Dorrit is a mid-sized asteroid with an orbit that crosses the orbit of Mars. NASA JPL has not classified Dorrit as potentially hazardous because its orbit does not bring it close to Earth.
Dorrit orbits the sun every 970 days (2.66 years), coming as close as 1.52 AU and reaching as far as 2.31 AU from the sun. Based on its brightness and the way it reflects light, Dorrit is probably between 5.255 to 11.750 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.
The rotation of Dorrit has been observed. It completes a rotation on its axis every 2.57 hours.
Dorrit's spectral type None (Tholen) / Sa (SMASSII) indicates that it is likely to contain and .
Dorrit's orbit is 0.62 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.
Dorrit's orbit is determined by observations dating back to Nov. 8, 1931. It was last officially observed on June 30, 2023. The IAU Minor Planet Center records 3,909 observations used to determine its orbit.
The position of Dorrit 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 Dorrit 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.