1 00:00:00,000 --> 00:00:03,497 Using NASA’s James Webb Space Telescope, 2 00:00:03,497 --> 00:00:06,520 a team of astrophysicists has gained the longest,   3 00:00:06,520 --> 00:00:08,975 most detailed glimpse yet of the void 4 00:00:08,975 --> 00:00:11,560 that lurks in the middle of our galaxy. 5 00:00:11,560 --> 00:00:14,437 They found that the swirling disk of gas and dust 6 00:00:14,437 --> 00:00:17,266 orbiting the central supermassive black hole, 7 00:00:17,266 --> 00:00:19,070 called Sagittarius A*, 8 00:00:19,070 --> 00:00:23,360 is emitting a constant  stream of flares with no periods of rest. 9 00:00:23,360 --> 00:00:26,528 Using Webb’s NIRCam (Near-Infrared Camera) 10 00:00:26,528 --> 00:00:30,200 to observe Sagittarius A* for a total of 48 hours   11 00:00:30,200 --> 00:00:32,957 in 8- to 10-hour increments across one  year, 12 00:00:32,957 --> 00:00:35,320 astronomers saw constantly changing, 13 00:00:35,320 --> 00:00:37,589 bubbling brightness, and then suddenly 14 00:00:37,589 --> 00:00:39,992 a big burst of brightness popped up. 15 00:00:39,992 --> 00:00:41,843 Then, it calmed down again. 16 00:00:41,843 --> 00:00:45,353 They couldn’t find a  pattern, it appeared to be random. 17 00:00:45,353 --> 00:00:47,753 The activity profile of the black hole 18 00:00:47,753 --> 00:00:51,360 was new and exciting  every time that the astronomers looked at it.  19 00:00:51,360 --> 00:00:55,196 While the team expected to see flares, Sagittarius A* 20 00:00:55,196 --> 00:00:57,604 was more active than they anticipated. 21 00:00:57,604 --> 00:01:00,040 The observations revealed ongoing fireworks 22 00:01:00,040 --> 00:01:02,778 of various brightnesses and durations. 23 00:01:02,778 --> 00:01:04,960 The accretion disk surrounding the black hole   24 00:01:04,960 --> 00:01:07,793 generated five to six big flares per day 25 00:01:07,793 --> 00:01:12,120 and several small sub-flares or bursts in between.  26 00:01:12,120 --> 00:01:16,640 Although astrophysicists do not yet  fully understand the processes at play,   27 00:01:16,640 --> 00:01:19,604 they suspect two separate causes are responsible 28 00:01:19,604 --> 00:01:22,840 for the short bursts and longer flares. 29 00:01:22,840 --> 00:01:25,273 They believe that minor disturbances within 30 00:01:25,273 --> 00:01:28,436 the accretion disk likely generate the faint flickers. 31 00:01:28,436 --> 00:01:32,520 Specifically, turbulent  fluctuations within the disk can compress   32 00:01:32,520 --> 00:01:36,259 plasma to cause a temporary burst of radiation. 33 00:01:36,259 --> 00:01:38,840 For the big, bright flares astronomers think the 34 00:01:38,840 --> 00:01:41,593 cause is magnetic reconnection events, 35 00:01:41,593 --> 00:01:44,353 a process where two magnetic fields collide, releasing   36 00:01:44,353 --> 00:01:47,731 releasing energy in the form of accelerated particles. 37 00:01:47,731 --> 00:01:50,640 Traveling at velocities near the speed of light, 38 00:01:50,640 --> 00:01:54,000 these particles emit bright bursts of radiation. 39 00:01:54,000 --> 00:01:56,640 These new findings could help physicists better 40 00:01:56,640 --> 00:01:59,960 understand the fundamental nature  of black holes, how they interact   41 00:01:59,960 --> 00:02:01,714 with their surrounding environments, 42 00:02:01,714 --> 00:02:05,050 and the dynamics and evolution of our own galactic home. 43 00:02:05,050 --> 00:02:09,242 "Webb Space Telescope" 44 00:02:09,242 --> 00:02:15,268 [ NASA Meatball ]