試卷名稱:110年 - 110 國立中山大學碩士暨碩士專班招生考試_物理系碩士班:普通物理#105961
年份:110年
科目:研究所、轉學考(插大)◆普通物理學
19. There is an interesting experiment that enables us to estimate the mass density of the sun. Consider (see Figure 5) an experimental setup that can get an image of the sun through a pinhole. The distance between the pinhole and the screen is d, and the diameter of the image is D. Because light propagates in a straight line (neglect geometrical distortions), you can obtain the angle θin terms of d and D. Therefore, the relationship between R and r can be exhibited, where R is the radius of the sun and r is the distance between the earth and the sun. It is known that the earth orbits the sun by the period
days. Assume that the earth makes a circular orbit around the sun, and the sun is a perfect sphere. From these hints, the mass density of the sun p is given by

(A)
(B)
(C)
(D)
, where G=
is the gravitational constant.