Key Facts

Overview

13811 (1998 XP92) is a large asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified 1998 XP92 as potentially hazardous because its orbit does not bring it close to Earth.

1998 XP92 orbits the sun every 1,920 days (5.26 years), coming as close as 2.66 AU and reaching as far as 3.38 AU from the sun. 1998 XP92 is about 12.1 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the city of Cleveland, Ohio.

No Close Approaches

1998 XP92's orbit is 1.67 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

1998 XP92's orbit is determined by observations dating back to Nov. 13, 1982. It was last officially observed on July 4, 2023. The IAU Minor Planet Center records 3,055 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 1998 XP92:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 3.021 AU
  • Eccentricity: 0.1203
  • Inclination: 9.7°
  • Longitude of Ascending Node: 237.99°
  • Argument of Periapsis: 149.55°
  • Mean Anomaly: 307.72°

Physical Characteristics

  • Diameter: 12.11800 km
  • Magnitude: 12.57
  • Albedo: 0.132

Derived Characteristics

  • Orbit Period: 1,920 days (5.26 years)
  • Avg. Orbit Speed: 17.12 km/s
  • Aphelion Distance: 3.38 AU
  • Perihelion Distance: 2.66 AU

Map Comparison

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Orbit Simulation

Sky Map

The position of 13811 (1998 XP92) 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.