Astronomy:214 Aschera

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Short description: Main-belt asteroid
214 Aschera
000214-asteroid shape model (214) Aschera.png
3D convex shape model of 214 Aschera
Discovery
Discovered byJohann Palisa
Discovery date29 February 1880
Designations
(214) Aschera
Pronunciation/əˈʃɪərə/[1]
A880 DB, 1903 SE
1947 BP, 1948 JE
1949 QG2, 1949 SX1
1950 XH, 1953 OO
Minor planet categoryMain belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc136.09 yr (49707 d)
|{{{apsis}}}|helion}}2.6938 astronomical unit|AU (402.99 Gm)
|{{{apsis}}}|helion}}2.5279 AU (378.17 Gm)
2.6108 AU (390.57 Gm)
Eccentricity0.031762
Orbital period4.22 yr (1540.9 d)
Average Orbital speed18.43 km/s
Mean anomaly167.065°
Mean motion0° 14m 1.068s / day
Inclination3.4364°
Longitude of ascending node341.997°
131.579°
Physical characteristics
Dimensions23.16±1.0 km
Rotation period6.835 h (0.2848 d)
Geometric albedo0.5220±0.048
E
Absolute magnitude (H)9.2


Aschera (minor planet designation: 214 Aschera) is a Main belt asteroid. It was discovered by Austrian astronomer Johann Palisa on February 29, 1880, in Pola and was named after the Sidonian goddess Asherah.

It is classified as a rare E-type asteroid and is fairly faint for an object of its type. The overall diameter is estimated to be 23 km and it has a geometric albedo of 0.52.[3] Photometric observations show a rotation period of 6.835 ± 0.001 hours with a brightness variation of 0.20 in magnitude. Using a tri-axial ellipsoidal model derived from light curve data, the overall shape of the asteroid is estimated to be a/b = 1.24 ± 0.12 and b/c = 1.83 ± 0.10, where a, b, c are the three axes of an ellipsoid.[4]

References

  1. "Asherah". Merriam-Webster Dictionary. https://www.merriam-webster.com/dictionary/Asherah. 
  2. "214 Aschera". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=214;cad=1. 
  3. Mishchenko, Michael I.; Rosenbush, Vera K. (2011), "Opposition Optical Phenomenon in Planetary Astrophysics: Observational Results", Polarimetric Detection, Characterization and Remote Sensing (Springer Science & Business Media): p. 417, ISBN 978-9400716353, https://books.google.com/books?id=tdPBENFJTe0C&pg=PA417. 
  4. Shevchenko, V. G. et al. (August 2003), "Rotation and photometric properties of E-type asteroids", Planetary and Space Science 51 (9–10): 525–532, doi:10.1016/S0032-0633(03)00076-X, Bibcode2003P&SS...51..525S. 

External links