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Keterangan
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)
Tarikh
Sumber https://hubblesite.org/contents/media/images/2001/13/1044-Image.html
Pengarang Illustration Credit: NASA, ESA, and A. Feild (STScI)

Perlesenan

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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Illustration of the dynamics of a proplyd

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semasa03:04, 22 November 2025Gambar kenit bagi versi pada 03:04, 22 November 20252,400 × 2,000 (270 KB)wikimediacommons>OptimusPrimeBot#Spacemedia - Upload of https://www.spacetelescope.org/static/archives/images/original/opo0113i.jpg via Commons:Spacemedia

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