1453 Fennia
| Discovery | |
|---|---|
| Discovered by | Vaisala, Y. |
| Discovery site | Turku |
| Discovery date | 8 March 1938 |
| Designations | |
| MPC designation | 1453 |
Named after | Finland |
| 1938 ED1 | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 78.04 yr (28504 days) |
| Aphelion | 1.9508111 AU (291.83719 Gm) |
| Perihelion | 1.8436697 AU (275.80906 Gm) |
| 1.897240 AU (283.8231 Gm) | |
| Eccentricity | 0.0282361 |
| 2.61 yr (954.51 d) | |
| 282.31178° | |
| 0° 22m 37.76s / day | |
| Inclination | 23.67528° |
| 7.090332° | |
| 254.44215° | |
| Earth MOID | 0.876603 AU (131.1379 Gm) |
| Jupiter MOID | 3.04724 AU (455.861 Gm) |
| Jupiter Tisserand parameter | 3.848 |
| Physical characteristics | |
Mean radius | 3.615±0.2 km |
| 4.4121 h (0.18384 d) | |
| 0.2494±0.032 | |
| 12.5 | |
|
| |
1453 Fennia (provisional designation: 1938 ED1) is an inner main belt asteroid. It was discovered on March 8, 1938, by the Finnish astronomer Yrjö Väisälä at Iso-Heikkilä Observatory in Turku, Finland. The asteroid's name is the Latin word for Finland.[2]
In 2007, a team of astronomers made photometric observations of Fennia, and discovered that it is orbited by a moon. The moon is at least a quarter the size of Fennia itself, and has an orbital period of approximately 23 hours. The team also found that Fennia has a rotation period of 4.4 hours and is likely spheroidal in shape.[3]
References
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