Other Worlds
Other planets
Planets around the neutron star PSR B1257+12
(A. Wolszczan, Penn State University)
- PSR B1257+12 has three planets on 25, 66, 98-day, nearly coplanar orbits,
with masses of 0.02, 3.9 and 4.2 M
- All three orbits almost fit within the orbit of Mercury
- Relative separations of the orbits are to sale wih those of Mercury,
Venus and Earth
- Planets B and C are in a near 3:2 mean motion resonance
- The system is dynamically stable over > 1 Gyr timescale
previous next