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4923 Clarke

From Wikipedia, the free encyclopedia
Asteroid

4923 Clarke
Orbital diagram ofClarke
Discovery[1]
Discovered byS. J. Bus
Discovery siteSiding Spring Obs.
Discovery date2 March 1981
Designations
(4923) Clarke
Named after
Arthur C. Clarke[1]
(British science fiction writer)
1981 EO27 · 1972 NJ
main-belt[1][2] · (inner)
background[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc45.53yr (16,631 d)
Aphelion2.5774AU
Perihelion1.7121 AU
2.1448 AU
Eccentricity0.2017
3.14 yr (1,147 d)
187.58°
0° 18m 49.68s / day
Inclination6.6759°
188.51°
108.65°
Physical characteristics
3.367±0.033 km[4]
3.532±0.033 km[5]
4.10 km(calculated)[6]
3.143±0.016 h[7]
3.1787±0.0009 h[a]
27.253±0.0553 h[8]
0.20(assumed)[6]
0.3259±0.0644[5]
0.366±0.066[4]
SMASS =S[2][6]
13.98±0.31[9]
14.1[5]
14.222±0.004(R)[8]
14.3[2][6]

4923 Clarke, provisional designation1981 EO27, is a stony backgroundasteroid from the inner regions of theasteroid belt, approximately 3.5 kilometers (2.2 miles) in diameter. It was discovered on 2 March 1981, by American astronomerSchelte Bus at theSiding Spring Observatory in Australia.[1] The spheroidalS-type asteroid has arotation period of 3.14 hours.[6] It was named after British science fiction writerArthur C. Clarke.[1] On the same night, Schelte Bus also discovered5020 Asimov.

Orbit and classification

[edit]

Clarke is a non-family asteroid from the main belt'sbackground population.[3] It orbits the Sun in theinner main-belt at a distance of 1.7–2.6 AU once every 3 years and 2 months (1,147 days;semi-major axis of 2.14 AU). Its orbit has aneccentricity of 0.20 and aninclination of 7° with respect to theecliptic.[2]

The asteroid was first observed as1972 NJ atCrimea–Nauchnij in July 1972. The body'sobservation arc begins at the Siding Spring Observatory two weeks prior to its official discovery observation on 12 February 1981.[1]

Physical characteristics

[edit]

In theSMASS classification,Clarke is a common, stonyS-type asteroid.[2][6]

Rotation period

[edit]

Three rotationallightcurves ofClarke have been obtained fromphotometric observations by the APT Observatory Group in Spain, by astronomers at thePalomar Transient Factory in California, and by Czech astronomerPetr Pravec atOndřejov Observatory (U=2/1/2-).[7][8][a] Analysis of the best-rated lightcurve gave arotation period of 3.143 hours with a consolidated brightness amplitude between 0.03 and 0.14magnitude, which indicates that the body has a nearly spheroidal, non-elongated shape (U=2).[6][7]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Clarke measures between 3.367 and 3.532 kilometers in diameter and its surface has analbedo between 0.3259 and 0.366.[4][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.20 and calculates a diameter of 4.10 kilometers based on anabsolute magnitude of 14.3.[6]

Naming

[edit]

Thisminor planet was named after thescience fiction writerArthur C. Clarke (1917–2008), author of2001: A Space Odyssey.[1] The official naming citation was prepared with assistance fromRichard Binzel and published by theMinor Planet Center on 3 May 1996 (M.P.C. 27127). The asteroid's name independently suggested byDuncan Steel (M.P.C. 27147).[10]

In the postscript to his novel3001: The Final Odyssey, Clarke jokingly expresses disappointment that he did not receiveasteroid 2001 as his namesake; instead, it was named forAlbert Einstein.[citation needed]

Notes

[edit]
  1. ^abLightcurve plot of (4923) Clarke, (Pravec 2013) from August 2013 web: rotation period3.18±0.0008 hours with a brightness amplitude of0.03±0.01 mag. Quality code is 2-. Summary figures at theLCDB andPravec, P.; Wolf, M.; Sarounova, L. (2013).

References

[edit]
  1. ^abcdefg"4923 Clarke (1981 EO27)".Minor Planet Center. Retrieved3 May 2018.
  2. ^abcdef"JPL Small-Body Database Browser: 4923 Clarke (1981 EO27)" (2018-01-24 last obs.).Jet Propulsion Laboratory. Retrieved3 May 2018.
  3. ^ab"Asteroid 4923 Clarke – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  4. ^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.S2CID 119293330.
  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. (catalog)
  6. ^abcdefgh"LCDB Data for (4923) Clarke". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2018.
  7. ^abcAznar Macias, Amadeo (January 2017). "Lightcurve Analysis from APT Observatory Group for Nine Mainbelt Asteroids: 2016 July-September. Rotation Period and Physical Parameters".The Minor Planet Bulletin.44 (1):60–63.Bibcode:2017MPBu...44...60A.ISSN 1052-8091.
  8. ^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.
  9. ^Veres, 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. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2018.

External links

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