A reaction that involves two atomic nuclei merging to create the nucleus of a new atom. The reaction is accompanied by a tremendous release of energy. The Sun's energy, as with all stars, comes from nuclear fusion reactions that happen in its core. The reactions fuse hydrogen nuclei into helium nuclei. About 0.7 percent of the mass of the hydrogen is converted to energy, which makes the star shine.
Resources
Radio Programs
Polaris II
The un-steady beat of the North Star
Wednesday, February 20, 2013
The Sun II
The long trip before the journey begins
Tuesday, December 18, 2012
The Sun
Powering up the Sun
Monday, December 17, 2012
Triangulum
Aging stars in the triangle
Saturday, November 3, 2012
Capella
A quick exit for a “heavy” star
Friday, April 27, 2012
White Dwarfs
Squeezing the heart of a dead star
Wednesday, February 1, 2012
Betelgeuse
A superstar among supergiants
Thursday, December 1, 2011
Alpha Persei
A young but aging star
Saturday, October 8, 2011
Pollux
Forging the element of life
Sunday, May 15, 2011
Gienah
A young-but-old star
Saturday, April 2, 2011
Denebola
Shining through the moonlight
Friday, March 18, 2011
Stellar Factory
Forging elements in a stellar factory
Tuesday, February 15, 2011
The Sun Shines
Stoking the fires of the Sun
Wednesday, December 22, 2010
Rigel
A star with a bright but short future
Monday, August 16, 2010
Moon and Spica
The long beginning of a long journey
Monday, May 24, 2010
Alkaid
Getting a handle on the Big Dipper
Sunday, May 9, 2010
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