149 Medusa

Medusa (minor planet designation: 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. It is orbiting the Sun at a distance of 2.17 AU with a period of 3.21 years and an eccentricity of 0.065. The orbital plane is tilted slightly at an angle of 0.94° to the plane of the ecliptic.

149 Medusa
A three-dimensional model of 149 Medusa based on its light curve.
Discovery
Discovered byHenri Joseph Perrotin
Discovery date21 September 1875
Designations
MPC designation
(149) Medusa
Pronunciation/mɪˈdjsə/
Named after
Medusa
Alternative designations
A875 SA; 1905 BA;
1906 HB
Minor planet category
Main belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc124.55 yr (45493 d)
Aphelion2.32 AU (346.60 Gm)
Perihelion2.03 AU (304.06 Gm)
Semi-major axis
2.17 AU (325.33 Gm)
Eccentricity0.065386
Orbital period (sidereal)
3.21 yr (1,171.4 d)
Average orbital speed
20.18 km/s
Mean anomaly
280.686°
Mean motion
0° 18m 26.374s / day
Inclination0.93927°
Longitude of ascending node
159.615°
250.609°
Earth MOID1.04 AU (155.77 Gm)
Jupiter MOID2.88 AU (430.38 Gm)
TJupiter3.683
Physical characteristics
Dimensions19.75±0.9 km
Mass8.0×1015 kg
Mean density
2.0 g/cm3
Equatorial surface gravity
0.0055 m/s2
Equatorial escape velocity
0.0104 km/s
Synodic rotation period
26.023 h (1.0843 d)
26.038 h
0.2334±0.022
Temperature~189 K
S
10.79

    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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