Main Sequence Flashcards

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

A

Gamma ray

19
Q

electron or positron

A

Beta particle

20
Q

The splitting of a nucleus into two smaller parts

A

Fission

21
Q

Merger of light nucleus, results in tightly bound nucleus

A

Fusion

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
Q

Main sequence start characteristic

A

Stably burning H in its core

26
Q

High neutron flux

A

R-process

27
Q

Low neutron flux

A

S-process

28
Q

Thermonuclear reactions are also called

A

Burning

29
Q

The line connecting set of points where stars first appear on the main sequence

A

Zero-age main sequence

30
Q

Weight of each layer supported by pressure across each layer

A

Hydrostatic equilibrium

31
Q

When atoms collide with nearby atoms and transports energy

A

Conduction

32
Q

Hot parcels rise, cool parcels fall (in fluid)

A

Convection

33
Q

Photons scatter and are absorbed by ions and atoms

A

Radiative transport

34
Q

Star’s structure is governed by…

A

Mass continuity

35
Q

Photons carry energy outward through absorption and re-emission

A

Energy transfer