2017 HT2 is a small asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2017 HT2 as a "Potentially Hazardous Asteroid" due to its predicted close pass(es) with Earth.
2017 HT2 orbits the sun every 1,260 days (3.45 years), coming as close as 1.00 AU and reaching as far as 3.57 AU from the sun. Based on its brightness and the way it reflects light, 2017 HT2 is probably between 0.563 to 1.259 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 HT2's orbit is 0.01 AU from Earth's orbit at its closest point. This means that its orbit is relatively close to Earth's orbit.
2017 HT2 has 6 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
Aug. 23, 2031 | 25,013,751 | 11.796 |
July 6, 2069 | 15,746,786 | 14.065 |
Aug. 13, 2100 | 18,749,512 | 11.064 |
July 16, 2138 | 3,421,339 | 12.429 |
Sept. 2, 2162 | 29,547,718 | 12.075 |
July 8, 2193 | 13,356,448 | 13.821 |
2017 HT2's orbit is determined by observations dating back to Jan. 17, 2015. It was last officially observed on Dec. 1, 2021. The IAU Minor Planet Center records 86 observations used to determine its orbit.
The position of 2017 HT2 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 HT2 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.