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141 Lumen

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141 Lumen
Discovery A
Discoverer P. P. Henry
Discovery date January 13, 1875
Alternate
designations
B
none
Category Main belt
Orbital elements C
Epoch March 6, 2006 (JD 2453800.5)
Eccentricity (e) 0.215
Semi-major axis (a) 398.786 Gm (2.666 AU)
Perihelion (q) 313.194 Gm (2.094 AU)
Aphelion (Q) 484.378 Gm (3.238 AU)
Orbital period (P) 1589.717 d (4.35 a)
Mean orbital speed 18.03 km/s
Inclination (i) 11.882°
Longitude of the
ascending node
(Ω)
318.776°
Argument of
perihelion
(ω)
57.659°
Mean anomaly (M) 152.721°
Physical characteristics D
Dimensions 130 km<ref name="IRAS">Supplemental IRAS Minor Planet Survey</ref>
Mass ~1.6×1018 (estimate)
Density ~1.4 g/cm³ (estimate)<ref name="Krasinsky">See Georgij A. Krasinsky et al Hidden Mass in the Asteroid Belt, Icarus, Vol. 158, p. 98 (2002), for density estimates</ref>
Surface gravity ~0.025 m/s² (estimate)
Escape velocity ~0.06 km/s (estimate)
Rotation period 0.820 d (19.67 h) <ref>PDS lightcurve data</ref>
Spectral class C-type asteroid
Absolute magnitude 8.20
Albedo (geometric) 0.054 <ref name="IRAS"/>
Mean surface
temperature
~173 K
max: 275K (+2° C)

141 Lumen is a dark (C-type), large rocky asteroid 130 km in diameter orbiting in the Main belt near the Eunomia family of asteroids. It is not, however, physically related to the group, being of the wrong spectral class.

It was discovered on January 13, 1875 by the brothers Paul Henry and Prosper Henry, but Paul is the one who was given the credit for this discovery. It is named after Lumen : Récits de l'infini, a book by the astronomer Camille Flammarion.

[edit] References

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Minor planets
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Small Solar System bodies
Vulcanoids | Near-Earth asteroids | Main belt | Jupiter Trojans | Centaurs | Damocloids | Comets | Trans-Neptunians (Kuiper belt · Scattered disc · Oort cloud)
For other objects and regions, see: asteroid groups and families, binary asteroids, asteroid moons and the Solar system
For a complete listing, see: List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names.
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