Key Facts

Overview

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

Suzannehawley orbits the sun every 1,550 days (4.24 years), coming as close as 2.31 AU and reaching as far as 2.93 AU from the sun. Based on its brightness and the way it reflects light, Suzannehawley is probably between 1.441 to 3.221 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to Mount Everest.

No Close Approaches

Suzannehawley's orbit is 1.35 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

Suzannehawley's orbit is determined by observations dating back to Oct. 28, 2001. It was last officially observed on Dec. 15, 2022. The IAU Minor Planet Center records 334 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 Suzannehawley:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.619 AU
  • Eccentricity: 0.1173
  • Inclination: 13.37°
  • Longitude of Ascending Node: 166.32°
  • Argument of Periapsis: 311.0°
  • Mean Anomaly: 5.8°

Physical Characteristics

  • Diameter: ~1.860 km
  • Magnitude: 16.33

Derived Characteristics

  • Orbit Period: 1,550 days (4.24 years)
  • Avg. Orbit Speed: 18.38 km/s
  • Aphelion Distance: 2.93 AU
  • Perihelion Distance: 2.31 AU

Map Comparison

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Orbit Simulation

Sky Map

The position of Suzannehawley 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 Suzannehawley 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.