Astronomy 210
Lecture 30, Nov 5
Fall 2010
Lecture Notes:
pdf file
Fusion in the Sun
Reactions and products
deuterium
positrons
neutrinos
Where does the
energy
come from?
A
prizewinning
theory
The Evidence: Solar
Neutrinos
Radiochemical experiments
The pioneer:
Ray Davis
and the
Homestake Mine
experiment
GALLEX
experiment (
Gran Sasso
, Italy):
gallium tank
Scattering experiments
Super-Kamiokande
(Japan); Super-K
neutrino image
of the Sun
Sudbury Neutrino Observatory
(Canada);
detector image
The 2002 Nobel Prize in Physics
Coda:
Cosmic Gall
, by
John Updike
Changing Gears:
The Big Picture
Stars
Physical Properties
Apparent brightness
data on the
125 (apparently) brightest stars
Luminosity
Distance: parallax
data on the
100 nearest stars
searchable
database
of nearby stars
Mass: from binary systems
visual binaries
spectroscopic
binaries
Lecture Archive
Brian D. Fields
Last modified: Fri Apr 6 13:22:25 CDT 2007