File:Hops383-1.jpg

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X-Ray image of HOPS 383 while flaring.

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	00:27, 11 September 2021		864 × 864 (89 KB)	RiverWalker88 (talk \| contribs)	X-Ray image of HOPS 383 while flaring.

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Astronomy/DSOs

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Image title	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.
Author	Chandra X-ray Observatory Center
Date and time of data generation	18 June 2020
Orientation	Normal
Exif version	2.31
Color space	Uncalibrated
Source	Chandra X-ray Observatory
Headline	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.
Credit/Provider	X-ray: NASA/CXC/Aix-Marseille University/N. Grosso et al.; Illustration: NASA/CXC/M. Weiss
Unique ID of original document	5D095F52C15A27FBCB7FE013006EE232
Date metadata was last modified	08:54, 10 August 2020
Keywords	HOPS 383
Short title	X-rays From a Newborn Star Hint at Our Sun's Earliest Days
Contact information	cxcpub@cfa.harvard.edu http://chandra.harvard.edu 60 Garden St. Cambridge, MA, 02138 USA 617.496.7941
Usage terms	http://chandra.harvard.edu/photo/image_use.html
IIM version	4