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The Lifecycle of Stars.

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Presentation on theme: "The Lifecycle of Stars."— Presentation transcript:

1 The Lifecycle of Stars

2 Measuring stars Constellations are groups of stars that make a picture: big dipper Orion

3 Measuring distance A Light year is the distance light travels in one Earth year It is a measure of distance NOT speed!

4 Measuring brightness Magnitude is the brightness
Absolute magnitude is the actual brightness of a star Apparent magnitude is how bright a star appears from Earth Luminosity is the energy output from the surface of a star per second

5 All stars have nearly identical composition
Their differences in appearance is a result of their differences in surface temperatures Blue 40,000K (~71,000oF) White 10,000K Yellow 7,000K Orange 5,000K Red 3,000K (~4,900oF)

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7 Star size (mass) can also vary Our sun = 1 solar mass (2x1030kg)
Giants = are 8-30 solar masses Super giants = solar masses Also called “super massive”

8 H-R Diagram Plots data of mass, diameter, temperature, luminosity
Y-axis plots absolute magnitude X-axis temperature (and spectral type) Main sequence—90% of all stars fall w/i this band of stars on the diagram These stars all have similar properties of structure and function

9 HR Diagram

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11 Stellar Evolution Stars have a lifecycle Birth of the star is a nebula
Maturity is main sequence Old age are red giants or super giants Death are white dwarf, neutron star, black hole

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13 Star Formation All stars begin the same way but their evolution is determined by their mass

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18 Black Hole Warping of space due to gravity

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