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1841 Masaryk

From Wikipedia, the free encyclopedia
Carbonaceous background asteroid

1841 Masaryk
Shape model ofMasaryk from itslightcurve
Discovery[1]
Discovered byL. Kohoutek
Discovery siteBergedorf Obs.
Discovery date26 October 1971
Designations
(1841) Masaryk
Named after
Tomáš Garrigue Masaryk(Czechoslovak President)[2]
1971 UO1 · 1936 FW
1955 DE · 1959 VJ
1968 FG · 1970 QN
main-belt · (outer)[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc81.02 yr (29,591 days)
Aphelion3.7629AU
Perihelion3.0796 AU
3.4213 AU
Eccentricity0.0999
6.33yr (2,311 days)
313.50°
0° 9m 20.52s / day
Inclination2.6203°
45.323°
119.95°
Physical characteristics
Dimensions38.642±0.544 km[3]
40.240±0.504[4]
43.77±0.83 km[5]
46.04 km(derived)[6]
46.07±2.5 km[7]
7.53±0.04h[8]
7.54301±0.00001 h[9]
0.0364(derived)[6]
0.0398±0.005[7]
0.045±0.002[5]
0.052±0.005[4]
0.0567±0.0036[3]
P[3] · CX[10] · C[6]
10.8[3][5][7] · 10.9[1][6] · 10.94±0.19[10]

1841 Masaryk (prov. designation:1971 UO1) is a carbonaceousbackground asteroid from the outer region of theasteroid belt, approximately 46 kilometers in diameter. It was discovered on 26 October 1971, by Czech astronomerLuboš Kohoutek atBergedorf Observatory in Hamburg, Germany.[11] The asteroid was named after the first President ofCzechoslovakia,Tomáš Garrigue Masaryk.[2]

Orbit and classification

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Masaryk orbits the Sun in theouter main-belt at a distance of 3.1–3.8 AU once every 6 years and 4 months (2,311 days). Its orbit has aneccentricity of 0.10 and aninclination of 3° with respect to theecliptic.[1] First identified as1936 FW atUccle Observatory,Masaryk's first used observation was taken atGoethe Link Observatory in 1955, extending the body'sobservation arc by 16 years prior to its official discovery observation.[11]

Naming

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Thisminor planet was named in honor of the first president of the independent Czechoslovak Republic,Tomáš Garrigue Masaryk (1850–1937), statesman, philosopher and known for his humanistic ideas.[2] The officialnaming citation was published by theMinor Planet Center on 20 December 1974 (M.P.C. 3757).[12]

Physical characteristics

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Thecarbonaceous asteroid is characterized as a (darker)P-type and as a transitional CX-type byNEOWISE andPanSTARRS, respectively.[3][10]

Rotation period

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In April 2006, a rotationallightcurve ofMasaryk was obtained from photometric observations made by French amateur astronomerPierre Antonini. It gave arotation period of 7.53 hours with a brightness variation of 0.52magnitude (U=2+).[8] The result agrees with a lightcurve published in March 2016, using sparse-in-time photometry data from the Lowell Photometric Database (U=n.a.).[9]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Masaryk measures between 38.6 and 46.1 kilometers in diameter, and its surface has analbedo between 0.039 and 0.057.[3][4][5][7] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.036 and a diameter of 46.0 kilometers with anabsolute magnitude of 10.9.[6]

References

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  1. ^abcde"JPL Small-Body Database Browser: 1841 Masaryk (1971 UO1)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1841) Masaryk".Dictionary of Minor Planet Names – (1841) Masaryk.Springer Berlin Heidelberg. p. 147.doi:10.1007/978-3-540-29925-7_1842.ISBN 978-3-540-00238-3.
  3. ^abcdefMainzer, 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.
  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. Retrieved14 December 2016.
  5. ^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)
  6. ^abcde"LCDB Data for (1841) Masaryk". Asteroid Lightcurve Database (LCDB). Retrieved14 December 2016.
  7. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1841) Masaryk".Geneva Observatory. Retrieved14 December 2016.
  9. ^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. Retrieved14 December 2016.
  10. ^abcVeres, 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. Retrieved14 December 2016.
  11. ^ab"1841 Masaryk (1971 UO1)".Minor Planet Center. Retrieved14 December 2016.
  12. ^Schmadel, Lutz D. (2009). "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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