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Ay 112 Midterm review
Ay 112 Midterm review

... As  pressure  increases,  the  density  increases  and  atoms  tend  to  be  more  neutral.  Also   as  the  density  increases  lines  are  broadened  by  “pressure  broadening”  or  the  Stark   effect,  as  the  quantum  levels  beco ...
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... The most accurate measurements of the stars and planets was made by a Danish astronomer named Tycho Brahe. Unfortunately, Brahe was a believer of Ptolemy’s geocentric vision of the universe. At the same time, though, he had to concede that some observations fit a heliocentric view. In a way to keep ...
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... of the solar system? Close your eyes and imagine… Don’t look at it! The Sun has a great amount of energy. You should never look directly at it. The Sun is the fiery center of our solar system. This huge ball of energy holds our solar system together. But what’s going on underneath its surface? ...
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Life Cycles of Stars

< 1 ... 145 146 147 148 149 150 151 152 153 ... 237 >

Standard solar model

The standard solar model (SSM) is a mathematical treatment of the Sun as a spherical ball of gas (in varying states of ionisation, with the hydrogen in the deep interior being a completely ionised plasma). This model, technically the spherically symmetric quasi-static model of a star, has stellar structure described by several differential equations derived from basic physical principles. The model is constrained by boundary conditions, namely the luminosity, radius, age and composition of the Sun, which are well determined. The age of the Sun cannot be measured directly; one way to estimate it is from the age of the oldest meteorites, and models of the evolution of the Solar System. The composition in the photosphere of the modern-day Sun, by mass, is 74.9% hydrogen and 23.8% helium. All heavier elements, called metals in astronomy, account for less than 2 percent of the mass. The SSM is used to test the validity of stellar evolution theory. In fact, the only way to determine the two free parameters of the stellar evolution model, the helium abundance and the mixing length parameter (used to model convection in the Sun), are to adjust the SSM to ""fit"" the observed Sun.
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