The deflection angle of a ray grazing the sun refers to the amount by which the path of a light ray is bent when it passes near the sun. This phenomenon is known as gravitational lensing and is a result of the sun's massive gravitational pull.
The deflection angle of a ray grazing the sun can be calculated using Einstein's general theory of relativity. This theory predicts the amount of deflection based on the mass of the sun and the distance between the ray of light and the center of the sun.
The deflection angle of a ray grazing the sun is significant because it provides evidence for the theory of relativity and helps us understand the effects of gravity on light. It also allows us to observe and study distant objects that would otherwise be hidden behind the sun.
Yes, the deflection angle of a ray grazing the sun can be observed during a solar eclipse. When the moon passes in front of the sun, it blocks out the light from the sun, allowing us to see the light from distant stars that have been deflected by the sun's gravity.
Yes, the deflection angle of a ray grazing the sun can change over time due to fluctuations in the sun's mass and the distance between the ray of light and the sun. However, these changes are very small and can only be measured with advanced technology.