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38 Leda

Main-belt asteroid


Summary

Main-belt asteroid

FieldValue
background#D6D6D6
name38 Leda
image38Leda (Lightcurve Inversion).png
captionA three-dimensional model of 38 Leda based on its light curve
discovererJ. Chacornac
discoveredJanuary 12, 1856
mpc_name(38) Leda
pronounced
adjectiveLedean (Latin Lēdæ-us)
alt_namesA904 SF;
named_afterLeda
mp_categoryMain belt
epochDecember 31, 2006 (JD 2454100.5)
semimajor410.409 million km (2.743 AU)
perihelion348.232 million km (2.328 AU)
aphelion472.587 million km (3.159 AU)
eccentricity0.152
period1659.725 d (4.54 a)
inclination6.955°
asc_node295.890°
arg_peri168.804°
mean_anomaly107.567°
avg_speed17.88 km/s
dimensions92.255 ± 0.490 km
mass(7.16 ± 3.38/2.24) kg
density1.743 ± 0.822/0.544 g/cm3
surface_gravm/s²
escape_velocitykm/s
rotation0.5350 d (12.84 h)
spectral_typeC
abs_magnitude8.32
albedo0.055
single_temperature~170 K

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. The spectra of the asteroid displays evidence of aqueous alteration.

Leda has been studied by radar. 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. 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.

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. "38 Leda".
Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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