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NGC 346 - From Hubble to Webb Space Telescopes
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This video compares images of star-forming region NGC 346 taken in visible light with the Hubble Space Telescope’s ACS instrument, near-infrared with the James Webb Space Telescope’s NIRCam instrument, and mid-infrared with Webb’s MIRI instrument.
Hubble’s visible-light image is filled with thousands of stars, as well as curtains of hydrogen and oxygen gas colored blue. In Webb’s near-infrared image, pink represents energized hydrogen, while orange represents dense, molecular hydrogen. Webb’s mid-infrared image highlights bright patches of star formation, diffuse pink emission from warm dust, and blue filaments of dusty and sooty material.
Credit: NASA, ESA, CSA, A. Pagan (STScI)
#Hubble #hubbletelescope #webb #NASAWebb #JWST #astronomy #MIRI #infrared #space
Hubble’s visible-light image is filled with thousands of stars, as well as curtains of hydrogen and oxygen gas colored blue. In Webb’s near-infrared image, pink represents energized hydrogen, while orange represents dense, molecular hydrogen. Webb’s mid-infrared image highlights bright patches of star formation, diffuse pink emission from warm dust, and blue filaments of dusty and sooty material.
Credit: NASA, ESA, CSA, A. Pagan (STScI)
#Hubble #hubbletelescope #webb #NASAWebb #JWST #astronomy #MIRI #infrared #space