When we look at close objects, we see what is happening now, but when we look at distant objects, we see what happens in the future.
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Q38: Why does fusion cease in a star
Q39: The _ brightness of a star is
Q40: A _ is a large volume of
Q41: A concentration of older stars that shared
Q42: Helium fusion requires a higher temperature than
Q44: The Universe was perfectly homogeneous, or uniform,
Q45: Hubble's law states that the _.
A) most
Q46: The expansion of the Universe is slowing
Q47: Until about 300,000 years after the big
Q48: Five billion years from now, the hydrogen
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