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193 Ambrosia

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Asteroid in the main belt of asteroids

193 Ambrosia
A three-dimensional model of 193 Ambrosia based on its light curve.
Discovery
Discovered byJ. Coggia, 1879
Discovery date28 February 1879
Designations
MPC designation(193) Ambrosia
Pronunciation/æmˈbroʊʒiə/
Alternative designationsA879 DB; 1915 RB
Minor planet categoryMain belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc100.12 yr (36569 d)
Aphelion3.3720 AU (504.44 Gm)
Perihelion1.8302 AU (273.79 Gm)
Semi-major axis2.6011 AU (389.12 Gm)
Eccentricity0.29638
Orbital period (sidereal)4.20 yr (1532.2 d)
Mean anomaly331.40°
Mean motion0° 14 5.82 / day
Inclination12.010°
Longitude of ascending node349.97°
Argument of perihelion81.365°
Physical characteristics
Mean diameter26 km
Synodic rotation period6.580 hours
6.581 h (0.2742 d)
Geometric albedo0.10
Absolute magnitude (H)9.68

193 Ambrosia (Symbol:) is a main belt asteroid that was discovered by the Corsican-born French astronomer J. Coggia on February 28, 1879, and named after Ambrosia, the food of the gods in Greek mythology.

In 2009, photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting light curve shows a synodic rotation period of 6.580 ± 0.001 hours with a brightness variation of 0.11 ± 0.02 in magnitude. This result is consistent with an independent study performed in 1996.

References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ Yeomans, Donald K., "193 Ambrosia", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 6 May 2016.
  3. ^ Warner, Brian D. (October 2009), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 March-June", The Minor Planet Bulletin, 36 (4): 172–176, arXiv:1203.4336, Bibcode:2009MPBu...36..172W, doi:10.1016/j.pss.2012.03.009, S2CID 119226456.
  4. "193 Ambrosia".

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