21ST CENT.ASTRONOMY(LL)W/CODE WKBK PKG.
21ST CENT.ASTRONOMY(LL)W/CODE WKBK PKG.
6th Edition
ISBN: 9780393874921
Author: PALEN
Publisher: Norton, W. W. & Company, Inc.
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Chapter 5, Problem 43QP

(a)

To determine

The average temperature on the planet.

(a)

Expert Solution
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Answer to Problem 43QP

The average temperature on the planet is 271.7K_.

Explanation of Solution

The black body temperature of a planet is given by,

    T=[Lsun(1a)16πσ]141d        (I)

Here, T is the temperature, Lsun is the luminosity of sun, a is the fraction of sunlight that reflects from a planet, σ is the Stefan’s constant, d is the distance.

All factors except the albedo are equal so that the change in temperature compared with zero albedo is given by,

    TT0=[Lsun(1a)16πσ]141d[Lsun(1a0)16πσ]141d=(1a)14(1a0)14        (II)

Conclusion:

Substitute 279K for T0 and 0 for a0 in equation (II) to find T.

    T=2791a4        (III)

Substitute 0.1 for a in equation (III) to find T.

    T=2791(0.1)4=271.7K

Therefore, the average temperature on the planet is 271.7K_.

(b)

To determine

The average temperature on the planet if its albedo were 0.9

(b)

Expert Solution
Check Mark

Answer to Problem 43QP

The average temperature on the planet is 156.9K_.

Explanation of Solution

The black body temperature of a planet is  given by,

    T=[Lsun(1a)16πσ]141d        (I)

Here, T is the temperature, Lsun is the luminosity of sun, a is the fraction of sunlight that reflects from a planet, σ is the Stefan’s constant, d is the distance.

All factors except the albedo are equal so that the change in temperature compared with zero albedo is given by,

    TT0=[Lsun(1a)16πσ]141d[Lsun(1a0)16πσ]141d=(1a)14(1a0)14        (II)

Conclusion:

Substitute 279K for T0 and 0 for a0 in equation (II) to find T.

    T=2791a4        (III)

Substitute 0.9 for a in equation (III) to find T.

    T=2791(0.9)4=156.9K

Therefore, the average temperature on the planet is 156.9K_.

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3. Suppose a planet has a surface temperature of 500 °K. (a)What is the total emission from the planet's surface (Wm²) over all wavelengths assuming it emits as a blackbody? (b) What is the wavelength of maximum emission for this planet? (c) Assume Earth has an average surface temperature of 300°K and emits as a black body. Earth's total emission would be what percent of that of the other planet? (d) What would the emissivity of the other planet have to be to have the same total emission as earth? (e) What would the brightness temperature of the other planet be in (a) and in (d)?
d&e
Consider a planet where Solar constant = 1360 W /m2 and albedo =0.30.  If n=0, what is the equilibrium surface temperature of the planet? If S increases to 1370 W/m2 and n remains zero, what is the new equilibrium surface temperature? If the planet has a water vapor feedback so that the number of layers n is a function of surface temperature nT = (T – 254.5)/100, what is the equilibrium surface temperature? Considering the answers above, calculate the climate feedback factor g for this planet.
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