An eclipse is an astronomical event that can be seen from space and Earth and has unique characteristics that change depending on the observer’s location. This happens when the sun, moon and Earth are in a certain alignment and causes rings such as the red moon and even turns day into night. Next, check out the difference between a solar eclipse and a lunar eclipse.
Read more:
Learn the difference between a solar eclipse and a lunar eclipse
As mentioned earlier, the eclipse seen from our planet is the result of the alignment of three stars: the Sun, Moon, and Earth. This event is only possible because most objects in our solar system, except for the Moon, revolve around the Sun, and this causes the stars to take different positions from time to time.
Although the Moon does not revolve around the Sun, it revolves around the Earth, so it also moves. As a result, these space objects (the Sun, Moon, and Earth) rotate and eventually line up in front of each other, causing an astronomical event called an eclipse.
Through this alignment, it is possible to observe different events, as the position of each star directly reflects what we can observe. Hey Solar eclipse It occurs when the Moon passes in front of the Earth, completely or partially blocking the sun’s brightness. In this way, it is possible to observe three different forms of solar eclipse:
Hey Lunar eclipse It occurs when the Earth passes between the Sun and the Moon, causing it to cast its shadow on the satellite. This movement can cause two different variations.
- Penumbral lunar eclipse: It occurs when the Moon travels a path through the Earth’s penumbra, changing its appearance in a way that is very subtle to those on Earth. In other words, it is as if the moon has become darker;
- Umbrella lunar eclipse: This occurs when the moon passes into the darkest part of the Earth’s shadow, causing a drastic change in its appearance, as the satellite begins to display a reddish or coppery glow due to scattering sunlight.
