Star Cluster Duo of NGC 460 and NGC 456 (Webb & Hubble composite) - section
Star Cluster Duo of NGC 460 and NGC 456 (Webb & Hubble composite) - section
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Two neighboring star clusters, NGC 460 and NGC 456, shine in this striking composite created from the combined observations of NASA’s Hubble Space Telescope and the James Webb Space Telescope. Together, the two reveal both the bright, glowing gas shaped by stellar radiation and the intricate web of dust where new stars continue to form.
Open clusters like these are groups of stars loosely bound by gravity, often numbering in the hundreds or thousands. Within them, gas and dust collapse under gravity to create new stars. As young, massive stars emit intense winds and radiation, they carve out cavities and ignite nearby material, triggering even more star formation.
Hubble’s visible and near-infrared view captures the brilliant blue glow of ionized gas, while Webb’s infrared vision unveils the red, dusty regions rich with stellar birth. Together, they offer a dynamic view of how energy and matter interact to shape the evolution of galaxies.
Image courtesy of NASA, ESA/Webb
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