MathgeomGLS

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-633.351072039666	-32979170.433223	22439.9161766168	584878115.761119	-633.351072039666	-32979170.433223	22439.9161766168	584878115.761119	0.25	Tahoma		12	2	8	8	80	80	1	1	1	1	1	64000	1	15793151	12632256	255	32768	8421504	32896	32896	8421376	15780518	128	0	0	1	1
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5.6704e-8*x^4	5.6704e-8 x^4	1	2	16711680	0.100000001490116	0	10000	10327.5723843863	574083075.817333	-1	-1	-1	0	-1
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Stefan-Boltzmann	10000	550000000	20	Tahoma		12	128	-1
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The Stefan-Boltzmann law, also known as Stefan's law, describes the power radiated	128
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from a black body in terms of its temperature, in degrees Kelvin.	128
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It states that the total energy radiated per unit surface area of a black body across	128
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all wavelengths per unit time (also known as the black-body irradiance or emissive power),	128
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is directly proportional to the fourth power of the black body's thermodynamic temperature (°K).	128
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Formula	13000	480000000	12	Symbol		16	32768	-1
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2
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       2p	16711680
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s = -----  = 	16711680
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Formula	13000	479500000	26	Constantia		16	16711680	-1
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2
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             k	16711680
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      15c  h	16711680
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numbers	13000	480000000	28	Constantia		10	16711680	-1
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2
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                 5    4	16711680
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                 2    3	16711680
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numbers	15100	468000000	20	Tahoma		12	16711680	-1
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1
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5.670400 x10   x k	16711680
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numbers	16460	472000000	17	Times New Roman		11	16711680	-1
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20
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    -8      4	16711680
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	16711680
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  -34	16711680
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                  -8        -2  -4	16711680
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Symbols	11000	440000000	20	Tahoma		12	16711680	-1
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4
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Where  k is the thermodynamic temperature in °K (0°C = 273.15 °K)	16711680
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          c is the velocity of light (299,792,458 metres per second)	16711680
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          h is Planck's constant (6.62606957×10     Js)	16711680
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 	4210816
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Temperature of the sun	10000	400000000	20	Tahoma		12	128	-1
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The temperature of the Sun is 5778 K.	128
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If you click on the Evaluate button and enter 5778 for the value of x then y = 63200984.8547802	128
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Thus the Suns emissive power is 6.3200984 x 10  Joules per second per square metre at its surface.	128
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numbers	15900	377000000	15	Tahoma		9	128	-1
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7	128
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Star temperature	10000	350000000	20	Tahoma		12	128	-1
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Star temperature can be estimated by treating the emitted energy as a black body radiation	128
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and using the following function.	128
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Formula	11900	317400000	27	Symbol		16	16711680	-1
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4
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               = 4p     s	16711680
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	16711680
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	16711680
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s	16711680
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Formula	13000	315000000	23	Tahoma		14	16711680	-1
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1
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L        R    T	16711680
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numbers	14170	315000000	15	Tahoma		9	16711680	-1
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1
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2       4	16711680
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Text Block	11000	300000000	20	Tahoma		12	16711680	-1
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4
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Where  L is the luminosity of the star	16711680
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          R is its radius	16711680
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          T is its temperature in kelvin degrees	16711680
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             is the Stefan-Boltzmann constant 5.670400 x10   W m  K	16711680
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Text Block	10000	-2000000	20	Tahoma		12	16711680	-1
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1
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Temperature °K	16711680
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Text Block	-300	400000000	15	Tahoma		12	16711680	-1
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14
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E	16711680
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m	16711680
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i	16711680
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s	16711680
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s	16711680
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i	16711680
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v	16711680
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e	16711680
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	16711680
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P	16711680
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o	16711680
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w	16711680
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e	16711680
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r	16711680
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