Towards an inky black backdrop, the blue swirls of spiral galaxy NGC 6956 stand out radiantly. NGC 6956 is a barred spiral galaxy, a standard kind of spiral galaxy with a bar-shaped construction of stars in its middle. This galaxy exists 214 million light-years away within the constellation Delphinus.
Scientists used NASA’s Hubble Area Telescope to picture NGC 6956 to review its Cepheid variable stars, that are stars that brighten and dim at common intervals. Because the interval of Cepheid variable stars is a perform of their brightness, scientists can measure how vibrant these stars seem from Earth and examine it to their precise brightness to calculate their distance. Consequently, these stars are extraordinarily helpful in figuring out the space of cosmic objects, which is without doubt one of the hardest items of data to measure for extragalactic objects.
This galaxy additionally accommodates a Sort Ia supernova, which is the explosion of a white dwarf star that was step by step accreting matter from a companion star. Like Cepheid variable stars, the brightness of these kinds of supernovae and how briskly they dim over time permits scientists to calculate their distance. Scientists can use the measurements gleaned from Cepheid variable stars and Sort Ia supernovae to refine our understanding of the speed of growth of the universe, often known as the Hubble Fixed.
Supplied by
NASA’s Goddard Space Flight Center
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Hubble captures majestic barred spiral galaxy NGC 6956 (2022, December 16)
retrieved 16 December 2022
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