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This Java applet is designed to simulate the diffusion process which occurs when gases of different temperatures are mixed.
This is the process which fuels the Sun and other stars which have core temperatures less than 15 million Kelvin. A reaction cycle yields about 15 MeV of energy.
Introduction to colligative properties of solutions - complex equations included!
Viewing the sun at different wavelengths and temperatures can reveal different information about what's going on at the sun and it's structure.
An ADIABATIC process deals with the changing temperature of a parcel of air due to rising or sinking the air. The DIABATIC process on the other hand is changing the temperature of a parcel of air ...
This page explains different ways that water can remain unfrozen at low temperatures - including dissolved solutes and supercooling.
Discusses creation of a new state of matter at near absolute zero - Bose Einstein condensates. Sponsored by University of Colorado.
The Ising model can be explored to observe the magnetic spins at different temperatures
Sir John Cockcroft was interested in the production of intense magnetic fields and low temperatures. Both he and Ernest Thomas Sinton Walton were awarded the Nobel Prize for Physics in 1951.
A profile of female astronomer Cecilia Payne-Gaposchkin who's PhD thesis related the differentl classes of stars to their temperatures.
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