WEBVTT FILE

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 ]

