The observed proportions and distribution of hydrogen and helium are consistent with what would be expected if the Big Bang model were accurate. The Big Bang model describes how, from the cooling universe, the simplest atoms would have condensed from the hot broth of fundamental particles most easily: a proton and an electron, forming hydrogen. Far fewer particles would have combined to form helium, requiring two protons and one or two neutrons. The likelihood of spontaneous condensation of elements then decreases rapidly with the complexity of the element, so very few heavier elements could have formed that way. Initially, almost all of the visible matter in the universe consisted of hydrogen and helium, according to the Big Bang model. Heavier elements would have been formed through nucleosynthesis in the cores of stars and supernovae. When we look at the proportions and distribution of the elements, especially hydrogen and helium, this is indeed what we find.
Hydrogen and helium are the first elements produced in the universe after the big-bang.
The minimum hydrogen-to-helium ratio observed is approximately 25% hydrogen to 75% helium. This ratio is consistent with predictions based on the conditions of the early universe during the Big Bang.
It wasn't. Right after the Big Bang, there was only hydrogen (including deuterium), helium, and minute amounts of lithium. Apart from that, all the so-called metals - i.e., elements other than hydrogen or helium - were created in supernovae.
The big bang produced the helium no present in the sun's core. The universe cooled down enough after the big bang to form the formation of helium and hydrogen.
The process is called nucleosynthesis. After the Big Bang, the nucleosynthesis process involved the fusion of hydrogen and helium nuclei to form elements like lithium, beryllium, and some trace amounts of heavier elements.
Hydrogen and helium are the first elements produced in the universe after the big-bang.
The minimum hydrogen-to-helium ratio observed is approximately 25% hydrogen to 75% helium. This ratio is consistent with predictions based on the conditions of the early universe during the Big Bang.
Hydrogen and helium were the two main elements created in abundance during the Big Bang nucleosynthesis. These elements were formed in the first few minutes after the Big Bang, when the universe was hot and dense enough to support nuclear fusion.
No. The hydrogen in the universe was formed during the Big Bang. Stars consume hydrogen, fusing it into helium.
It wasn't. Right after the Big Bang, there was only hydrogen (including deuterium), helium, and minute amounts of lithium. Apart from that, all the so-called metals - i.e., elements other than hydrogen or helium - were created in supernovae.
No element "started" the big bang. The big band eventually produced mainly hydrogen and helium, which may be the answer you were looking for.
Hydrogen was initially formed in the 'Big Bang' which initiated this universe. Helium is formed by the fusion of hydrogen atoms, inside stars. This reaction is what causes stars to shine, and give off heat.
The big bang produced the helium no present in the sun's core. The universe cooled down enough after the big bang to form the formation of helium and hydrogen.
Some was made in the big bang and the rest is made by the process of hydrogen fusion in the cores of stars.
Hydrogen and helium are the two most abundant elements in the universe.
The process is called nucleosynthesis. After the Big Bang, the nucleosynthesis process involved the fusion of hydrogen and helium nuclei to form elements like lithium, beryllium, and some trace amounts of heavier elements.
The Big Bang leads to huge clouds of hydrogen and helium, which eventually condense into galaxies.