•Temperature
changes relatively simple
–Starts
out large and relatively cool Must
be on red side of diagram
–It
heats up as it contracts Must
towards the blue
–
•Luminosity
more complicated because it depends on T and R
–Not
much energy to start with Luminosity
must start out low
–Collapse
releases grav. energy Luminosity
will rise
–Fusion
begins, releases more energy Luminosity
at a peak
–Collapse
slows, only have fusion now Luminosity
declines
•
•Finally
stabilizes on the main sequence