Above: Sun before eclipse starts --Note: a few sunspots are visible
Above: Beginning of eclipse
Above: Continues with some hazines as cloud coverage increases
Above:: About half the sun is now covered by the moon
Above: Close to Maximum Coverage by Moon during Solar Eclipse in NYC April 8,2024
Above: Maximum Coverage by Moon during Solar Eclipse in NYC April 8,2024
Above: Moon starts to pull away
Never look directly at the Sun
The Sun is a star -- ”the closest one to Earth. It is a large ball of very hot gas. The air we breathe and the helium in a balloon are both gases. The Sun is very hot. It is over 5,000 °F at the surface, and much hotter at the center. The Sun is made of mostly hydrogen (70%) and helium (28%). It turns more hydrogen into helium every second.
The Sun makes light and heat that warms the surface of the Earth and makes plants grow. We can get food from plants, and we can burn wood and other parts of plants to cook, warm our houses, and make cars go. Without the Sun there would be no life on Earth.
The Sun is very big - much, MUCH bigger than the Earth! It is more than a million kilometers or 109 Earths across and contains more than 99.9% of the Solar System's mass. If you could stand on the surface of the Sun, you would weigh 28 times as much as you do on Earth because the Sun is so big.
More than a million Earths could fit beneath the surface of the Sun! It doesn't look that big from Earth, though. That's because the Sun is so far away. Compared to other stars, the Sun is about average-sized.
The entire Solar System is inside the atmosphere of the Sun. A very thin solar wind of gases blows from the Sun all the way to the edge of the Solar System, until it hits the wind between the stars.
Dark areas are sunspots
Sunspots look like dark spots on the Sun. But they are still bright — brighter than lightning. They are a little cooler, too. But they are still hot — about 2000 °C (3600 °F). Spots are caused by changes in the Sun's magnetic field, and usually form in groups which are carried around the Sun as it rotates.
The number of sunspots we see goes up and down every 11 years. Sometimes, prominences and solar flares form in or near sunspots.
Above the photosphere, the Sun’s gases are not very dense at all. There are two layers that we can see with special telescopes. Above that, gases stream out as solar wind that reaches to the edge of the Solar System.
A closeup view of a sunspot and prominencesIf you have a telescope with special filters, you can see bumps around the edge of the Sun. Each one of these is called a prominence. They look like volcanoes erupting. They are hundreds or thousands of kilometers long. Some are bigger than the Earth. They often seem to come from sunspots. Sometimes they get so far away from the Sun that they fly away from it. Then they are called solar flares.
Chromosphere means "color ball". It is just above the photosphere. It is not as bright as the photosphere, and you can’t normally see it. But you can see it just before a solar eclipse (only with special filters!). It looks like a flash of all the colors of light.
Solar eclipses occur when the moon passes in between the Earth and the Sun.
Above image courtesy of weather.com