508967 (2004 VC17) is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2004 VC17 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2004 VC17 orbits the sun every 953 days (2.61 years), coming as close as 0.36 AU and reaching as far as 3.43 AU from the sun. Its orbit is highly elliptical. Based on its brightness and the way it reflects light, 2004 VC17 is probably between 0.533 to 1.191 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.
2004 VC17'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.
2004 VC17 has 5 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
Nov. 15, 2064 | 12,159,171 | 32.116 |
Nov. 3, 2098 | 29,582,398 | 24.220 |
Nov. 21, 2111 | 25,801,740 | 34.802 |
Nov. 10, 2145 | 11,269,294 | 27.863 |
Nov. 4, 2192 | 29,587,816 | 24.406 |
2004 VC17's orbit is determined by observations dating back to Nov. 7, 2004. It was last officially observed on March 25, 2020. The IAU Minor Planet Center records 409 observations used to determine its orbit.
The position of 508967 (2004 VC17) 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 2004 VC17 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.