The figure below shows the energy balance for a planet with an atmosphere. The atmosphere is fully transparent to solar radiation and fully absorbing of infra-red radiation. Fill in values for the arrows in the figure assuming Ein=100 W/m². Doing arrows in the order labeled should help. Enter the values for 1-4 in the text box. What is the temperature of this planet (use E = L = oT* , o = 5.67 × 10-8 –W )? m² K+ 5. K 6. °C 7. °F Sun 2.

Principles of Heat Transfer (Activate Learning with these NEW titles from Engineering!)
8th Edition
ISBN:9781305387102
Author:Kreith, Frank; Manglik, Raj M.
Publisher:Kreith, Frank; Manglik, Raj M.
Chapter1: Basic Modes Of Heat Transfer
Section: Chapter Questions
Problem 1.46P
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The figure below shows the energy balance for a planet with an atmosphere. The atmosphere is fully transparent
to solar radiation and fully absorbing of infra-red radiation. Fill in values for the arrows in the figure assuming
Ein=100 W/m?. Doing arrows in the order labeled should help. Enter the values for 1-4 in the text box.
What is the temperature of this planet (use E = 2 = oTª , o =
= 5.67 x 10-8
W
)?
m K4
5.
K
6.
°C
7.
°F
Sun
2.
1.
3.
4.
Transcribed Image Text:The figure below shows the energy balance for a planet with an atmosphere. The atmosphere is fully transparent to solar radiation and fully absorbing of infra-red radiation. Fill in values for the arrows in the figure assuming Ein=100 W/m?. Doing arrows in the order labeled should help. Enter the values for 1-4 in the text box. What is the temperature of this planet (use E = 2 = oTª , o = = 5.67 x 10-8 W )? m K4 5. K 6. °C 7. °F Sun 2. 1. 3. 4.
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