What happens to a star when it runs out of hydrogen in its core? This
lecture describes the post main-sequence evolution of stars. What
happens depends on the star's mass. Low mass stars swell up into Red
Giants, and eventually shed their envelopes and end their lives as white
dwarf stars. High mass stars become Red Supergiants, and if large
enough, end ... Show More
Sep 2009
Lecture 2: Astronomical Numbers
An introduction and review of the basic notation and physical units we will be
using throughout this course. In particular, we will be using the
Metric (SI) system for lengths, masses, times, and temperatures, and
special astronomical units for distances (AU and Light Years) and ... Show More
43m 56s
Mar 2022
Comment calculer l'âge d'une étoile ?
La durée de vie d'une étoile peut nous renseigner sur sa composition et sur l'existence éventuelle de la vie dans le cosmos. mais, en dehors du Soleil, il est assez difficile de déterminer l'âge d'une étoile.
L'importance de la masse
En évaluant, grâce à la radioactivité, l'âge d ... Show More
1m 58s