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Pan Across NGC 1275’s Filaments
The red filaments seen near the center of galaxy NGC 1275 are fine threads of gas up to 20,000 light-years long, but only 200 light-years wide. These are sustained by magnetic fields.
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Hubble ACS image of NGC 1275
This Hubble Space Telescope image of galaxy NGC 1275 reveals the fine, thread-like filamentary structures in the gas surrounding the galaxy. The red filaments are composed of cool gas being suspended by a magnetic field, and are surrounded by the 100-million-degree Fahrenheit...
NGC 1275 (Perseus A) Multi-wavelength Composite
The active galaxy NGC 1275 is also a well-known radio source (Perseus A) and a strong emitter of X-rays due to the presence of a black hole in the center of the galaxy. The behemoth also lies at the center of the cluster of galaxies known as the Perseus Cluster. By combining...
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Last Updated
Feb 17, 2025
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Media
Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov