Main Sequence Flashcards

(35 cards)

1
Q

Approximate time it takes for a star to radiate all kinetic energy at current luminosity

A

Kelvin-Helmholtz timescale

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2
Q

Ordinary matter made up of two fundamental types of elementary particles

A

Quarks and leptons

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3
Q

Protons and neutrons made up of quarks called…

A

Hadrons

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4
Q

3 bound quarks

A

Baryons

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5
Q

2 bound quarks

A

Mesons

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6
Q

Quarks and leptons interact via which four fundamental forces?

A

Strong, electromagnetic, weak, and gravity

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7
Q

4 fundamental forces mediated by…

A

Bosons

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8
Q

Principle would not allow a baryon to have 2 quarks in the same state

A

Pauli Exclusion Principle

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9
Q

Particles with opposite charge, baryon, and lepton number

A

Antiparticles

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10
Q

Antiparticle counterpart to an electron

A

Positron

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11
Q

Protons and neutrons are bound by____(atomic nucleus)

A

Strong force

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12
Q

When protons and neutrons interact via weak force

A

Beta decay

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13
Q

Same # protons but different sum of protons and neutrons

A

Isotopes

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14
Q

Energy that hold nucleus together

A

Binding energy

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15
Q

Merge light nuclei–>more tightly bound–>energy released

A

Fusion

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16
Q

Reaction that emits alpha, beta, or gamma particles

A

Decay reactions

17
Q

He-4 nucleus

A

Alpha particle

18
Q

High energy photon

19
Q

electron or positron

A

Beta particle

20
Q

The splitting of a nucleus into two smaller parts

21
Q

Merger of light nucleus, results in tightly bound nucleus

22
Q

Most important reaction within the sun

A

Fusing of 4 hydrogen nuclei to 1 helium nuclei

23
Q

Nuclei must have enough ______to overcome the Coulomb potential (coulomb holds nucleus)

A

Kinetic energy

24
Q

Momentum accuracy =greater uncertainty in position

A

Heisenberg Uncertainty Principle

25
Main sequence start characteristic
Stably burning H in its core
26
High neutron flux
R-process
27
Low neutron flux
S-process
28
Thermonuclear reactions are also called
Burning
29
The line connecting set of points where stars first appear on the main sequence
Zero-age main sequence
30
Weight of each layer supported by pressure across each layer
Hydrostatic equilibrium
31
When atoms collide with nearby atoms and transports energy
Conduction
32
Hot parcels rise, cool parcels fall (in fluid)
Convection
33
Photons scatter and are absorbed by ions and atoms
Radiative transport
34
Star's structure is governed by...
Mass continuity
35
Photons carry energy outward through absorption and re-emission
Energy transfer