Home
Class 12
PHYSICS
The incident intensity on a horizontal s...

The incident intensity on a horizontal surface at sea level from the sun is about `1kW m^(-2)`.
Assuming that 50 per cent of this intensity is reflected and 50 per cent is absorbed, determine the radiation pressure on this horizontal surface (in pascals).

A

`8.2xx10^(-2)`

B

`5xx10^(-6)`

C

`6xx10^(-12)`

D

`8xx10^(-11)`

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem of determining the radiation pressure on a horizontal surface due to sunlight, we can follow these steps: ### Step 1: Understand the Given Data The intensity of sunlight incident on the surface is given as: - \( S = 1 \, \text{kW/m}^2 = 1000 \, \text{W/m}^2 \) It is stated that: - 50% of this intensity is reflected. - 50% of this intensity is absorbed. ### Step 2: Calculate the Pressure from Absorbed Light The pressure exerted by the absorbed light can be calculated using the formula: \[ P_{\text{absorbed}} = \frac{S_{\text{absorbed}}}{c} \] Where: - \( S_{\text{absorbed}} = 0.5 \times S = 0.5 \times 1000 \, \text{W/m}^2 = 500 \, \text{W/m}^2 \) - \( c \) is the speed of light, approximately \( 3 \times 10^8 \, \text{m/s} \). Thus, the pressure from absorbed light is: \[ P_{\text{absorbed}} = \frac{500}{3 \times 10^8} \, \text{Pa} \] ### Step 3: Calculate the Pressure from Reflected Light The pressure exerted by the reflected light is given by: \[ P_{\text{reflected}} = \frac{2S_{\text{reflected}}}{c} \] Where: - \( S_{\text{reflected}} = 0.5 \times S = 500 \, \text{W/m}^2 \) Thus, the pressure from reflected light is: \[ P_{\text{reflected}} = \frac{2 \times 500}{3 \times 10^8} \, \text{Pa} = \frac{1000}{3 \times 10^8} \, \text{Pa} \] ### Step 4: Calculate Total Radiation Pressure The total radiation pressure \( P_{\text{total}} \) on the surface is the sum of the pressures from absorbed and reflected light: \[ P_{\text{total}} = P_{\text{absorbed}} + P_{\text{reflected}} \] Substituting the values we calculated: \[ P_{\text{total}} = \frac{500}{3 \times 10^8} + \frac{1000}{3 \times 10^8} \] \[ P_{\text{total}} = \frac{1500}{3 \times 10^8} \, \text{Pa} \] \[ P_{\text{total}} = \frac{1500}{3} \times 10^{-8} \, \text{Pa} = 500 \times 10^{-8} \, \text{Pa} = 5 \times 10^{-6} \, \text{Pa} \] ### Final Answer The radiation pressure on the horizontal surface is: \[ P_{\text{total}} = 5 \times 10^{-6} \, \text{Pa} \]

To solve the problem of determining the radiation pressure on a horizontal surface due to sunlight, we can follow these steps: ### Step 1: Understand the Given Data The intensity of sunlight incident on the surface is given as: - \( S = 1 \, \text{kW/m}^2 = 1000 \, \text{W/m}^2 \) It is stated that: - 50% of this intensity is reflected. ...
Promotional Banner

Topper's Solved these Questions

  • PHOTOELECTRIC EFFECT

    CENGAGE PHYSICS ENGLISH|Exercise Integer|9 Videos
  • PHOTOELECTRIC EFFECT

    CENGAGE PHYSICS ENGLISH|Exercise Single Correct Answer Type|7 Videos
  • PHOTOELECTRIC EFFECT

    CENGAGE PHYSICS ENGLISH|Exercise Multiple Correct|10 Videos
  • NUCLEAR PHYSICS

    CENGAGE PHYSICS ENGLISH|Exercise ddp.5.5|14 Videos
  • RAY OPTICS

    CENGAGE PHYSICS ENGLISH|Exercise DPP 1.6|12 Videos

Similar Questions

Explore conceptually related problems

The incident intensity on a horizontal surface at sea level from the sun is about 1kW m^(-2) . Q. Find the ratio of this pressure to atmospheric pressure p_0 (about 1xx10^(5) Pa) at sea level

The mean intensity of radiation on the surface of the Sun is about 10^(s)W//m^2 . The rms value of the corresponding magnetic field is closed to :

A monochromatic beam of light (lamda=4900A) incident normally upon a surface produces a pressure of 5xx10^(-7)Nm^(-2) on it. Assume that 25% of the light incident in reflected and the rest absorbed. Find the number of photons falling per second on a unit area of thin surface

When the sun is directly overhead, the surface of the earth receives 1.4 xx (10^3) W (m^-2) of sunlight. Assume that the light is monochromatic with average wavelength 500mn and that no light is absorbed in between the sun and the earth's surface. The distance between the sun and the earth is 1.5 xx (10^11) m. (a) Calculate the number of photons falling per second on each square metre of earth's surface directly below the sun. (b) How many photons are there in each cubic metre near the earth's surface at any instant? (c) How many photons does the sun emit per second?

A block A of mass 2 kg rests on a horizontal surface. Another block B of mass 1 kg moving at a speed of m/s when at a distance of 16 cm from A. collides elastically with A. The coefficeint of friction between the horizontal surface and earth of the blocks is 0.2. Then (g = 10 m//s^(2))

The intensity of direct sunlight befor it passes through the earth's atmosphere is 1.4kW|m^2 . If it is completely absorbed, find the corresponding radiation pressure.

A block slides with a velocity of 10 m/sec. on a rough horizontal surface. It comes to rest after covering of 50 m. If g is 10 m/ sec^(2) , then the coefficient of dynamic friction between the block and surface is

The intensity of sound from a point source is 1.0 xx 10^-8 Wm^-2 , at a distance of 5.0 m from the source. What will be the intensity at a distance of 25 m from the source ?

A family uses 8kW of power. (a) Direct solar energy is incident on the horizontal surface at an average rate of 200 W per square metre. If 20% of this energy can be converted to useful electrical energy, how large an area is needed to supply 8kW? (a) Compare this area to that of the roof of a typical house.

Express : 80 cm as a per cent of 2 m 50 cm

CENGAGE PHYSICS ENGLISH-PHOTOELECTRIC EFFECT-Linked Comprehension
  1. in an experimental set up to study the photoelectric effect a point so...

    Text Solution

    |

  2. in an experimental set up to study the photoelectric effect a point so...

    Text Solution

    |

  3. The incident intensity on a horizontal surface at sea level from the s...

    Text Solution

    |

  4. The incident intensity on a horizontal surface at sea level from the s...

    Text Solution

    |

  5. Light of intensity I falls along the axis on a perfectly reflecting ri...

    Text Solution

    |

  6. Light of intensity I falls along the axis on a perfectly refleccting r...

    Text Solution

    |

  7. An experimental setup of verification of photoelectric effect is shown...

    Text Solution

    |

  8. An experimental setup of verification of photoelectric effect is shown...

    Text Solution

    |

  9. An experimental setup of verification of photoelectric effect is shown...

    Text Solution

    |

  10. An experimental setup of verification of photoelectric effect is shown...

    Text Solution

    |

  11. An experimental setup of verification of photoelectric effect is shown...

    Text Solution

    |

  12. Light having photon energy hupsilon is incident on a metallic plate ha...

    Text Solution

    |

  13. Light having photon energy hupsilon is incident on a metallic plate ha...

    Text Solution

    |

  14. Light having photon energy hupsilon is incident on a metallic plate ha...

    Text Solution

    |

  15. When light of sufficiently high frequency is incident on a metallic su...

    Text Solution

    |

  16. When light of sufficiently high frequency is incident on a metallic su...

    Text Solution

    |

  17. When light of sufficiently high frequency is incident on a metallic su...

    Text Solution

    |

  18. The energy reveived from the sun by the earth and surrounding atmosphe...

    Text Solution

    |

  19. The energy reveived from the sun by the earth and surrounding atmosphe...

    Text Solution

    |

  20. The energy reveived from the sun by the earth and surrounding atmosphe...

    Text Solution

    |