2015 BO519 is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2015 BO519 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2015 BO519 orbits the sun every 2,490 days (6.82 years), coming as close as 0.53 AU and reaching as far as 6.66 AU from the sun. Its orbit is highly elliptical. Based on its brightness and the way it reflects light, 2015 BO519 is probably between 0.638 to 1.426 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.
2015 BO519's orbit is 0.02 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.
Orbital simulations conducted by NASA JPL's CNEOS do not show any close approaches to Earth.
2015 BO519's orbit is determined by observations dating back to Jan. 20, 2015. It was last officially observed on Jan. 23, 2015. The IAU Minor Planet Center records 16 observations used to determine its orbit.
The position of 2015 BO519 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 2015 BO519 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.