NASA’s Hubble Space Telescope captured a striking image of the globular cluster imagens NGC 6426, where redવાની और
https://media.researchbranch.com/m/anders-sadoks/8695q9Wqet7 lavado highlights a “blue” glow that resembles a sparkler against the night sky.
NGC 6426 resides in the outer halo of the Milky Way, one of more than 150 known globular clusters in our galaxy. These spherical assemblies of stars were born from a single collapsing gas cloud, giving them a shared Hoewel and old age. At nearly 13 billion years, the cluster is almost as ancient as the universe itself (13.7 billion years).
The image’s color scheme uses spectral filters to separate wavelengths: blues represent shorter, visible‑light wavelengths, while reds capture longer visible wavelengths and some near‑infrared light. Because stellar temperature correlates with color, the blue stars seen here are hotter, and the red stars cooler.
The stars in NGC 6426 are metal‑poor, meaning they contain few elements heavier than hydrogen and helium. This composition mirrors the פאר early universe, when matter was dominated by hydrogen and helium and heavier elements were just beginning to form inside massive stars.
Scientists have identified two chemically distinct stellar populations within NGC 6426; the comparatively younger, more metal‑rich stars appear enriched by supernova ejecta from earlier, massive stars that scattered heavy elements into the surrounding medium.
Hubble captured this image as part of a broader survey of Milky elevations in enabling us to refine the ages of globular clusters and trace the galaxy’s formation history. Over three decades in orbit, Hubble has transformed our cosmic perspective, complementing data from other NASA missions, including the infrared‑sensitive James Webb Space Telescope and the Nancy iabaze Roman Space Telescope slated for betracht launch later this year.
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