Sormano

Key Facts

• Categorized as a Main-belt Asteroid
• Comparable in size to the San Francisco Bay (8.10 km diameter)
• Not a Near Earth Object
• Not a Potentially Hazardous Object
• See orbit simulation

Overview

Sormano is a mid-sized asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified Sormano as potentially hazardous because its orbit does not bring it close to Earth.

Sormano orbits the sun every 1,490 days (4.08 years), coming as close as 2.29 AU and reaching as far as 2.81 AU from the sun. Sormano is about 8.1 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.

The rotation of Sormano has been observed. It completes a rotation on its axis every 3.69 hours.

No Close Approaches

Sormano's orbit is 1.28 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.

Images and Observations

Sormano's orbit is determined by observations dating back to July 29, 1989. It was last officially observed on Feb. 19, 2023. The IAU Minor Planet Center records 2,965 observations used to determine its orbit.

Scientists have been able to determine this object's shape:

View asteroid Sormano in 3D.

Accessibility and Exploration

This asteroid is not considered a viable target for human exploration by the NHATS study.

Similar Objects

These objects have orbits that share similar characteristics to the orbit of Sormano:

• 29 Amphitrite (A854 EB)
• 89 Julia (A866 PA)
• 170 Maria (A877 AA)

References

• JPL Small Body Database
• Mission Design
• Sky Finder Chart

Orbit Simulation

Sky Map

The position of Sormano 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.