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239 Adrastea

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Main-belt asteroid For the satellite of Jupiter, see Adrastea (moon).

239 Adrastea
3D model based on lightcurve data
Discovery
Discovered byJohann Palisa
Discovery date18 August 1884
Designations
MPC designation(239) Adrastea
Pronunciation/ædrəˈstiːə/
Named afterAdrasteia
Alternative designationsA884 QA, 1915 TD
1955 MK1, 1956 UJ
Minor planet categoryMain belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc131.66 yr (48,087 d)
Aphelion3.66279 AU (547.946 Gm)
Perihelion2.2695 AU (339.51 Gm)
Semi-major axis2.96616 AU (443.731 Gm)
Eccentricity0.23486
Orbital period (sidereal)5.11 yr (1,865.9 d)
Average orbital speed17.25 km/s
Mean anomaly233.617°
Mean motion0° 11 34.584 / day
Inclination6.1746°
Longitude of ascending node180.634°
Argument of perihelion210.15°
Physical characteristics
Dimensions41.52±1.4 km
Synodic rotation period18.4707 h (0.76961 d)
Geometric albedo0.0777±0.006
Temperatureunknown
Spectral typeunknown
Absolute magnitude (H)10.4
Orbit of Adrastea (blue ring)

239 Adrastea is a main belt asteroid. It was discovered by Johann Palisa on 18 August 1884 in Vienna, and was named after the Greek nymph Adrasteia. This asteroid is orbiting the Sun at a distance of 2.97 AU with a period of 5.11 years and an eccentricity (ovalness) of 0.23. The orbital plane is tilted at an angle of 6.17° to the plane of the ecliptic.

Photometric data collected during 2009 were used for light curve analysis of this asteroid, yielding a rotation period of 18.48±0.03 h with a brightness variation of 0.45±0.05 in magnitude. The result is close to the 18.347±0.003 h period from a study performed in 2003. The asteroid is roughly 42 km in diameter.

References

  1. ^ "JPL Small-Body Database Browser: 239 Adrastea". Jet Propulsion Laboratory. Retrieved 12 May 2016.
  2. Carbo, Landry; et al. (October 2009), "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2008 October thru 2009 March", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 36 (4): 152–157, Bibcode:2009MPBu...36..152C.

External links

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