New imagery of the Large Magellanic Cloud reveals the structural layers of star formation.
The James Webb Space Telescope has released a new image of LHA 120-N 159, a star-forming region located 161,000 light-years away in the Large Magellanic Cloud. Spanning 230 light-years, the photograph captures an H II region filled with ionized hydrogen gas. The visual data highlights thick orange clouds composed of polycyclic aromatic hydrocarbons and pale blue areas representing ionized gas. Dark red filaments of cool molecular hydrogen appear as dense structures that protect growing stars from radiation and stellar winds. The image also features the Papillon Nebula, a compact blob of ionized hydrogen first documented by Hubble in 1999. These new observations show stars as points of light embedded within orange gas pillars and molecular filaments. The region is estimated to be less than three million years old, providing a detailed look at active cosmic birth and molecular distribution.
Image-makers can study how different light wavelengths distinguish chemical compositions and physical depths within a single frame. The clear separation of orange hydrocarbons, blue ionized gas, and red filaments provides a reference for complex color grading and layered compositions.
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