494658 (2000 UG11) is a very small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2000 UG11 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2000 UG11 orbits the sun every 979 days (2.68 years), coming as close as 0.83 AU and reaching as far as 3.03 AU from the sun. Based on its brightness and the way it reflects light, 2000 UG11 is probably between 0.192 to 0.429 kilometers in diameter, making it a small to average asteroid, very roughly comparable in size to a football field.
The rotation of 2000 UG11 has been observed. It completes a rotation on its axis every 4.44 hours.
2000 UG11's orbit is 0.01 AU from Earth's orbit at its closest point. This means that its orbit is relatively close to Earth's orbit.
2000 UG11 has 7 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
March 12, 2025 | 23,201,947 | 15.642 |
Nov. 3, 2067 | 12,151,677 | 16.191 |
Nov. 20, 2075 | 12,932,450 | 11.621 |
March 4, 2092 | 19,846,695 | 12.526 |
Nov. 12, 2142 | 2,982,772 | 13.558 |
March 8, 2159 | 18,979,124 | 12.937 |
Nov. 2, 2193 | 17,862,677 | 17.178 |
2000 UG11's orbit is determined by observations dating back to Oct. 21, 2000. It was last officially observed on May 14, 2017. The IAU Minor Planet Center records 433 observations used to determine its orbit.
The position of 494658 (2000 UG11) is indicated by a ◯ pink circle. Note that the object may not be in your current field of view. Use the controls below to adjust position, location, and time.
The below comparison is an artistic rendering that uses available data on the diameter of 2000 UG11 to create an approximate landscape rendering with New York City in the background. This approximation is built for full-resolution desktop browsers. Shape, color, and texture of asteroid are imagined.