The Sun Flashcards

1
Q

What holds sun together?

A

Sun made of gas so no rigidity. Held together by gravity

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2
Q

What stops sun collapsing?

A

Thermal pressure(atoms bouncing)

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3
Q

What is balance of pressure and gravity called?

A

Hydrostatic equilibrium

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4
Q

Why do we need hydrostatic equilibrium?

A

•if gravity too strong sun will collapse
•if pressure too strong sun will expand

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5
Q

Where is energy in sun generated?

A

The core

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6
Q

Explain nuclear fusion

A

•At high T atoms bounce very fast
•so fast 4 hydrogen fuse into helium
•releases tiny amount of energy
•so much hydrogen happens a lot powering entire sun

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7
Q

Where does the energy released in fusion come from?

A

Comes from binding energy of He

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8
Q

What are 3 ways of transporting energy?

A

Conduction, convection, radiation

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9
Q

What is radiation in sun?

A

Photons carrying energy

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10
Q

What is scattering?

A

Gas so dense so photons constantly getting absorbed and re-emitted. Photons random walk outwards

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11
Q

What is convection?

A

Boiling

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12
Q

Explain convection in sun

A

Lower parts of sun hotter so water expands becoming less dense than stuff above it so floats upwards transporting energy to top very fast

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13
Q

Ratio of radiation vs convection in sun

A

Radiation dominates lower 70%
Convection dominates upper 30%

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14
Q

What is helioseismology?

A

Measure of vibration patterns on suns surface

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15
Q

What is the photosphere?

A

Surface from which suns light comes to us

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16
Q

What is outside the photosphere?

A

The chromosphere and the corona

17
Q

What does convection cause magnetic fields to do?

A

Bubble out of solar surface.
Sunspots and solar prominences

18
Q

What do magnetic fields do?

A

Prevent hot surrounding plasma from entering the sunspot.

19
Q

Are sunspots cooler or hotter than surrounding regions?

A

Cooler

20
Q

Typical sunspot cycle

A

10-11 years

21
Q

What happens to sunspots cycle when sun is hotter?

A

Cycle is shorter as more activity

22
Q

When is sun most active?

A

When magnetic field lines tightly wound

23
Q

What causes solar flares?

A

When magnetic field lines become too twisted they reconnect and release lots of energy

24
Q

What is solar wind?

A

Continuous flow of charged particles caused by photons streaming out and pushing a tiny bit of matter along with it

25
Q

What is CME?

A

Coronal mass ejection. Bubbles of gas erupting from solar surface

26
Q

How is earth protected from solar wind and CMEs?

A

Magnetosphere. Charged particles can’t cross magnetic field lines so solar wind deflected. Visible as aurorae

27
Q

When can one see solar corona?

A

X-rays or during solar eclipse

28
Q

How is heliosphere inflated?

A

Solar wind

29
Q

What does the heliosphere protect us from?

A

Very energetic galactic cosmic rays

30
Q

What is heliopause?

A

End of heliosphere. Where wind buffets interstellar gas