Astronomers learn by looking May 2006April 2004 Belinda Wilkes
Life Cycle of a Star The Sun: our nearest star May 2006April 2004 Belinda Wilkes
Stars have different colors B: blue – hottest A: green – warm C: red - cool What can we measure? May 2006April 2004 Belinda Wilkes
Color, Brightness + Count them May 2006April 2004 Belinda Wilkes
What makes the Sun Shine? May 2006April 2004 Belinda Wilkes
Where are Stars Born? Clusters: Pleiades May 2006April 2004 Belinda Wilkes
Stellar Nurseries Optical Infrared: 30 Doradus in LMC May 2006April 2004 Belinda Wilkes
The Crab Nebula Chandra X-ray Observatory: X-ray Hubble Space T/p: Optical May 2006April 2004 Belinda Wilkes
May 2006April 2004 Belinda Wilkes
Stellar Life Star burns fuel in its core (fusion: H→Helium) Initially fuel is H, star is on Main Sequence “Adult” (e.g. The Sun) When H runs out, core heats up and He, burns: “Middle Age” (Giant star) then He runs out, it burns heavier elements, e.g. Fe May 2006April 2004 Belinda Wilkes
HR Diagram shows age and mass May 2006April 2004 Belinda Wilkes
Death of a Star When all fuel runs out, the core collapses Outer regions of star explode outwards: Supernova SN shine more brightly than a galaxy for a few hours/days May 2006April 2004 Belinda Wilkes
We are made of stardust! May 2006April 2004 Belinda Wilkes
Cassiopeia A: X-rays May 2006April 2004 Belinda Wilkes
What are X-rays? May 2006April 2004 Belinda Wilkes
Supernovae by Chandra May 2006April 2004 Belinda Wilkes