Key Facts

Overview

16886 (1998 BC26) is a mid-sized asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified 1998 BC26 as potentially hazardous because its orbit does not bring it close to Earth.

1998 BC26 orbits the sun every 1,370 days (3.75 years), coming as close as 1.98 AU and reaching as far as 2.85 AU from the sun. 1998 BC26 is about 6.1 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to the San Francisco Bay.

The rotation of 1998 BC26 has been observed. It completes a rotation on its axis every 5.99 hours.

No Close Approaches

1998 BC26's orbit is 0.99 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

1998 BC26's orbit is determined by observations dating back to Dec. 19, 1974. It was last officially observed on Dec. 13, 2022. The IAU Minor Planet Center records 2,960 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 1998 BC26:

References

Search

   or view a random object

Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.414 AU
  • Eccentricity: 0.1807
  • Inclination: 8.71°
  • Longitude of Ascending Node: 64.37°
  • Argument of Periapsis: 319.85°
  • Mean Anomaly: 37.31°

Physical Characteristics

  • Diameter: 6.06900 km
  • Magnitude: 13.2
  • Albedo: 0.282

Derived Characteristics

  • Orbit Period: 1,370 days (3.75 years)
  • Avg. Orbit Speed: 19.17 km/s
  • Aphelion Distance: 2.85 AU
  • Perihelion Distance: 1.98 AU
  • Rotation Period: 5.99 hours

Map Comparison

Click to load map

Orbit Simulation

Sky Map

The position of 16886 (1998 BC26) 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 1998 BC26 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.