How Large Should a Solar Sail Be to Counteract the Sun's Gravitational Pull?

In summary, a proposed method for propelling a spaceship in the solar system using radiation pressure and a large sail made of foil requires a sail with a surface area of approximately 1.14 million square meters in order to equal the magnitude of the Sun's gravitational attraction. This calculation is based on the assumptions of a perfectly reflecting sail and perpendicular orientation to the Sun's rays, as well as given values for the Sun's mass, rate of energy emission, and the gravitational constant.
  • #1
ft92
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Homework Statement


t has been proposed that a spaceship might be propelled in the solar system by radiation pressure, using a large sail made of foil.

Assume that the mass of the ship + sail is 1780.4 kg, that the sail is perfectly reflecting, and that the sail is oriented perpendicular to the Sun's rays. How large must the surface area of the sail be if the radiation force is to be equal in magnitude to the Sun's gravitational attraction?

The rate at which the Sun emits energy is 3.90 × 1026 W. The Sun's mass is 1.99 × 1030 kg. The gravitational constant is 6.67 × 10-11 N m2/kg2.

Homework Equations


Preflect= 2Ef cos2ϑ /c

The Attempt at a Solution



Ef= (3.9×1026 W)/A = (3.9 ×1026)/ 4πR2 = 3.1×1025/R2

let surface area be Af :

force on ship= Preflect Af= (2×3.1×1025×cos20)(Af)/ 3×108×R2

F= 2.07×1017 (Af)/R2

Fgravitational at R= GMm/R2 = (6.67×10-11×1.99×1030×1780.4)/R2

let F=Fgrav =(6.67×10-11×1.99×1030×1780.4)/(2.07×1017)= 1.14 ×106m2 do you agree with my result?
 
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  • #2
The result looks reasonable. Just over a kilometer square.
 
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FAQ: How Large Should a Solar Sail Be to Counteract the Sun's Gravitational Pull?

What is radiation pressure?

Radiation pressure is the pressure exerted by electromagnetic radiation on a surface. It is caused by the transfer of momentum from photons (particles of light) to the surface they strike.

How is radiation pressure calculated?

Radiation pressure is calculated using the equation P = F/A, where P is the pressure, F is the force exerted by the radiation, and A is the area of the surface. The force can be calculated using the equation F = Δp/Δt, where Δp is the change in momentum and Δt is the change in time.

What are the potential applications of radiation pressure?

Radiation pressure has a variety of potential applications, including solar sails for spacecraft propulsion, optical tweezers for manipulating tiny particles, and pressure sensors for measuring small forces.

How does radiation pressure affect objects in space?

In space, radiation pressure can have a significant impact on objects such as comets and asteroids. As they travel closer to the sun, they may experience radiation pressure from solar wind, which can cause their orbits to change.

Can radiation pressure be harmful to humans?

Radiation pressure from visible light is generally not harmful to humans, as it is very small compared to other forces we experience. However, high levels of radiation pressure from sources such as X-rays and gamma rays can be dangerous and can cause damage to cells and tissues.

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