Question

The solar constant, equal to 1370 W/m2, is the amount of light energy from the Sunfalling...

The solar constant, equal to 1370 W/m2, is the amount of light energy from the Sunfalling on 1 square metre of the Earth’s surface each second. Given that the Sun’s radiusis roughly 700,000 km, determine (a) its luminosity, (b) its surface temperature, and (c) its wavelength of maximum emission.

0 0
Add a comment Improve this question Transcribed image text
Know the answer?
Add Answer to:
The solar constant, equal to 1370 W/m2, is the amount of light energy from the Sunfalling...
Your Answer:

Post as a guest

Your Name:

What's your source?

Earn Coins

Coins can be redeemed for fabulous gifts.

Not the answer you're looking for? Ask your own homework help question. Our experts will answer your question WITHIN MINUTES for Free.
Similar Homework Help Questions
  • At our distance from the Sun, the intensity of solar radiation is 1370 W/m2. The temperature...

    At our distance from the Sun, the intensity of solar radiation is 1370 W/m2. The temperature of the Earth is affected by the greenhouse effect of the atmosphere. This phenomenon describes the ef- fect of absorption of infrared light emitted by the surface so as to make the surface temperature of the Earth higher than if it were airless. For comparison, consider a spherical object of radius r with no atmosphere at the same distance from the Sun as the...

  • The Intensity of solar radiation at the Earth's orbit is 1370 W/m2. However, because of the...

    The Intensity of solar radiation at the Earth's orbit is 1370 W/m2. However, because of the atmosphere, the curvature of the Earth, and rotation (night and day), the actual intensity at the Earth's surface is much lower. At this moment, let us assume the intensity of solar radiation is 350 W/m2. You have installed solar panels on your roof to convert the sunlight to electricity. If the area of your solar panels is 3 m2, How much power is incident...

  • (a) Calculate the sun’s energy output assuming the sun is a black body radiator at 5800K...

    (a) Calculate the sun’s energy output assuming the sun is a black body radiator at 5800K surface temperature, and its diameter is 1.39E+06 km. (b) (And) from the earth orbit diameter calculate the energy actually reaching the top of the earth’s atmosphere, and compare it to the solar constant.

  • At our distance from the Sun, the intensity of solar radiation is 1370 W/m^2 . As...

    At our distance from the Sun, the intensity of solar radiation is 1370 W/m^2 . As discussed in class and in the textbook, the temperature of the Earth is affected by the greenhouse effect of the atmosphere. This phenomenon describes the effect of absorption of infrared radiation by the surface so as to make the surface temperature of the Earth higher than if it were airless. The average global surface temperature of the Earth is ~288 K. Calculate the surface...

  • Assume a planet with a solar constant S=2000 W/m2, an albedo α=0.4 and radius of 3,000...

    Assume a planet with a solar constant S=2000 W/m2, an albedo α=0.4 and radius of 3,000 km. What is the planet’s surface temperature? What would happen to the temperature if the planet’s radius doubles?

  • 7. Ultraviolet light with wavelength equal to 350 nm and intensity of 1.0 W/m2 is directed...

    7. Ultraviolet light with wavelength equal to 350 nm and intensity of 1.0 W/m2 is directed at a ted as a calcium surface. What is the maximum possible kinetic energy of electrons ejec result of this type of radiation? Give answer in units of eV? [10 points]

  • A watt is a unit of energy per unit time, and one watt (W) is equal...

    A watt is a unit of energy per unit time, and one watt (W) is equal to one joule per second (1 J s). A 80.0- W incandescent light bulb produces about 4.00% of its energy as visible light. Assuming that the light has an average wavelength of 510.0 nm, calculate how many such photons are emitted per second by a 80.0-W incandescent light bulb Number 1.03 x 1019 photons/s

  • 2. The average person has 1.4 m2 of skin at a skin temperature of roughly 305...

    2. The average person has 1.4 m2 of skin at a skin temperature of roughly 305 K (90°F) Consider the average person to be an ideal radiator standing in a room at a temperature of 293 K (68°F) (a) Calculate the power (energy per uni i) radiated by the average person in the form of blackbody radiation; express your answer in erg s-1. What is the person's "wattage"? (1 W = 107 erg s-1) Compare this to a typical incandescent...

  • Question 16 (1 point) Visible light has wavelengths ranging between approximately 4000 and 7000 Angstroms (400...

    Question 16 (1 point) Visible light has wavelengths ranging between approximately 4000 and 7000 Angstroms (400 to 700 nanometres). Which of the following statements is true regarding the surface temperature of a star for which the wavelength of maximum intensity falls in the visible range t could never be cooler than 8000 K It must always be cooler than 5500 K t must lie between 8000 K and 5500 K It must always be hotter than 3500 K Question 17...

  • #2 please ! Ro le Astronomy 1F03 Problem Set 3 Thursday, Nov 10th, 2019 Write your...

    #2 please ! Ro le Astronomy 1F03 Problem Set 3 Thursday, Nov 10th, 2019 Write your answers on a separate sheet and show your work 1. The protesproton chain effectively c erta hyre en into hem according to 4 He. A Helium wus weighs 6.64518 x 10 IT kg and Hydrogen mucha proton) welches 1.67262 x 10 Workout the change in a when I kg of Hydrogen is converted completely into Helium 4. Convert the change in mass Per burning...

ADVERTISEMENT
Free Homework Help App
Download From Google Play
Scan Your Homework
to Get Instant Free Answers
Need Online Homework Help?
Ask a Question
Get Answers For Free
Most questions answered within 3 hours.
ADVERTISEMENT
ADVERTISEMENT
ADVERTISEMENT