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English: Anatomy of a protoplanetary disk: As fine dust particles clump together deep inside the protoplanetary disk, ultraviolet radiation from a neaby hot star eats away at the disk. The outer portions of the gas bubble are then heated and removed by energetic ultraviolet radiation. Material falling from the disk toward the central object fuels twin gas jets. Links: NASA Press release Protoplanetary Disks in the Orion Nebula Proplyd in the Orion Nebula (1) Proplyd in the Orion Nebula (2) Proplyd in the Orion Nebula (3) Proplyd in the Orion Nebula (4) Proplyd in the Orion Nebula (5)
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Mkpọlọ́gwụ̀ https://hubblesite.org/contents/media/images/2001/13/1044-Image.html
Odé ákwụ́kwọ́ Illustration Credit: NASA, ESA, and A. Feild (STScI)

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Nkowapụta

Tinye nkọwa otu ahịrị ihe faịlụ a na-anochi anya ya.
Illustration of the dynamics of a proplyd

Ihe ndị egosiri na faịlụ a

depicts Bekee

image/jpeg

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dị ùgbu â20:03, 13 Septemba 2022NvóÁká màkà otù ȯ dị nà 20:03, 13 Septemba 20221,280 × 1,067 (198 KB)Nsae CompUploaded a work by Illustration Credit: NASA, ESA, and A. Feild (STScI) from https://hubblesite.org/contents/media/images/2001/13/1044-Image.html with UploadWizard

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