Term
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Definition
The total mass of the star must equal the sum of the masses in its shells. Of course, no shell can be empty, and there is no such thing as a negative mass |
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Term
Conservation of Energy Law |
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Definition
says the amount of energy flowing out of the top of a shell in the star must be equal to the amount of energy coming in at the bottom of the shell pluss whatever energy is generated within the shell |
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Term
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Definition
the weight on each layer is balanced by the pressure in that layer |
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Term
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Definition
Energy moves from hot to cool by radiation, convection, or conduction |
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Term
Zero-Age main sequence (ZAMS) |
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Definition
Once nuclear fusion of hydrogen becomes the dominant energy production process and the excess energy gained from gravitational contraction has been lost,[14] the star lies along a curve on the Hertzsprung-Russell diagram (or HR diagram) called the standard main sequence |
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Term
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Definition
When a gas is so dense that the electrons are not free to change their energy |
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Term
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Definition
100 million Kelvin He nuclei fuse together to form Carbon - thus three He nuclei (alpha particles) He fusion is triple alpha process |
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Term
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Definition
Start He fusion with an explosion is caused by the density of the He core which can reach 1,000,000 g/cm^3 |
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Term
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Definition
1:) Open and Globular look different but evolve the same 2:) Estimate the age of a cluster by oberving the turnoff point 3:) Compare the stars and see how they are different |
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Term
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Definition
changes its brightness in a periodic way |
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Term
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Definition
more or less luminous because of an internal process |
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Term
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Definition
Cepheid variables are supergiants or bright giant stars of spectral type F or G, complete cycle in 2-60 days |
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Term
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Definition
star with a period of less than one day |
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Term
Period Luminosity Relation |
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Definition
Longer Period cephid 40,000 time brighter Shorter Period only 100's of times brighter |
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Term
Period Luminosity Relation |
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Definition
Longer Period cephid 40,000 time brighter Shorter Period only 100's of times brighter |
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Term
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Definition
The region where size and temperataure lead to pulsation on the HR diagram |
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Term
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Definition
The region where size and temperataure lead to pulsation on the HR diagram |
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Term
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Definition
The region where size and temperataure lead to pulsation on the HR diagram |
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Term
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Definition
The region where size and temperataure lead to pulsation on the HR diagram |
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Term
Period Luminosity Relation |
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Definition
Longer Period cephid 40,000 time brighter Shorter Period only 100's of times brighter |
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Term
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Definition
The region where size and temperataure lead to pulsation on the HR diagram |
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