An Introduction to Modern Astrophysics · Problem 1.9
Celestial Mechanics — Carroll & Ostlie
Physics — Astrophysics · precession-proper-motion
Problem
(a) Using the information in Problem 1.8, precess the coordinates of Proxima Centauri to epoch J2010.0.
(b) The proper motion of Proxima Centauri is 3.84′′yr−1 with the position angle 282∘. Calculate the change in α and δ due to proper motion between 2000.0 and 2010.0.
(c) Which effect makes the largest contribution to changes in the coordinates of Proxima Centauri: precession or proper motion?