2017 VV14 is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2017 VV14 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2017 VV14 orbits the sun every 1,220 days (3.34 years), coming as close as 0.35 AU and reaching as far as 4.13 AU from the sun. Its orbit is highly elliptical. Based on its brightness and the way it reflects light, 2017 VV14 is probably between 0.555 to 1.242 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.
2017 VV14's orbit is 0.05 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.
2017 VV14 has 4 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
Nov. 29, 2057 | 6,591,512 | 29.771 |
Nov. 24, 2114 | 24,784,831 | 25.585 |
Dec. 7, 2124 | 19,384,302 | 34.255 |
April 10, 2188 | 26,042,072 | 30.574 |
2017 VV14's orbit is determined by observations dating back to Jan. 31, 2017. It was last officially observed on Feb. 11, 2021. The IAU Minor Planet Center records 94 observations used to determine its orbit.
The position of 2017 VV14 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 2017 VV14 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.