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1958 Chandra

From Wikipedia, the free encyclopedia
Main-belt asteroid

1958 Chandra
Modelled shape ofChandra from itslightcurve
Discovery[1]
Discovered byC. U. Cesco
Discovery siteEl Leoncito
(Yale–Columbia Station)
Discovery date24 September 1970
Designations
(1958) Chandra
Named after
Subrahmanyan Chandrasekhar
(astrophysicist)[2]
1970 SB · 1947 HD
1959 RG1 · 1965 UN
1971 XA
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.66 yr (22,887 days)
Aphelion3.6220AU
Perihelion2.5840 AU
3.1030 AU
Eccentricity0.1673
5.47yr (1,997 days)
233.69°
0° 10m 49.08s / day
Inclination10.559°
345.04°
318.95°
Physical characteristics
Dimensions33.82 km(derived)[3]
34.278±0.220[4]
36.167±0.349 km[5]
7.0571±0.0029h[6]
7.070±0.004 h[7]
0.0511(derived)[3]
0.0709±0.0138[5]
0.082±0.007[4]
C[3]
10.7[5] · 11.102±0.003(R)[6] · 11.18±0.18[8] · 11.2[1][3]

1958 Chandra (prov. designation:1970 SB) is a darkbackground asteroid from the outer region of theasteroid belt, approximately 35 kilometers (22 miles) in diameter. It was discovered on 24 September 1970, by Argentinian astronomerCarlos Cesco at the Yale–Columbia Southern Station of theLeoncito Astronomical Complex in San Juan, Argentina(also seeFélix Aguilar Observatory).[9] It was named after astrophysicistSubrahmanyan Chandrasekhar.[2]

Orbit and classification

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Chandra is a darkC-type asteroid that orbits the Sun in theouter main-belt at a distance of 2.6–3.6 AU once every 5 years and 6 months (1,997 days). Its orbit has aneccentricity of 0.17 and aninclination of 11° with respect to theecliptic.[1] In April 1947, the asteroid was first identified as1947 HD atAlgiers Observatory. The body'sobservation arc begins 16 years prior to its official discovery observation with aprecovery taken atPalomar Observatory in 1954.[9]

Naming

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Thisminor planet was named in honor ofSubrahmanyan Chandrasekhar (1910–1995), the Nobel Prize winning Indian–American theoreticalastrophysicist(also seeChandrasekhar limit).[2] The approved naming citation was published by theMinor Planet Center on 1 November 1979 (M.P.C. 5013).[10]

Physical characteristics

[edit]

Photometry

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In December 2010, a rotationallightcurve was obtained for this asteroid from photometric observations at the U.S.Palomar Transient Factory, California. It gave arotation period of7.0571±0.0029 hours with a brightness variation of 0.35magnitude (U=2).[6] A second lightcurve, obtained by Italian amateur astronomerSilvano Casulli in August 2014, gave a concurring period of7.070±0.004 hours with an amplitude of 0.38 in magnitude (U=3-).[7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the asteroid measures 36.2 kilometers in diameter and its surface has analbedo of 0.07,[5] while theCollaborative Asteroid Lightcurve Link derives an albedo of 0.05 and a diameter of 33.8 kilometers with anabsolute magnitude of 11.2.[3]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1958 Chandra (1970 SB)" (2017-06-04 last obs.).Jet Propulsion Laboratory. Retrieved2 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1958) Chandra".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 157.doi:10.1007/978-3-540-29925-7_1959.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1958) Chandra". Asteroid Lightcurve Database (LCDB). Retrieved25 August 2016.
  4. ^abMasiero, 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. Retrieved8 December 2016.
  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.
  6. ^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. Retrieved25 August 2016.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1958) Chandra".Geneva Observatory. Retrieved25 August 2016.
  8. ^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. Retrieved25 August 2016.
  9. ^ab"1958 Chandra (1970 SB)".Minor Planet Center. Retrieved25 August 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved25 August 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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