Pela Seri - Wikimedia Commons

Wikimedia Commons

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A close-in image of a protoplanetary disc HH 30 around a newly formed star produced by NASA/ESA/CSA James Webb Space Telescope. It is surrounded by jets and a disc wind, and is located in the dark cloud LDN 1551 in the Taurus Molecular Cloud. Herbig-Haro objects are small nebulae found in star formation regions, marking the locations where gas outflowing from young stars is heated into luminescence by shockwaves. HH 30 is an example of where this outflowing gas takes the form of a narrow jet. The source star is located on one end of the jet, hidden behind an edge-on protoplanetary disc that the star is illuminating.

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Cıkewtış

geyrayış?: zewmi gırey, geyrayışi rê butonê seri bıtıknê. Atom warikerdıs.
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Xısusiyeti

Şıma yi ya sıfte yeni commons se, resimi wesi'ra, resimi qelite'dı yana zi resimi hususi'ra dewam keri. tayzi resme wesi esti bewni re: Fotrafberan u xizberana bere bıslas ni.

Zerrek

Images from August 13