Lucretia is a large asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified Lucretia as potentially hazardous because its orbit does not bring it close to Earth.
Lucretia orbits the sun every 1,180 days (3.23 years), coming as close as 1.90 AU and reaching as far as 2.48 AU from the sun. Lucretia is about 11.0 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the city of Boston.
The rotation of Lucretia has been observed. It completes a rotation on its axis every 4.35 days.
Lucretia's orbit is 0.91 AU from Earth's orbit at its closest point. This means that there is an 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.
Lucretia's orbit is determined by observations dating back to April 16, 1890. It was last officially observed on June 1, 2020. The IAU Minor Planet Center records 3,263 observations used to determine its orbit.
Scientists have been able to determine this object's shape.
View asteroid Lucretia in 3D.
The position of Lucretia 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.