2012 AA11 is a very small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2012 AA11 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2012 AA11 orbits the sun every 1,020 days (2.79 years), coming as close as 1.02 AU and reaching as far as 2.94 AU from the sun. Based on its brightness and the way it reflects light, 2012 AA11 is probably between 0.249 to 0.557 kilometers in diameter, making it larger than 90% of asteroids but tiny compared to large asteroids, very roughly comparable in size to a football field.
The rotation of 2012 AA11 has been observed. It completes a rotation on its axis every 14.19 hours.
2012 AA11's orbit is 0.05 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.
2012 AA11 has 5 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
April 19, 2037 | 29,777,949 | 12.715 |
Feb. 22, 2076 | 16,383,217 | 7.848 |
Feb. 22, 2101 | 17,183,475 | 7.935 |
Feb. 8, 2126 | 28,550,241 | 10.878 |
April 10, 2187 | 13,205,226 | 9.148 |
2012 AA11's orbit is determined by observations dating back to Jan. 14, 2012. It was last officially observed on Nov. 26, 2022. The IAU Minor Planet Center records 718 observations used to determine its orbit.
The position of 2012 AA11 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 2012 AA11 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.