47035 (1998 WS) is a mid-sized asteroid with an orbit that crosses the orbit of Mars. NASA JPL has not classified 1998 WS as potentially hazardous because its orbit does not bring it close to Earth.
1998 WS orbits the sun every 1,580 days (4.33 years), coming as close as 1.61 AU and reaching as far as 3.70 AU from the sun. Based on its brightness and the way it reflects light, 1998 WS is probably between 6.991 to 15.633 kilometers in diameter, making it larger than 99% of asteroids, very roughly comparable in size to the San Francisco Bay.
The rotation of 1998 WS has been observed. It completes a rotation on its axis every 3.99 hours.
1998 WS's spectral type None (Tholen) / Sr (SMASSII) indicates that it is likely to contain and .
1998 WS's orbit is 0.84 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.
1998 WS's orbit is determined by observations dating back to Oct. 25, 1976. It was last officially observed on July 1, 2023. The IAU Minor Planet Center records 1,922 observations used to determine its orbit.
Scientists have been able to determine this object's shape:
View asteroid 47035 (1998 WS) in 3D.
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