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1855 Korolev

From Wikipedia, the free encyclopedia
Main-belt asteroid

1855 Korolev
Shape model ofKorolev from itslightcurve
Discovery[1]
Discovered byL. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date8 October 1969
Designations
(1855) Korolev
Named after
Sergey Korolyov
(Soviet rocket engineer)[2]
1969 TU1 · 1961 JD
1964 DD
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc55.74 yr (20,358 days)
Aphelion2.4363AU
Perihelion2.0583 AU
2.2473 AU
Eccentricity0.0841
3.37yr (1,231 days)
286.81°
0° 17m 33.36s / day
Inclination3.0793°
191.03°
349.40°
Physical characteristics
Dimensions6.789±0.253 km[4]
7.47 km(calculated)[3]
4.65±0.01 h[5]
4.656199±0.000001 h[6]
4.6568±0.0001h[a]
4.66±0.01 h[7]
0.24(assumed)[3]
0.319±0.032[4]
S[3]
12.70[4] · 12.8[1][3]

1855 Korolev (prov. designation:1969 TU1) is a stonyFlora asteroid from the inner regions of theasteroid belt, approximately 7 kilometers in diameter. Discovered in 1969, it was later named after Soviet rocket engineerSergei Korolev.[2]

Discovery

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Korolev was discovered by Russian astronomerLyudmila Chernykh at theCrimean Astrophysical Observatory in Nauchnyj on 8 October 1969.[8] On the same night, she also discovered1856 Růžena.[2]

It was first identified as1961 JD atGoethe Link Observatory in 1961, extending the body'sobservation arc by 8 years prior to its official discovery observation.[8]

Orbit and classification

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The asteroid orbits the Sun in theinner main-belt at a distance of 2.1–2.4 AU once every 3 years and 4 months (1,231 days). Its orbit has aneccentricity of 0.08 and aninclination of 3° with respect to theecliptic.[1]

Naming

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Thisminor planet was named in honor ofSergei Korolev (1907–1966), a designer, integrator, organizer and strategic planner. He was the lead Soviet rocket engineer and spacecraft designer in theSpace Race between the United States and the Soviet Union during the 1950s and 1960s until his early death. Thelunar andMartian cratersKorolev are also named in his honour.[2] The officialnaming citation was published by theMinor Planet Center on 1 June 1975 (M.P.C. 3825).[9]

Physical characteristics

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Korolev is characterized as a common stonyS-type asteroid.[3]

Diameter and albedo

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According to the surveys carried out by NASA's space-basedWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Korolev measures 6.79 kilometers in diameter, and its surface has a highalbedo of 0.319,[4] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its orbital family – and calculates a diameter of 7.47 kilometers with anabsolute magnitude of 12.8.[3]

Rotation period

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In March 2008, three rotationallightcurves ofKorolev were obtained from photometric observation made by astronomers James W. Brinsfield,Petr Pravec andRené Roy, giving a well-definedrotation period of 4.65–4.66 hours with a brightness variation 0.75 and 0.76magnitude, respectively (U=3/2/3).[5][7][a] Another concurring lightcurve was published in March 2016, using sparse-in-time photometry data from the Lowell Photometric Database (U=n.a.).[6]

Notes

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  1. ^abLightcurve plot by Pravec (2008) with rotation period4.6568±0.0001 hours with a brightness amplitude of0.75 mag and a quality code of 3. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1855) Korolev. UnpublishedOndrejov data obtained by the NEO Photometric Program and collaborating projects

References

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  1. ^abcd"JPL Small-Body Database Browser: 1855 Korolev (1969 TU1)" (2017-02-04 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1855) Korolev".Dictionary of Minor Planet Names – (1855) Korolev.Springer Berlin Heidelberg. p. 149.doi:10.1007/978-3-540-29925-7_1856.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1855) Korolev". Asteroid Lightcurve Database (LCDB). Retrieved13 December 2016.
  4. ^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. Retrieved13 December 2016.
  5. ^abBrinsfield, James W. (September 2008)."Asteroid Lightcurve Analysis at the Via Capote Observatory: First Quarter 2008".The Minor Planet Bulletin.35 (3):119–122.Bibcode:2008MPBu...35..119B.ISSN 1052-8091. Retrieved13 December 2016.
  6. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved13 December 2016.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1855) Korolev".Geneva Observatory. Retrieved13 December 2016.
  8. ^ab"1855 Korolev (1969 TU1)".Minor Planet Center. Retrieved13 December 2016.
  9. ^Schmadel, Lutz D. "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.

External links

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Authority control databasesEdit this at Wikidata
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