2010 ST19

Key Facts

• Categorized as a Outer Main-belt Asteroid
• Comparable in size to Mount Everest
• Not a Near Earth Object
• Not a Potentially Hazardous Object
• See orbit simulation

Overview

2010 ST19 is a mid-sized asteroid that orbits between Mars and Jupiter in the outer reaches of the main asteroid belt. NASA JPL has not classified 2010 ST19 as potentially hazardous because its orbit does not bring it close to Earth.

2010 ST19 orbits the sun every 3,390 days (9.28 years), coming as close as 3.47 AU and reaching as far as 5.37 AU from the sun. Based on its brightness and the way it reflects light, 2010 ST19 is probably between 1.822 to 4.074 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to Mount Everest.

No Close Approaches

2010 ST19's orbit is 2.47 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

2010 ST19's orbit is determined by observations dating back to July 30, 2000. It was last officially observed on Jan. 31, 2022. The IAU Minor Planet Center records 77 observations used to determine its orbit.

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 2010 ST19:

• 2001 FW220
• 2009 VD78
• 2010 EL9

References

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

Orbit Simulation

Sky Map

The position of 2010 ST19 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.

Size Rendering

The above comparison is an artistic rendering that uses available data on the diameter of 2010 ST19 to create an approximate landscape rendering with Mount Everest in the background. This approximation is built for full-resolution desktop browsers. Shape, color, and texture of asteroid are imagined.