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Astronomy 100 Section 2

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John Updike. scant. Photons take 106 years to escape. Neutrinos escape right away. very much ... Ray Davis & John Bahcall. Only ~ 1/3 of the electron neutrinos ... – PowerPoint PPT presentation

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Title: Astronomy 100 Section 2


1
Astronomy 100 Section 2 As Presented by Paul
Ricker
This class The Sun II Interior
2
Life Depends on the Sun
Wind and weather
Liquid water
Photosynthesis
3
Human Cultural Acknowledgment of the Suns Role
Zia sun symbol New Mexico
Ancient Egypt Akhenaton
Van Gogh Olive Trees with Yellow Sky and Sun
4
Helioseismology
  • Trapped sound waves refract from regions of
    different density
  • Produce characteristic pattern of oscillations on
    surface

5
The Interior of the Sun
6
Internal Rotation Speed
Base of the convective zone
7
The Battle between Gravity and Pressure
8
What Holds Up the Sun?
  • Without an energy source, Sun would rapidly cool
    contract
  • Mid-1800s
  • Darwin evolution needs Sun Earth to be 108
    years old
  • Lyell geological changes also needs 108
    years
  • Kelvin gravitational heating gives only a few
    million years!
  • No physical process then known would work!

Charles Darwin
Charles Lyell
William Thomson, Lord Kelvin
9
Atomic Nuclei and Radioactivity
10
Nuclear Reactions
  • Atomic nuclei can combine or split
  • Release energy in process (E mc2)
  • Light nuclei fusion
  • Heavy nuclei fission

11
Nuclear Fusion in the Suns Interior
  • Proton-proton in stars like the Sun
  • Hydrogen fused to make helium
  • 0.7 of mass converted to energy
  • CNO cycle in more massive stars

12
Why Nuclear Fusion Doesnt Occur in Your Coffee
  • Fusion requires
  • High enough temperature ( 5 million K)
  • High enough density
  • Enough time

13
Neutrinos
  • An extremely lightweight, weakly interacting
    neutral particle
  • Produced in radioactive decays and nuclear
    fusion
  • Three different types or flavors

n
p
e
?
A free neutron
spontaneously decays into a proton, an
electron, and an (anti)neutrino (half-life 10
minutes)
Flavors
Electron neutrino
Muon neutrino
Tau neutrino
14
Photons take 106 years to escape
COSMIC GALL Neutrinos, they are very small. Th
ey have no charge and have no mass
And do not interact at all. The earth is just a s
illy ball To them, through which they simply pass
, Like dustmaids down a drafty hall Or photons t
hrough a sheet of glass. They snub the most exqui
site gas, Ignore the most substantial wall, Cold
shoulder steel and sounding brass,
Insult the stallion in his stall,
And, scorning barriers of class,
Infiltrate you and me. Like tall
And painless guillotines they fall
Down through our heads into the grass.
At night, they enter at Nepal And pierce the love
r and his lass From underneath the bed you call
It wonderful I call it crass. John Updike
scant
very much
Neutrinos escape right away
15
Detecting Neutrinos
Neutrinos
Super Kamiokande Mozumi Mine, Japan 50,000 tons
of water
40 meters
16
The Sun as Seen in Neutrinos by Super-Kamiokande
500 days of data
90 degrees
90 degrees
17
The Solar Neutrino Problem
  • Only 1/3 of the electron neutrinos expected are
    seen!

Homestake Neutrino Detector
Ray Davis John Bahcall
18
The Solar Neutrino Problem Resolution
  • Neutrinos have (a little) mass
  • Neutrinos of one flavor can change into the others

Detector
19
Questions?
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