WEBVTT FILE

﻿1
00:00:00.000 --> 00:00:01.634
[Music throughout]

2
00:00:01.634 --> 00:00:04.137
When superdense neutron stars crash,

3
00:00:04.137 --> 00:00:07.841
the event can be felt across the cosmos.

4
00:00:09.242 --> 00:00:13.313
But astronomers would love
to find these systems before they collide.

5
00:00:13.747 --> 00:00:16.750
And new simulations are guiding the way.

6
00:00:17.584 --> 00:00:20.553
Neutron stars pack the mass of our Sun

7
00:00:20.687 --> 00:00:22.956
into a ball the size of a city.

8
00:00:22.956 --> 00:00:25.258
And have superstrong magnetic fields

9
00:00:25.258 --> 00:00:27.727
filled with energetic particles.

10
00:00:28.795 --> 00:00:31.664
New simulations run on NASA Ames’

11
00:00:31.664 --> 00:00:33.633
Pleiades supercomputer show

12
00:00:33.700 --> 00:00:35.935
how these fields begin interacting

13
00:00:35.935 --> 00:00:37.904
long before the stars crash.

14
00:00:39.472 --> 00:00:41.674
As the magnetic fields intertwine,

15
00:00:41.674 --> 00:00:42.909
they produce a glow

16
00:00:42.909 --> 00:00:44.644
that steadily increases

17
00:00:44.644 --> 00:00:46.813
as the stars spiral closer together.

18
00:00:49.682 --> 00:00:51.317
These simulations

19
00:00:51.317 --> 00:00:53.620
map where the most energetic gamma rays

20
00:00:54.054 --> 00:00:55.989
produce a distinctive glow

21
00:00:55.989 --> 00:00:57.624
we could detect from Earth,

22
00:00:57.991 --> 00:01:00.660
a goal for next-generation telescopes.

23
00:01:01.694 --> 00:01:03.630
Simulations like these

24
00:01:03.630 --> 00:01:07.367
will help astronomers better understand
how these fields interact

25
00:01:07.634 --> 00:01:09.035
and better predict

26
00:01:09.035 --> 00:01:10.837
the electromagnetic signals

27
00:01:10.837 --> 00:01:12.005
that will point

28
00:01:12.005 --> 00:01:14.474
to imminent neutron star collisions.

29
00:01:17.177 --> 00:01:21.381
[NASA]
