Sequoia is a mid-sized asteroid orbiting between Mars and Jupiter within the inner portion of the asteroid belt. NASA JPL has not classified Sequoia as potentially hazardous because its orbit does not bring it close to Earth.
Sequoia orbits the sun every 982 days (2.69 years), coming as close as 1.75 AU and reaching as far as 2.12 AU from the sun. Sequoia is about 6.7 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.
The rotation of Sequoia has been observed. It completes a rotation on its axis every 3.04 days.
Sequoia's orbit is 0.81 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.
Sequoia's orbit is determined by observations dating back to Dec. 30, 1928. It was last officially observed on Feb. 4, 2020. The IAU Minor Planet Center records 2,094 observations used to determine its orbit.
Scientists have been able to determine this object's shape.
View asteroid Sequoia in 3D.
The position of Sequoia 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.