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lilacbat112Lv1
31 Mar 2019
Assuming the light is emitted uniformly in all
directions, at what distance from the lamp will
the rate of green photons flowing outward (the
“intensity”) be 106 photons.cm-2
.s-1 (i.e. 1
million photons per square cm per second)?
This is approximately the apparent brightness
of a bright star.
Assuming the light is emitted uniformly in all
directions, at what distance from the lamp will
the rate of green photons flowing outward (the
“intensity”) be 106 photons.cm-2
.s-1 (i.e. 1
million photons per square cm per second)?
This is approximately the apparent brightness
of a bright star.
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Elin HesselLv2
1 Apr 2019
Related textbook solutions
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Solar Sail
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A solar sail allows a spacecraft to use radiation pressure for propulsion, similar to the way wind propels a sailboat. The sails of such spacecraft are made out of enormous reflecting panels. The area of the panels is maximized to catch the largest number of incident photons, thus maximizing the momentum transfer from the incident radiation.
For such spacecraft to work, the force from the radiation pressure exerted by the photons must be greater than the gravitational attraction to the star emitting the photons. The critical parameter is the area density (mass per unit area) of the sail.
To solve the second part of this problem you will need to know the following:
Isun(R) = 3.2 x10251/R2 (W/m2)
and
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