2011 EF17 is a very small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2011 EF17 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2011 EF17 orbits the sun every 1,310 days (3.59 years), coming as close as 0.60 AU and reaching as far as 4.08 AU from the sun. Its orbit is highly elliptical. Based on its brightness and the way it reflects light, 2011 EF17 is probably between 0.384 to 0.859 kilometers in diameter, making it larger than 90% of asteroids but tiny compared to large asteroids, very roughly comparable in size to the Golden Gate Bridge.
2011 EF17's orbit is 0.01 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.
2011 EF17 has 6 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
Sept. 24, 2072 | 25,105,353 | 17.469 |
April 4, 2083 | 17,588,123 | 25.473 |
April 9, 2126 | 11,565,494 | 23.966 |
Oct. 11, 2158 | 13,118,852 | 24.157 |
Oct. 8, 2176 | 5,839,239 | 22.244 |
April 12, 2187 | 7,745,165 | 22.685 |
2011 EF17's orbit is determined by observations dating back to March 5, 2011. It was last officially observed on Nov. 19, 2018. The IAU Minor Planet Center records 72 observations used to determine its orbit.
The position of 2011 EF17 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 below comparison is an artistic rendering that uses available data on the diameter of 2011 EF17 to create an approximate landscape rendering with New York City in the background. This approximation is built for full-resolution desktop browsers. Shape, color, and texture of asteroid are imagined.