Aethra (minor planet designation: 132 Aethra) is a metallic asteroid and Mars-crosser on an eccentric orbit from the asteroid belt. It measures approximately 40 kilometers in diameter.
![]() Lightcurve-based 3D-model of Aethra | |
Discovery | |
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Discovered by | James C. Watson |
Discovery date | 13 June 1873 |
Designations | |
MPC designation | (132) Aethra |
Pronunciation | /ˈiːθrə/[1] |
Named after | Aethra |
Alternative designations | A873 LA; 1922 XB; 1949 MD; 1953 LF |
Minor planet category | Mars crosser |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 142.50 yr (52049 d) |
Aphelion | 3.6250 AU (542.29 Gm) |
Perihelion | 1.5895 AU (237.79 Gm) |
Semi-major axis | 2.6073 AU (390.05 Gm) |
Eccentricity | 0.39036 |
Orbital period (sidereal) | 4.21 yr (1537.7 d) |
Average orbital speed | 17.72 km/s |
Mean anomaly | 38.271° |
Mean motion | 0° 14m 2.796s / day |
Inclination | 24.997° |
Longitude of ascending node | 258.408° |
Argument of perihelion | 255.216° |
Physical characteristics | |
Dimensions | 35.83±6.59 km[3] 42.87±1.6 km[2] |
Mass | (0.41±2.71)×1018 kg[3] |
Synodic rotation period | 5.1684 h (0.21535 d)[2] |
Geometric albedo | 0.1990±0.015[2] |
Spectral type | M |
Absolute magnitude (H) | 9.38[2] |
It was discovered by James Craig Watson in 1873 and is the first such Mars-crosser asteroid to be identified. As a Mars-crosser asteroid, Aethra is the lowest numbered asteroid to not have proper orbital elements due to recurring perturbations by Mars. It has a rather eccentric orbit that sometimes brings it closer to the Sun than the planet Mars.
With an original observation arc of only 22 days, 132 Aethra was a lost asteroid between 1873 and 1922.[4][5]
The varying light curve of the asteroid implies an elongated or irregular shape for its body.
It is named after Aethra, the mother of Theseus in Greek mythology.
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