417211 (2005 XL80) is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2005 XL80 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2005 XL80 orbits the sun every 829 days (2.27 years), coming as close as 0.89 AU and reaching as far as 2.57 AU from the sun. Based on its brightness and the way it reflects light, 2005 XL80 is probably between 0.595 to 1.331 kilometers in diameter, making it larger than ~97% of asteroids but small compared to large asteroids, very roughly comparable in size to the Golden Gate Bridge.
2005 XL80's orbit is 0.04 AU from Earth's orbit at its closest point. This means that there is a wide berth between this asteroid and Earth at all times.
2005 XL80 has 9 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
May 3, 2040 | 16,087,784 | 10.478 |
Feb. 22, 2065 | 27,851,976 | 11.207 |
May 25, 2074 | 6,654,980 | 11.973 |
April 7, 2099 | 24,018,651 | 10.456 |
June 12, 2108 | 26,278,237 | 16.275 |
May 17, 2133 | 10,278,946 | 10.940 |
Feb. 27, 2158 | 27,602,346 | 11.015 |
May 26, 2167 | 7,111,933 | 11.851 |
March 20, 2192 | 26,009,845 | 10.318 |
2005 XL80's orbit is determined by observations dating back to Dec. 8, 2005. It was last officially observed on Oct. 16, 2022. The IAU Minor Planet Center records 346 observations used to determine its orbit.
The position of 417211 (2005 XL80) 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 above comparison is an artistic rendering that uses available data on the diameter of 2005 XL80 to create an approximate landscape rendering with Mount Everest in the background. This approximation is built for full-resolution desktop browsers. Shape, color, and texture of asteroid are imagined.