127535 (2002 XL14)

Key Facts

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

Overview

127535 (2002 XL14) is a mid-sized asteroid with an orbit that crosses the orbit of Mars. NASA JPL has not classified 2002 XL14 as potentially hazardous because its orbit does not bring it close to Earth.

2002 XL14 orbits the sun every 1,160 days (3.18 years), coming as close as 1.60 AU and reaching as far as 2.71 AU from the sun. Based on its brightness and the way it reflects light, 2002 XL14 is probably between 1.226 to 2.742 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to Mount Everest.

No Close Approaches

2002 XL14's orbit is 0.61 AU from Earth's orbit at its closest point. This means that there is a 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.

Images and Observations

2002 XL14's orbit is determined by observations dating back to Dec. 8, 1996. It was last officially observed on April 28, 2023. The IAU Minor Planet Center records 558 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 2002 XL14:

• 1818 Brahms (1939 PE)
• 1917 Cuyo (1968 AA)
• 1988 Delores (1952 SV)

References

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

Orbit Simulation

Sky Map

The position of 127535 (2002 XL14) 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 2002 XL14 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.