Original: It is a retrograde rotator, although its pole points almost parallel to the ecliptic towards ecliptic coordinates (Î, Î ") = (-15 Â, 253 Â) with a 10 Â uncertainty.
Simplified: It is a retrograde rotator, although its pole points almost parallel to the ecliptic towards ecliptic coordinates (Î, Î ") = (-15 Â, 235 Â) with a 10 Â uncertainty (2).