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Main Evidence for the Big Bang
The Hubble Law The existence and properties of the blackbody cosmic microwave background Primordial nucleosynthesis and the observed light element abundances
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Modern-Day Hubble Law
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Too Much Helium Our Sun is about 28% helium by mass.
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Nuclear Reactions in the Early Universe
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Primordial Nucleosynthesis
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“Cooling” of the Cosmic Microwave Background
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Arno Penzias and Robert Wilson
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Cosmic Background Explorer (COBE)
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Spectrum of the Cosmic Microwave Background
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Anisotropy of the Cosmic Microwave Background
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Current Maps of the Cosmic Microwave Background
WMAP
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