C/1885 X2 (Barnard) is a large comet with a trajectory through the solar system likely originating from the Oort Cloud. NASA JPL has not classified Barnard as potentially hazardous because its orbit does not bring it close to Earth.
Barnard orbits the sun every 0 days (0.00 years), coming as close as 0.48 AU and reaching as far as -4774.48 AU from the sun. Its orbit is highly elliptical. Based on its brightness and the way it reflects light, Barnard is probably between 2658.000 to 5943.469 kilometers in diameter, making it the largest asteroid/dwarf planet, very roughly comparable in size to the U.S. state of Alaska.
Barnard's orbit is 0.33 AU from Earth's orbit at its closest point. This means that there is an 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.
Barnard's orbit is determined by observations dating back to Dec. 5, 1885. It was last officially observed on May 4, 1886. The IAU Minor Planet Center records 56 observations used to determine its orbit.
The position of C/1885 X2 (Barnard) 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.