The 55 Cancri planetary system: fully self-consistent N-body constraints and a dynamical analysis
Type
Publication
MNRAS
![[ An illustration of the orbital distances and relative sizes of the four innermost planets known to orbit the star 55 Cancri A (bottom) in comparison with planets in own inner Solar System (top). Both Jupiter and the Jupiter-mass planet 55 Cancri d are outside this picture, orbiting their host star with a distance of nearly 5 astronomical units (au), where one au is equal to the average between earth and sun. Credit: Center for Exoplanets Habitable Worlds, Penn State University ]](../../img/outreach_files/image_preview(1))
Press Coverage
- The 55 Cancri Planetary System: Fully Self-Consistent N-body Constraints and a Dynamical Analysis
- Solved: Mysteries of a Nearby Planetary System's Dynamics: Penn State pres release, April 22, 2014
- Mysteries of a nearby planetary systems dynamics now are solved: Astronomy Magazine, April 22, 2014
- Mysteries of Nearby Planetary Systems Dynamics: Astrobiology Magazine, April 23, 2014
