495190 (2012 VS113) is a large asteroid whose orbit extends beyond the orbit of Neptune. NASA JPL has not classified 2012 VS113 as potentially hazardous because its orbit does not bring it close to Earth.
2012 VS113 orbits the sun every 152,000 days (416.15 years), coming as close as 38.05 AU and reaching as far as 73.43 AU from the sun. Based on its brightness and the way it reflects light, 2012 VS113 is probably between 98.300 to 219.806 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the U.S. state of Connecticut.
2012 VS113's orbit is 37.10 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.
2012 VS113's orbit is determined by observations dating back to Dec. 22, 2008. It was last officially observed on Dec. 23, 2017. The IAU Minor Planet Center records 227 observations used to determine its orbit.
The position of 495190 (2012 VS113) 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.