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Galaxies
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Galaxies Huge (>1000’s ly across) Gravitationally bound
Collections of gas, stars, planets, ice & dust.
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Galaxies Different shapes & sizes.
Dwarf containing tens of millions (107) of stars, Supergiants containing up to a trillion stars (1012). > 100 billion (1011 ) galaxies in the observable universe.
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Galaxies Ecosystems of the Universe Gas Stars (& vice versa)
No star formation between galaxies (intergalactic space)
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Edwin Hubble In 1924, he divided galaxies into different
“classes” based on their appearance.
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Galaxy Types
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Hubble’s Classification Scheme
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Elliptical Galaxies ~ 50% of all galaxies They are gas poor
little star formation smooth featureless light distribution & appear elliptically shaped in found near the center of rich galaxy clusters.
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Elliptical Classification Scheme
Identified by the letter E 0 -7 O is the most spherical, 7 is the most elliptical
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by amount of flattening
Elliptical Examples 0-7 determined by amount of flattening
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Lenticular Galaxies* About 20% of all galaxies
Between elliptical & spiral Have central bulge but no arms Aging, little star formation * Hubble added later
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Spiral Galaxies ~ 20% of all galaxies* They are gas rich
But 70% of visible galaxies due to their brightness. They are gas rich Lots of star formation More isolated
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Spiral Classification Scheme
Identified by the letter S B is added if barred spiral
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Spiral Examples: Sa very tightly wound spiral arms
bright central bulge Ex: Messier 81 “Bode’s Galaxy”
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Spiral Examples: Sb Ex: M51 “Whirpool Galaxy”
less tightly wound spiral arms fainter central bulge.
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Spiral Examples: Sc loosely wound spiral arms
smaller, fainter central bulge. Ex: NGC 6946 New general catalogue of galaxies and nebulae 1886 originally but updated since, most recent 2009
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Barred Spiral Examples
classified in the same way as non-barred spiral galaxies.
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Irregular Galaxies about 5% No symmetry
Lots of young, blue stars and interstellar material Smaller than most spirals and elliptical galaxies
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Irregular Galaxies Large & Small Magellenic “Clouds” LMC, SMC
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