Home https://server7.kproxy.com/servlet/redirect.srv/sruj/smyrwpoii/p2/ World https://server7.kproxy.com/servlet/redirect.srv/sruj/smyrwpoii/p2/ NASA news: The sun spewed only COLD MATERIAL in the room – What happens? | Science | News

NASA news: The sun spewed only COLD MATERIAL in the room – What happens? | Science | News

The sun is the only hottest object in our solar system, with a core bearing at an incredible 15 million degrees Celsius. The surface temperatures of the Sun are just as scary and reach as high as 5.540C (10,000 Fahrenheit). And the sun's corona – the outer layer of the star's atmosphere – burns hundreds of times warmer than the sun's surface. So how did NASA on Friday, June 28, see a violent outbreak of cold material in the Sun's upper atmosphere?

The sunrise was a so-called sunrise or a light function that extends from the sun.

Sun prominences are ejected from the sun as a whip or tentacle attached to the sun's surface.

These events are typically played during a day, but have been known to hang around for months at a time.

When solar energy highlights the sun, it runs back to the star, and sometimes extends hundreds of thousands of miles in space.

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On Friday, June 28, NASA's Solar Dynamics Observatory (SDO) registered a of these highlights on the Sun.

Seen from the Earth, these features resemble a loop of loose thread that moves out of a jacket lining.

But how exactly are these solar observations cold?

NASA explains oath: "Solar prominence is loosening of relatively cold, dense solar material that is suspended in the sun's super-warm outer atmosphere.

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9659002] "Because they are colder and denser than their surroundings, they are easily observed by SDO's 304 Angstrom telescope."

NASA's Angstrom telescope is a modern instrument that observes the light that The helium gas burns at an incredible 5,000C (9,000F) while the surrounding corona can reach "a few million degrees Fahrenheit."

NASA said, "Prominences like the Most sun blinds form over active areas: places where the sun's magnetic field is particularly intense and complex.

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"Active regions can last several months, making more trips around the sun – every complete sun shift is known as a Carrington rotation and takes about 27 days. "

These events are quite difficult to track unless the sun experiences a solar minimum when solar activity falls.

But, the sun is below its solar minimum right now.

So the appearance was not cold in the same way as the ice is cold on Earth, but was considerably colder than the peak temperatures in the sun's corona.

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