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2384 Schulhof

From Wikipedia, the free encyclopedia
Asteroid

2384 Schulhof
Shape model ofSchulhof from itslightcurve
Discovery[1]
Discovered byM. Laugier
Discovery siteNice Obs.
Discovery date2 March 1943
Designations
(2384) Schulhof
Named after
Lipót Schulhof[2]
(Hungarian astronomer)
1943 EC1 · 1943 GV
1960 FE · 1962 WL1
1970 RP · 1981 FF
A909 BF
main-belt[1][3] · (middle)
Schulhof[4]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc108.97yr (39,803 d)
Aphelion2.9231AU
Perihelion2.2989 AU
2.6110 AU
Eccentricity0.1195
4.22 yr (1,541 d)
256.37°
0° 14m 0.96s / day
Inclination13.530°
7.9084°
205.72°
Physical characteristics
11.485±0.174 km[5]
11.721±0.138 km[6]
12.66 km(calculated)[7]
3.294±0.006 h[8]
0.21(assumed)[7]
0.2733±0.0217[6]
0.280±0.045[5]
S(assumed)[7]
11.7[6]
11.8[3][7]

2384 Schulhof (prov. designation:1943 EC1) is a mid-sizedasteroid and the namesake of theSchulhof family, located in the Eunomian region of the intermediateasteroid belt. It was discovered on 2 March 1943, by French astronomerMarguerite Laugier atNice Observatory in southeastern France.[1] The asteroid was later named after Hungarian astronomerLipót Schulhof.[2] The presumedS-type asteroid has a shortrotation period of 3.3 hours and measures approximately 12 kilometers (7.5 miles) in diameter.

Orbit and classification

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Schulhof is the principal body and namesake of theSchulhof family, a smallasteroid family within the region of theEunomia family of the main-belt.[4][9] It orbits the Sun in thecentral asteroid belt at a distance of 2.3–2.9 AU once every 4 years and 3 months (1,541 days). Its orbit has aneccentricity of 0.12 and aninclination of 14° with respect to theecliptic.[3] It was first observed asA909 BF atHeidelberg Observatory in 1909. The body'sobservation arc begins with its official discovery observation at Nice in 1943.[1]

Naming

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Thisminor planet was named in memory of Austrian–Hungarian astronomerLipót Schulhof (1847–1921), observer of asteroids and comets, discoverer of the main-belt asteroid147 Protogeneia, and awardee of theLalande Prize.[2] The official naming citation was published by theMinor Planet Center on 17 February 1984, based on a suggestion byBrian G. Marsden (M.P.C. 8541).[10]

Physical characteristics

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Schulhof is an assumedS-type asteroid.[7]

Rotation period

[edit]
Lightcurve-based 3D-model ofSchulhof

In April 2002, a rotationallightcurve ofSchulhof was obtained from photometric observations at the U.S.Oakley Observatory. It gave a well-definedrotation period of3.294±0.006 hours with a brightness variation of 0.43magnitude (U=3).[8]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Schulhof measures 11.5 and 11.7 kilometers in diameter and its surface has analbedo of 0.27 and 0.28, respectively.[5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived form15 Eunomia, the family's largest member and namesake – and calculates a diameter of 12.7 kilometers with anabsolute magnitude of 11.8.[7]

References

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  1. ^abcd"2384 Schulhof (1943 EC1)".Minor Planet Center. Retrieved9 August 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(2384) Schulhof".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 194.doi:10.1007/978-3-540-29925-7_2385.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 2384 Schulhof (1943 EC1)" (2018-01-20 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 September 2020. Retrieved9 August 2018.
  4. ^ab"Asteroid 2384 Schulhof".Small Bodies Data Ferret. Retrieved9 August 2018.
  5. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved7 December 2016.
  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.
  7. ^abcdef"LCDB Data for (2384) Schulhof". Asteroid Lightcurve Database (LCDB). Retrieved5 July 2016.
  8. ^abDitteon, R.; Bixby, A. R.; Sarros, A. M.; Waters, C. T. (December 2002)."Rotation Periods and Lightcurves of 1858 Lobachevskij, 2384 Schulhof and (5515) 1989 EL1"(PDF).Minor Planet Bulletin.29 (1): 69.Bibcode:2002MPBu...29...69D. Archived fromthe original(PDF) on 4 October 2021. Retrieved18 March 2020.
  9. ^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.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved5 July 2016.

External links

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