21374 (1997 WS22) is a mid-sized asteroid whose orbit approaches the orbit of Earth but does not cross it. NASA JPL has classified 1997 WS22 as a "Near Earth Asteroid" due to its orbit's proximity to Earth, but it is not considered potentially hazardous because computer simulations have not indicated any imminent likelihood of future collision.
1997 WS22 orbits the sun every 522 days (1.43 years), coming as close as 1.12 AU and reaching as far as 1.42 AU from the sun. Based on its brightness and the way it reflects light, 1997 WS22 is probably between 0.852 to 1.906 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the Golden Gate Bridge.
The rotation of 1997 WS22 has been observed. It completes a rotation on its axis every 3.41 hours.
1997 WS22's orbit is 0.11 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.
1997 WS22 has 7 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
May 21, 2024 | 16,527,326 | 12.314 |
May 22, 2034 | 21,051,540 | 12.315 |
May 21, 2097 | 28,755,940 | 13.296 |
May 23, 2107 | 19,900,958 | 12.674 |
May 22, 2117 | 16,402,035 | 12.359 |
May 23, 2127 | 19,283,797 | 12.283 |
May 23, 2137 | 27,514,663 | 12.479 |
1997 WS22's orbit is determined by observations dating back to Sept. 22, 1974. It was last officially observed on July 1, 2021. The IAU Minor Planet Center records 1,352 observations used to determine its orbit.
The position of 21374 (1997 WS22) 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 1997 WS22 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.