Astronomy:152 Atala

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Short description: Main-belt asteroid
152 Atala
152Atala (Lightcurve Inversion).png
A three-dimensional model of 152 Atala based on its light curve.
Discovery[1]
Discovered byP. P. Henry
Discovery date2 November 1875
Designations
(152) Atala
Pronunciation/əˈtɑːlə/
French: [atala]
Named afterAtala
A875 VB
Minor planet categoryMain belt
Orbital characteristics[2][3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc130.69 yr (47735 d)
|{{{apsis}}}|helion}}3.3855 astronomical unit|AU (506.46 Gm)
|{{{apsis}}}|helion}}2.8984 AU (433.59 Gm)
3.1420 AU (470.04 Gm)
Eccentricity0.077507
Orbital period5.57 yr (2034.2 d)
Mean anomaly52.593°
Mean motion0° 10m 37.092s / day
Inclination12.114°
Longitude of ascending node39.945°
59.807°
Earth MOID1.93567 AU (289.572 Gm)
Jupiter MOID1.85235 AU (277.108 Gm)
TJupiter3.171
Physical characteristics
Dimensions65 ± 8 km[4]
71–122 km[5]
Mass(5.43 ± 1.24) × 1018 kg[6]
Rotation period6.246 h (0.2603 d)
Sidereal rotation period5.28-6.25 hours
Geometric albedo0.054
D[7]
Absolute magnitude (H)8.33


Atala (minor planet designation: 152 Atala) is a large main belt asteroid that was discovered by brothers Paul Henry and Prosper Henry on 2 November 1875, but the discovery was credited to Paul. It is a type D asteroid, meaning that it is composed of carbon, organic rich silicates and possibly water ice.

The asteroid is named for the eponymous heroine of the 1801 novella Atala by François-René de Chateaubriand.[8] The Henry brothers also named the last of their discoveries, 186 Celuta, after another Chateaubriand heroine.[9] Both Atala and Céluta are American Indian fictional characters.[10]

An occultation of a star by Atala was observed from Japan on 11 March 1994. Subsequent occultations have been observed as recently as 2006.[citation needed]

Photometric of this asteroid made in 1981 gave a light curve with a period of 5.282 ± 0.004 hours with a brightness variation of 0.50 in magnitude.[11]

References

  1. Hardard's Numbered MPs
  2. "The Asteroid Orbital Elements Database". Lowell Observatory. http://ftp.lowell.edu/pub/elgb/astorb.html. 
  3. Yeomans, Donald K., "152 Atala", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=152, retrieved 12 May 2016. 
  4. Ďurech, Josef; Kaasalainen, Mikko; Herald, David; Dunham, David; Timerson, Brad; Hanuš, Josef et al. (2011). "Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes". Icarus 214 (2): 652–670. doi:10.1016/j.icarus.2011.03.016. Bibcode2011Icar..214..652D. http://astro.troja.mff.cuni.cz/projects/asteroids3D/download/durech_et_al_2011_occ_paper.pdf. Retrieved 26 January 2012. 
  5. Asterodoccultation.com
  6. Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  7. SPIFF LCSUMPUB
  8. Schmadel, Lutz D.; International Astronomical Union (2003). Dictionary of minor planet names. Berlin; New York: Springer-Verlag. p. 29. ISBN 978-3-540-00238-3. https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA29. 
  9. Schmadel, Lutz D.; International Astronomical Union (2012). Dictionary of minor planet names (6th ed.). Berlin; New York: Springer-Verlag. p. 29. ISBN 9783642297182. https://books.google.com/books?id=aeAg1X7afOoC&q&pg=PA29. Retrieved 4 April 2014. 
  10. Chateaubriand, François-René (1801). Atala. ; Chateaubriand, François-René (1802). René. 
  11. Schober, H. J. (July 1983), "The large C-type asteroids 146 Lucina and 410 Chloris, and the small S-type asteroids 152 Atala and 631 Philippina - Rotation periods and lightcurves", Astronomy and Astrophysics Supplement Series 53: 71–75, Bibcode1983A&AS...53...71S. 

External links