Kepler's First Law of Planetary Motion
Kepler's Second Law of Planetary Motion
Reduced Mass Coordinates: Isolated Two-body Problem
Kepler's Third Law of Planetary Motion
Gravitation Between Spherically Symmetric Masses
Circular Orbits and Critical Velocity for Satellites
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Updated: Apr 26, 2026

Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
Eric L N Jensen1, Rachel Akeson2
1Department of Physics and Astronomy, Swarthmore College, 500 College Avenue, Swarthmore, Pennsylvania 19081, USA.
Many giant planets have unusual orbits, possibly due to interactions with binary stars. We found significant disk misalignment in the HK Tauri binary system, supporting this theory during planet formation.
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