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
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Discovery | |||||||||||||
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Discovered by | H. Goldschmidt | ||||||||||||
Discovery date | 27 June 1857 | ||||||||||||
Designations | |||||||||||||
MPC designation | (45) Eugenia | ||||||||||||
Pronunciation | /juːˈdʒiːniə/ ew-JEE-nee-ə | ||||||||||||
Named after
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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
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18.03 km/s | ||||||||||||
45.254° | |||||||||||||
Inclination | 6.610° | ||||||||||||
147.939° | |||||||||||||
85.137° | |||||||||||||
Known satellites |
Petit-Prince S/2004 (45) 1 |
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Physical characteristics | |||||||||||||
Dimensions |
232 × 193 × 161 km 305 × 220 × 145 km |
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Mean radius
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107.3 ± 2.1 km | ||||||||||||
Mass |
(5.69 ± 0.1) ×1018 kg (5.8 ± 0.2) ×1018 kg |
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Mean density
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1.1 ± 0.1 g/cm³ 1.1 ± 0.3 g/cm³ |
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Equatorial surface gravity
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0.017 m/s² | ||||||||||||
Equatorial escape velocity
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0.071 km/s | ||||||||||||
Sidereal rotation period
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0.2375 d (5.699 h) | ||||||||||||
117 ± 10° | |||||||||||||
Pole ecliptic latitude
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-30 ± 10° | ||||||||||||
Pole ecliptic longitude
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124 ± 10° | ||||||||||||
0.040 ± 0.002 | |||||||||||||
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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.