The Sun and Nuclear Chemistry Flashcards

1
Q

photosphere

A

the surface of the sun/ what we see

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2
Q

chromosphere

A

is the lower atmosphere of the sun

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3
Q

corona

A

the upper atmosphere of the sun

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4
Q

what is the average temp of the photosphere

A
  • 5800 kelvin

- we know this because of weins law

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5
Q

what is luminosity

A

-total energy given off by an object each second

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6
Q

solar constant

A
  • we measure this to get luminosity

- and is the solar energy reaching earth per square meter

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7
Q

what us the sun made of

A

hydrogen and helium

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8
Q

what is the radiave zone

A

the interior of the sun

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9
Q

what is the temp of the core of the sun

A

15 million kelvin

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10
Q

what causes the gas bubbles of the sun

A

the convection of the ionized atoms

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11
Q

what do we see and what is covered up when a solar eclipse happens

A

the bright photospheres blocked and the faint chromosphere and corona is visible

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12
Q

what are the atoms of the corona like?

A

highly ionized

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13
Q

what is solar wind

A
  • the heat of the suns gas is being escaping

- mostly protons and electrons moving very fast

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14
Q

if corona is very hot, what is a good wavelength to look t

A
  • x rays

- we see hot white spots and dark cool spots when we did this

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15
Q

sunspots

A
  • each is about the size of earth
  • they have a black color but that is deceiving because they are still very hot
  • they only last a few days
  • usually in pairs
  • have large magnetic feilds
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16
Q

magnetic field of the sun

A

magnetism gets twisted by differential rotation because. the equator rotates father than the rest of the star

17
Q

Polarity of the sunspots

A
  • every other sunspot has the reverse polarity
  • north becomes south
  • thus a true sun cycle is 22 years
18
Q

solar maximum

A
  • when the max number of sunspot occur

- and the sun get every active around this time

19
Q

prominences

A

giant loops of hot gas that follow field lines

20
Q

solar flares

A

more violent bursts of hot gas

21
Q

Nuclear Fusion

A
  • the sun combines light nuclei into heavier ones

- when mass is lost and energy is gained

22
Q

nuclear force

A

at high temps in the center of the sun, velocity of atoms is very high and atoms can collide after going through electrical repulsion to fuse together

23
Q

Positron

A
  • a positively charged electron

- when it collides with an electron it creates energy

24
Q

Neutrino

A
  • have no charge and have no mass so they rarely interact with each other
  • and easily escape the sun
  • can go through anything
25
Q

Deuteron

A
  • aka the nucleus of a heavy hydrogen
  • has an extra neutron
  • also called an isotope
26
Q

isotope

A

when you have more or less neutrons that normal

27
Q

what happens when 2 protons collide

A

after collision, it pops out a deuteron (which is a proton +neutron) and slo a positron

28
Q

how does sun create energy

A

through a string of reactions called the proton-proton chain

29
Q

proton-proton chain

A

creates a net result of 4H —-> 1He + energy

30
Q

what is the sun always gradually doing

A

turning H in its core to He

31
Q

what evidence do we have that the sun is turning H into He

A

we see evidence by the neutrino detectors

32
Q

where do we test these neutrinos

A
  • giant underground tanks of chlorine-rich chemicals which neutrinos interact more strongly with
  • abut 2 or 3 neutrinos are detected every week here