Key Facts

Overview

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

Femariebustos orbits the sun every 1,770 days (4.85 years), coming as close as 2.38 AU and reaching as far as 3.35 AU from the sun. Femariebustos is about 7.1 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.

No Close Approaches

Femariebustos's orbit is 1.39 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

Femariebustos's orbit is determined by observations dating back to March 19, 1993. It was last officially observed on May 27, 2022. The IAU Minor Planet Center records 1,335 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 Femariebustos:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.864 AU
  • Eccentricity: 0.169
  • Inclination: 2.15°
  • Longitude of Ascending Node: 7.13°
  • Argument of Periapsis: 119.7°
  • Mean Anomaly: 143.94°

Physical Characteristics

  • Diameter: 7.07500 km
  • Magnitude: 15.05
  • Albedo: 0.056

Derived Characteristics

  • Orbit Period: 1,770 days (4.85 years)
  • Avg. Orbit Speed: 17.60 km/s
  • Aphelion Distance: 3.35 AU
  • Perihelion Distance: 2.38 AU

Map Comparison

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Orbit Simulation

Sky Map

The position of Femariebustos 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.