Authors: Allen Graycek
Extending from galaxies are huge halos of gas and dust, much larger than previously thought. Mass estimates of these halos indicate a mass about equal to the galaxy’s stars. Material type verifies these halos to be the exudate of the galaxy’s supernovae (SNs). It is known stars that explode give considerable force and speed to the gas and dust they blow off. The rate of SNs when searched for was found to be very low. Simple calculations using this data results in a very great age for a Milky Way size galaxy and provides answers to current research on mysteries such as dark matter. It is known it takes trillions of years for stars to cool down, and once cool they would emit millions of times less heat, and no light. They might be IR detectable within a few light years from us.
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[v1] 2016-09-08 08:31:43
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