Key Facts

Overview

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

Veniamina orbits the sun every 1,630 days (4.46 years), coming as close as 2.14 AU and reaching as far as 3.29 AU from the sun. Veniamina is about 11.4 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the city of Cleveland, Ohio.

No Close Approaches

Veniamina's orbit is 1.17 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

Veniamina's orbit is determined by observations dating back to Oct. 9, 1958. It was last officially observed on June 8, 2023. The IAU Minor Planet Center records 2,676 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 Veniamina:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.715 AU
  • Eccentricity: 0.2112
  • Inclination: 8.01°
  • Longitude of Ascending Node: 180.44°
  • Argument of Periapsis: 262.7°
  • Mean Anomaly: 143.01°

Physical Characteristics

  • Diameter: 11.35300 km
  • Magnitude: 13.58
  • Albedo: 0.079

Derived Characteristics

  • Orbit Period: 1,630 days (4.46 years)
  • Avg. Orbit Speed: 18.12 km/s
  • Aphelion Distance: 3.29 AU
  • Perihelion Distance: 2.14 AU

Map Comparison

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Orbit Simulation

Sky Map

The position of Veniamina 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.