Key Facts

Overview

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

Misterrogers orbits the sun every 1,310 days (3.59 years), coming as close as 1.53 AU and reaching as far as 3.15 AU from the sun. Misterrogers is about 6.3 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.

The rotation of Misterrogers has been observed. It completes a rotation on its axis every 8.07 hours.

No Close Approaches

Misterrogers's orbit is 0.66 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

Misterrogers's orbit is determined by observations dating back to Sept. 25, 1952. It was last officially observed on May 7, 2023. The IAU Minor Planet Center records 2,877 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 Misterrogers:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.341 AU
  • Eccentricity: 0.3451
  • Inclination: 21.87°
  • Longitude of Ascending Node: 203.64°
  • Argument of Periapsis: 247.81°
  • Mean Anomaly: 244.73°

Physical Characteristics

  • Diameter: 6.33300 km
  • Magnitude: 13.0
  • Albedo: 0.282

Derived Characteristics

  • Orbit Period: 1,310 days (3.59 years)
  • Avg. Orbit Speed: 19.44 km/s
  • Aphelion Distance: 3.15 AU
  • Perihelion Distance: 1.53 AU
  • Rotation Period: 8.07 hours

Map Comparison

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Orbit Simulation

Sky Map

The position of Misterrogers 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 Misterrogers 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.