Problem
Our Galaxy completes one full rotation in the galactic plane in about million years. The Sun is about from the galactic centre. Assuming a circular orbit and that most of the galactic mass is concentrated within the Sun’s orbit, estimate the order of magnitude of the Galaxy’s mass and comment on the comparison with the visible stellar mass ().
Solution
Setting up. We treat the Sun as a satellite in circular orbit around the mass enclosed within its orbital radius. Gravity provides the centripetal force; equivalently, we use Kepler’s third law:
Converting the period. With :
Numerical substitution. With and :
Comment. The visible stellar mass is , of the same order of magnitude as the dynamical mass estimated here within the Sun’s orbit. However, extending the same reasoning to more distant stars, rotation curves remain flat instead of declining: this requires much more non-luminous mass (dark matter) in the galactic halo. Kepler’s estimate is therefore only a lower bound on the Galaxy’s total mass.
Links
Topics: Gravitazione Concepts: Leggi di Keplero · Moto circolare uniforme · Legge di gravitazione universale · Forza centripeta Skills: Stime di Fermi · Impostazione simbolica