Riema is a mid-sized asteroid orbiting between Mars and Jupiter within the inner portion of the asteroid belt. NASA JPL has not classified Riema as potentially hazardous because its orbit does not bring it close to Earth.
Riema orbits the sun every 1,020 days (2.79 years), coming as close as 1.90 AU and reaching as far as 2.06 AU from the sun. Riema is about 4.6 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.
The rotation of Riema has been observed. It completes a rotation on its axis every 3.59 hours.
Riema's spectral type E (Tholen) / Xe (SMASSII) indicates that it is likely to contain iron, nickel, and cobalt.
Riema's orbit is 0.91 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.
Riema's orbit is determined by observations dating back to Aug. 13, 1923. It was last officially observed on May 25, 2022. The IAU Minor Planet Center records 3,482 observations used to determine its orbit.
The position of Riema 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 Riema 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.