James Webb Telescope: NASA's James Webb Space Telescope has captured a stunning new image of the Phantom Galaxy, which is otherwise called M74. The picture revealed the delicate filaments of gas and dust in the grandiose spiral arms which wind outwards from the centre of this image. 
Webb's sharp vision pictured an unobscured view of the nuclear star cluster at the galaxy's centre, complimented by lack of gas in the nuclear region.

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What is M74?

M74 is a spiral galaxy of a particular segment, which is classified as a ‘grand design spiral’. The galaxy's arms are prominent and well-defined unlike other galaxies in space which have patchy and ragged structure.

M74, also called Phantom Galaxy, is about 32 million light-years away from Earth and lies almost face-on to Earth. The prominent spiral arms of this galaxy make it a most-chosen target for astronomers studying the origin and structure of galactic spirals.

Webb noticed M74 with its Mid-InfraRed Instrument (MIRI) to learn more about the earliest phases of star formation in the local universe. To study nearby star-forming galaxies, these observations were made by PHANGS (Physics at High Angular resolution in Nearby Galaxies) collaboration. The neighboring galaxies have already been observed using the NASA/ESA Hubble Space Telescope and ground-based observatories.

The recent James Webb's addition of well-defined observations at longer wavelengths will give astronomers an opportunity to pinpoint star-forming regions in the galaxies. Furthermore, accurate measurement of the masses and ages of star clusters and insights into the nature of the small grains of dust drifting in interstellar space, will also be possible.

Earlier observations of M74 revealed bright areas of star formation known as HII regions. Scientists gain greater insight into astronomical objects by accumulating data from telescopes operating across the electromagnetic spectrum.