On the Origin of the 3:2 Almost Resonance Between the Two Earth-like Planets Orbiting Pulsar PSR 1257 + 12

Details On the Origin of the 3:2 Almost Resonance Between the Two Earth-like Planets Orbiting Pulsar PSR 1257 + 12 On the Origin of the 3:2 Almost Resonance Between the Two Earth-like Planets Orbiting Pulsar PSR 1257 + 12

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1120m&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1120

Computer Science

Scientific paper

We suggest that the 3:2 near-resonance between the two more massive
planets orbiting pulsar PSR1257 + 12 might be a consequence of two
independent resonances (2:1 and 3:1) with a low--mass stellar companion,
now completely evaporated.

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