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1834 Palach

From Wikipedia, the free encyclopedia
Main-belt asteroid

1834 Palach
Discovery[1]
Discovered byL. Kohoutek
Discovery siteBergedorf Obs.
Discovery date22 August 1969
Designations
(1834) Palach
Named after
Jan Palach(Czech student)[2]
1969 QP
main-belt ·  · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc47.26 yr (17,260 days)
Aphelion3.2373AU
Perihelion2.8142 AU
3.0258 AU
Eccentricity0.0699
5.26yr (1,922 days)
102.36°
0° 11m 14.28s / day
Inclination9.4352°
268.16°
358.39°
Physical characteristics
Dimensions17.156±0.414[5]
18.059±0.264 km[6]
19.52 km(calculated)[3]
20.23±0.87 km[7]
3.1358±0.0009h[8]
3.139±0.001 h[9]
0.109±0.010[7]
0.1364±0.0190[6]
0.14(assumed)[3]
0.151±0.020[5]
S(assumed)[3]
11.3[1][3] · 11.50[6][7] · 11.54±0.20[10]

1834 Palach, provisional designation1969 QP, is a stony Eoanasteroid from the outer region of theasteroid belt, approximately 19 kilometers in diameter. It was discovered on 22 August 1969 by Czech astronomerLuboš Kohoutek atBergedorf Observatory in Hamburg, Germany, and named after Czech studentJan Palach.[2][11]

Orbit and classification

[edit]

Palach is a member of theEos family (606), the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids.[4][12]: 23 

It orbits the Sun in theouter main-belt at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,922 days). Its orbit has aneccentricity of 0.07 and aninclination of 9° with respect to theecliptic.[1] As noprecoveries were taken, and no prior identifications were made,Palach'sobservation arc begins with its official discovery observation in 1969.[11]

Physical characteristics

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Rotation period

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In September 2006, a rotationallightcurve forPalach was obtained from photometric observations made by French amateur astronomerLaurent Bernasconi at St. Michel sur Meu. It gave arotation period of 3.139 hours with a brightness amplitude of 0.16magnitude (U=2).[9] In May 2010, a second lightcurve, obtained by Zachary Pligge at Oakley Southern Sky Observatory, Australia, gave a period of 3.1358 hours with an amplitude of 0.13 (U=2).[8]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Palach measures between 17.16 and 20.23 kilometers in diameter, and its surface has analbedo between 0.109 and 0.151.[5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for Eoan asteroids of 0.14 and calculates a diameter of 19.52 kilometers with anabsolute magnitude of 11.3.[3]

Naming

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It was named in memory of Czech studentJan Palach (1948–1969), who burned himself to death, as a protest against the Soviet occupation of Czechoslovakia that followed and ended the national reform movement known as thePrague Spring.[2] The official naming citation was published by theMinor Planet Center on 25 August 1991 (M.P.C. 18643).[13]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1834 Palach (1969 QP)" (2016-11-23 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1834) Palach".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 147.doi:10.1007/978-3-540-29925-7_1835.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1834) Palach". Asteroid Lightcurve Database (LCDB). Retrieved15 December 2016.
  4. ^ab"Asteroid 1834 Palach – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved15 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.
  7. ^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)
  8. ^abPligge, Zachary; Monnier, Adam; Pharo, John; Stolze, Kellen; Yim, Arnold; Ditteon, Richard (January 2011)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2010 May".The Minor Planet Bulletin.38 (1):5–7.Bibcode:2011MPBu...38....5P.ISSN 1052-8091. Retrieved15 December 2016.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1834) Palach".Geneva Observatory. Retrieved15 December 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. Retrieved15 December 2016.
  11. ^ab"1834 Palach (1969 QP)".Minor Planet Center. Retrieved15 December 2016.
  12. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 December 2016.

External links

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