Key Facts

Overview

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

Takeshima orbits the sun every 1,280 days (3.50 years), coming as close as 2.20 AU and reaching as far as 2.42 AU from the sun. Takeshima is about 4.3 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the island of Manhattan.

The rotation of Takeshima has been observed. It completes a rotation on its axis every 1069.00 hours.

No Close Approaches

Takeshima's orbit is 1.21 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

Takeshima's orbit is determined by observations dating back to Oct. 18, 1966. It was last officially observed on Feb. 9, 2023. The IAU Minor Planet Center records 4,055 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 Takeshima:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.311 AU
  • Eccentricity: 0.0463
  • Inclination: 6.28°
  • Longitude of Ascending Node: 331.03°
  • Argument of Periapsis: 204.43°
  • Mean Anomaly: 275.2°

Physical Characteristics

  • Diameter: 4.30800 km
  • Magnitude: 13.84
  • Albedo: 0.416

Derived Characteristics

  • Orbit Period: 1,280 days (3.50 years)
  • Avg. Orbit Speed: 19.64 km/s
  • Aphelion Distance: 2.42 AU
  • Perihelion Distance: 2.20 AU
  • Rotation Period: 1,069.00 hours

Map Comparison

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Orbit Simulation

Sky Map

The position of Takeshima 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 Takeshima 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.