Key Facts

Overview

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

Bignonia orbits the sun every 1,890 days (5.17 years), coming as close as 2.74 AU and reaching as far as 3.25 AU from the sun. Based on its brightness and the way it reflects light, Bignonia is probably between 6.801 to 15.207 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.

No Close Approaches

Bignonia's orbit is 1.74 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

Bignonia's orbit is determined by observations dating back to Nov. 15, 1990. It was last officially observed on June 8, 2023. The IAU Minor Planet Center records 3,086 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 Bignonia:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.991 AU
  • Eccentricity: 0.0854
  • Inclination: 10.64°
  • Longitude of Ascending Node: 118.2°
  • Argument of Periapsis: 234.01°
  • Mean Anomaly: 187.61°

Physical Characteristics

  • Diameter: ~8.780 km
  • Magnitude: 12.96

Derived Characteristics

  • Orbit Period: 1,890 days (5.17 years)
  • Avg. Orbit Speed: 17.22 km/s
  • Aphelion Distance: 3.25 AU
  • Perihelion Distance: 2.74 AU

Map Comparison

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Orbit Simulation

Sky Map

The position of Bignonia 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.