eclips
????? I'd call that IMPOSSIBLE. The only time there would be equal amounts of sun on all parts of the earth would be during a solar eclipse, at which time there would be no sunlight reaching anypart of the earth.
A bit over 8 minutes, it is the time it takes sunlight to reach the earth.
Sunlight And Time Of Day
Mars is a little over half the size of Earth.
The angle of sunlight hitting the earth affects the amount of energy the earth receives because sunlight is spread over a larger area when it hits at a lower angle, resulting in less concentrated energy. This can impact the intensity of heat and light received at the surface, influencing weather patterns and climate.
there classified as one of the sperm parts that go all over and don't insert
When sunlight hits Earth at an angle smaller than ninety degrees, the energy is spread over a larger surface area, resulting in less energy per unit area. This leads to lower intensity of sunlight and reduced heating compared to when sunlight hits directly overhead.
An isohel on a map joins places of equal amount of sunlight received over a specific period of time, typically in a day. It is used to display the distribution of light and helps identify areas receiving similar levels of sunlight.
The equator receives the most direct sunlight, that is, the most Wm-2. The sun shines most directly over the Tropics, and specifically the equator, throughout the year, creating a net surplus in energy which is redistributed towards the poles. In terms of the number of hours of sunlight, all points on Earth receive the same amount over the course of a year, but the angle at which it is received is very different at different latitudes.
"To reflect the sun to the moon?" Your question does not make sense as worded. It takes a little over a second for sunlight to reflect from the moon to earth, if that is what you are asking. The sun does not reflect anything--it can't. Sunlight takes 8.3 minutes to reach the moon, then a bit over a second to get from the moon to earth.
The latitude of an area on Earth affects the amount of sunlight it receives because it determines the angle at which sunlight hits the surface. Areas closer to the equator receive more direct sunlight as the sun is overhead, leading to warmer temperatures. In contrast, areas closer to the poles receive sunlight at a lower angle, spreading the energy over a larger area and resulting in colder temperatures.
Sunlight that lands directly on the equator is spread out the least across the Earth's surface since it is perpendicular, providing the most energy (heat) per unit area. Near the poles, the angle of incidence of the sun's rays spread them out over a much greater area, providing less energy (heat) per unit area.