This beautiful picture from the NASA/ESA Hubble House Telescope reveals the arms of the spiral galaxy M74 studded with rosy pink areas of contemporary star formation. M74 — often known as the Phantom Galaxy — lies round 32 million light-years away from Earth within the constellation Pisces. It's a acquainted sight for Hubble.
The attractive reddish blooms that unfold all through M74 are literally large clouds of hydrogen gasoline. They're made to glow by the ultraviolet radiation from scorching, younger stars embedded inside them. These areas — which astronomers seek advice from as H II areas — mark the situation of latest star formation and are an vital goal for each space- and ground-based telescopes. Hubble’s Superior Digital camera for Surveys, which collected the information on this picture, even has a filter specifically tailor-made to select solely this particular purple wavelength of sunshine!
A set of observations exploring the evolution of native spiral galaxies similar to M74 equipped the information for this picture. This exploration goals to realize insights into the historical past of star formation in these spirals. To do that, astronomers analyzed star clusters so far the completely different components of spiral galaxies, enabling them to know how the galaxies assembled over time. Moreover, they explored the distribution of mud in spiral galaxies. This mud is seen on this picture because the darkish threads winding alongside the spiral arms of M74.
Other than their quest to know the historical past of spiral galaxies, astronomers additionally noticed M74 to enhance observations from different telescopes. Combining observations of the identical object from completely different telescopes throughout the electromagnetic spectrum gives way more perception to astronomers than observations from a single telescope would. Hubble’s observations additionally paved the best way for future devices; M74 was one of many first targets of the highly effective new NASA/ESA/CSA James Webb House Telescope.
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