125 Liberatrix

Liberatrix (minor planet designation: 125 Liberatrix) is a main-belt asteroid. It has a relatively reflective surface and an M-type spectrum. Liberatrix is a member of an asteroid family bearing its own name.

125 Liberatrix
A three-dimensional model of 125 Liberatrix based on its light curve.
Discovery
Discovered byPaul Henry and Prosper Henry
Discovery date11 September 1872
Designations
MPC designation
(125) Liberatrix
Pronunciation/ˈlɪbərtrɪks/
Alternative designations
A872 RA; 1902 EG;
1943 FE; 1949 OE1;
1949 SM; 1954 TD1
Minor planet category
Main belt
(liberatrix)
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc143.54 yr (52428 d)
Aphelion2.95698 AU (442.358 Gm)
Perihelion2.53084 AU (378.608 Gm)
Semi-major axis
2.74391 AU (410.483 Gm)
Eccentricity0.077651
Orbital period (sidereal)
4.55 yr (1660.2 d)
Average orbital speed
17.96 km/s
Mean anomaly
307.971°
Mean motion
0° 13m 0.642s / day
Inclination4.66407°
Longitude of ascending node
169.003°
109.288°
Earth MOID1.51912 AU (227.257 Gm)
Jupiter MOID2.13019 AU (318.672 Gm)
TJupiter3.340
Physical characteristics
Dimensions43.58±2.3 km
61.058 km
Mass8.7×1016 kg
Mean density
2.0 g/cm3
Equatorial surface gravity
0.0122 m/s2
Equatorial escape velocity
0.0231 km/s
Synodic rotation period
3.968 h (0.1653 d)
0.2253±0.026
0.1305 ± 0.0269
Temperature~168 K
M (Tholen)
9.04, 8.90

    It was discovered by Prosper Henry on 11 September 1872, from Paris. Some sources give Paul Henry sole credit for its discovery. The asteroid's name is a feminine version of the word "liberator". Henry may have chosen the name to mark the liberation of France from Prussia during the Franco-Prussian War in 1870. More specifically, it may honor Adolphe Thiers, the first President of the French Republic, who arranged a loan that enabled the Prussian troops to be removed from France.

    In the late 1990s, a network of astronomers worldwide gathered lightcurve data to derive the spin states and shape models of 10 asteroids, including Liberatrix. Liberatrix's lightcurve has a large amplitude of 0.4 in magnitude, indicating an elongated or irregular shape.

    The spectrum of this asteroid matches a M-type asteroid. It may be the remnant of an asteroid that had undergone differentiation, with orthopyroxene minerals scattered evenly across the surface. There is no indication of hydration.

    To date, there have been at least two observed occultations by Liberatrix. Early on 11 December 2014, Liberatrix occulted a 9th magnitude star and will be visible over the majority of Southern California and a swath of Mexico.

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