Балкански 2007, Теория — Задача 2. The solar sail
Concours Général de Physiques “Minko Balkanski” — 20 mai 2007 · 20 май 2007 г.
Указания
The two exercices are independent.
All the answers must be given in English or in French*. The clarity and the precision will be taken into account for the final note.*
The exam is 4 hours long.
Условие
2. We are now interested by the launching of the sail. In the following table we plot the solar energy flow, in , at the vicinity of a planet, as a function of the planet-sun distance in Astronomical Units A.U. We recall that one astronomical unit is the distance between the Sun and the Earth : 1 A.U. .
| Planet | Distance to the Sun (A.U.) | Sun energy flow () | Flow Distance |
|---|---|---|---|
| Mercury | 0.387 | 9134 | |
| Venus | 0.723 | 2617 | |
| Earth | 1 | 1368 | |
| Mars | 1.524 | 589 | |
| Jupiter | 5.203 | 50.53 | |
| Saturn | 9.539 | 15.03 | |
| Uranus | 19.182 | 3.718 | |
| Neptune | 30.057 | 1.514 | |
| Pluto | 39.750 | 0.8657 |
2.a) What is the relationship between the energy flow and the flow of photons , if the mean energy per photon is ? Give then a simplified expression of the radiation force on the sail.
2.b) If the sail is to attain a high speed, is it more advantageous to launch it in the vicinity of Mercury or Neptune ? Why ?
2.c) Fill up the forth column of the table by the product of the energy flow times the square of the planet-sun distance. What is to be noticed ? Provide an explanation.
2.d) Show then that the radiation fore can be written :
with the planet-Sun distance and a constant that will be calculated numerically, in S.I. units.
Решение
Внимание: Непълно решение
В архива няма официално решение на тази задача.
Оригинал в Архива: CGP_2007_en.pdf