Observed BrightnessThe flux due to a light emitting object measured at the observer (in most cases, at the earth or a satellite).
Omega, ΩThe ratio of the average total density of matter to the critical density required to make the universe flat and eventually stop its expansion.
Opaque to RadiationA condition when radiation is absorbed or scattered many times. For the first 400,000 years the universe was so hot that the matter was ionized and…
Open Universe , ΩA universe where the geometry of space is curved like an infinite saddle-shaped surface.