Main Sequence Flashcards
Approximate time it takes for a star to radiate all kinetic energy at current luminosity
Kelvin-Helmholtz timescale
Ordinary matter made up of two fundamental types of elementary particles
Quarks and leptons
Protons and neutrons made up of quarks called…
Hadrons
3 bound quarks
Baryons
2 bound quarks
Mesons
Quarks and leptons interact via which four fundamental forces?
Strong, electromagnetic, weak, and gravity
4 fundamental forces mediated by…
Bosons
Principle would not allow a baryon to have 2 quarks in the same state
Pauli Exclusion Principle
Particles with opposite charge, baryon, and lepton number
Antiparticles
Antiparticle counterpart to an electron
Positron
Protons and neutrons are bound by____(atomic nucleus)
Strong force
When protons and neutrons interact via weak force
Beta decay
Same # protons but different sum of protons and neutrons
Isotopes
Energy that hold nucleus together
Binding energy
Merge light nuclei–>more tightly bound–>energy released
Fusion
Reaction that emits alpha, beta, or gamma particles
Decay reactions
He-4 nucleus
Alpha particle
High energy photon
Gamma ray
electron or positron
Beta particle
The splitting of a nucleus into two smaller parts
Fission
Merger of light nucleus, results in tightly bound nucleus
Fusion
Most important reaction within the sun
Fusing of 4 hydrogen nuclei to 1 helium nuclei
Nuclei must have enough ______to overcome the Coulomb potential (coulomb holds nucleus)
Kinetic energy
Momentum accuracy =greater uncertainty in position
Heisenberg Uncertainty Principle
Main sequence start characteristic
Stably burning H in its core
High neutron flux
R-process
Low neutron flux
S-process
Thermonuclear reactions are also called
Burning
The line connecting set of points where stars first appear on the main sequence
Zero-age main sequence
Weight of each layer supported by pressure across each layer
Hydrostatic equilibrium
When atoms collide with nearby atoms and transports energy
Conduction
Hot parcels rise, cool parcels fall (in fluid)
Convection
Photons scatter and are absorbed by ions and atoms
Radiative transport
Star’s structure is governed by…
Mass continuity
Photons carry energy outward through absorption and re-emission
Energy transfer