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Jovian Planet Systems
Jovian Planet Systems

... • The first geologic eon of Earth and lies before the Archean. It began with the formation of the Earth about 4.5 billion years ago and ended about 4,000 million ...
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... Andromeda, and determined their distance. Andromeda contains a spiral-shaped galaxy that, at a distance of 2.2 million light-years, is the farthest object visible to the naked eye. He calculated that Andromeda must be at least 10 times farther away than the farthest stars in the Milky Way. The Andro ...
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regan-kent-25nov09a

... • BUT!!! 4He can fuse with 2 other 4He (8Be) stuck together for a short time (~10-16sec) to make 12C…complicated but understood. ...
Origin of Life - BlackSage.com
Origin of Life - BlackSage.com

... • Galaxies have a red shift in light produced by the Doppler effect similar to sound (also used in radar) • The movement of galaxies away from us corresponds to an equation called "Hubble's Law" • The time elements in Hubble's Law permit the estimation of the age of the universe – about 13 billion y ...
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... Stars can make Lithium in nuclear reactions but most stars actually DESTROY lithium. Why? 1.  It gets fused into other elements 2.  No energy is released by the fusion of lithium 3.  Lots of energy is released by the fusion of lithium 4.  Lithium reacts chemically to make molecules 5.  Stars hate l ...
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... __F__  the  total  star  formation  rate  in  the  Universe  has  been  relatively  steady  since   about  1  billion  years  after  the  Big  Bang   __T__  Quasars  were  much  more  common  in  the  period  between  1  and  3  b ...
Getting to Know: Theories About How the Universe Formed
Getting to Know: Theories About How the Universe Formed

... behind. Future scientific studies may add more ideas to the Big Bang Theory. However, today, many scientists believe that the Big Bang Theory is the best scientific answer for how the universe formed. ...
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Big Bang nucleosynthesis

In physical cosmology, Big Bang nucleosynthesis (abbreviated BBN, also known as primordial nucleosynthesis) refers to the production of nuclei other than those of the lightest isotope of hydrogen (hydrogen-1, 1H, having a single proton as a nucleus) during the early phases of the universe. Primordial nucleosynthesis is believed by most cosmologists to have taken place from 10 seconds to 20 minutes after the Big Bang, and is calculated to be responsible for the formation of most of the universe's helium as the isotope helium-4 (4He), along with small amounts of the hydrogen isotope deuterium (2H or D), the helium isotope helium-3 (3He), and a very small amount of the lithium isotope lithium-7 (7Li). In addition to these stable nuclei, two unstable or radioactive isotopes were also produced: the heavy hydrogen isotope tritium (3H or T); and the beryllium isotope beryllium-7 (7Be); but these unstable isotopes later decayed into 3He and 7Li, as above.Essentially all of the elements that are heavier than lithium and beryllium were created much later, by stellar nucleosynthesis in evolving and exploding stars.
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