1 00:00:00,000 --> 00:00:04,909 NASA’s Hubble Space Telescope captured three separate moments 2 00:00:04,909 --> 00:00:09,510 in a far-off supernova explosion in a single snapshot. 3 00:00:09,510 --> 00:00:15,200 These moments provide a unique glimpse into the supernova’s early life. 4 00:00:15,200 --> 00:00:20,209 It is quite rare to detect a supernova explosion at a very early stage, 5 00:00:20,209 --> 00:00:22,610 because that stage is so short. 6 00:00:22,610 --> 00:00:28,260 It only lasts for hours to a few days, and it can be easily missed. 7 00:00:28,260 --> 00:00:33,969 The star exploded more than 11 billion years ago, when the universe was less than one fifth 8 00:00:33,969 --> 00:00:38,110 of its current age of 13.8 billion years. 9 00:00:38,110 --> 00:00:43,039 In a single exposure, Hubble captured the supernova’s rapid change of color, which 10 00:00:43,039 --> 00:00:45,480 indicates temperature change. 11 00:00:45,480 --> 00:00:48,390 The early, hotter phase appears blue. 12 00:00:48,390 --> 00:00:52,000 As the supernova cooled, its light turned redder. 13 00:00:52,000 --> 00:00:57,530 This detection was possible through a phenomenon called gravitational lensing, as first predicted 14 00:00:57,530 --> 00:01:01,210 by Einstein’s theory of general relativity. 15 00:01:01,210 --> 00:01:07,580 In this case, the immense gravity of the galaxy cluster Abell 370 both bent and magnified 16 00:01:07,580 --> 00:01:11,528 the light from the more distant supernova located behind the cluster, 17 00:01:11,528 --> 00:01:14,556 like a giant cosmic lens. 18 00:01:14,556 --> 00:01:18,234 This lensing effect split and warped the supernova’s light, 19 00:01:18,234 --> 00:01:22,479 bending it along separate pathways of varying lengths. 20 00:01:22,479 --> 00:01:27,790 The different travel times between each path created a time delay that produced three distinct 21 00:01:27,790 --> 00:01:35,330 images of the explosion at different times that arrived at Earth simultaneously. 22 00:01:35,330 --> 00:01:38,497 This is the first detailed look at a supernova 23 00:01:38,497 --> 00:01:42,009 at such an early time of the universe’s evolution. 24 00:01:42,009 --> 00:01:46,799 The research could help scientists learn more about the formation of stars and galaxies 25 00:01:46,799 --> 00:01:51,011 in the young universe. 26 00:01:51,011 --> 00:01:58,051 Follow us on social media @NASAHubble!