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The Sun Erupts Credit: Skylab, NASA
Explanation: The Sun is a seething ball of extremely hot gas. Above, the Sun was captured by Skylab in 1973 throwing off one the largest eruptive prominences in recorded history. The Sun has survived for about 5 billion years, and
will
likely survive for another 5 billion. The Sun is not on fire, will never
explode, and a solar flare will never destroy the Earth. The Sun continues to
present many unanswered questions. For example: Why is the Sun's corona so
hot? What causes the Sun's unusual magnetic field? Why does the Sun's center
emit so few neutrinos?
You can find this photo and other exciting images on the
Astronomy Picture of the Day web site. Each day a different image or
photograph of our
fascinating universe is featured, along with a brief explanation written
by a
professional astronomer.


NASA's Solar Dynamics Observatory
It's a "coronal hole," a vast region where the sun's magnetic field has opened
up and allowed the solar wind to escape.
Indeed, a solar wind stream flowing from this hole is heading toward Earth, due
to arrive on June 7th or 8th
Award winning astrophotographer Thierry
Legault wanted to image the Hubble Space Telescope and space shuttle
Atlantis traveling together around Earth.
The suns core is at a temperature of 15.6 million
Kelvin,
the surface is 5800 and the pressure is 250 billion
Atmospheres

Russian astronomy amateur - Alexei Prudnikov.
Prominences on North-West of Sun, 4 September 2008.
Scope - TAL-75 as 2x afocal before Coronado PST, Barlow 3x.
Feefctive focal length is 2400mm.
Camera:
DMK 31AU.AS, 15 frames per second at 1024×768.
Scale is 100% of original.
Time of imaging is given by Moscow time (GMT+4h).
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