SP-436 Project Orion: A Design Study of a System for Detecting
Extrasolar Planets
Figure 4. Maximum angular displacement () of a star due to a Jovian mass
companion shown as a function of its distance (D) from an observer.
Present level of observational accuracy indicated by dashed line;
various slanting lines refer to differing values of
Rp/M*.
) of a star due to a Jovian mass
companion shown as a function of its distance (D) from an observer.
Present level of observational accuracy indicated by dashed line;
various slanting lines refer to differing values of
Rp/M*.