Glarona

Key Facts

• Categorized as a Main-belt Asteroid
• Comparable in size to the city of Houston (37.85 km diameter)
• Not a Near Earth Object
• Not a Potentially Hazardous Object
• See orbit simulation

Overview

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

Glarona orbits the sun every 2,060 days (5.64 years), coming as close as 2.63 AU and reaching as far as 3.70 AU from the sun. Glarona is about 37.9 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the city of Houston.

The rotation of Glarona has been observed. It completes a rotation on its axis every 6.50 hours.

No Close Approaches

Glarona's orbit is 1.64 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

Glarona's orbit is determined by observations dating back to Oct. 17, 1909. It was last officially observed on June 2, 2023. The IAU Minor Planet Center records 4,290 observations used to determine its orbit.

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

View asteroid Glarona 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 Glarona:

• 31 Euphrosyne (A854 RA)
• 199 Byblis (A879 NA)
• 227 Philosophia (A882 PA)

References

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

Orbit Simulation

Sky Map

The position of Glarona 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.