Key Facts

Overview

2019 OT44 is a small asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified 2019 OT44 as potentially hazardous because its orbit does not bring it close to Earth.

2019 OT44 orbits the sun every 1,770 days (4.85 years), coming as close as 2.65 AU and reaching as far as 3.08 AU from the sun. Based on its brightness and the way it reflects light, 2019 OT44 is probably between 0.690 to 1.542 kilometers in diameter, making it larger than ~97% of asteroids but small compared to large asteroids, very roughly comparable in size to the Golden Gate Bridge.

No Close Approaches

2019 OT44's orbit is 1.64 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

2019 OT44's orbit is determined by observations dating back to Sept. 22, 1995. It was last officially observed on May 16, 2023. The IAU Minor Planet Center records 30 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 2019 OT44:

References

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Orbital Elements

  • Epoch: 2460200.5 JD
  • Semi-major axis: 2.865 AU
  • Eccentricity: 0.0741
  • Inclination: 1.34°
  • Longitude of Ascending Node: 336.34°
  • Argument of Periapsis: 9.4°
  • Mean Anomaly: 283.82°

Physical Characteristics

  • Diameter: ~0.890 km
  • Magnitude: 17.93

Derived Characteristics

  • Orbit Period: 1,770 days (4.85 years)
  • Avg. Orbit Speed: 17.61 km/s
  • Aphelion Distance: 3.08 AU
  • Perihelion Distance: 2.65 AU

Map Comparison

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Orbit Simulation

Sky Map

The position of 2019 OT44 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 2019 OT44 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.