It is now believed the majority of mass for most galaxies lies in their dark halos.
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Q15: A large cluster's mass can be over
Q16: Most large spirals and ellipticals are comparable
Q17: While quasars may have now vanished, the
Q18: Spiral galaxies are much more common in
Q19: For nearby spirals, their rotation curves help
Q21: Due to the galaxy density and collisions,
Q22: The largest voids may span 300 million
Q23: Based on galactic rotation curves and cluster
Q24: Gravity lensing lets us map the distribution
Q25: The distance between adjacent galaxies in a
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