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Definitions and explanations of dark matter, dark energy, their respective compositions in the universe, orbital velocity, rotation curves, evidence, gravitational lensing, wimps, machos, formation of structure, critical density, and different types of universes. It also discusses the role of gravity and the impact of these phenomena on the expansion of the universe.
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undetected form of mass that emits little or no light infer from gravitational influence 90% mass of universe is dark matter detectable only through gravitational forces on luminous matter (gas and stars) TERM 2
DEFINITION 2 source of repulsive force causing expansion of universe to accelerate TERM 3
DEFINITION 3 Normal Matter - 4. dark matter - 23% dark energy - 73% TERM 4
DEFINITION 4 found to measure mass TERM 5
DEFINITION 5 Speed of rotation from center planets in our solar systemm: dramatic fall of curves means orbital speed decreases with distance milky way: flat curve so speed remains large at large distances
galaxy velocities are too large in cluster X-ray emitting gas in cluster Gravitational Lenses distorts view of galaxies TERM 7
DEFINITION 7 bends light due to gravity of galaxy clusters TERM 8
DEFINITION 8 WIMPS (nonbaryonic) MACHOS (baryonic) TERM 9
DEFINITION 9 MASSIVE COMPACT halo objects atoms, protons, neutrons brown dwarfs, black holes, black dwarfs, cold neutron stars etc. when passing in front of a star, it suddenly brightens TERM 10
DEFINITION 10 weakly interacting massive particles non baryonic matter neutrinos unknown particles
dark energy exists overpowers gravity and accelerates with time