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Hydrogen burning
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Physics
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Astrophysics
Stellar astrophysics
Stellar nuclear fusion
2026-09-28
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Hydrogen
burning converts
hydrogen
into
helium
through the
proton–proton chain
or
CNO cycle
.
Table of contents
Hydrogen-burning shell
Hydrogen burning
Hydrogen-burning shell
0
0
0
Hydrogen burning
A
hydrogen-burning
shell converts
hydrogen
into
helium
in
a
layer surrounding
a
hydrogen
-exhausted stellar core. It moves outward in
enclosed mass
as
it supplies fresh
helium
to that core; its movement in
radius
need not have the same
sign
.
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Stellar nuclear fusion
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Bethe stellar energy-production theory
Composition-dependent temperature selection of hydrogen burning
Contraction-limited central temperature
Helium mass fraction
Homogeneous fuel-depletion luminosity feedback
Hot-bottom burning
Low-mass main-sequence star
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Past exam of the mathematics course of the University of Cambridge
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Paper 63
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Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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Paper 63
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Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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2012
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iii
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Paper 63
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1
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c
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Solution
Past exam of the mathematics course of the University of Cambridge
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2012
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Paper 63
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4
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Solution
Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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Past exam of the mathematics course of the University of Cambridge
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Protostar
Radiative homology with fifth-power hydrogen burning and inverse-cubic opacity
Red giant
Stellar nuclear timescale
Stellar nucleosynthesis
Terminal-age main sequence
Turnoff mass of a homogeneously mixed proton-proton-burning population
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