51-55 Flashcards

1
Q

Photosphere

A

where light can escape into space as the light we see from the sun

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2
Q

Plasma

A

sun is at such a high temp that atoms are ionized in what is called plasma

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3
Q

hydrostatic equilibrium

A

balance between pressure and gravity

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4
Q

Ideal Gas Law

A

Pressure=Tdc

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5
Q

Radiative zone

A

where photons carry energy through

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6
Q

convection zone

A

hot gas rises and cools, then sinks back to this region

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7
Q

granulation

A

bright area where bubbles of hot gas rise

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8
Q

sun’s atmosphere

A

the lower density gasses that lie above the photosphere

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9
Q

chromosphere

A

immediately above photosphere
contains spikes called spicules
red zone during a total eclipse

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10
Q

corona

A

the sun’s outer atmosphere
hotter than photosphere and chromosphere
contains little energy despite temp

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11
Q

magnetic fields

A

exert a force on charged particles making them follow the path of the field

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12
Q

coronal holes

A

larger cooler regions of corona where magnetic field is weak

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13
Q

solar wind

A

flow of gas away from the sun

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14
Q

proton-proton chain

A

(1) p + p yields 1 2H
(2) p + 2H yields 1 3He
(3) 3He + 3He yields 4He

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15
Q

cosmic rays

A

particles constantly showering earth from exploded stars

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16
Q

neutrino telescope

A

neutrino collides with neutron in water breaking neutron into a proton and an electron

17
Q

Fusion of H summary

A

4 1H yields 1 4He + E + 2v

18
Q

sunspots

A

indicator of solar activity

large, dark regions ranging in size, come in pairs

19
Q

Zeeman effect

A

physical process in which the magnetic field causes some of the spectral lines produced by atoms to split into 3 or 2 or more components

20
Q

prominences

A

huge plumes of glowing gas that jut from the lower chromosphere and into the corona

21
Q

solar flares

A

brief, bright eruptions of hot gas in the chromosphere

arise when the magnetic field near a sunspot gets twisted by gas motion

22
Q

coronal mass ejection

A

enormous bubbles of hot gas blasted from corona into space

23
Q

sunspot cycle

A

sunspot and flare activity changing from year to year

cycle is about 11 years

24
Q

Maunder Minimum

A

period where very little sunspots are seen causing cold winters

25
Q

parallax

A

d (in parsecs) = 1/P (in arcseconds)

26
Q

Proper motion

A

shifting positions of stars

27
Q

transverse velocity

A

actual speed of star across our line of sight

28
Q

Space velocity

A

vector addition of a stars radial and transverse velocity

29
Q

aberration of light

A

shift in the positions of stars

30
Q

brightness

A

Luminosity/4pi x d^2

31
Q

Photometer

A

way to measure B