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Published byKelley Garrison Modified over 8 years ago
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A universe that stops expanding only after an infinite Amount of time
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Flat Universe
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A universe with enough matter to eventually stop The expansion and recollapse
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Closed Universe
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A universe with too little matter to stop the expansion.
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Open Universe
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An assumption that the universe is everywhere Uniform and looks the same in any direction in all space and Time.
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Perfect Cosmological Principle
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An estimate of the age of the universe obtained by Taking the inverse of a specific constant, only valid If the expansion rate of the universe is constant at all Times in its history.
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Hubble Time
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Period of time before 1 million years after the start of the Expansion of the universe, when energy was more Dominant than matter.
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Radiation Era
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Radio energy that is nearly uniform in all directions and has a nearly perfect thermal spectrum.
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Cosmic Microwave Background Radiation
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The problem that if the universe is infinite in size and age, then the night sky should everywhere be as bright as the sun no matter the direction being looked at
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Olbers’ Paradox
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The time about a million years after expansion of the universe began when it became transparent
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Decoupling Epoch
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The time about 1 million years after the big bang’s beginning, when most of the ions and electrons In the universe combined to form atoms
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Recombination Epoch
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A type of matter that destroys ordinary matter when they come into contact with one another
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Antimatter
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The force that caused the expansion of the universe to expand and accelerate
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Dark Energy
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The undetectable quantity that helps hold galaxies together. It can be deduced due to gravity.
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Dark Matter
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The value of the average density of the universe must equal or exceed if the universe is closed.
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Critical Density
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When the charges on the two particles cancel and the Mass of the particles is entirely converted to energy
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Annihilation
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The explosive event at the beginning of the universe
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Big Bang
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The self-repelling property of space first proposed by Einstein
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Cosmological Constant
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Everywhere uniform in appearance so that there is no preferred observing position
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Homogeneous
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A brief period of extremely rapid and enormous expansion that may have occurred very early in the history of the universe.
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Inflation
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Looking the same in all directions
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Isotropic
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Coach Villegas’s favorite NFL team
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49ers
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Coach Villegas’s age
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30
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Coach Villegas’s favorite NBA team
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Mavericks
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What do you call a fly with not wings?
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A walk
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What gets wetter as it dries?
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A towel
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