Question

Assuming that Earth (and its atmosphere) behaves like a flat disk perpendicular to the Sun's rays...

Assuming that Earth (and its atmosphere) behaves like a flat disk perpendicular to the Sun's rays and that all the incident energy is absorbed, calculate the force on Earth due to radiation pressure. What would it be for Pluto? What is the force on the Earth due to the sun's gravitational attraction? What is it for Pluto?

Homework Answers

Answer #1

here the sun reaching earth has an intensity 1400 w/m^2

1. Intensity at Pluto = 1400/(39.48^2) = 0.900 W/m^2[Distance of Pluto from Sun 39.48 AU]
2. Radiation pressure = I/c =1400/(3*10^8)
Force on earth = [pi*(6.0*10^6)^2*1400]/(3*10^8) N = 5.28*10^8 N
3. Force on Pluto = (5.28*10^8)*(0.900/14000)*(1.180/6.0)^2 = 1.31*10^4 N
4. Gravitational force on Earth = [(6.67*10^-11)*(1.989*10^30)*(6.0*10^24)...
= 3.58*10^26 N
5. Gravitational force on Pluto = (3.58*10^26)/[(39.48^2)*(600/1.3)] = 4.97*10^20 N
{mass of Pluto = 1.3*10^22 kg)

Know the answer?
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
Similar Questions
A particle in the solar system is under the combined influence of the Sun's gravitational attraction...
A particle in the solar system is under the combined influence of the Sun's gravitational attraction and the radiation force due to the Sun's rays. Assume that the particle is a sphere of density 830 kg/m3 and that all the incident light is absorbed. If its radius is less than some critical radius R, the particle will be blown out of the solar system. Calculate this critical radius. Note that the total radiation power of the Sun is 3.90 ×...
A particle in the solar system is under the combined influence of the Sun's gravitational attraction...
A particle in the solar system is under the combined influence of the Sun's gravitational attraction and the radiation force due to the Sun's rays. Assume that the particle is a sphere of density 1100 kg/m3 and that all the incident light is absorbed. If its radius is less than some critical radius R, the particle will be blown out of the solar system. Calculate this critical radius. Note that the total radiation power of the Sun is 3.90 ×...
At high noon (sun rays fall perpendicular to the surface of the earth), the sun delivers...
At high noon (sun rays fall perpendicular to the surface of the earth), the sun delivers 990 W to each square meter of a blacktop road, emissivity of 1 (blackbody). If the hot asphalt loses energy only by radiation, what is its equilibrium temperature?
It looks like there is an earth sized planet in the habitable zone of Proxima Centauri,...
It looks like there is an earth sized planet in the habitable zone of Proxima Centauri, located 4.2 ly from the solar system. It would be cool to send a probe to check it out. Perhaps the most reasonable way of doing this is to construct a very small micro-spaceship connected to a large flat screen which absorbs radiation: a solar sail. We will model the sail as a perfectly absorbing flat screen, and the sun's radiation as plane waves....
Like all light, the light from the sun is an electromagnetic wave. In the vicinity of...
Like all light, the light from the sun is an electromagnetic wave. In the vicinity of Earth, the average intensity of sunlight is about 1400W/m^2. For this problem, assume that sunlight is a monochromatic plane wave, so you can apply the equations for the energy and pressure of an EM wave. (a) What is the amplitude of the electric field at Earth? (b) If I go outside on a sunny day, the magnetic field sensor on my phone tells me...
Problem 2 a) What is the radiant power of the sun? b) What is the radiant...
Problem 2 a) What is the radiant power of the sun? b) What is the radiant power at the surface of the earth? c) Calculation of the solar constant d) How much energy does the earth absorb? e) Using the equilibrium condition to calculate the earth’s temperature (W/O atmosphere) ? (Give a brief comment regarding your findings) f) Using the equilibrium condition to calculate the earth’s real temperature (W/ atmosphere)? (Give a brief comment regarding your findings) Problem 3 (Very...
This is from Principles of Planetary Climate, Problem 1.13 The thick CO2 atmosphere of Venus is...
This is from Principles of Planetary Climate, Problem 1.13 The thick CO2 atmosphere of Venus is nearly opaque in the infrared, so observations of Venus in the infrared spectrum provide no direct information about the temperature of the ground. However, the atmosphere is nearly transparent to microwave radiation, so the microwave emission of the planet can be used to infer its surface temperature. Indeed, this is how it was inferred in the 1960s that the surface of the planet was...
1. Inside a Red Giant, denser elements fuse and emit sufficient energy to balance thermal expansion...
1. Inside a Red Giant, denser elements fuse and emit sufficient energy to balance thermal expansion versus gravity, until fusion of: silica & sulphur helium carbon & oxygen iron deuterium & tritium 2. Structure of the Universe: 2dF and the Sloan Microwave Digital Survey plotted clusters of galaxies. What kind of structure was seen among super-clusters of galaxies? Filaments of galaxies surround voids that have no or very few galaxies inside. Super-clusters expand outward from a Big Bang source. Super-clusters...
A grey body is one whose absorptivity 1. does not vary with temperature and wavelength of...
A grey body is one whose absorptivity 1. does not vary with temperature and wavelength of the incident ray 2. is equal to its emissivity 3. varies with temperature 4. varies with wavelength of the incident ray A liquid is in equilibrium with its vapor at its boiling point. On an average, the molecules in the liquid and gaseous phases have equal 1. potential energy. 2. kinetic energy. 3.temperature. 4. intermolecular forces of attraction. A liquid of density 1000 kg/m3...
ch 6 1: It is generally a good idea to gain an understanding of the "size"...
ch 6 1: It is generally a good idea to gain an understanding of the "size" of units. Consider the objects and calculate the kinetic energy of each one. A ladybug weighing 37.3 mg flies by your head at 3.83 km/h . ×10 J A 7.15 kg bowling ball slides (not rolls) down an alley at 17.5 km/h . J A car weighing 1260 kg moves at a speed of 49.5 km/h. 5: The graph shows the ?-directed force ??...