteroid 1831 Nicholson".Small Bodies Data Ferret. Retrieved7 December 2018.
  5. ^abcdef"LCDB Data for (1831) Nicholson". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2018.
  6. ^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.
  7. ^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.
  8. ^abcdMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0.Bibcode:2016PDSS..247.....M. Retrieved7 December 2018.
  9. ^abGarcerà; n, Alfonso Carreñ; o; Macias, Amadeo Aznar; Mansego, Enrique Arce; Rodriguez, Pedro Brines; et al. (October 2015)."Lightcurve Analysis of Six Asteroids".The Minor Planet Bulletin.42 (4):235–237.Bibcode:2015MPBu...42..235G.ISSN 1052-8091. Retrieved7 December 2018.
  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.
  11. ^"Asteroid (1831) Nicholson – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved20 October 2019.
  12. ^Schmadel, Lutz D. (2009). "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.
  13. ^Benishek, Vladimir (January 2016)."Rotation Periods of 1831 Nicholson, 2929 Harris, 8463 Naomimurdoch, and (34173) 2000 QY37".The Minor Planet Bulletin.43 (1):89–90.Bibcode:2016MPBu...43...89B.ISSN 1052-8091. Retrieved7 December 2018.

External links

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