Exif MM * z > ; ! i An X-ray flare from a very young star, or "protostar," detected by Chandra may reset the timeline for when scientists think Sun-like stars start blasting high-energy radiation into space. This illustration shows HOPS 383 surrounded by a donut-shaped cocoon of material (dark brown) that is falling in towards the central star. Much of the light from the infant star is unable to pierce this material, but X-rays from the flare (blue) can. Infrared light is scattered off the inside of the cocoon (white and yellow). An inset shows the Chandra image of the flare, which lasted over 3 hours, taken during observations in December 2017. Chandra X-ray Observatory Center 0231 http://ns.adobe.com/xap/1.0/
Chandra X-ray Observatory Center
HOPS 383
An X-ray flare from a very young star, or "protostar," detected by Chandra may reset the timeline for when scientists think Sun-like stars start blasting high-energy radiation into space. This illustration shows HOPS 383 surrounded by a donut-shaped cocoon of material (dark brown) that is falling in towards the central star. Much of the light from the infant star is unable to pierce this material, but X-rays from the flare (blue) can. Infrared light is scattered off the inside of the cocoon (white and yellow). An inset shows the Chandra image of the flare, which lasted over 3 hours, taken during observations in December 2017.
X-rays From a Newborn Star Hint at Our Sun's Earliest Days
B.3.1.1
1,400
Chandra X-ray Observatory
ACIS
Blue
X-ray
83870
18927, 20882,20883
8.3882938723006E+01
-4.9921994577078E+00
296
346
69.5
258.5
http://chandra.harvard.edu/photo/image_use.html
VPhotoshop 3.0 8BIM Z %G :X-rays From a Newborn Star Hint at Our Sun's Earliest Days HOPS 3837 20200618P Chandra X-ray Observatory Centeri By detecting an X-ray flare from a very young star using NASA's Chandra X-ray Observatory, researchers have reset the timeline for when stars like the Sun start blasting high-energy radiation into space.n X-ray: NASA/CXC/Aix-Marseille Uns Chandra X-ray ObservatoryxyAn X-ray flare from a very young star, or "protostar," detected by Chandra may reset the timeline for when scientists think Sun-like stars start blasting high-energy radiation into space. This illustration shows HOPS 383 surrounded by a donut-shaped cocoon of material (dark brown) that is falling in towards the central star. Much of the light from the infant star is unable to pierce this material, but X-rays from the flare (blue) can. Infrared light is scattered off the inside of the cocoon (white and yellow). An inset shows the Chandra image of the flare, which lasted over 3 hours, taken during observations in December 2017.8BIM% r]?[+[n$ l Adobe d `
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