2010 CB19 is a very small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2010 CB19 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.
2010 CB19 orbits the sun every 380 days (1.04 years), coming as close as 0.71 AU and reaching as far as 1.34 AU from the sun. Based on its brightness and the way it reflects light, 2010 CB19 is probably between 0.022 to 0.098 kilometers in diameter, making it a small to average asteroid, very roughly comparable in size to a school bus or smaller.
2010 CB19's orbit is 0.00 AU from Earth's orbit at its closest point. This means that its orbit is relatively close to Earth's orbit.
2010 CB19 has 6 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
July 8, 2030 | 23,982,571 | 13.982 |
July 22, 2031 | 15,116,895 | 7.243 |
Feb. 6, 2036 | 6,941,656 | 8.412 |
Feb. 15, 2037 | 29,558,292 | 15.521 |
July 12, 2057 | 12,320,361 | 11.482 |
Feb. 7, 2063 | 485,425 | 9.821 |
2010 CB19's orbit is determined by observations dating back to Feb. 13, 2010. It was last officially observed on March 4, 2010. The IAU Minor Planet Center records 36 observations used to determine its orbit.
2010 CB19 can be reached with a journey of 394 days. This trajectory would require a delta-v of 11.065 km/s. To put this into perspective, the delta-v to launch a rocket to Low-Earth Orbit is 9.7 km/s. There are 518 potential trajectories and launch windows to this asteroid.
See more at the NHATS Mission Trajectories table for 2010 CB19.
The position of 2010 CB19 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 2010 CB19 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.