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214 Aschera

From Wikipedia, the free encyclopedia
Main-belt asteroid

214 Aschera
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
Main belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc136.09 yr (49707 d)
Aphelion2.6938 AU (402.99 Gm)
Perihelion2.5279 AU (378.17 Gm)
2.6108 AU (390.57 Gm)
Eccentricity0.031762
4.22 yr (1,540.9 d)
18.43 km/s
167.065°
0° 14m 1.068s / day
Inclination3.4364°
341.997°
131.579°
Physical characteristics
Dimensions23.16±1.0 km
6.835 h (0.2848 d)
0.5220±0.048
E
9.2

214 Aschera is aMain beltasteroid. It was discovered byAustrian astronomerJohann Palisa on February 29, 1880, inPola and was named after theSidonian goddessAsherah. This minor planet is orbiting theSun at a distance of2.61 AU with a loweccentricity of 0.032 and anorbital period of 4.22 yr. Theorbital plane is inclined at an angle of 3.44° to theplane of the ecliptic.[2]

It is classified as a rareE-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 data collected during September 2021 was used the generate alightcurve for 214 Aschera. This showed arotation period of6.833±0.004 h with a brightness variation of 0.20 magnitude.[4] Using a tri-axialellipsoidal model derived fromlight curve data, the overall shape of the asteroid is estimated to bea/b = 1.24 ± 0.12 andb/c = 1.83 ± 0.10, wherea,b,c are the threeaxes of anellipsoid.[5]

References

[edit]
  1. ^"Asherah".Merriam-Webster.com Dictionary. Merriam-Webster.
  2. ^ab"214 Aschera".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved12 May 2016.
  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.
  4. ^Farfan, Rafael Gonzalez; et al. (April 2022), "The Rotation Periods of 3 Juno, 28 Bellona, 129 Antigone, 214 Aschera, 237 Coelestina, 246 Asporina, 382 Dodona, 523 Ada, 670 Ottegebe, 918 Itha, 1242 Zambesia, 1352 Wawel, 1358 Gaika, 4155 Watanabe, and 6097 Koishikawa",Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers,49 (2):136–140,Bibcode:2022MPBu...49..136F.
  5. ^Shevchenko, V. G.; et al. (August 2003), "Rotation and photometric properties of E-type asteroids",Planetary and Space Science,51 (9–10):525–532,Bibcode:2003P&SS...51..525S,doi:10.1016/S0032-0633(03)00076-X.

External links

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