Magnetic Monster: Galaxy NGC 1275 | Hubble
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 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 a gaping 200,000 light-years long. The entire image is approximately 260,000 light-years across.
Also seen in the image are impressive lanes of dust from a separate spiral galaxy. It lies partly in front of the giant elliptical central cluster galaxy and has been completed disrupted by the tidal gravitational forces within the galaxy cluster. Several striking filaments of blue newborn stars are seen crossing the image.
Credit: NASA, European Space Agency (ESA) and Andy Fabian (University of Cambridge, UK)
Release Date: August 20, 2008
#NASA #ESA #Astronomy #Space #Science #Hubble #Stars #Galaxy #SeyfertGalaxy #Filaments #NGC1275 #PerseusCluster #Perseus #Constellation #Cosmos #Universe #SpaceTelescope #GSFC #STScI #UnitedStates #Europe #STEM #Education
No comments:
Post a Comment