pipplo_imp
JWST - NGC 2070 - The Tarantula Nebula - MIRI - Magnification and reconstruction via AI
Reconstruction using our artificial intelligence model of the photo acquired by the JWST through the MIRI.
This is a different image from the one obtained, again from, JWST, via the NIRCam. The MIRI (Mid-Infrared Instrument) was used here. We can see the central part of the Tarantula nebula under a new mode. In this light, the cluster's hot young stars lose their brilliance and glowing gas and dust come forward. Abundant hydrocarbons illuminate the surfaces of the dust clouds, highlighted in blue and violet. Much of the nebula takes on a more spectral and diffuse appearance because the mid-infrared light is better able to show what is happening in the depths of the clouds.
The file is available at 170.56 million pixels for download at a resolution of 15000x11371 pixels.
Credit:NASA/ESA/CSA/STScI/PipploIMP(for AI upscaling)
Our Facebook Page: bit.ly/PipploFB
Our YouTube Channel: bit.ly/PipploYT
JWST - NGC 2070 - The Tarantula Nebula - MIRI - Magnification and reconstruction via AI
Reconstruction using our artificial intelligence model of the photo acquired by the JWST through the MIRI.
This is a different image from the one obtained, again from, JWST, via the NIRCam. The MIRI (Mid-Infrared Instrument) was used here. We can see the central part of the Tarantula nebula under a new mode. In this light, the cluster's hot young stars lose their brilliance and glowing gas and dust come forward. Abundant hydrocarbons illuminate the surfaces of the dust clouds, highlighted in blue and violet. Much of the nebula takes on a more spectral and diffuse appearance because the mid-infrared light is better able to show what is happening in the depths of the clouds.
The file is available at 170.56 million pixels for download at a resolution of 15000x11371 pixels.
Credit:NASA/ESA/CSA/STScI/PipploIMP(for AI upscaling)
Our Facebook Page: bit.ly/PipploFB
Our YouTube Channel: bit.ly/PipploYT