450894 (2008 BT18) is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2008 BT18 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2008 BT18 orbits the sun every 1,210 days (3.31 years), coming as close as 0.90 AU and reaching as far as 3.54 AU from the sun. Based on its brightness and the way it reflects light, 2008 BT18 is probably between 0.617 to 1.381 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.
The rotation of 2008 BT18 has been observed. It completes a rotation on its axis every 2.57 hours.
2008 BT18's orbit is 0.01 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.
2008 BT18 has 7 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
July 31, 2051 | 27,976,223 | 18.013 |
June 17, 2061 | 17,842,767 | 11.083 |
July 30, 2094 | 23,663,386 | 17.393 |
June 26, 2104 | 13,585,497 | 11.037 |
April 8, 2114 | 25,854,272 | 14.702 |
June 30, 2147 | 13,528,035 | 11.360 |
May 29, 2190 | 21,460,472 | 11.114 |
2008 BT18's orbit is determined by observations dating back to March 14, 1955. It was last officially observed on Jan. 15, 2021. The IAU Minor Planet Center records 435 observations used to determine its orbit.
The position of 450894 (2008 BT18) 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 2008 BT18 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.