Galaxies
Galaxies Huge (>1000’s ly across) Gravitationally bound Collections of gas, stars, planets, ice & dust.
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.
Galaxies Ecosystems of the Universe Gas Stars (& vice versa) No star formation between galaxies (intergalactic space)
Edwin Hubble In 1924, he divided galaxies into different “classes” based on their appearance.
Galaxy Types
Hubble’s Classification Scheme
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.
Elliptical Classification Scheme Identified by the letter E 0 -7 O is the most spherical, 7 is the most elliptical
by amount of flattening Elliptical Examples 0-7 determined by amount of flattening
Lenticular Galaxies* About 20% of all galaxies Between elliptical & spiral Have central bulge but no arms Aging, little star formation * Hubble added later
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
Spiral Classification Scheme Identified by the letter S B is added if barred spiral
Spiral Examples: Sa very tightly wound spiral arms bright central bulge Ex: Messier 81 “Bode’s Galaxy”
Spiral Examples: Sb Ex: M51 “Whirpool Galaxy” less tightly wound spiral arms fainter central bulge.
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
Barred Spiral Examples classified in the same way as non-barred spiral galaxies.
Irregular Galaxies about 5% No symmetry Lots of young, blue stars and interstellar material Smaller than most spirals and elliptical galaxies
Irregular Galaxies Large & Small Magellenic “Clouds” LMC, SMC