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149 Medusa

149 Medusa
149Medusa (Lightcurve Inversion).png
A three-dimensional model of 149 Medusa based on its light curve.
Discovery 
Discovered by Henri Joseph Perrotin
Discovery date 21 September 1875
Designations
MPC designation (149) Medusa
Named after
Medusa
Main belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 124.55 yr (45493 d)
Aphelion 2.3169 AU (346.60 Gm)
Perihelion 2.03252 AU (304.061 Gm)
2.17472 AU (325.333 Gm)
Eccentricity 0.065386
3.21 yr (1171.4 d)
Average orbital speed
20.18 km/s
280.686°
0° 18m 26.374s / day
Inclination 0.93927°
159.615°
250.609°
Earth MOID 1.04123 AU (155.766 Gm)
Jupiter MOID 2.87692 AU (430.381 Gm)
Jupiter Tisserand parameter 3.683
Physical characteristics
Dimensions 19.75±0.9 km
Mass 8.0×1015 kg
Mean density
2.0 g/cm³
Equatorial surface gravity
0.0055 m/s²
Equatorial escape velocity
0.0104 km/s
26.023 h (1.0843 d) 
26.038 h 
0.2334±0.022
Temperature ~ 189 K
S
10.79

149 Medusa is a bright-coloured, stony main-belt asteroid that was discovered by French astronomer J. Perrotin on September 21, 1875, and named after the Gorgon Medusa, a snake-haired monster in Greek mythology.

When it was discovered, Medusa was by far the smallest asteroid found (although this was not known at that time). Since then, many thousands of smaller asteroids have been found. It was also the closest asteroid to the Sun discovered up to that point, beating the long-held record of 8 Flora. It remained the closest asteroid to the Sun until 433 Eros and 434 Hungaria were found in 1898, leading to the discovery of two new families of asteroids inward from the 4:1 Kirkwood gap which forms the boundary of the main belt.

Photometric observations of this asteroid at the Organ Mesa Observatory in Las Cruces, New Mexico, during 2010 gave a light curve with a rather long rotation period of 26.038 ± 0.002 hours and a brightness variation of 0.56 ± 0.03 in magnitude.



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