the sun Flashcards

1
Q

how does sun make energy

A

fusion

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2
Q

where does fusion happen

A

core

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3
Q

how does it happen

A
  • hot
  • pressure
  • hydrogen becomes helium
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4
Q

whats the input of pp chain

A

4 hydrogens

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5
Q

output of pp chain

A

1 helium + energy

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6
Q

how long will sun last

A

another 5 billion years

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7
Q

solar neutrino problem

A

only detect 1/3 of neutrinos than predictions

by the time they hit earth 2//3 transform into the other types

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8
Q

equilibrium

A

due to fusion there is outward presure of radiation that counters the gravity

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9
Q

radiation zone

A

energy transported from core to convection zone using radiation

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10
Q

convection zone

A

energy moved through air convection to surface

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11
Q

bright spots on sun

A

hot gas is rising

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12
Q

why is corona so hot

A

mag field

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13
Q

what are sun spots

A

due to mag flux, cool spots

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14
Q

parallax

A
  • to measure distance to objects
  • aparent shift of location
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15
Q

temp of hottest stars

A

50000k

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16
Q

temp of coolest stars

A

3000k

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17
Q

how to measure mass of binary

A

2 out of 3:
- period
- speration of orbit
- velocity

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18
Q

mass range of stars

A

0.08Msun to 150Msun

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19
Q

size on HR

A

top right is largest, bottom left is smallest

20
Q

lifetimes on HR

A

shortest lifetime is top left, longest is bottom right

21
Q

mass on HR

A

hotter = more mass

22
Q

why does high mass = short life

A

burns fuel faster

23
Q

props for high mass

A
  • bright
  • blue
  • short life
  • large radius
24
Q

how is a giant or super giant created

A

when star burns all its fuel

25
open star cluster
- few thousand stars - young - in disk of our galaxy - 10s of lt-yr across
26
globular clusters
million stars very old found in halo
27
composition of interstellar medium
- hydrogen - helium - dust
28
molecular clouds
- cold - dense - hydrogen - dust
29
interstellar extinction
dust blocks view of stars
30
interstellar redding
dust allows IR to pass
31
how does a star form
grav collapse of molecular cloud, by overcoming force of thermal pressure
32
what stabalizes a molecular cloud
- turbulent motion - mag fields - thermal pressure
33
where did the first stars come from
formed with only H and He
34
what is the primary coolent in the early universe
- molecular hydrogen - only at high temps - so only massive stars are formed
35
what is a protostar
- when the cloud gets too dense for light to escape. it stops cooling and heats up. it stops collaping - hot clump formed inside cloud - no fusion
36
what are the jets that shoot from protostar
- out of the rotation axis - high speed gas - maybe created by mag field
37
steps of star evolution
1. protostar forms from cloud 2. it shrinks and heats up as it converts grav potential to heat 3. when its hot enough fusion can become the energy maker 4. fusion inc until it balences
38
what is brown dwarfs
- failed star - not big enough for fusion to start - degeneracy pressure halts contraction - emits IR - luminosity gradually declines
39
distribution of masses of stars
lots of low mass, few high mass
40
what mass is a low mass star
2 Solar mass
41
what mass is intermediate mass star
2 - 8 S mass
42
high mass
8+ S mass
43
evolution for small mass (red dwarf)
straight to white dwarf
44
evoution for sun like stars
giant -> white dwarf
45
evolution for high mass star
supernova explosion to neutron star or black hole
46
how is giant formed
hydrogen is gone, grav collapses, and it heats up pushes outer layer outwards star gets bigger and brighter