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NGC 1275

NGC 1275


Date: 20 August 2008
Satellite: Hubble Space Telescope
Depicts: NGC 1275
Copyright: NASA, ESA and Andy Fabian (University of Cambridge, UK)

This stunning image of NGC 1275 was taken using the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS) in July and August 2006. It provides amazing detail and resolution of the fragile filamentary structures, which show up as a reddish lacy structure surrounding the central bright galaxy NGC 1275. These filaments are cool despite being surrounded by gas that is around 55 million degrees hot. They are suspended in a magnetic field which maintains their structure and demonstrates how energy from the central black hole is transferred to the surrounding gas.

By observing the filamentary structure, astronomers were, for the first time, able to estimate the magnetic field's strength. Using this information they demonstrated how the extragalactic magnetic fields have maintained the structure of the filaments against collapse caused by either gravitational forces or the violence of the surrounding cluster of galaxies during their 100-million-year lifetime.

This is the first time astronomers have been able to differentiate the individual threads making up such filaments to this degree. Astonishingly, they distinguished threads a mere 200 light-years across. By contrast, the filaments seen here can be 200 000 light-years long. The entire image is approximately 260 000 light-years across.

NGC 1275 is a giant elliptical galaxy and lies in the centre of the Perseus cluster of galaxies. Also seen in the image are impressive lanes of dust from a separate spiral galaxy. It lies partly in front of NGC 1275 and has been completly disrupted by the tidal gravitational forces within the Perseus galaxy cluster. Several striking filaments of blue newborn stars are seen crossing the image.

Last Update: 1 September 2019
25-Sep-2021 16:31 UT

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https://sci.esa.int/s/A2qP998

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