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Estimate the surface temperature of sun....

Estimate the surface temperature of sun. Given for solar radiations, `lambda_(m)=4753Å`. (`b=2.89xx10^(-3)` meter Kelvin)

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To estimate the surface temperature of the Sun using Wien's Displacement Law, we can follow these steps: ### Step-by-Step Solution: 1. **Understand Wien's Displacement Law**: Wien's Displacement Law states that the wavelength of maximum intensity of radiation emitted by a black body is inversely proportional to its temperature. The formula is given by: \[ \lambda_m \cdot T = b ...
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Experimental investigations show that the intensity of solar radiation is maximum for a wavelength 480 nm in the visible ragion. Estimate the surface temperature of sun. (Given Wien's constant b = 2.88 xx 10^(-3) m K ).

The wavelength of maximum intensity of emission of solar radiation is lambda_(m) = 4753Å and from moon it is 14 mm . The surface temperature of sun and moon are: (Given b = 2.898 xx 10^(-3) "metre"// "Kelvin")

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The intensity of the solar radiation is maximum for wavelength lamda_(m)=4753Å in the visible region. The surface temepratureof the sun, is (Assume the sun to be a black body. Wien's constant (b) =2.892xx10^(-3)mK )

Obtain the temperature ranges for ultraviolet part of radiation of EM waves. Use the formulae lambda_m T=2.9xx10^-3mK . Take frequency of ultraviolet part of radiations as 8xx10^14Hz to 5xx10^17Hz .

Compute the surface temperature of the sun from the following data: Distance of earth from the sun R=1.469xx10^(11)m Radius of the sun r=6.928xx10^(8)m Solar constant S=1.39xx10^(3)Wm^(-2) Stefan's constant sigma=5.73xx10^(-8)Wm^(-2)K^(-4)

The sun radiates maximum energy at wavelength 4753Å . The surface temperature of the sun if b=2.888xx10^(-3)mK , is

The solar energy received by the Earth persquare metre per minute is 8.315 xx 10^(4)Jm^(-2)min^(-1) . If the radius of the Sun is 7.5 xx 10^(5) km and the distance of the Earth from the Sun is 1.5 xx10^(8) km, calculate the surface temperature of Sun. Assume the Sun as a perfect black body. Given that Stefen constanta sigma = 5.7 xx 10^(-8)Wm^(-2)K^(-4).

Consider the sun to be a perfect sphere of radius 6.8 xx 10^(8)m . Calculate the energy radiated by sun in one minute. Surface temperature of the sun = 6200 K . Stefan's constant = 5.67 xx 10^(-8) J m^(-2) s^(-1) K^(-4) .

BANSAL-HEAT TRANSFER-Exercise
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  14. During total solar eclipse Fraunhoffer's lines appear bright because -

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  19. If the rate of emission of radiation by a body at temperature TK is E ...

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  20. A liquid takes 10 minutes to cool from 80^(@)C to 50^(@)C. The tempera...

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