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45 Eugenia

45 Eugenia
45 eugenia-01.jpg
CFHT time-lapse image of Eugenia and Petit-Prince, showing five stages in the moon's orbit. The 'flare' around them is an imaging artifact
Discovery
Discovered by H. Goldschmidt
Discovery date 27 June 1857
Designations
MPC designation (45) Eugenia
Pronunciation /juːˈniə/ ew-JEE-nee-ə
Named after
Empress Eugénie
1941 BN
Main belt
Orbital characteristics
Epoch November 26, 2005 (JD 2453701.5)
Aphelion 440.305 Gm (2.943 AU)
Perihelion 373.488 Gm (2.497 AU)
406.897 Gm (2.720 AU)
Eccentricity 0.082
1638.462 d (4.49 a)
Average orbital speed
18.03 km/s
45.254°
Inclination 6.610°
147.939°
85.137°
Known satellites Petit-Prince
S/2004 (45) 1
Physical characteristics
Dimensions 232 × 193 × 161 km
305 × 220 × 145 km
Mean radius
107.3 ± 2.1 km
Mass (5.69 ± 0.1) ×1018 kg
(5.8 ± 0.2) ×1018 kg
Mean density
1.1 ± 0.1 g/cm³
1.1 ± 0.3 g/cm³
Equatorial surface gravity
0.017 m/s²
Equatorial escape velocity
0.071 km/s
Sidereal rotation period
0.2375 d (5.699 h)
117 ± 10°
-30 ± 10°
124 ± 10°
0.040 ± 0.002
Surface temp. min mean max
Kelvin ~171 253
Celsius -22°
F
7.46

45 Eugenia is a large asteroid of the asteroid belt. It is famed as one of the first asteroids to be found to have a moon orbiting it. It is also the second known triple asteroid, after 87 Sylvia.

Eugenia was discovered on June 28, 1857 by the Franco-German amateur astronomer Hermann Goldschmidt. His instrument of discovery was a 4-inch aperture telescope located in his sixth floor apartment in the Latin Quarter of Paris. It was the forty-fifth minor planet to be discovered. The preliminary orbital elements were computed by Wilhelm Forster in Berlin, based on three observations in July, 1857.

The asteroid was named by its discoverer after Empress Eugenia di Montijo, the wife of Napoleon III. It was the first asteroid to be definitely named after a real person, rather than a figure from classical legend, although there was some controversy about whether 12 Victoria was really named for the mythological figure or for Queen Victoria.

Eugenia is a large asteroid, with a diameter of 214 km. It is an F-type asteroid, which means that it is very dark in colouring (darker than soot) with a carbonaceous composition. Like Mathilde, its density appears to be unusually low, indicating that it may be a loosely packed rubble pile, not a monolithic object. Eugenia appears to be almost anhydrous. Lightcurve analysis indicates that Eugenia's pole most likely points towards ecliptic coordinates (β, λ) = (-30°, 124°) with a 10° uncertainty, which gives it an axial tilt of 117°. Eugenia's rotation is then retrograde.


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