WEBVTT FILE

﻿1
00:00:11.136 --> 00:00:11.594
That's right.

2
00:00:11.594 --> 00:00:15.473
So NASA's Parker Solar Probe,
which launched in 2018,

3
00:00:15.724 --> 00:00:20.061
has been using Venus gravity assist
to get closer and closer to the sun.

4
00:00:20.437 --> 00:00:23.023
And most recently,
it had a Venus gravity assist.

5
00:00:23.023 --> 00:00:27.736
And so now it's going to fly within 3.83
million miles of the surface of the sun,

6
00:00:27.736 --> 00:00:30.822
which is closer than any human made
object has ever gone

7
00:00:30.822 --> 00:00:33.825
before.

8
00:00:41.833 --> 00:00:42.375
That's right.

9
00:00:42.375 --> 00:00:42.709
Even though

10
00:00:42.709 --> 00:00:46.421
the sun is a constant in our sky,
the sun is not constant at all.

11
00:00:46.421 --> 00:00:50.925
The sun constantly has magnetic explosions
and little bursts of energy

12
00:00:50.925 --> 00:00:54.471
that come out, and sometimes
big burst of energy like the solar storms.

13
00:00:54.888 --> 00:00:58.516
And by measuring that process,
as it happens,

14
00:00:58.516 --> 00:01:02.979
so close to where its original energy
source was, we can really understand

15
00:01:03.271 --> 00:01:06.691
more about the energization and the

16
00:01:06.691 --> 00:01:09.819
the structures
as they evolve through the solar system.

17
00:01:19.746 --> 00:01:21.498
I am so excited about

18
00:01:21.498 --> 00:01:24.501
Parker touching the top edges of the,

19
00:01:25.043 --> 00:01:28.296
corona, the solar corona,
the outer atmosphere of the sun,

20
00:01:28.671 --> 00:01:32.383
and by measuring it in such detail
so close,

21
00:01:32.634 --> 00:01:35.929
we can combine that
with what we already know about the sun

22
00:01:36.304 --> 00:01:39.099
and the solar system
and that that material as that

23
00:01:39.099 --> 00:01:41.893
fills the solar system
from our other spacecraft.

24
00:01:41.893 --> 00:01:45.522
But by putting all of these pieces
together, we can really learn more

25
00:01:45.522 --> 00:01:49.025
about the solar corona
and that material as it fills

26
00:01:49.025 --> 00:01:52.028
our solar system.

27
00:01:58.451 --> 00:02:01.412
So during a total solar eclipse,
that's when the moon comes

28
00:02:01.412 --> 00:02:04.749
between us here on the Earth and the sun,
and it blocks out the main bright

29
00:02:04.749 --> 00:02:05.834
part of the sun

30
00:02:05.834 --> 00:02:09.796
so that we can see the solar corona,
the outer atmosphere of the sun.

31
00:02:10.046 --> 00:02:12.465
That outer atmosphere is extremely hot

32
00:02:12.465 --> 00:02:16.094
and it flows outwards,
filling our solar system.

33
00:02:16.845 --> 00:02:20.682
And Parker is flying through the outer
reaches of that solar corona.

34
00:02:20.890 --> 00:02:26.229
Really understanding how that energy is
put into that material in the first place.

35
00:02:34.445 --> 00:02:37.448
Yeah, NASA has a number of cool
missions coming up.

36
00:02:37.532 --> 00:02:39.284
One of the missions is called Punch.

37
00:02:39.284 --> 00:02:41.202
Punch has,

38
00:02:41.202 --> 00:02:43.121
3D imaging capability.

39
00:02:43.121 --> 00:02:43.872
So it's going to be able

40
00:02:43.872 --> 00:02:47.792
to see the corona in three dimensions,
the outer atmosphere of the sun,

41
00:02:48.042 --> 00:02:52.088
and watch that corona as it
expands outwards into the solar system

42
00:02:52.505 --> 00:02:57.218
and CODEX, which is, coronagraph
that's on the International Space Station.

43
00:02:57.552 --> 00:03:00.638
So that also is going to be looking
at the corona

44
00:03:01.306 --> 00:03:04.642
and measuring the temperature
and the velocity of that,

45
00:03:05.977 --> 00:03:09.314
of that material as it flows outwards,
which we can compare directly

46
00:03:09.314 --> 00:03:12.567
with what Parker measures in detail
in those outer

47
00:03:12.567 --> 00:03:15.570
reaches of the corona.

48
00:03:21.492 --> 00:03:22.243
We have

49
00:03:22.243 --> 00:03:26.247
never had a human made object
so close to the sun.

50
00:03:26.623 --> 00:03:31.336
To get that close, we had to use
Venus to have our gravity assist,

51
00:03:31.336 --> 00:03:34.339
to slow Parker down
so that it can get that close.

52
00:03:34.714 --> 00:03:36.216
Also, we had to not melt.

53
00:03:36.216 --> 00:03:40.053
That's why the Parker has this heat shield
that holds the instruments

54
00:03:40.053 --> 00:03:43.056
at room temperature
and keeps the heat of the sun away.

55
00:03:43.431 --> 00:03:45.308
And these are just amazing feats.

56
00:03:45.308 --> 00:03:47.393
And so it's so amazing
that we are so close

57
00:03:47.393 --> 00:03:52.315
and really getting to measure in detail
this material up close.

58
00:04:02.158 --> 00:04:02.784
You can learn

59
00:04:02.784 --> 00:04:06.579
more about Parker Solar Probe at NASA.gov/parker

60
00:04:06.579 --> 00:04:10.875
and you can also check
us out on @NASASun.
