159 Aemilia

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159 Aemilia
Discovery A
Discoverer P. P. Henry
Discovery date January 26, 1876
Alternate
designations
B
1904 OK, 1959 EG1
Category Main belt (Hygiea family)
Orbital elements C
Epoch 26 November 2005 (JD 2453700.5)
Eccentricity (e) 0.111
Semi-major axis (a) 463.794 Gm (3.100 AU)
Perihelion (q) 412.241 Gm (2.756 AU)
Aphelion (Q) 515.348 Gm (3.445 AU)
Orbital period (P) 1993.879 d (5.46 a)
Mean orbital speed 16.86 km/s
Inclination (i) 6.128°
Longitude of the
ascending node
(Ω)
134.336°
Argument of
perihelion
(ω)
335.594°
Mean anomaly (M) 227.956°
Physical characteristics D
Dimensions 125 km[1]
Mass ~1.4×1018 kg (estimate)
Density ~1.4 g/cm³ (estimate)[4]
Surface gravity ~0.024 m/s² (estimate)
Escape velocity ~0.055 km/s (estimate)
Rotation period ~1.05 d [2]
Spectral class C-type asteroid
Absolute magnitude 8.12
Albedo (geometric) 0.0639 [1]
Mean surface
temperature
~160 K
max: 239K (-34° C)
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159 Aemilia is a large Main belt asteroid. This slowly rotating, dark asteroid has a primitive carbonaceous composition.

It orbits within the Hygiea family, although it may be an unrelated interloping asteroid, as it is too big to have arisen from the cratering process that most likely produced that family.

Aemilia was discovered by the brothers Paul Henry and Prosper Henry on January 26, 1876. The credit for this discovery was given to Paul. It is probably named after the Via Aemilia, a Roman road in Italy that runs from Piacenza to Rimini.

Two stellar occultations by Aemilia have been recorded so far, the first in 2001 and the second in 2003 [3].

[edit] References

  1. PDS lightcurve data
  2. PDS occultation data
  3. G. A. Krasinsky et al Hidden Mass in the Asteroid Belt, Icarus, Vol. 158, p. 98 (2002).


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