17409 (1988 BA4) is a mid-sized asteroid orbiting between Mars and Jupiter in the main portion of the asteroid belt. NASA JPL has not classified 1988 BA4 as potentially hazardous because its orbit does not bring it close to Earth.
1988 BA4 orbits the sun every 1,280 days (3.50 years), coming as close as 2.20 AU and reaching as far as 2.41 AU from the sun. 1988 BA4 is about 2.5 kilometers in diameter, making it larger than 99% of asteroids, comparable in size to Mount Everest.
The rotation of 1988 BA4 has been observed. It completes a rotation on its axis every 3.85 hours.
1988 BA4's orbit is 1.22 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.
1988 BA4's orbit is determined by observations dating back to Oct. 2, 1986. It was last officially observed on June 5, 2023. The IAU Minor Planet Center records 2,659 observations used to determine its orbit.
The position of 17409 (1988 BA4) 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.
The above comparison is an artistic rendering that uses available data on the diameter of 1988 BA4 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.