Climenhaga is a mid-sized asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified Climenhaga as potentially hazardous because its orbit does not bring it close to Earth.
Climenhaga orbits the sun every 1,290 days (3.53 years), coming as close as 1.84 AU and reaching as far as 2.81 AU from the sun. Based on its brightness and the way it reflects light, Climenhaga is probably between 7.355 to 16.445 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.
The rotation of Climenhaga has been observed. It completes a rotation on its axis every 2.74 hours.
Climenhaga's orbit is 0.83 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.
Climenhaga's orbit is determined by observations dating back to Sept. 24, 1917. It was last officially observed on June 17, 2023. The IAU Minor Planet Center records 3,735 observations used to determine its orbit.
The position of Climenhaga 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.