Martha (minor planet designation: 205 Martha) is a large main belt asteroid. It is a dark, primitive carbonaceous C-type asteroid. This object was discovered by Johann Palisa on 13 October 1879, in Pola and was named after Martha, a woman in the New Testament.
| Discovery | |
|---|---|
| Discovered by | Johann Palisa |
| Discovery date | 13 October 1879 |
| Designations | |
MPC designation | (205) Martha |
| Pronunciation | /ˈmɑːrθə/[1] |
Named after | Martha |
Alternative designations | A879 TB |
Minor planet category | Main belt |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 136.51 yr (49860 d) |
| Aphelion | 2.8758 AU (430.21 Gm) |
| Perihelion | 2.6783 AU (400.67 Gm) |
Semi-major axis | 2.7771 AU (415.45 Gm) |
| Eccentricity | 0.035571 |
Orbital period (sidereal) | 4.63 yr (1690.3 d) |
Average orbital speed | 17.87 km/s |
Mean anomaly | 198.37° |
Mean motion | 0° 12m 46.692s / day |
| Inclination | 10.696° |
Longitude of ascending node | 211.792° |
Argument of perihelion | 177.281° |
| Physical characteristics | |
| Dimensions | 80.58±1.4 km |
Synodic rotation period | 14.911 h (0.6213 d) |
Geometric albedo | 0.0553±0.002 |
Spectral type | C |
Absolute magnitude (H) | 9.23 |
Efforts to determine the rotation period for this asteroid have produced wildly different results, in large part because the actual period is close to half of an Earth day. A study performed during 2013 showed that the light curve changed significantly during the observation period, adding to the difficulty. This study gave a synodic rotation period of 14.905 ± 0.001 h.[3]
| |
|---|---|
|
Small Solar System bodies | |||||||
|---|---|---|---|---|---|---|---|
| Minor planets |
| ||||||
| Comets |
| ||||||
| Other |
| ||||||
This article about a C-type asteroid native to the asteroid belt is a stub. You can help Wikipedia by expanding it. |