Berenike is a large asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified Berenike as potentially hazardous because its orbit does not bring it close to Earth.
Berenike orbits the sun every 1,910 days (5.23 years), coming as close as 2.88 AU and reaching as far as 3.15 AU from the sun. Berenike is about 49.8 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the U.S. state of Rhode Island.
The rotation of Berenike has been observed. It completes a rotation on its axis every 12.49 hours.
Berenike's spectral type S (Tholen) / K (SMASSII) indicates that it is likely to contain water, iron, nickel, cobalt, nitrogen, and ammonia.
Berenike's orbit is 1.90 AU from Earth's orbit at its closest point. This means that there is an extremely 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.
Berenike's orbit is determined by observations dating back to Jan. 13, 1893. It was last officially observed on April 1, 2023. The IAU Minor Planet Center records 5,638 observations used to determine its orbit.
The position of Berenike 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.