Radiation Pressure and Solar Sail

AI Thread Summary
To propel a spacecraft with a solar sail, the area of the sail must be calculated based on the momentum and pressure of sunlight. The pressure exerted on the sail can be derived from the relationship between force, area, and momentum. The gravitational force from the Sun must be countered by the force generated by the solar sail, which involves understanding the energy output of the Sun and its intensity at a given distance, such as Earth's orbit. The discussion highlights the need to connect concepts of luminosity, pressure, and impulse to determine the required sail area. Overall, a clear understanding of these relationships is essential for calculating the necessary parameters for effective propulsion.
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Consider a spacecraft attached to a sheet of material, a "sail," that absorbs sunlight. Assume that the sail is positioned to face the Sun and that the combined mass of the spacecraft and the sail is m. How large does the area of the sail have to be to propel the spacecraft away from the Sun? m = 1000 kg.

My thoughts on how to figure this out...

Calculate the momentum per unit area per unit time of the radiation leaving the Sun, which seems to me to be the pressure by this relation:

Pressure = Force/Area = momentum/(area*time)

Then find the force that arises from the pressure on the solar sail, and this needs to oppose the gravitational force of the Sun.

I think it is this: F = GMm/r2 = Ut/c
where momentum p = U/c, and it's derivative is F = Ut/c

And U is energy coming from the Sun. This is more of my confusion. I know Luminosity is energy per unit time, I just don't really know how to use all of this to get what I need. I think I am just missing some of the conceptual part that would help me relate everything and simply plug in the given mass.
 
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I think of it via the impulse formula F*Δt = change in momentum
For light, E = p*c so p = E/c and F = (E/Δt)/c = Intensity*Area/c.
The question doesn't say what distance from the sun. Earth orbit would be convenient; there the intensity is called the solar constant and it can be looked up in Wikipedia.
 
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