Astrophysics. Aim: To determine the luminosity of the Sun using calculations.

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Brionna Wilson

HL Physics

12/11/2009

Determining the Luminosity of the Sun

Aim:

        To determine the luminosity of the Sun using calculations.

Diagram:

Equations Used:

b  apparent brightness

L  luminosity (of the sun)

d  =

 

BUT:  

                                          AND  

SO: 

   ∴

Initial Information:

Mass of Water (m) = 0.937810 kg ±1 x 10-6 kg

Specific Heat Capacity (C) = 4200 J Kg-1 K-1

Change in Temperature (∆T) = 319.5 – 298.5

                                   = 21.0 K ±1 K

Distance between Sun and Earth (d2) = (1.496 x 1011)2

                                                = 2.238 x 1022 m

Radius of Beaker (r2) = (0.0525)2

                         = 0.00276 m ±0.002 m

Time Taken for 21.0 K Temperature Change (∆t) = 5700 s ± 600 s

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Calculations:

 =    4. d2. C. m. ∆T

                        r2. ∆t

  =     4 x (2.238 x 1022) x 4200 x (0.937810) x 21.0

                                         0.00276 x 5700

  =    4.707 x 1026 Watts

Uncertainty:

±  = (1 x 10-6) + 1 + 0.002 + 600

            = 601.002001 ≈ ±601

Luminosity of Sun = 4.707 x 1026 ±601 W


Conclusion & Evaluation:

Based on the results and my calculations, the luminosity of the Sun is 4.707 x 1026 ±601 Watts. The accepted value for the ...

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