Davidgavine is a mid-sized asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified Davidgavine as potentially hazardous because its orbit does not bring it close to Earth.
Davidgavine orbits the sun every 1,770 days (4.85 years), coming as close as 2.71 AU and reaching as far as 3.01 AU from the sun. Based on its brightness and the way it reflects light, Davidgavine is probably between 5.788 to 12.943 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.
The rotation of Davidgavine has been observed. It completes a rotation on its axis every 2.87 hours.
Davidgavine's orbit is 1.72 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.
Davidgavine's orbit is determined by observations dating back to Dec. 22, 1954. It was last officially observed on June 5, 2023. The IAU Minor Planet Center records 3,271 observations used to determine its orbit.
The position of Davidgavine 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.