Eckert is a mid-sized asteroid with an orbit that crosses the orbit of Mars. NASA JPL has not classified Eckert as potentially hazardous because its orbit does not bring it close to Earth.
Eckert orbits the sun every 977 days (2.67 years), coming as close as 1.59 AU and reaching as far as 2.26 AU from the sun. Based on its brightness and the way it reflects light, Eckert is probably between 4.023 to 8.996 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.
The rotation of Eckert has been observed. It completes a rotation on its axis every 375.00 days.
Eckert's orbit is 0.69 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.
Eckert's orbit is determined by observations dating back to July 15, 1950. It was last officially observed on Sept. 15, 2019. The IAU Minor Planet Center records 3,136 observations used to determine its orbit.
Scientists have been able to determine this object's shape.
View asteroid Eckert in 3D.
The position of Eckert 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.