13541 (1991 VP3)

Mid-sized Main-belt Asteroid

Space Reference » Main-belt Asteroids » 13541 (1991 VP3)

Key Facts

Overview

13541 (1991 VP3) is a mid-sized asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified 1991 VP3 as potentially hazardous because its orbit does not bring it close to Earth.

1991 VP3 orbits the sun every 1,330 days (3.64 years), coming as close as 2.15 AU and reaching as far as 2.58 AU from the sun. Based on its brightness and the way it reflects light, 1991 VP3 is probably between 3.737 to 8.357 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.

No Close Approaches

1991 VP3's orbit is 1.18 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

1991 VP3's orbit is determined by observations dating back to March 6, 1978. It was last officially observed on June 29, 2023. The IAU Minor Planet Center records 2,635 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 1991 VP3:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.366 AU
  • Eccentricity: 0.0925
  • Inclination: 7.87°
  • Longitude of Ascending Node: 49.46°
  • Argument of Periapsis: 81.72°
  • Mean Anomaly: 189.05°

Physical Characteristics

  • Diameter: ~4.825 km
  • Magnitude: 14.26

Derived Characteristics

  • Orbit Period: 1,330 days (3.64 years)
  • Avg. Orbit Speed: 19.35 km/s
  • Aphelion Distance: 2.58 AU
  • Perihelion Distance: 2.15 AU

Map Comparison

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Orbit Simulation

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Sky Map

The position of 13541 (1991 VP3) 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 1991 VP3 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.