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![]() A three-dimensional model of 38 Leda based on its light curve | |
Discovery | |
---|---|
Discovered by | J. Chacornac |
Discovery date | January 12, 1856 |
Designations | |
Designation | (38) Leda |
Pronunciation | /ˈliːdə/[1] |
Named after | Leda |
A904 SF; 1949 QO2 | |
Main belt | |
Adjectives | Ledean /lɪˈdiːən/ (Latin Lēdæ-us) |
Orbital characteristics | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 472.587 Gm (3.159 AU) |
Perihelion | 348.232 Gm (2.328 AU) |
410.409 Gm (2.743 AU) | |
Eccentricity | 0.152 |
1659.725 d (4.54 a) | |
Average orbital speed | 17.88 km/s |
107.567° | |
Inclination | 6.955° |
295.890° | |
168.804° | |
Physical characteristics | |
Dimensions | 92.255 ± 0.490 km[2] |
Mass | (7.16 ± 3.38/2.24)×1017 kg[3] |
Mean density | 1.743 ± 0.822/0.544 g/cm3[3] |
0.0225 m/s² | |
0.0455 km/s | |
0.5350 d (12.84 h) [2] | |
Albedo | 0.055 [2] |
Temperature | ~170 K |
Spectral type | C[2] |
8.32 | |
38 Leda is a large, dark main-belt asteroid that was discovered by French astronomer J. Chacornac on January 12, 1856, and named after Leda, the mother of Helen of Troy in Greek mythology. In the Tholen classification system, it is categorized as a carbonaceous C-type asteroid, while the Bus asteroid taxonomy system lists it as a Cgh asteroid.[4] The spectra of the asteroid displays evidence of aqueous alteration.[5]
Leda has been studied by radar.[6] During 2002, 38 Leda was observed by radar from the Arecibo Observatory. The return signal matched an effective diameter of 116 ± 13 km. This is consistent with some asteroid dimensions computed through other means.[7][8] Based upon a light curve that was generated from photometric observations of this asteroid at Pulkovo Observatory, it has a rotation period of 12.834 ± 0.001 hours and varies in brightness by 0.15 ± 0.01 in magnitude.[9]