Beckman is a mid-sized asteroid with an orbit that crosses the orbit of Mars. NASA JPL has not classified Beckman as potentially hazardous because its orbit does not bring it close to Earth.
Beckman orbits the sun every 1,360 days (3.72 years), coming as close as 1.45 AU and reaching as far as 3.36 AU from the sun. Beckman is about 7.0 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.
The rotation of Beckman has been observed. It completes a rotation on its axis every 3.12 hours.
Beckman's spectral type None (Tholen) / S (SMASSII) indicates that it is likely to contain and .
Beckman's orbit is 0.61 AU from Earth's orbit at its closest point. This means that there is a very wide berth between this asteroid and Earth at all times.
Orbital simulations conducted by NASA JPL's CNEOS do not show any close approaches to Earth.
Beckman's orbit is determined by observations dating back to Aug. 8, 1983. It was last officially observed on June 21, 2023. The IAU Minor Planet Center records 2,659 observations used to determine its orbit.
The position of Beckman 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.