Key Facts


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

Smetana orbits the sun every 935 days (2.56 years), coming as close as 1.87 AU and reaching as far as 1.88 AU from the sun. Smetana is about 3.1 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the island of Manhattan.

The rotation of Smetana has been observed. It completes a rotation on its axis every 2.50 hours.

No Close Approaches

Smetana's orbit is 0.87 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

Smetana's orbit is determined by observations dating back to Oct. 26, 1971. It was last officially observed on Feb. 19, 2023. The IAU Minor Planet Center records 3,272 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 Smetana:



   or view a random object

Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 1.872 AU
  • Eccentricity: 0.0035
  • Inclination: 25.28°
  • Longitude of Ascending Node: 36.58°
  • Argument of Periapsis: 301.91°
  • Mean Anomaly: 148.92°

Physical Characteristics

  • Diameter: 3.13100 km
  • Magnitude: 14.1
  • Albedo: 0.544

Derived Characteristics

  • Orbit Period: 935 days (2.56 years)
  • Avg. Orbit Speed: 21.78 km/s
  • Aphelion Distance: 1.88 AU
  • Perihelion Distance: 1.87 AU
  • Rotation Period: 2.50 hours

Map Comparison

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Orbit Simulation

Sky Map

The position of Smetana 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 Smetana 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.