2011 DO is a very small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2011 DO as a "Near Earth Asteroid" due to its orbit's proximity to Earth, but it is not considered potentially hazardous because computer simulations have not indicated any imminent likelihood of future collision.
2011 DO orbits the sun every 524 days (1.43 years), coming as close as 0.69 AU and reaching as far as 1.85 AU from the sun. Based on its brightness and the way it reflects light, 2011 DO is probably between 0.073 to 0.164 kilometers in diameter, making it a small to average asteroid, very roughly comparable in size to a school bus or smaller.
2011 DO's orbit is 0.04 AU from Earth's orbit at its closest point. This means that there is an wide berth between this asteroid and Earth at all times.
2011 DO has 6 close approaches predicted in the coming decades:
|Date||Distance from Earth (km)||Velocity (km/s)|
|Feb. 8, 2077||26,802,539||11.291|
|Aug. 31, 2079||19,373,492||12.537|
|Feb. 22, 2087||24,390,082||19.660|
|Feb. 10, 2146||22,455,851||11.951|
|Sept. 6, 2148||27,172,493||11.515|
|Aug. 12, 2161||29,397,409||20.524|
2011 DO's orbit is determined by observations dating back to Feb. 23, 2011. It was last officially observed on March 11, 2011. The IAU Minor Planet Center records 60 observations used to determine its orbit.
The position of 2011 DO 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 2011 DO 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.