Episode Transcript
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0:00
On April 8th, parts of Canada,
0:02
Mexico, and the United States will
0:04
experience a total solar eclipse. For
0:07
those of us in the path of totality, the
0:09
skies will darken. And if it's
0:11
not cloudy, you might even be able to
0:13
see the corona, the outer atmosphere of the
0:15
sun. I'll be at
0:17
the Fairbanks Museum with Planetarium Director
0:19
Mark Breen for a live special
0:21
broadcast, and you can listen. Or
0:24
watch! It's live on April
0:26
8th from 3 to 4 p.m. Eastern
0:28
time. Join us online from
0:30
anywhere in the world at vermontpublic.org.
0:34
You'll be able to call in and
0:36
ask your questions live. That's April 8th
0:38
from 3 to 4 p.m. Eastern. Just
0:40
go to vermontpublic.org. But
0:44
why is supported by Progressive? Progressive helps
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1:01
in all states or situations. This
1:24
is But Why, a podcast for curious
1:26
kids from Vermont Public. I'm Jane Lindholm.
1:29
On this show we take questions from curious
1:31
kids just like you, and we find interesting
1:33
people to answer them. On
1:36
April 8th, 2024, something
1:39
is happening in the skies over
1:41
North America. A
1:43
total solar eclipse. It's
1:46
being called the Great American Eclipse because
1:48
the path of the total eclipse cuts
1:50
across parts of Mexico, almost
1:53
all the way across the U.S. from west to
1:55
east, and then into eastern Canada. I
1:58
think it should be called the Great North American Eclipse. eclipse,
2:00
personally, but they're calling it
2:02
the Great American Eclipse. What's
2:04
happening during a solar eclipse is that
2:07
the moon lines up perfectly between the
2:09
Earth and the sun to block out
2:11
our view of the sun. And
2:14
it creates a shadow on the Earth, making it
2:16
look kind of like nighttime, but just for a
2:18
couple of minutes. When
2:20
the moon completely blocks the sun,
2:22
that's called totality. Eclipses
2:25
of the US states of
2:27
Texas, Oklahoma, Arkansas, Missouri, the
2:30
teeniest sliver of Tennessee, Illinois,
2:32
a tiny bit of Kentucky, Indiana,
2:34
Ohio, a really tiny bit of
2:37
Michigan, Pennsylvania, New York, Vermont,
2:39
New Hampshire, and Maine are all in
2:41
the path of totality. But
2:44
even if you're not in the path of
2:46
totality, if you live in North America, almost
2:48
all of you will have a chance to
2:50
see at least a partial eclipse. Today
2:53
we're going to learn more about what's happening during
2:55
a solar eclipse and what you can expect on
2:57
April 8th. And we're also
3:00
going to talk about how to watch the
3:02
eclipse safely, because you can't just watch it
3:04
happening with your bare eyes any
3:06
more than you would look at the sun on a normal
3:08
day with your bare eyes. So
3:10
let's start with the basics. Hello,
3:13
my name is Jake. I
3:15
am five years old and I live in
3:18
Altoona, Pennsylvania. And
3:24
my question is, why
3:26
does the moon, sun,
3:28
and earth all line
3:30
up for an eclipse? Hi,
3:33
my name is Camila. I
3:35
live in Dursbury, New York. And my
3:38
question is, what is a
3:40
solar eclipse and why people are going to
3:42
it? Hi, my name is
3:44
Frederick. I'm nine years old. I live
3:46
in Dallas, Texas. And my question is,
3:48
where are eclipses and how do they
3:50
happen? As I mentioned, an eclipse happens
3:52
when the moon passes between the earth
3:54
and the sun and blocks the light
3:56
of the sun. But to
3:59
get more details, we'd talk to Martina
4:01
Arndt, who's an astrophysicist. So
4:03
I study the sky and
4:05
the stars, and I really
4:07
focus actually on the sun these days, so
4:10
that makes me a solar physicist. Professor
4:12
Arndt knows a lot about solar eclipses, and
4:15
she has even seen a lot of them.
4:17
So we thought she'd be a great person to help
4:19
answer your questions. The basic definition
4:21
of an eclipse is that one
4:25
celestial body moves in front of the
4:27
other one, and in doing so, blocks
4:29
some of that object's light, and
4:32
it eclipses some of that light. And so
4:34
we have what are called eclipsing binary stars,
4:36
where you might have two stars that are
4:38
orbiting around each other, and when one passes
4:40
in front of the other, it
4:43
blocks some of the light. Or
4:47
there are stars that have exoplanets
4:49
going around them, and those planets will block
4:52
out some of the light, and that's how
4:54
we actually detect a lot of
4:57
these exoplanets that are being discovered, is that there's
4:59
something moving in front of a star, eclipsing it,
5:01
and blocking some of the light. And the one
5:04
that you're referring to is
5:07
a total solar eclipse, where we have
5:09
the moon coming between the sun and
5:11
the Earth, and blocking this
5:14
really, really bright star. Because
5:17
you mentioned celestial bodies,
5:20
and celestial just means up in the
5:22
sky, and so these are two things
5:24
that move in front of one another,
5:26
or one moves in front of the
5:28
other, and somebody at a third location
5:30
can see what's happening, or see the
5:33
shadow. So when a
5:35
solar eclipse happens for
5:38
us to see it on Earth, it's the moon
5:40
moving in front of the sun, and blocking the
5:42
light. And sometimes you get
5:44
a partial eclipse, where you only have
5:46
a part of the moon blocking the
5:48
sun, because the path is not direct.
5:51
But on April 8th, for many people,
5:53
they're going to see totality, where the
5:55
sun is totally blocked. And
5:58
Nora wants to know, what is the sun?
6:00
Why do the edges of the sun get so
6:02
bright in a solar eclipse? Given
6:05
that the moon is blocking out
6:07
the entire sun, why do
6:09
the edges of the sun get so
6:12
bright? If it's
6:14
supposedly all blocked out? Yeah, and
6:16
I love this question that Nora has. The
6:18
sun is always bright, okay, and then there's
6:21
the surface of the sun, and
6:23
then above that is an atmosphere,
6:25
like the Earth has an atmosphere.
6:27
The atmosphere is not as dense,
6:29
which means there's not as many
6:31
particles smooshed together in one place,
6:34
and as a result it's very hard to
6:36
see unless we block out the sun. And
6:39
when the moon does block the sun, what we do
6:41
get to see is a tiny,
6:43
tiny little bit of the sun's
6:46
surface, the
6:48
chromosphere and the photosphere, and that part is
6:50
really the bright part that I think she's
6:52
talking about, and it can look very red,
6:55
and it's
6:57
just that that material is denser
7:00
than the upper atmosphere, which
7:02
is the one that we're studying. One
7:04
thing we should probably note even
7:06
before that question is when
7:08
we study the Earth and the moon
7:11
and the sun in school, we learn
7:13
that the Earth is much smaller than the
7:16
sun, and the moon is even smaller than
7:18
that. So if the moon
7:20
is very, very, very small compared to
7:22
the sun, how can it block out
7:24
all the light of the sun? Yeah,
7:28
so what I do in my
7:30
classes is I have students hold
7:32
their thumb up and try to
7:34
maybe block out a light bulb, and if you
7:36
hold the thumb far away, it doesn't do as
7:38
nice of a job of blocking out the light
7:40
bulb as if you bring your thumb
7:43
really close to your eye, and it looks so
7:45
much bigger, right? And the fact that
7:47
the sun is so far away, it looks
7:49
smaller, and because the moon is much closer
7:51
to us, even though it's small, it looks
7:53
bigger, and the geometry
7:55
works out perfectly that we have the
7:58
moon being essentially looking like a star. the same size
8:00
as the Sun. Okay, so what
8:02
do we know so far? In
8:05
a solar eclipse, the moon blocks out
8:07
the light of the Sun, but you
8:09
can still see the Sun's atmosphere radiating
8:11
out from the shadow created by the
8:13
moon. Now not everyone
8:15
will get to experience this total eclipse,
8:18
but most people living in North America will
8:20
see, as we said, at least a partial
8:22
eclipse. But it actually starts out
8:24
in the Pacific. That's Mark Breen. He's
8:27
a meteorologist, someone who studies the
8:29
weather, and he's also the director
8:31
of a planetarium at the Fairbanks
8:33
Museum in St. John's Bay, Vermont.
8:36
He knows a lot about the path this solar
8:38
eclipse is going to take. It
8:40
takes a few thousand miles before it
8:42
gets to Mexico. It cuts across northern
8:44
Mexico and then through Texas.
8:46
It goes through big cities like Indianapolis,
8:50
then into Cleveland, Buffalo, and
8:52
then right across northern Vermont.
8:55
And then slightly into Canada for a little while
8:57
as well. Yes, it continues on right
8:59
into Atlantic Canada. If you live
9:01
right in the center of that path, you'll get
9:03
three minutes or more of totality when the moon
9:05
is totally covering the Sun. If
9:07
you're on the outer edge of totality, you might only
9:10
get a minute or even less. And
9:12
if you're outside the path of totality, you'll
9:14
see a partial eclipse, which is
9:16
still pretty cool. Jimmy
9:19
asks, why do eclipses happen
9:21
very rarely? So they
9:23
worked out an average that in any one
9:25
location, it's about every 400 years. Oh
9:28
my gosh, every 400 years. Yes. But
9:30
there's a place in Tennessee where the
9:33
eclipse in 2017 will
9:35
basically happen again this year. So they
9:37
get two eclipses in seven years. Martina
9:40
Arndt says there are a lot of factors
9:42
that need to line up for an eclipse
9:44
to be visible in any one location. Well,
9:47
I have good news for Jimmy because actually
9:50
an eclipse happens every month. And
9:53
I want to have to clarify this. It happens
9:55
every month because the moon comes between the Sun
9:57
and the Earth every month and it casts the
9:59
shadow. And unfortunately though, the
10:02
shadow is most of the time either
10:04
above the Earth or below the
10:06
Earth, so we'd have to jump really high to try
10:08
and see it, which we can't do. So
10:10
what we do is we wait for those two
10:13
times a year where the moon and the sun
10:15
and the Earth are lined up so that the
10:17
shadow from the eclipse falls on the Earth. Okay?
10:21
Now, so
10:23
that says that we should in principle
10:25
have two solar eclipses every year, and
10:27
sometimes we do. However, just like with
10:30
this conversation, this example I gave with
10:32
the thumb, that if the
10:35
moon is farther away, it looks smaller, and if
10:37
the moon is closer, it looks bigger, and in
10:39
fact the moon isn't always the exact same distance
10:42
away from us. So we need the perfect combination
10:44
of the shadow falling on the Earth
10:46
and the moon being the right distance
10:48
away from us to be able to
10:50
get a total solar eclipse. And that's
10:52
why they feel rare, right, because we
10:54
need those conditions to happen. But
10:58
I like to think of the fact that if I could jump really
11:00
high, I'd get an eclipse every month. Well,
11:02
and then you also have to be in
11:04
the right part of the world at the right
11:06
time. So a total solar eclipse could be a
11:08
once-in-a-lifetime event depending on where you live. Yes.
11:11
Or if you have the
11:15
ability to travel the world like I have,
11:17
you get to travel wherever the eclipse shadow
11:19
takes you. What happens if
11:22
there's bad weather, clouds or snow or rain
11:24
during an eclipse? What do you see? Well,
11:27
we can't see the sun, but we can
11:29
see that when the sun gets covered by
11:31
the moon, it's still covering the sun even
11:33
though we can't see it. So it still
11:35
makes the skies darker. And so
11:38
you will notice, even if it's
11:40
cloudy, that the skies will darken.
11:43
And it's an interesting
11:45
kind of darkness. It's not like middle of
11:47
the night darkness, but it's a
11:50
grayish darkness, a dark gray, if that
11:52
makes any sense. A
11:54
few of you have questions
11:56
about animals and eclipses. I've
12:08
seen animals respond to the
12:11
change in light in different ways. My
12:13
favorite was when I was in Zambia,
12:16
one of the eclipses, there were some hippos
12:18
near where we were set up. And the
12:20
hippos, because it's so hot out, like during
12:22
the day, they like to sit and sleep
12:25
while they lie down and they sleep. And
12:28
they relax and they tend to do more
12:30
things at night. And when it got dark
12:32
during the eclipse, they started to kind of
12:34
get up and move around and they were
12:37
like, oh, it's not so hot anymore.
12:39
Because you'll also find out that the
12:41
temperature goes down. So you'll see the
12:43
skies get darker, but you'll also feel
12:45
a difference in temperature, by quite
12:48
a few degrees actually. Hello, my
12:50
name is Charlotte. I am seven years
12:52
old. I was in Scottsdale, Arizona. My
12:55
question is, do animals have their
12:57
eyes on the solar eclipse? Charlotte,
13:00
I hope these animals listen to me. They
13:03
need to be wearing eclipse glasses during
13:05
the one and a half hours before the
13:07
sun is totally covered and for the one
13:09
and a half hours after the sun is
13:11
totally covered. Because
13:14
that's the time when you can hurt your eyes.
13:16
And so yes, animals could. I
13:18
don't think that many of them look up though. Or
13:21
if they do and it starts to be
13:23
a little too much, then they look down. If it
13:25
starts to hurt, then they look down. Sure. I
13:28
mean, I have to tell the truth. I've sometimes
13:30
looked at the sun by accident. They know if
13:33
I take off my
13:35
sunglasses or something and I look up to see
13:37
if I can see a bird that's going by
13:39
or where the helicopter might be coming from. And
13:42
I look at the sun and I know how
13:44
uncomfortable it is. And I'm sure if
13:46
it's ever happened to any of the
13:48
listeners, they know how uncomfortable it is. And
13:51
you're absolutely right. They're probably smart enough to say, you know,
13:53
that's not good for me. I'm not going to
13:55
do it anymore. We're animals too, of course. And
13:57
we should definitely not be looking at the sun.
14:00
even during an eclipse without
14:02
taking safety precautions. Let
14:04
me say that very clearly. You
14:06
should never look at a partially
14:09
eclipsed sun without protection for your
14:11
eyes. Looking at a
14:13
partial eclipse without eye protection can lead
14:15
to permanent and serious eye damage. And
14:18
you may not know it's happening because your
14:20
eyes won't necessarily feel pain. So
14:23
if you can get a pair of solar
14:25
eclipse glasses, you could put those on
14:27
and then you can look up at the sun safely.
14:30
Maybe your school or local library
14:32
or community organization has some solar
14:34
eclipse glasses. And there
14:36
may be a group nearby that has special telescopes
14:39
with solar filters that are safe to look through.
14:42
But any camera or binoculars or
14:44
telescope or even cell phone that you
14:46
wanna take pictures of or look at the
14:48
eclipse through needs to have a solar filter
14:50
too. Now, if
14:52
you're in the path of totality and the
14:54
sun is fully covered, meaning there is no
14:57
light showing, just that corona we talked about,
15:00
then it is safe to remove your eclipse
15:02
glasses and take a brief look. You
15:04
might even see that corona, the outer atmosphere
15:06
of the sun. But before
15:09
you take off your eclipse glasses, check in with
15:11
an adult and make sure they tell you
15:13
it's safe to do so. Now,
15:15
if you don't have a pair of eclipse
15:18
glasses, that doesn't mean you're out of luck
15:20
for viewing the eclipse. It just might mean
15:22
that you have to look down instead of
15:24
up in order to see it. You can
15:27
find things around your house that
15:29
have little holes in them. So I'm thinking like
15:32
a cracker that might have holes in it
15:34
or the pasta strainer that your parents might
15:36
use to strain their pasta. There's lots of
15:38
little holes in there. If
15:41
you take something that has a small, lots
15:44
of small holes on it, and if you don't have
15:46
any of that, then take a pen and poke some
15:48
holes through a piece of paper and
15:51
you put that out there
15:53
so that the sky is above the
15:55
paper and you look below the paper and
15:57
look below the colander and you will see
15:59
little tiny... images of partial solar eclipses. And you
16:01
can take a picture of that if you wanted
16:03
to. But it's a nice, safe way to do
16:05
it, because you're looking down at the ground and
16:07
not up at the sky. And
16:09
another thing, if you don't have any of those
16:12
things, maybe there are trees near you. Because trees,
16:14
when they have leaves, and in April, hopefully there'll
16:16
be some trees with leaves, those
16:19
leaves overlap. And they make little tiny
16:21
pinhole cameras just naturally. And so if
16:23
you look under a tree, you should
16:25
see lots of little partial solar eclipses
16:28
on the ground, dancing around as the leaves
16:30
move. And it can be really beautiful. Coming
16:33
up, we'll learn more about the
16:35
corona, the sun's atmosphere, that's still
16:38
visible during a total solar eclipse.
16:42
But first, a message for the adults who are listening. Support
16:44
for our show comes from Oak Meadow. How
16:47
is school going this year? If
16:49
the answer is not great, maybe
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it's time to rediscover the joy of learning.
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Oak Meadow provides student-centered homeschooling
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for K through 12. To
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learn how homeschooling can work for
17:04
your family, visit oakmeadow.com. This
17:07
is But Why, a podcast for curious kids.
17:10
I'm Jane Lindholm, and today we're learning
17:12
about solar eclipses, how they happen,
17:14
and why people are so excited about the
17:17
Great American eclipse on April 8. Scientists
17:20
are especially excited about solar eclipses
17:22
because it's a chance for them
17:24
to observe the atmosphere of the
17:26
sun, which is tough to
17:28
do normally. That's one of
17:31
the things Martina aren't studies. The sun
17:33
itself has two main
17:35
parts. It has the
17:38
sphere, the ball itself, which is the part
17:40
that you might see at sunrise or sunset
17:42
in the clouds. And above that,
17:44
we have an atmosphere, like the Earth has an
17:47
atmosphere. And this
17:49
atmosphere is called the corona on the
17:51
sun, and it's a
17:53
lot fainter than the surface of the sun.
17:57
And if we want to study this
17:59
corona, upper atmosphere, we have to
18:01
block out the surface of the sun
18:03
because we have some interesting
18:05
problems we're trying to solve. The corona
18:08
is hotter than the surface of the
18:10
sun. The sun is spitting out particles
18:13
in two categories of speeds. We got fast
18:15
and we've got slow and we don't know
18:17
why that happens. And so there's
18:19
a lot of scientists working to figure
18:22
out the answers to these questions and
18:24
they come up with models and ideas. And
18:26
anytime you have a theory like
18:29
this, you maybe do some computer
18:31
simulations, you do the math and you
18:33
say, okay, I think this is the
18:35
explanation. And then what we need to
18:37
do is to get data to test
18:39
this hypothesis and see how close we
18:41
are. And then if
18:43
it's not right, then we go back and do it
18:45
again. So the only way to get
18:47
data from the corona is
18:49
during a total solar eclipse because the
18:52
sun is so, so, so bright, okay,
18:56
that we can get data
18:58
close to the solar surface and further away.
19:01
Now, there are some instruments in
19:03
space that take
19:07
– they have their own version of their thumb and
19:09
they block out the sun, right? But
19:11
even space images don't get
19:13
us enough information about what's happening
19:15
between the surface of the sun
19:17
and the atmosphere of the sun.
19:19
We need that information in that
19:22
crucial zone between the two. Why
19:25
is it important to learn these things about the
19:27
sun? Well, I
19:29
just like learning personally. I think it's a
19:32
wonderful thing to try and understand the world
19:34
around us. So there's two ways to answer
19:36
this. I would say
19:38
that if we want to understand
19:40
the universe around us and how things
19:42
work, we have a sun, which
19:45
is a star, literally in our
19:48
backyard, that we can take data from on a
19:50
regular basis. And if we can understand
19:53
our star, then we can understand what
19:55
happens in other places. And
19:57
I just think that's human nature to
19:59
try and understand. understand the universe
20:01
in which we live. That
20:04
being said, there are also reasons for
20:06
us to understand the sun because it
20:08
interacts with the earth that affects us.
20:10
I mean, we've got sunburns, we've got,
20:13
you know, other things that the sun
20:15
does for us and does to
20:17
us. One of them
20:19
is that all these particles that are being sent
20:21
out by the wind are
20:23
interacting with the earth's magnetic field, and
20:25
that's how we get the northern lights
20:28
and the southern lights, and so to
20:30
understand that, we,
20:33
those particles can also knock out power grids,
20:35
and so then our TVs wouldn't
20:37
work, and you know, all this, that
20:39
would be bad. And then there's another
20:41
component, too, that if we can predict
20:43
when the sun is
20:46
going to be sending us a
20:48
large quantity of charged particles, it
20:50
allows us the opportunity to protect any satellites.
20:52
You know, we can have them turn their
20:54
back on the sun for a little bit.
20:56
It also is a way to, you know,
20:59
alert maybe astronauts who are up in space
21:01
that a big storm is coming, and I
21:03
think also the
21:05
more we understand, it'll help us kind
21:07
of be prepared for, let's say,
21:09
if we ever do make it to Mars, right,
21:12
to be able to go to Mars and understand
21:14
and predict what might be happening when the sun
21:16
does a particular something. Well, that
21:18
has me convinced. Martina Arndt has
21:21
already seen a dozen total eclipses around
21:23
the world, all as part of her
21:25
work, but for most
21:27
of us, a total eclipse is
21:29
a once-in-a-lifetime experience. That's
21:32
been true throughout human history, and
21:34
throughout human history, we've been trying to
21:37
make sense of what's happening in the
21:39
sky. Before people
21:41
understood the science of eclipses, they
21:43
attached many different meanings and myths
21:45
to them. Thomas
21:47
Hockey is a professor of astronomy at
21:49
the University of Northern Iowa and the
21:52
author of a book called America's First
21:54
Eclipse Chasers. We asked
21:56
him to tell us a little bit about some
21:58
of the earliest written records of human humans experiencing
22:01
eclipses. We find
22:03
this in civilizations all over
22:06
the world, trying
22:08
to keep track of
22:11
eclipses, Mesopotamia and China,
22:14
India, the Mayans
22:16
and other cultures. The
22:19
goal was always the same, to try
22:21
to find some pattern in eclipses.
22:25
You're saying early civilizations realized this
22:27
was likely not a one-time event,
22:30
or something that they wanted to make
22:32
sure that they could be prepared for, should it happen
22:35
again. Exactly. If
22:39
you over many centuries kept track
22:42
of them, you might have a
22:44
chance of at least,
22:46
if not predicting, at least saying
22:48
when an eclipse might
22:51
occur, and then take what you
22:53
consider to be necessary steps,
22:56
which involved certain
22:58
rights, loud
23:01
noises to scare, whatever was
23:03
taking the eclipse away, or
23:06
in the case of the Babylonians,
23:08
who thought this was an omen
23:10
directed at the king, they
23:13
would pull someone off the street, put
23:15
him on the throne, crown on
23:17
his head, hide the real king.
23:20
And during that eclipse
23:22
peril, it was this
23:25
nobody who was the pretend
23:27
king, and supposedly would take whatever
23:30
bad effect the
23:33
eclipse had in store. Tell
23:35
us a little bit about some
23:38
of the other associations that civilizations
23:40
had with eclipses before we
23:42
had the science to know what
23:45
was actually happening. It
23:47
often involved something,
23:50
China, for instance, a dragon devouring
23:53
the sun, the
23:57
partial eclipse before a
23:59
total eclipse. kind of looks
24:01
like someone has taken a bite
24:04
out of the Sun and
24:09
the eclipses of course would end.
24:12
They would eventually, the
24:15
monster would disgorge
24:17
the Sun but there
24:19
was no guarantee of
24:22
that. A fire
24:24
after all will not
24:26
necessarily rekindle itself
24:29
so I'm sure there was a great deal of relief when
24:32
whatever had the Sun let go. How did
24:35
we start to gain the
24:37
knowledge about what's actually happening
24:39
scientifically and astronomically during an
24:42
eclipse? While many
24:44
civilizations reached the point of
24:46
at least being able to
24:48
anticipate possible eclipse,
24:52
it was the Greeks who had a
24:56
theory of science
24:58
that probably got closest. It
25:00
involved great shelves
25:04
spinning about the earth with
25:06
the various bodies involved, mounted
25:09
on them, the ideas they were made
25:11
of crystals so you could see through
25:13
them or some preferred
25:15
a wheel-on-wheel arrangement kind of
25:17
like a carnival
25:20
ride. Such systems did
25:23
do a fair job of predicting
25:26
where things were in the sky
25:28
under normal times, less
25:31
successful in the
25:33
exact alignment that was
25:36
necessary to predict an
25:38
actual solar eclipse. You
25:41
know today we teach
25:43
our children that this is
25:46
the moon moving in between
25:48
the earth and the Sun and just
25:50
temporarily blocking out the light of the
25:53
Sun because of the specific place the
25:55
moon is at this moment. And there's
25:57
a lot of hard facts, hard
25:59
facts. science that
26:01
we use to describe language around
26:04
the solar eclipse. And yet,
26:06
there are also still cultural
26:08
significances to a solar eclipse that
26:10
go beyond just what we know
26:12
about the path of the Earth
26:14
and the Moon. What
26:16
is the central gut feeling that
26:19
people have when they see this
26:21
remarkable we still have
26:23
within us, I think, that primal
26:27
feeling about eclipses from
26:30
as long as we
26:32
have those records going on for
26:34
millennia. And that is a not
26:38
just, oh,
26:40
that's interesting in the sky, but
26:43
it evokes a
26:46
very visceral, all
26:48
body feeling that is difficult
26:51
to describe. And
26:53
I'm always not successful
26:55
in telling people about
26:57
that. I end up just
27:00
saying, yeah, you got to go, you got to
27:02
go check out one of these. And then
27:04
you'll see why people's interaction
27:10
with total solar eclipses
27:13
since the beginning has
27:15
been strong. That's
27:18
true of Martina Arndt. Remember how
27:20
I said she has chased a whole bunch of eclipses? She
27:22
says the feeling of wonder at seeing one doesn't go away.
27:25
But having good weather certainly helps
27:28
the experience. I have traveled to 12 and it's
27:30
brought me to six of the seven continents on
27:36
the Earth. The only one I haven't been to
27:38
is Antarctica. And I would say of those 12
27:40
eclipses, we had good weather for probably half of
27:43
them. When we were in Australia, we thought we
27:46
had clear skies. But then because the sun was getting
27:48
covered and we were by the ocean, it was almost
27:51
like a little weather change instantaneously happened. And then it was
27:53
windy and raining and blowing
27:56
and we didn't get to see anything. And I think
27:58
that's a very interesting question. anything. And at my
28:01
first eclipse in Mongolia, it snowed. Here we
28:03
went, we traveled all halfway around the world
28:05
with all of this equipment and we set
28:07
up and it was snowing and you couldn't
28:09
see anything. But then, you know, in
28:11
2017, in the
28:14
last Great American eclipse that came across the
28:17
United States in the other way, we
28:20
had beautiful clear weather and it
28:22
was perfect. Given that you've seen
28:24
so many of these, is it
28:26
still exciting in a visceral human
28:28
way to see a total eclipse?
28:31
Yes, it absolutely is. And I'll tell
28:33
you that people have a variety of
28:35
responses to these sorts of
28:37
events. Some people
28:39
really are just overwhelmed,
28:41
some people are scared.
28:44
And for me, I have to be honest with you,
28:47
I see it as beautiful but I have a job
28:49
to do when I'm there which is taking the data.
28:51
And I usually stand there and go, oh my
28:53
goodness, we got it right. We were in the
28:55
right place at the right time. And it just
28:57
gives me a real appreciation for how
29:00
we understand already so much about
29:02
nature that we can predict where to stand and
29:04
it works. It's pretty amazing. I
29:06
hope those of you in the Path of Totality
29:08
get to see this amazing site. Get
29:11
your eclipse glasses ready or make a
29:13
pinhole viewer. We have a video
29:15
up on our But Why YouTube channel and
29:17
on our Instagram page showing you how to
29:19
make one. Even if
29:21
you're outside the Path of Totality, you
29:23
may be able to see a partial
29:26
eclipse. So have an adult help you
29:28
look up your location and find out
29:30
what you'll see. And if you go
29:32
to aboutwhykids.org or vermontpublic.org, you can listen
29:34
to me broadcast live during the
29:36
solar eclipse from 3 to 4 p.m.
29:39
Eastern Time on April 8th. That's
29:42
it for today. Thanks to Martina Art,
29:44
Mark Breen and Thomas Hockey for teaching
29:46
us about eclipses. As
29:48
always, if you have a question about
29:50
anything, have an adult record it. It's
29:52
easy to do on a smartphone using a
29:55
voice memo or voice recording app. Then
29:57
your adult can email the question to
29:59
questions. at butwhykids.org.
30:02
We can't answer every question we get, but
30:04
we love hearing from you. But
30:07
Why is produced by Melody Baudette, Kiana
30:09
Haskin, and me, Jane Lindholm at Vermont
30:12
Public. We're distributed by
30:14
PRX. Our theme music is by
30:16
Luke Reynolds. Special thanks this
30:18
week to David Littlefield, Joey
30:20
Palumbo, Kaylee Mumford, and Kyle
30:22
Ambus. We'll be back
30:24
in two weeks with an all
30:26
new episode. Until then, stay curious.
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