A three-dimensional model of 345 Tercidina based on its light curve.
|
|
Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 23 November 1892 |
Designations | |
MPC designation | (345) Tercidina |
1892 O | |
Main belt | |
Orbital characteristics | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 122.88 yr (44882 d) |
Aphelion | 2.46765 AU (369.155 Gm) |
Perihelion | 2.18337 AU (326.628 Gm) |
2.32551 AU (347.891 Gm) | |
Eccentricity | 0.061120 |
3.55 yr (1295.3 d) | |
Average orbital speed
|
19.53 km/s |
288.675° | |
0° 16m 40.526s / day | |
Inclination | 9.74765° |
212.629° | |
230.279° | |
Earth MOID | 1.2087 AU (180.82 Gm) |
Jupiter MOID | 2.69073 AU (402.527 Gm) |
Jupiter Tisserand parameter | 3.553 |
Physical characteristics | |
Dimensions | 126x94x90 km 94 km 98.78 ± 2.63 km |
Mean radius
|
±2.45 47.06km |
Mass | (2.68 ± 1.18) × 1018 kg |
Mean density
|
5.30 ± 2.37 g/cm3 |
12.371 h (0.5155 d) | |
±0.007 0.0654 | |
C | |
8.71 | |
345 Tercidina is a large main-belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material.
It was discovered by Auguste Charlois on November 23, 1892, in Nice.
Observations of an occultation of a bright 5.5 magnitude star on September 17, 2002, produced seventy-five chords indicating an ellipsoid of 111×90 km.
Observations of an occultation on November 15, 2005, near Grass Valley, CA, produced five chords indicating an incomplete outline of 126×111 km. This larger result may be caused by a different orientation of the asteroid as it passed in front of the star.