835 Olivia
835 Olivia is a dark background asteroid orbiting in the outer regions of the main asteroid belt between Mars and Jupiter. It carries the provisional designation A916 SH, and it belongs to the main belt's background population rather than any collisional asteroid family.
| Key fact | Detail |
|---|---|
| Distance from the Sun | Orbits at 2.9–3.5 AU, with a semi-major axis of 3.22 AU1 |
| Orbit shape | Eccentricity of 0.09 and an inclination of 4° with respect to the ecliptic2 |
| Earliest observation | Observation arc begins at Bergedorf Observatory on 30 September 1916, one week after the official discovery observation at Heidelberg2 |
| Hazard status | Not classified as potentially hazardous, because its orbit does not bring it close to Earth1 |
Orbit and classification
Olivia circles the Sun in the outer asteroid belt, at distances ranging from 2.9 to 3.5 AU. One AU, or astronomical unit, is the average Earth–Sun distance, so the asteroid travels between roughly two and three and a half times farther from the Sun than Earth does. Completing one orbit takes 5 years and 9 months, equivalent to 2,109 days, and its semi-major axis, the average of its closest and farthest orbital distances, is 3.22 AU. The orbit is nearly circular, with an eccentricity of 0.09, and tilted 4° to the plane of the Solar System (the ecliptic).2
When astronomers apply the hierarchical clustering method, a technique that groups asteroids with similar proper orbital elements to identify collisional families, Olivia falls outside every family.
Discovery and observation
The asteroid's official discovery observation was made at Heidelberg, and the earliest recorded observation in its arc comes from the Bergedorf Observatory on 30 September 1916, one week after that discovery.
Naming
The origin of the name Olivia is unknown.
Hazard status
JPL has not classified Olivia as a potentially hazardous asteroid, because its orbit does not bring it close to Earth. Potentially hazardous status is reserved for objects whose orbits approach Earth's closely enough to warrant monitoring.1
References
Topic: Encyclopedia › Places and geography › Extraterrestrial places › Small bodies of the Solar System › Main-belt asteroids and numbered minor planets › Outer-belt asteroids
Initially written Oct 20, 2026 · Edited: Oct 25, 2026
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