The Sun is Earth’s major source of energy, yet the planet only receives a small portion of its energy and the Sun is just an ordinary star. Many stars produce much more energy than the Sun. The energy source for all stars is nuclear fusion.
Stars are made mostly of hydrogen and helium, which are packed so densely in a star that in the star’s center the pressure is great enough to initiate nuclear fusion reactions. In a nuclear fusion reaction, the nuclei of two atoms combine to create a new atom. Most commonly, in the core of a star, two hydrogen atoms fuse to become a helium atom. Although nuclear fusion reactions require a lot of energy to get started, once they are going they produce enormous amounts of energy (Figure below).
A thermonuclear bomb is an uncontrolled fusion reaction in which enormous amounts of energy are released.
In a star, the energy from fusion reactions in the core pushes outward to balance the inward pull of gravity. This energy moves outward through the layers of the star until it finally reaches the star’s outer surface. The outer layer of the star glows brightly, sending the energy out into space as electromagnetic radiation, including visible light, heat, ultraviolet light, and radio waves (Figure below).
A diagram of a star like the Sun.
In particle accelerators, subatomic particles are propelled until they have attained almost the same amount of energy as found in the core of a star (Figure below). When these particles collide head-on, new particles are created. This process simulates the nuclear fusion that takes place in the cores of stars. The process also simulates the conditions that allowed for the first helium atom to be produced from the collision of two hydrogen atoms in the first few minutes of the universe.
The SLAC National Accelerator Lab in California can propel particles a straight 2 mi (3.2 km).
The CERN Particle Accelerator presented in this video is the world’s largest and most powerful particle accelerator and can boost subatomic particles to energy levels that simulate conditions in the stars and in the early history of the universe before stars formed (2e):http://www.youtube.com/watch?v=sxAxV7g3yf8 (6:16).
An interactive or media element has been excluded from this version of the text. You can view it online here: http://pb.libretexts.org/es/?p=166
- Provided by: CK12.org. Located at: http://www.ck12.org/book/CK-12-Earth-Science-For-High-School/section/26.1/. License: CC BY-NC: Attribution-NonCommercial