Sobolev

Key Facts

• Categorized as a Main-belt Asteroid
• Comparable in size to the city of Philadelphia (18.60 km diameter)
• Not a Near Earth Object
• Not a Potentially Hazardous Object
• See orbit simulation

Overview

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

Sobolev orbits the sun every 1,900 days (5.20 years), coming as close as 2.73 AU and reaching as far as 3.27 AU from the sun. Sobolev is about 18.6 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the city of Philadelphia.

The rotation of Sobolev has been observed. It completes a rotation on its axis every 4.75 hours.

No Close Approaches

Sobolev'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.

Images and Observations

Sobolev's orbit is determined by observations dating back to Aug. 21, 1930. It was last officially observed on June 17, 2023. The IAU Minor Planet Center records 4,245 observations used to determine its orbit.

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

View asteroid Sobolev 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 Sobolev:

• 35 Leukothea (A855 HA)
• 256 Walpurga (A886 GA)
• 271 Penthesilea (A887 TB)

References

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

Orbit Simulation

Sky Map

The position of Sobolev 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.