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4003 Schumann

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4003 Schumann
Discovery [1]
Discovered byF. Börngen
Discovery siteKarl Schwarzschild Obs.
Discovery date8 March 1964
Designations
(4003) Schumann
Named after
Robert Schumann
(German composer)[2]
1964 ED · 1933 FG1
1967 RK1 · 1968 UL3
1974 SE2 · 1978 GM4
1980 RH2 · 1980 TP6
1981 WV8
main-belt · (outer)[1][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc84.20 yr (30,753 days)
Aphelion3.7477AU
Perihelion3.1040 AU
3.4258 AU
Eccentricity0.0939
6.34yr (2,316 days)
343.35°
0° 9m 19.44s / day
Inclination5.0589°
189.31°
116.48°
Physical characteristics
Dimensions32.03 km(calculated)[3]
35.00±0.89 km[4]
36.115±0.245[5]
38.207±0.611 km[6]
5.5984±0.0019h[7]
5.601±0.001 h[8]
5.6040±0.0019 h[7]
5.7502±0.0007 h[9]
0.0439±0.0089[6]
0.049±0.008[5]
0.057(assumed)[3]
0.072±0.004[4]
C[3]
10.80[4] · 11.1[6] · 11.154±0.003(R)[7] · 11.186±0.002(R)[7] · 11.2[1][3] · 11.40±0.20[10]

4003 Schumann, provisional designation1964 ED, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 35 kilometers in diameter.

The asteroid was discovered on 8 March 1964, by German astronomerFreimut Börngen at theKarl Schwarzschild Observatory in Tautenburg, Eastern Germany.[11] It was named after German composerRobert Schumann.[2]

Orbit and classification

[edit]

Schumann orbits the Sun in theouter main-belt at a distance of 3.1–3.7 AU once every 6 years and 4 months (2,316 days). Its orbit has aneccentricity of 0.09 and aninclination of 5° with respect to theecliptic.[1] The firstprecovery was obtained atHeidelberg Observatory in 1933, extending the asteroid'sobservation arc by 31 years prior to its discovery.[11]

Physical characteristics

[edit]

Schumann has been characterized as a darkC-type asteroid.[3]

Diameter and albedo

[edit]

According to the space-based surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with itsNEOWISE mission,Schumann's surface has analbedo of 0.04 and 0.07, and an estimated diameter of 35.0 and 38.2 kilometers, respectively.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous bodies of 0.057, and calculates a diameter of 32.0 kilometers.[3]

Rotation period

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Several photometriclightcurves ofSchumann gave arotation period between 5.60 and 5.75 hours with a brightness amplitude in the range of 0.20 to 0.23 inmagnitude (U=3-/2+/2).[9][8][7]

Naming

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Thisminor planet was named in honor of German composer of theRomantic era,Robert Schumann (1810–1856), known for hisLieder,chamber works and cello concerti. He was born in Zwickau, in proximity to the discovering observatory in Tautenburg.[2] The official naming citation was published by theMinor Planet Center on 20 May 1989 (M.P.C. 14634).[12]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 4003 Schumann (1964 ED)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved19 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4003) Schumann".Dictionary of Minor Planet Names – (4003) Schumann.Springer Berlin Heidelberg. p. 341.doi:10.1007/978-3-540-29925-7_3988.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (4003) Schumann". Asteroid Lightcurve Database (LCDB). Retrieved2 May 2016.
  4. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  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. Retrieved5 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. Retrieved2 May 2016.
  7. ^abcdeWaszczak, 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. Retrieved2 May 2016.
  8. ^abBrinsfield, J. W. (April 2011)."Asteroid Lightcurve Analysis at the Via Capote Observatory: 4th Quarter 2010".The Minor Planet Bulletin.38 (2):73–74.Bibcode:2011MPBu...38...73B.ISSN 1052-8091. Retrieved2 May 2016.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (4003) Schumann".Geneva Observatory. Retrieved2 May 2016.
  10. ^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. Retrieved2 May 2016.
  11. ^ab"4003 Schumann (1964 ED)".Minor Planet Center. Retrieved2 May 2016.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved2 May 2016.

External links

[edit]
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