154278 (2002 TB9) is a mid-sized asteroid whose orbit crosses the orbit of Earth. NASA JPL has classified 2002 TB9 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.
2002 TB9 orbits the sun every 885 days (2.42 years), coming as close as 0.74 AU and reaching as far as 2.87 AU from the sun. Based on its brightness and the way it reflects light, 2002 TB9 is probably between 1.290 to 2.884 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to Mount Everest.
The rotation of 2002 TB9 has been observed. It completes a rotation on its axis every 7.85 hours.
2002 TB9's orbit is 0.19 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.
2002 TB9 has 3 close approaches predicted in the coming decades:
Date | Distance from Earth (km) | Velocity (km/s) |
---|---|---|
April 19, 2054 | 28,084,505 | 22.818 |
April 19, 2117 | 27,733,912 | 22.846 |
April 17, 2180 | 27,376,757 | 22.734 |
2002 TB9's orbit is determined by observations dating back to May 16, 1991. It was last officially observed on July 27, 2023. The IAU Minor Planet Center records 691 observations used to determine its orbit.
The position of 154278 (2002 TB9) 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 2002 TB9 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.