Universe: Stars And Galaxies
Universe: Stars And Galaxies
6th Edition
ISBN: 9781319115098
Author: Roger Freedman, Robert Geller, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 5, Problem 12Q
To determine

The reason why astronomer prefer to work on Kelvin scale in their work rather than Celsius or Fahrenheit.

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Our Sun shines bright with a luminosity of 3.828 x 1026 Watt. Her energy is responsible for many processes and the habitable temperatures on the Earth that make our life possible. Calculate the amount of energy arriving on the Earth in a single day. To how many litres of heating oil (energy density: 37.3 x 106 J/litre) is this equivalent? The Earth reflects 30% of this energy: Determine the temperature on Earth’s surface. What other factors should be considered to get an even more precise temperature estimate? Note: The Earth’s radius is 6370 km; the Sun’s radius is 696 x 103 km; 1 AU is 1.495 x 108 km.
Calculate the amount of radiation emitted for a unit surface (1 m2) for a white ball at 53°C and £≈0.12. Express your Answer SI units (in W).
The amount of radiant energy emitted by a surface is given by q = ɛ0 AT+ where q represents the rate of thermal energy (per unit time) emitted by the surface in watts; e = the emissivity of the surface 0<ɛ<1 and is unitless o = Stefan-Boltzman constant (o = 5.67×10% ) A represents the area of the surface in m² Ty = surface temperature of the object expressed in kelvin What are the appropriate units for o if the equation is to be homogeneous in units?
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