505657 (2014 SR339) is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2014 SR339 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2014 SR339 orbits the sun every 541 days (1.48 years), coming as close as 0.90 AU and reaching as far as 1.70 AU from the sun. 2014 SR339 is about 1.0 kilometers in diameter, making it larger than ~97% of asteroids but small compared to large asteroids, comparable in size to the Golden Gate Bridge.
The rotation of 2014 SR339 has been observed. It completes a rotation on its axis every 8.71 hours.
2014 SR339's orbit is 0.03 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.
2014 SR339 has 7 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
Jan. 30, 2021 | 29,074,397 | 15.925 |
Feb. 5, 2058 | 6,335,085 | 17.136 |
Feb. 8, 2095 | 7,643,357 | 17.869 |
Jan. 30, 2098 | 29,590,021 | 15.935 |
Feb. 7, 2135 | 5,726,132 | 17.223 |
Feb. 12, 2172 | 15,641,447 | 18.739 |
Feb. 3, 2175 | 20,856,201 | 16.205 |
2014 SR339's orbit is determined by observations dating back to Sept. 30, 2014. It was last officially observed on July 29, 2023. The IAU Minor Planet Center records 1,474 observations used to determine its orbit.
The position of 505657 (2014 SR339) 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 2014 SR339 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.