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physical phenomena > energy source > exothermic fusion process > hydrogen burning > proton-proton chain
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proton-proton chain
(p-p chain)
subjectfact 
proton-proton chainhas required reactant concentration high2001-09-27 09:29:42.0
has optimum temperature 5 million Kelvin2001-09-27 09:29:42.0
has part intermediate product deuterium2001-09-27 09:29:42.0
has part intermediate product tritium2001-09-27 09:29:42.0
has part product helium2001-09-27 09:29:42.0
has part reactant proton2001-09-27 09:29:42.0
has next higher temperature reaction carbon cycle2001-09-27 09:29:42.0
has temperature dependence ET4has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:29:42.0
has minimum temperature 107 Khas source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:29:42.0
has synonym p-p chain2001-09-27 09:29:42.0
has location the center of the Sun an other stars2001-09-27 09:29:42.0
has definition thermonuclear reaction in which two protons collide a very high velocities and combine to form deuteurium, the deuteurium can capture a proton to form tritium and tritium can capture a proton to form heliumhas source: Talbot, J. 2001, 2001-09-27 09:29:42.0
has definition A series of thermonuclear reactions in which hydrogen nuclei are transformed into helium nuclei. The temperature and density required are about 107 K and 100 g cm-3. It is the main source of energy in the Sun, where 1038 of these reactions occur every second. All parts of this reaction have been observed in the laboratory, except for the first step 1H(p, β+v)2D, which occurs only a few times in 1012 collisions of protons. But the first two reactions provide about one-third of the Sun's total energy release. The p-p chain divides into three main branches: PP I, PP II and PP III.has source: Hopkins, J. 1976 Glossary of Astronomy and Astrophysics, University of Chicago Press, 2001-09-27 09:29:42.0
has definition Process of nuclear fusion by which relatively cooler stars produce and radiate energy; hotter stars commonly achieve the same result by means of the carbon-nitrogen cycle.has source: Abbot, D. 1984 Astronomers, Peter Bedrick Books, New York, 2001-09-27 09:29:42.0
has definition The nuclear sequence by which the Sun and all other main-sequence stars with less than 1.5 solar masses fuse hydrogen into helium.has source: Croswell, K. 1995 The Alchemy of the Heavens, Anchor Books, 2001-09-27 09:29:42.0
has definition An important nuclear fusion reaction that occurs in stars. It begins with the fusion of two hydrogen nuclei, each of which consists of a single proton.has source: Ferris, T. 1988 Coming of Age in the Milky Way, Morrow, 2001-09-27 09:29:42.0
is a kind of hydrogen burning2001-09-27 09:29:42.0
is a kind of pycnonuclear reaction2001-09-27 09:29:42.0
hydrogen burninghas minimum mass 0.08 solar masses2001-09-27 09:29:41.0
has product helium2001-09-27 09:29:41.0
has catalyst2001-09-27 09:29:41.0
has reactant hydrogen2001-09-27 09:29:41.0
exothermic fusion processliberates energy2001-09-27 09:29:41.0
fusionhas antonym fission2001-09-27 09:29:41.0
produces energy2001-09-27 09:29:41.0
has reaction probability2001-09-27 09:29:41.0
physical processhas domain physics2001-09-27 09:29:38.0

Kinds of proton-proton chain :

Next hydrogen burningcarbon cycle    Uphydrogen burning, pycnonuclear reaction