Astronomy:878 Mildred
| Discovery [1][2] | |
|---|---|
| Discovered by | S. B. Nicholson H. Shapley |
| Discovery site | Mount Wilson Obs. |
| Discovery date | 6 September 1916 |
| Designations | |
| (878) Mildred | |
| 1916 f, 1985 VG6, 1991 GZ8 | |
| Minor planet category | main-belt Nysa [3] |
| Orbital characteristics [1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 99.57 yr (36368 days) |
| |{{{apsis}}}|helion}} | 2.8953 astronomical unit|AU (433.13 Gm) |
| |{{{apsis}}}|helion}} | 1.8286 AU (273.55 Gm) |
| 2.3619 AU (353.34 Gm) | |
| Eccentricity | 0.22580 |
| Orbital period | 3.63 yr (1325.9 d) |
| Mean anomaly | 198.89° |
| Mean motion | 0° 16m 17.472s / day |
| Inclination | 2.0648° |
| Longitude of ascending node | 172.83° |
| 190.14° | |
| Physical characteristics | |
| Dimensions | ~4 km[4] |
| Rotation period | 2.660 h (0.1108 d)[1] |
| S[3] | |
| Absolute magnitude (H) | 14.7[1] |
878 Mildred is a minor planet in the main belt orbiting the Sun. It is the lowest numbered, and thus the namesake, of the Mildred family of asteroids, a subgroup of the Nysa family.[3] The Mildred subgroup, and by extension 878 Mildred itself, is thought to have been formed by a recent fragmentation event from a larger asteroid.[3]
Discovery
878 Mildred was originally discovered in 1916 using the 1.5 m Hale Telescope at the Mount Wilson Observatory, but was subsequently lost until it was again observed on single nights in 1985 and 1991 (a lost asteroid).[2] Initially only two observations of the asteroid were taken on 1916-09-06 which does not allow for an accurate orbital determination, however interest in the object prompted further investigation and more measurements were taken in late September and October.[4] The asteroid was re-discovered in 1991 by Gareth V. Williams.[5] It is named after Mildred Shapley Matthews.
Physical properties
By comparing the asteroid's perceived brightness and the then computed distance from the Sun they arrived at an absolute visual magnitude of 14.3, which if one assumes Mars-like albedo gives an approximate diameter of 3 to 5 kilometers.[4]
References
- ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 878 Mildred (1916 f)". https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=878+Mildred#content.
- ↑ 2.0 2.1 IAU Circular: IAUC 5275 (Report). IAU. 1991-05-25. http://www.cbat.eps.harvard.edu/iauc/05200/05275.html. Retrieved 2020-02-20.
- ↑ 3.0 3.1 3.2 3.3 Cellino, A. (August 2001). "The Puzzling Case of the Nysa–Polana Family". Icarus 152 (2): 225–237. doi:10.1006/icar.2001.6634. Bibcode: 2001Icar..152..225C.
- ↑ 4.0 4.1 4.2 Shapley, H.; Nicholson, S. B. (1917). "The Orbit and Probable Size of a Very Faint Asteroid (878) Mildred". Astronomical Journal 30 (710): 127–128. doi:10.1086/104199. Bibcode: 1917AJ.....30..127S.
- ↑ "MPC staff - Gareth Williams". International Astronomical Union. https://www.minorplanetcenter.net/about.
External links
- Minor Planet Center Database entry on (878) Mildred
- 878 Mildred at AstDyS-2, Asteroids—Dynamic Site
- 878 Mildred at the JPL Small-Body Database
 |  |
