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Monthly Notices of the Royal Astronomical Society: Letters
The Kepler mission has discovered a plethora of multiple transiting planet candidate exosystems, many of which feature putative pairs of planets near mean motion resonance commensurabilities. Identifying potentially resonant systems could help guide future observations and enhance our understanding of planetary formation scenarios. We develop and apply an algebraic method to determine which Kepler 2-planet systems cannot be in a 1st-4th order resonance, given the current, publicly availabledoi:10.1111/j.1745-3933.2011.01185.x fatcat:xv7zgbi2t5h7vjqjyznk2ousgi