111 Ate

Ate (minor planet designation: 111 Ate) is a main-belt asteroid discovered by the German-American astronomer C. H. F. Peters on August 14, 1870, and named after Ate, the goddess of mischief and destruction 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 an Ch asteroid.

111 Ate
Orbital diagram
Discovery
Discovered byChristian Heinrich Friedrich Peters
Discovery date14 August 1870
Designations
MPC designation
(111) Ate
Pronunciation/ˈt/
Named after
Ate
Alternative designations
A870 PA; 1911 KE;
1935 AA
Minor planet category
Main belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc145.66 yr (53202 d)
Aphelion2.8614 AU (428.06 Gm)
Perihelion2.32553 AU (347.894 Gm)
Semi-major axis
2.59349 AU (387.981 Gm)
Eccentricity0.10332
Orbital period (sidereal)
4.18 yr (1525.5 d)
Average orbital speed
18.44 km/s
Mean anomaly
190.607°
Mean motion
0° 14m 9.532s / day
Inclination4.9318°
Longitude of ascending node
305.757°
166.424°
Earth MOID1.34088 AU (200.593 Gm)
Jupiter MOID2.23131 AU (333.799 Gm)
TJupiter3.406
Physical characteristics
Dimensions126.34 km
142.85 ± 5.94 km
Mass(1.76 ± 0.44) × 1018 kg
Mean density
1.15 ± 0.32 g/cm3
Equatorial surface gravity
0.0376 m/s²
Equatorial escape velocity
0.0712 km/s
Synodic rotation period
22.072 h (0.9197 d)
22.072 ± 0.001 h
0.0605±0.004
Temperature~173 K
C
8.02

    Two stellar occultations by Ate were observed in 2000, two months apart. Its occultation of the star HIP 2559 was used to determine a chord length of 125.6 ± 7.2 km through the asteroid, giving a lower bound on the maximum dimension. During 2000, 111 Ate was observed by radar from the Arecibo Observatory. The return signal matched an effective diameter of 135 ± 15 km. The estimated size of this asteroid is 143 km, making it one of the larger asteroids.

    Based upon an irregular light curve generated from photometric observations of this asteroid at Pulkovo Observatory, it has a rotation period of 22.072 ± 0.001 hours and varies in brightness by 0.12 ± 0.01 in magnitude.

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