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Page 1: Putting the  Iron in

Putting the Iron in

Prof Martin HendryUniversity of Glasgow

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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How do stars and planets form?

fromNebulae

"Island Universe", NSEW 2012

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How do stars and planets form?

fromNebulae

"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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versus

Forming stars

"Island Universe", NSEW 2012

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Forming stars

versus

Gas pressure trying to expand the cloud

Gravity trying to collapse the cloud

"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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Spectral type (temperature)S

tella

r m

ass

"Island Universe", NSEW 2012

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We can use spectral lines, like fingerprints, to identify the chemicals that stars and planets are made of.

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Hydrogen fusion – fuelling a star’s nuclear furnace

E = mc 2

H = HydrogenHe = Helium

Speed of light

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"Island Universe", NSEW 2012

The CNO Cycle

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The CNO Cycle

But how did the carbon, nitrogen and oxygen get there?...

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Spectral type (temperature)

Lum

inos

ity

"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

The “triple alpha” process

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Inside a very massive starconditions are hot anddense enough tofuse even heavierelements,

all the way upto Iron

"Island Universe", NSEW 2012

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"Island Universe", NSEW 2012

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