Astronomy 162:
Introduction to Stellar, Galactic, & Extragalactic Astronomy
Lecture 13: Energy Generation in Stars
Key Ideas:
- Energy generation in stars:
- Nuclear Fusion in the core.
- Controlled by a Hydrostatic "thermostat".
Putting Stars Together
Physics needed to describe stars:
- Law of Gravity
- Equation of State ("gas law")
- Principle of Hydrostatic Equilibrium
- Source of Energy (e.g., Nuclear Fusion)
- Way to transport that energy to the surface.
Hydrostatic Equilibrium
Balance between Pressure & Gravity.
- If Pressure dominates, the star expands.
- If Gravity dominates, the star contracts.
Sets up a Core-Envelope Structure:
- Hot, dense, compact core.
- Cooler, low-density, extended envelope.
Energy Generation
Stars shine because they are hot.
To stay hot stars must make up for the energy lost by shining.
Energy sources available:
- Gravitational Contraction (Kelvin-Helmholtz)
- Nuclear Fusion in the hot core.
Main-Sequence Stars
Generate energy by fusion of 4 1H into 1 4He.
There are two nuclear reaction paths by which a star might accomplish
this fusion:
Proton-Proton Chain:
- Relies on proton-proton reactions
- Efficient at low core Temperature (TC<18M K)
CNO Cycle:
- Carbon acts as a catalyst
- Efficient at high core Temperature (TC>18M K)
Proton-Proton Chain:
Note that you use 6 protons in all, and end up with 1 4He nucleus
and 2 protons at the end, for a net conversion of 4 protons into 1 Helium,
with the release of energy as gamma-ray photons, neutrinos, and postirons.
CNO Cycle:
Note that you start with one 12C nucleus in step one, and
add 4 protons during steps 1, 3, 4, and 6, ending up with the 12C
nucleus back at the end with the 4He nucleus.
The result is a net conversion of 4 protons into 1 Helium nucleus, with a
release of energy in the form of gamma-ray photons, neutrinos, and
positrons.
Because 12C is not consumed by this process (it goes in &
comes out at the end), we say that it acts as a catalyst for the
nuclear reaction.
Because Carbon and Nitrogen have 6 and 7 protons, respectively, in order to
overcome the repulsion of all these positive charges the protons must be
moving fairly fast. This is why the CNO cycle occurs at higher
temperatures than the P-P chain.
Controlled Nuclear Fusion
Fusion reactions are Temperature sensitive:
- Higher Core Temperature = More Fusion
- Energy Generation Rate of PP Chain ~ T4
- Energy Generation Rate of CNO Cycle ~ T18
BUT,
- More fusion makes the core hotter,
- Hotter core leads to even more fusion,
So why doesn't it runaway and blow up like a Hydrogen Bomb?
Hydrostatic Thermostat
If fusion reactions run too fast:
- core heats up.
- pressure increases & core expands.
- expansion cools core, slowing
fusion reactions.
If fusion reactions run too slow:
- core cools down.
- pressure drops & gravity contracts
the core.
- contraction heats core, increasing
fusion.
Summary:
Energy generation in stars:
- Nuclear Fusion in the core.
- Controlled by a Hydrostatic "thermostat".