2015 BS16 is a small asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified 2015 BS16 as potentially hazardous because its orbit does not bring it close to Earth.
2015 BS16 orbits the sun every 1,330 days (3.64 years), coming as close as 2.05 AU and reaching as far as 2.67 AU from the sun. Based on its brightness and the way it reflects light, 2015 BS16 is probably between 0.612 to 1.368 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 BS16's orbit is 1.07 AU from Earth's orbit at its closest point. This means that there is an extremely 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 BS16's orbit is determined by observations dating back to April 5, 1997. It was last officially observed on June 17, 2023. The IAU Minor Planet Center records 168 observations used to determine its orbit.
The position of 2015 BS16 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 BS16 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.