101430 (1998 VE32) is a mid-sized asteroid with an orbit that crosses the orbit of Mars. NASA JPL has not classified 1998 VE32 as potentially hazardous because its orbit does not bring it close to Earth.
1998 VE32 orbits the sun every 924 days (2.53 years), coming as close as 1.32 AU and reaching as far as 2.40 AU from the sun. Based on its brightness and the way it reflects light, 1998 VE32 is probably between 2.180 to 4.876 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to Mount Everest.
The rotation of 1998 VE32 has been observed. It completes a rotation on its axis every 40.66 hours.
1998 VE32's orbit is 0.52 AU from Earth's orbit at its closest point. This means that there is a very 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.
1998 VE32's orbit is determined by observations dating back to Jan. 4, 1951. It was last officially observed on July 4, 2023. The IAU Minor Planet Center records 1,432 observations used to determine its orbit.
The position of 101430 (1998 VE32) 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 1998 VE32 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.