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Hey everyone, I'm Dan Kortler, the host
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of TED Climate. Each episode we unpack
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this. This
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is a CBC Podcast. Hi,
0:38
I'm Bob McDonald. Welcome to Quirks and
0:41
Quarks. On this week's show, one
0:44
species' feces is another one's
0:46
treasure. But this treasure
0:48
might be poisoned. We saw
0:50
many instances of chimps coming, black
0:53
and white colobus monkeys and
0:55
red diker. And they were all coming to
0:58
feast on this bat poop. And
1:01
five million years ago, a gigantic
1:03
salmon with tusks swam the seas
1:05
of the Pacific. They actually look more
1:07
like a warthog. Some people describe them almost
1:09
looking like a mustache. Looks like
1:11
they could have been spikes and used for tools.
1:14
Plus desperate measures might be
1:17
working for woodland caribou, the
1:19
Gulf oil spill and the fish we don't
1:22
see. And why
1:24
tiny black holes might be spinning through our
1:26
solar system. All this today on
1:29
Quirks and Quarks. A
1:32
few years ago, researchers working
1:34
in the lush tropical Budongo
1:37
rainforest in Uganda saw something
1:39
peculiar. A group of
1:41
chimps were huddled together at the base of a
1:43
big hollow tree. They were
1:45
reaching in and retrieving something that they
1:47
were then eating. And
1:49
upon closer inspection, what they were
1:51
eating was kind of nasty. It
1:54
was bat poop. Apart
1:56
from the obvious ick factor, it
1:58
made the researchers wonder. wonder why were
2:00
they eating it and what
2:02
were they being exposed to? Bats
2:05
are known to be carriers of
2:07
several nasty pathogens that can spread
2:10
to other wildlife and to humans.
2:12
So they recruited some epidemiologists
2:14
and began to investigate, and what
2:16
they found could have an impact
2:18
on our understanding of how diseases
2:20
escape wildlife into the wider world.
2:23
Dr. Tony Goldberg is a professor of
2:26
epidemiology in the School of Veterinary Medicine
2:28
at the University of Wisconsin-Madison. He was
2:30
part of the team. Dr.
2:33
Goldberg, welcome to Quirks in Quarks. Thank you for
2:35
having me. Now tell
2:37
me about these chimps eating bat poop
2:39
or bat guano. Is this a new
2:42
behavior for them? This
2:44
is a new behavior and you're right, ick.
2:47
When we first saw this a few
2:49
years ago, we had never seen it before, so
2:52
that's despite the fact that these chimps have been the
2:54
subjects of research for decades. So if they had been
2:57
doing it, we would have noticed. So
2:59
what do you do to try to understand this
3:01
behavior better? We thought
3:03
about it and we realized that chimpanzees
3:06
have a problem that they have to
3:08
solve on a daily basis. Where do
3:11
you get your minerals? And in forests
3:13
like Budongo in Uganda, natural sources that
3:15
are rich in minerals are rare. So
3:18
we thought, aha, maybe they're doing
3:20
this because they're in search of
3:22
minerals in their diet. Now
3:25
were the chimps the only animals doing this
3:27
or were other animals also attracted to the
3:29
bat poop? Over several months,
3:31
we saw many instances of
3:33
chimps coming, black and white
3:35
colobus monkeys and red
3:38
diker, a kind of small cute forest antelope.
3:40
And they were all coming to
3:42
feast on this bat poop. So
3:45
why would these animals decide to eat
3:47
bat poop? So we knew
3:49
from decades of research at this site
3:52
that animals eat weird things in
3:54
their pursuit of minerals. The
3:58
question that really got us interested though is why
4:00
did they just start doing this now? Chimpanzees
4:02
and other animals have their
4:05
preferred sources of natural dietary
4:07
minerals. One of those sources,
4:09
its scientific name is Raffia
4:11
farinifera, and it used
4:13
to be very abundant in this
4:15
environment. And when that tree died,
4:17
the rotting inner pith of the
4:19
tree was very rich in sodium
4:22
and other minerals, and chimpanzees loved
4:24
it. About 20
4:26
years ago, that tree all
4:29
but disappeared in Budongo. There was a
4:32
demand in the area for
4:34
the leaves of that tree to
4:36
make strings for drying
4:38
tobacco leaves that were
4:40
produced during tobacco farming.
4:43
And these animals lost dietary minerals, so
4:45
they had to find something else. And
4:49
that's when we started to see them eating guano,
4:51
which is rich in the minerals that they used
4:53
to get from this tree. Well,
4:56
how were they able to eat the bad
4:58
feces and not get horrendously sick to the
5:00
stomach? We have all wondered that.
5:03
I get horrendously sick to the stomach just
5:05
watching them eat the bad guano. All
5:07
I can say is that these
5:09
animals naturally eat
5:12
soil. It's a
5:15
behavior that we call geophagy. And
5:18
it's not too much of a stretch to
5:20
go from eating soil to eating a pile
5:22
of something that looks like soil. Well,
5:24
what minerals are the chimps getting
5:27
from the bad poop? They are
5:29
getting a lot of phosphorus, also
5:31
calcium and magnesium. They're getting sodium.
5:34
Not as much as we thought,
5:36
but phosphorus, magnesium, calcium, and sodium
5:39
are pretty essential elements for
5:41
a diet. Okay,
5:44
so if it's so nutritious, why
5:46
is it concerning that the animals are eating
5:48
these feces? It's
5:51
concerning because we know something else
5:53
about bats. We also know
5:56
that bats carry interesting and
5:58
sometimes dangerous animals. pathogens.
6:01
We think that bats are the
6:03
source of coronaviruses, many coronaviruses that
6:06
have caused outbreaks in humans like
6:08
the SARS coronaviruses. So
6:10
did you find any of those pathogens in
6:12
the bat guano? We sure did.
6:14
We found 27 viruses
6:17
in this bat guano. Two-thirds
6:19
of them are things you'd
6:21
expect to find in insects because
6:23
these bats are eating insects, so
6:25
that wasn't surprising. We found some
6:27
fairly obscure viruses of mammals, but
6:30
we also found something surprising,
6:33
a first cousin relative to
6:35
SARS coronavirus too. Wow.
6:38
Now are the chimps showing
6:40
any signs that they're getting
6:42
the coronavirus? They
6:45
are not. So we have not
6:47
seen chimps eating this
6:50
guano and then getting something that
6:52
looks like a coronavirus disease. That
6:54
being said, chimps in the wild
6:56
do get sick and they do
6:58
get respiratory infections, but they're rarely
7:00
diagnosed, so we rarely have the
7:02
opportunity to know what they're infected
7:04
with, but it's plausible. So
7:07
why might this be a problem for human health?
7:10
We think that a lot
7:12
of human epidemics and maybe
7:15
even pandemics begin in
7:17
wildlife. This is not a new
7:19
idea. We've seen this with
7:22
Ebola, for example. There's
7:25
decent evidence that some human
7:27
Ebola virus outbreaks begin
7:30
when animals in the forest get
7:33
Ebola die and then humans touch the
7:35
carcasses. And another thing
7:37
that we realized when we first saw
7:39
this behavior is that three of the
7:41
animals that have been implicated as
7:45
hosts in Ebola outbreaks are
7:47
chimpanzees, black and white colobus, and dyker,
7:49
which are the same three animals we
7:52
saw eating the bat poop. Well
7:54
what does this mean for our understanding
7:56
of how viruses can spread from bats
7:58
to other animals? and then eventually to
8:01
us. It's sort of a
8:03
missing link because it was
8:05
never clear how these sorts
8:07
of chains of events happen
8:10
in nature. Well, how could knowing
8:12
about this missing link help us
8:14
prevent future disease outbreaks? I
8:17
can't help but think, what
8:19
if the solution to
8:22
the potential problem of
8:24
these animals being exposed to bat viruses
8:27
was as simple as giving farmers a
8:29
ball of twine so they
8:32
didn't have to cut down this tree and
8:34
dry their tobacco leaves. What
8:36
an incredibly inexpensive and
8:38
simple solution to this problem.
8:41
Just another amazing example of
8:43
the unintended consequences of human
8:46
activity. Exactly. Dr.
8:50
Goldberg, thank you so much for your time. You
8:53
are very welcome. Dr. Tony Goldberg
8:55
is a professor of epidemiology at
8:57
the School of Veterinary Medicine at
8:59
the University of Wisconsin-Madison. Caribou
9:12
are an iconic Canadian animal with
9:14
a long history in our landscape,
9:17
but they also have a long history
9:20
of struggling when humans encroach on their
9:22
habitat. The Southern
9:24
Mountain Caribou of British Columbia
9:26
and Alberta are particularly vulnerable.
9:29
They live in small groups and
9:31
need large undisturbed swaths of old-growth
9:34
forest in order to survive. Conservation
9:38
groups started rallying to protect these Caribou back
9:40
in the 1950s, but decades of
9:44
half-measures did nothing, and
9:46
populations still continued to decline.
9:49
So in recent years, scientists have been
9:51
trying anything and everything to save these
9:53
animals from long-term programs
9:56
like habitat restoration to
9:58
short-term strategies that seem extreme,
10:01
like captive breeding programs, penning
10:04
mothers and offspring to keep them safe
10:07
and even killing predatory wolves. And
10:10
in a new study, they've looked at which, if
10:12
any of these measures, is working and
10:14
whether caribou were really better or worse
10:16
off as a result. Dr.
10:19
Clayton Lamb is a wildlife scientist
10:21
at Biodiversity Pathways and the University
10:23
of British Columbia, Okanagan. He led
10:25
the study. Dr. Lamb,
10:27
welcome back to our program. Thanks for having
10:29
me today. First of all,
10:32
tell me about these caribou. Most
10:34
of us are familiar with the caribou and the high Arctic.
10:37
What are these mountain caribou like? So
10:40
in British Columbia and Alberta, especially in
10:42
the southern half of the provinces, there's
10:44
a special type of caribou called a
10:46
mountain caribou. And these are caribou
10:48
that basically live up in the mountains of
10:50
the Rockies and the Purcell's and the Selkirk's
10:53
and they eat arboreal lichen,
10:55
so the lichen in trees and also
10:57
the lichen found along the ground. And
11:00
these are animals that migrate up and
11:02
down the slopes as opposed to these
11:04
far distances like we see in the
11:06
Arctic. Oh, so they stay within the
11:08
Rockies? Yeah, exactly. They actually
11:10
typically stay in fairly small areas, sort
11:12
of distinct herds right now, partly due
11:14
to how few there are left, but
11:16
they don't move nearly as far as
11:18
the high Arctic animals. Now, why
11:21
is it so challenging to keep their
11:23
populations healthy? Yeah,
11:25
so southern mountain caribou are one
11:27
of the most challenging conservation issues
11:29
that Canada has right now. So
11:31
their populations have declined dramatically over
11:33
the last 50 years or
11:35
so. And it really comes down
11:37
to a landscape that's just not working for these
11:39
caribou. The landscape has
11:42
been transformed from industrialized resource extraction,
11:44
so logging, which has basically produced
11:46
a landscape that is more attractive
11:49
for deer and moose. And
11:51
that's not necessarily a bad thing in that that can
11:53
be good for hunters and it is good for
11:55
deer and moose, but it brings in wolves.
11:58
And caribou basically... struggle to
12:00
coexist with high predator densities. And
12:02
those wolves prey on
12:05
caribou on sustainable race and have
12:07
precipitated very dramatic declines of caribou
12:09
populations across southern Canada. Well,
12:11
when you say dramatic decline, how much have
12:13
their populations gone down? By
12:16
over 50% in the last 30 years,
12:19
and a number of those distinct
12:21
herds have actually been completely lost.
12:23
So they've gone to zero and
12:25
the actual distribution of caribou is
12:27
shrinking quite dramatically. Wow. Take
12:30
me through some of the interventions that are being used
12:32
to help save the caribou. Yeah,
12:35
so there's a number of interventions
12:37
that are being used to keep
12:39
caribou on the landscape while habitat
12:41
restoration and protection is underway. And
12:43
the important thing there is to
12:45
sort of create a landscape that
12:47
works for caribou could take decades.
12:49
And so in that interim period,
12:51
we need to keep caribou around.
12:53
And those interventions are
12:56
largely focused on reducing this unsustainable
12:58
predation on caribou. And so
13:00
they range from maternal pens, which
13:02
is bringing caribou into sort of
13:05
a high elevation enclosure where they would sort of
13:07
naturally be at that time of year to have
13:09
their calves and safety. Some
13:11
of the other actions are reducing
13:13
the density of wolves. So, you
13:15
know, because this landscape has been
13:17
so dramatically transformed, the density of
13:19
wolves is much, much higher than
13:21
caribou historically co-existed with. So
13:24
there is the direct removal of wolves
13:26
and then also other ways to reduce
13:28
wolves through reducing the number of moose,
13:30
which eventually should reduce the density of
13:32
wolves. So, you know, people are trying
13:34
all sorts of different things, including also
13:36
feeding caribou and just trying to keep
13:39
these caribou around as best as they
13:41
can using the tools that we have in hand.
13:44
And what did you find? What we found
13:46
was that since 1990s,
13:48
the population of Southern Mountain Caribou has declined
13:50
quite dramatically by over 50%. So in the
13:52
1990s, there was around 10,000 caribou.
13:54
And today
13:58
there's just shy of 5,000. But
14:01
we did find that those recovery measures
14:03
that were applied have increased the population
14:05
by quite a bit, by over 1,500
14:07
animals compared to what would have been
14:09
here otherwise. And what
14:12
is really working for caribou is
14:14
the reduction of predators. So the
14:17
reduction of wolves and additional recovery
14:19
interventions that are supporting the recovery
14:21
of caribou on top of the
14:24
wolf productions are maternal penning, so
14:26
to keep those calves safe and
14:28
feeding caribou. So
14:31
would you consider the programs a success
14:33
then? I mean
14:35
from a caribou perspective and from
14:37
the perspective of trying to keep
14:39
caribou around and averting the loss
14:41
of those herds, yes, the wolf
14:44
reductions and the remainder of the
14:46
restoration or recovery actions that were
14:48
applied have avoided the excavation of a number of those
14:50
herds. Now we've
14:53
talked on this program a lot about the importance
14:55
of predators in an ecosystem. Are
14:58
you concerned that these
15:00
interventions of reducing the number of predators
15:02
could have other problems in the ecosystems?
15:05
Yeah, I think we have to consider that. I
15:07
mean we don't want to sort of trade one
15:10
problem for another. You know I
15:12
think we are seeing some shifts in
15:14
the landscape and the composition of species
15:16
on it and I think we have
15:18
to keep our mind to what the
15:20
additional ecological consequences could be. From
15:23
the wolf perspective, generally the wolf
15:25
density is brought quite low, like
15:27
the target is less than three
15:29
wolves per thousand square kilometers and
15:31
it generally quickly rebounds after they
15:33
are reduced due to dispersal from
15:35
outside the area. So there usually
15:38
remains some wolves in these areas
15:40
but not as many as there
15:42
were previously. Why
15:45
is it important to protect the caribou to
15:47
this extent? Well
15:50
in this case it's sort of this
15:52
binary option of if we don't protect
15:54
them, they will be lost.
15:57
There are a number of these herds that have already
15:59
been... been completely lost before these
16:01
interventions took place. And if
16:05
the interventions that did take place weren't
16:07
done, a number of the other herds
16:09
would have been lost. And so we're
16:11
essentially in the situation where we either
16:13
act to keep caribou on the landscape
16:15
or they will rapidly not be in
16:17
British Columbia and Alberta. It
16:20
does speak to the larger vision here
16:22
though that this is an interim action
16:24
and we don't necessarily want to be
16:26
solely sustaining a caribou population off these
16:29
interim actions. They are expensive,
16:31
they have ecosystem and ethical
16:33
concerns, especially on the wolf
16:35
cull side. And this
16:38
is an intervention to stave off extirpation,
16:40
but we need to be thinking forward
16:42
to restoration of course. So how do
16:44
we make a landscape that will work
16:46
for these caribou so that these are
16:48
truly interim actions and not, that doesn't
16:50
form the backbone of what keeps caribou
16:52
around forever. So what's
16:54
the next step for you now that you
16:56
have this information? I
16:58
mean, I think that the work here
17:01
can inform, you know, what are the
17:03
effective strategies to keep caribou around in
17:05
the interim? Like if folks are going
17:08
to be applying these interventions, then we
17:10
should use the ones that are working.
17:13
And for our research program
17:15
is certainly shifting rapidly towards
17:18
this restoration focus. So trying to
17:20
think about what does a landscape
17:22
that works for caribou look like
17:25
and how do we create it
17:27
as fast as possible, as
17:29
efficiently as possible and what are the strategies
17:31
that we haven't thought of that can help
17:33
us do that. Dr.
17:36
Lam, thank you very much for your time. Thank
17:39
you. Dr. Clayton Lam is a
17:41
wildlife scientist with Biodiversity Pathways and
17:43
the University of British Columbia, Okanagan.
17:56
The Chinook salmon is the biggest salmon living
17:58
in the Pacific North. Northwest today, it can
18:01
grow up to be a meter and a half
18:03
long and weigh over 100 pounds. But
18:07
once it had a relative that dwarfed it,
18:10
the now extinct Oncorhynchus rasterosus
18:12
was the largest salmon known
18:14
to science. It
18:16
was almost twice the length of the Pacific
18:18
salmon alive today, a full
18:20
three meters. And
18:23
if that wasn't impressive enough, it
18:25
also sported two oversized front teeth
18:28
that originally earned it the nickname
18:30
of the saber-toothed salmon. But
18:33
a new study by paleontologist Karen
18:35
Clason suggests that this name needs
18:38
a rethink, because those
18:40
teeth weren't fangs at all. Instead,
18:42
they stuck out of the side of
18:44
the salmon's head like tusks. Dr.
18:47
Clason is a paleo-ichthyologist and
18:49
professor of anatomy at the
18:51
Philadelphia College of Osteopathic Medicine.
18:54
Dr. Clason, welcome to Corks and Corks. Thank
18:57
you so much for having me. I'm really glad to talk
18:59
about this. When did we first
19:01
learn about these giant salmon? The
19:04
first giant salmon were found probably
19:06
in the 1960s, and then they
19:08
were ultimately published in the early 1970s. What
19:11
did they look like? So what
19:14
we can tell from most of
19:16
their bones is that they look like really
19:18
enormous versions of the salmon that we're aware
19:20
of now. And they
19:22
had this very unique bone
19:24
at the front of their mouths that would
19:26
have had this very large bulbous shape to
19:28
them and these enormous teeth
19:31
on them. And based on
19:33
what we think that most of the animals
19:35
would have been related to, we
19:37
assumed that they faced down like sabers.
19:39
So that was the original construction, to
19:41
have this very large head with big
19:43
fangs that faced into the mouth. When
19:46
did these salmon live? So
19:48
we have evidence that they would have
19:51
been around about five million years ago
19:53
at this point in time, probably transitioning
19:55
between the Miocene and the Pliocene. And
19:57
where were the fossils found? fossils
20:00
that we found around the time of 2011 till
20:02
2014, those were found in the same locality. It's
20:08
known as the Gateway locality in Oregon.
20:11
Oh, so they were Pacific
20:14
salmon then? Yes, definitely. They are
20:16
absolutely part of this entire group known
20:18
as the Pacific salmon. And you gave
20:21
the full scientific name earlier, which is
20:23
Oncorhynchus rastrosis. And Oncorhynchus is the genus
20:25
name for all of the living and
20:28
modern Pacific salmon as well. Well,
20:30
what made you reconsider these teeth that
20:33
were originally thought to look like fangs?
20:35
Well, the fact was that they found
20:38
remarkable specimens that had all of these
20:40
bones in place. So everything was in
20:42
situ. Everything was preserved in three dimension.
20:45
We had two fish very
20:47
closely situated together as if they
20:50
were in a breeding situation. And
20:52
they both had these enormous bones
20:54
plus their tusks and they were
20:56
all facing outwards. What do
20:59
you mean facing outwards? Tell me about that. So
21:01
as we thought with the saber tooth salmon
21:03
configuration, they would have faced down like we
21:05
have with all the modern salmon today. They
21:07
would have been able to grab at their
21:09
food and sliced it or grabbed and held
21:11
on really tight. It turns
21:13
out that these are filter feeding
21:16
salmon. And so they wouldn't
21:18
have used their teeth for that anyways. And
21:20
so now these teeth that are facing outwards.
21:22
They actually look more like a warthog. Some
21:25
people describe them almost looking like a mustache.
21:27
They have this completely unique configuration that looks
21:29
like they could have been spikes and used
21:31
for tools that if they
21:33
slash their head from side to
21:36
side, they would have created a
21:38
very, very unique aspect to these fish. So
21:40
what part of their face today stick out
21:42
of? So right at the tip of
21:44
their rostrum it's called. So right at the
21:46
front where we would expect the modern
21:49
salmon to have this major change happen during
21:51
metamorphosis. So if you've ever taken a look
21:54
at pictures of when they're breeding, they're this
21:56
bright red color and they have this kind
21:58
of greenish head. All of
22:00
the males have a very, very long russum.
22:02
Their nose almost looks like gonzo from the
22:04
Muppets. This is the
22:06
same bone that is changing in the
22:09
fish that we're describing. And
22:11
what's also interesting is though that males and females
22:13
are doing it in these fossils, which is unlike
22:15
what the modern do now. Boy.
22:19
And were they curved? Did they curve back
22:21
or curve forward or stick straight out? They
22:23
kind of blew up like balloons right at
22:26
the front, and then they just stuck
22:28
straight out towards the side. So instead of
22:30
creating this long hook in the front,
22:32
they actually more a tiny little
22:34
hammerhead almost if you will. Wow.
22:37
And you say both the males and the females had
22:39
this. They did. They
22:41
did. So unlike all of
22:44
the salmon that are around today, we
22:46
only see the changes occurring in a
22:48
few of the bones. And
22:50
so we still see the changes that are
22:52
occurring due to metamorphosis in
22:54
the males, but not on this particular
22:57
bone, not this pre-maxilla with these teeth.
22:59
So this is occurring in
23:01
both the male and the female on
23:03
this particular fossil, which is definitely unique.
23:06
Well, you said that these salmon
23:08
were filter feeders, sort of
23:10
like baleen whales. So they plankton and stuff like
23:12
that. They didn't eat other fish. So
23:15
why would they need these large teeth sticking up
23:17
the side of their head? That's
23:19
a great question. So the ideas
23:22
that we've been coming up with have a lot
23:24
to do with strategy for probably defense,
23:26
maybe a little bit of offense. And
23:29
these were really large. Perhaps they could have
23:31
been a very tasty meal for some type of predator. And
23:34
the fact that they were so large, they had
23:36
these very strong muscles that would have helped to
23:38
move their entire body while swimming. These
23:41
would also be able to move their head. And
23:43
so they could create a lot of force to
23:45
ward off some type of predator. They
23:47
could have created a lot of force to
23:49
keep other competition out of the way. It
23:51
makes me think a little bit of when you
23:53
think of the street races and the movie Grease
23:56
and their spikes coming out of their
23:58
tires or something to just keep them away from you. Perhaps
24:00
by the time that they got up
24:03
to the area where they were ready
24:05
to breed, they would have used them
24:07
for tools to actually build the nests
24:09
where the eggs on the sperm would
24:12
have been deposited. Once those
24:14
nests are in place and the fry exists,
24:16
they could have potentially protected that
24:19
nest from other sorts of predators as
24:21
well. Now, how can
24:23
you tell that this wasn't a one-off, that
24:26
not all of these giant salmon had these spiked
24:28
teeth? Well, the fact that we
24:31
didn't have only one specimen with this configuration
24:33
was a good tip-off. And
24:35
then we were actually using medical
24:37
imaging. We used CT scanning at
24:39
an industrial strength to look inside
24:42
the rock and start to remove
24:44
the sediment and the matrix that
24:46
was surrounding and protecting the really delicate parts
24:48
of the bones that we don't tend to
24:50
get to see otherwise
24:52
when the fossils are preserved.
24:55
So by using this technology to
24:58
appear inside the entire skull, we
25:00
were able to find the small processes that
25:02
fit together like puzzle pieces that
25:04
said that this is the actual configuration that
25:06
it should have been. What
25:08
went through your mind when you realized that these
25:10
salmon had this strange formation sticking out the sides
25:12
of their heads? I just thought it
25:14
was really fascinating and thought to myself, again, why
25:17
would you be doing this? And
25:19
why don't we see it in a lot of
25:21
other animals now? It's not a strategy that a
25:23
lot of animals are using at all. And
25:26
so it was pretty unique. Well, why
25:28
do you think modern day salmon don't have these
25:30
teeth? So if you think about
25:32
it from an evolutionary perspective, these are
25:34
not the ancestors to the modern salmon.
25:36
They're probably more derived
25:39
or as derived as some of the ones
25:41
that are around now. So it wouldn't have
25:43
been something that came first and then left
25:45
the modern ones around. These actually existed and
25:47
co-existed at the same time as some of
25:49
the species that are around today like the
25:51
sockeye. And
25:53
I think it was a very interesting experiment. And
25:56
so not a lot of the other ones though
25:58
would have tried it. seems, at least
26:00
based on what we can see in the fossil record. So
26:03
for any time travelers out there, if you go back
26:05
a million years or so, don't go swimming in the
26:08
ocean. Yeah, I know. Well,
26:11
there are some pretty large animals that are
26:13
in the ocean nowadays, but they don't school
26:15
quite as much as what we would think
26:18
about for those salmon as well.
26:20
So could you imagine seeing so many of
26:22
them all together at once coming and charging
26:24
at you? I don't know. That
26:27
would have been pretty crazy. Patrick Gleason, thank you so much for your time.
26:29
Thank you. Dr. Karen Gleason
26:31
is a paleo ichthyologist and an
26:33
anatomist at the Philadelphia College of
26:36
Osteopathic Medicine. I'm Jordan
26:38
Heathralling's host of The Big Story. For
26:41
six years now, we've been telling one
26:43
story a day, every one of them,
26:45
about something that matters to Canadians. This
26:47
spring, though, we're going deeper. The
26:50
Big Story presents Paydirt,
26:52
the inside story of Ontario's
26:54
Greenbelt scandal, from political games
26:57
to stag and doe parties,
26:59
endangered species, RCMP investigations and
27:01
Las Vegas massages. You
27:04
will hear the full story. The Big
27:06
Story presents Paydirt, new episodes
27:08
every Monday, and you can get
27:10
them all by following The Big
27:12
Story wherever you get your podcasts.
27:16
I'm Bob McDonald, and you're listening to Quarks
27:18
and Quarks on CBC Radio One. Coming
27:20
up later in the program. Could
27:22
the universe be full of tiny black holes
27:25
that occasionally blast through our planet? So it's
27:27
like a bullet through cotton candy. These things
27:29
enter one side of the planet, they're out
27:31
the other, and then they're off into space,
27:33
never to come back again. Fourteen
27:37
years ago this month, the
27:39
Deepwater Horizon oil well disaster
27:41
began, ultimately releasing
27:43
an estimated 800 million liters of
27:46
oil and gas into the Gulf
27:48
of Mexico. It was
27:50
the largest accidental marine oil spill
27:52
in history. At
27:55
the time, scientists flocked to the
27:57
scene to understand how this unprecedented
27:59
pollution Not just the
28:01
oil, but the chemical dispersants released to
28:03
break up the spill would affect
28:05
the rich ecosystem in those waters. Much
28:09
of the early research focus was
28:11
on the economically important species in
28:14
the area, like tuna, swordfish, shrimp
28:16
and oysters, and
28:18
these species fortunately recovered
28:21
quickly. That seemed like good news.
28:24
Canadian biologist Pro Santa Chakrabarti was also
28:26
on the scene at the time, but
28:29
he was focused on the rarer creatures that
28:31
live only in the deepest parts of the
28:33
Gulf, closest to where the
28:36
chaos was happening. And for
28:38
these animals, the picture is less rosy.
28:41
In his latest study, Dr. Chakrabarti and
28:43
his colleagues report that out of the
28:46
78 endemic species, 29 of
28:48
them haven't been spotted in the years since the
28:51
spill. Dr. Chakrabarti
28:53
is a professor and curator
28:55
of fishes at Louisiana State
28:57
University's Museum of Natural Science.
28:59
Hello and welcome to our program. Thanks for having me.
29:02
Now we've heard for a while how the
29:05
fish populations in the Gulf seem to be
29:07
holding steady after the spill, but
29:09
now you're saying that's not the whole story? Yeah,
29:12
unfortunately it's not. You know, we
29:14
typically focus on the food fish
29:16
that we eat, right? The fish
29:18
that are commercially important. But
29:21
those are only a handful of species while
29:23
there's actually 1,500 or
29:25
more species in the Gulf of Mexico of fishes.
29:28
And those are the ones I'm also
29:30
interested in that are often overlooked, and
29:32
that's the focus of these papers. Well,
29:35
why did you want to focus on the animals in the deep
29:37
ocean? Well, the oil spill happened in
29:40
the deep sea. So
29:42
that's the part of the world, not
29:44
just the Gulf of Mexico, but of
29:47
the world that we know the least
29:49
about, this deep sea, cold, perpetually dark
29:51
ecosystem that houses some amazing species that
29:53
are bioluminescent, that are doing all kinds
29:56
of things that we know very little
29:58
about, and, you know, they're endangered,
30:01
then somebody has to speak for them.
30:03
And that's our role as scientists. Well,
30:06
now 14 years after the disaster, what
30:08
do we know about the long-term effects
30:11
of the oil spill? Not
30:13
as much as we would suspect that we would
30:15
know by now. Still, 14 years
30:18
later, another spill were to happen
30:20
tomorrow. I'm afraid that we just
30:22
don't know the impacts of how
30:25
a deep sea environment would be
30:27
impacted and affected any better
30:29
than we were 14 years ago. And
30:32
that's problematic. And it's in part due
30:34
to the difficulty in studying the deep sea.
30:37
There have been efforts to make
30:40
new collections, to make new
30:42
environmental impact assessments. But
30:44
it's still a drop in the bucket compared
30:46
to how much we could know. Well,
30:49
you mean nobody's been down to actually look at
30:51
what's going on down there? Not
30:54
in a way that people would expect. So
30:56
it's not like we can easily get to
30:58
1,000 meters. Very
31:00
few submersibles exist that can
31:03
get to the bottom of the ocean still.
31:05
And long-term studies
31:08
are just difficult to do in these
31:10
perpetually dark environments. And so figuring
31:14
out populations of deep sea fishes
31:16
is almost impossible. Well,
31:18
tell me about how you've been looking at
31:21
the species that seem to be disappearing. Yeah,
31:24
for me, as a museum curator,
31:26
our collections are this library
31:29
of the Earth's biodiversity. And
31:32
these collections have specimens or
31:34
vouchers, as we call them,
31:36
of creatures from around the
31:39
world. And so I thought it'd be
31:41
useful to use this library. And
31:44
we all share our data. So
31:46
we can look online and see
31:48
where specimens from around where the
31:50
spill happened, where
31:52
were they collected, when were they collected,
31:55
and can we make a sort of
31:57
guesstimate or estimates of how
31:59
these populations are doing. So
32:02
I want to know what species
32:04
have we not seen since the time of
32:06
the spill or from before the spill that
32:08
we should know more about. And those
32:10
are the 29 species that you mentioned that
32:12
are still quote, missing, things
32:15
that we haven't seen from the time of the
32:17
spill or before. So how many
32:19
animals usually get added to a museum collection?
32:22
That's an interesting point. And so it
32:24
sort of depends if there's survey work
32:26
being done. So in my
32:28
own collections here, we have
32:30
about 300,000 fish from 60 or so different countries.
32:35
And 300,000 fish sounds like a lot. But
32:37
5 million fish are caught every minute
32:39
by the fishing industry. So
32:42
often what's being caught in the
32:44
Gulf and other parts of North
32:47
America, what's not the target
32:49
fish. So if they're targeting menhaden, all
32:51
that other fish gets thrown overboard, the
32:53
bycatch. And so that's
32:56
a larger portion of some
32:59
of the species that might be so-called missing
33:01
that we might not have data for. And
33:04
so they only become data when they're in a
33:06
museum collection. And that's what we're here for. Are
33:09
there any species that only exist in
33:11
the Gulf of Mexico? Yeah, in fact, those
33:14
are the species that we were targeting. So
33:16
there's 1,500 or so species
33:18
in the Gulf of Mexico. But many of them are
33:20
found in this very
33:22
wide range. I was
33:24
interested in those that are only found in
33:26
the Gulf of Mexico, so not even in
33:29
the Caribbean or on the eastern coast of
33:31
the US. So
33:33
those species, there's only 78 of those
33:35
species. And
33:38
so those are the ones that we focused on as
33:40
sort of a proxy for what's going on
33:42
in the entirety of the Gulf. Well,
33:45
tell me about some of these animals.
33:47
What are they like? Yeah, perhaps the
33:49
most well-known of these will be the
33:51
pocket shark. So that species was actually
33:53
described around the time of the oil
33:55
spill. And it's a
33:57
shark that's not even a foot long, big
34:00
old head. It's actually very cute as far
34:02
as sharks go. It's got
34:04
dark skin, it's bioluminescent, and
34:07
so it produces light. And there's
34:10
only been one specimen ever found, ever.
34:13
There's a fringe lantern shark,
34:15
which was only seen right before this
34:17
bill in 2009. There's an eel
34:21
pout and other sharks and rays and
34:23
hag fish, things that people don't eat
34:25
and most people don't think about, but
34:27
I do and other scientists
34:29
do. And some of those
34:31
that I mentioned haven't been seen since
34:33
the 60s, from well before the spill.
34:36
But even with targeted efforts, we would expect
34:39
to see one or two more specimens, but
34:41
they are only known from the Gulf and
34:43
we haven't seen them since. Now,
34:46
is it possible that the reason these
34:48
species haven't been seen is that, well,
34:50
they've just evaded capture all these years?
34:52
Oh, certainly, yeah. So some of these
34:54
species have, again, you know, haven't been
34:56
seen since the 60s. And
34:59
they're deep sea animals that are very hard
35:01
to get. The Gulf's a very big place
35:04
and so you just have
35:06
to get lucky sometimes. But with
35:08
more effort and especially around the region
35:11
of the spill, I think we can
35:13
learn more and we should learn more
35:15
about what exists. Now
35:17
you were on site at the oil spill 14
35:19
years ago. Did you think you'd still be calling
35:21
attention to the deep sea animals all these years
35:24
later? When I came
35:26
to Louisiana, and I'm a Canadian who
35:28
lived in New York for a long
35:30
time before I moved here in 2008,
35:33
I didn't really feel like a Louisiana until
35:35
the oil spill happened. It made me really
35:37
feel a connection to this place. And all
35:39
of a sudden, I just fell in love
35:41
with the Gulf, especially when it was endangered.
35:43
This 12 weeks of the spill made
35:46
me really feel like Louisiana was home.
35:48
And it's still very much home 15
35:51
years later since I've
35:53
been here. And I couldn't
35:56
imagine then how little we still
35:58
know. the remnants
36:00
of the oil at the surface was gone, it
36:02
was out of sight and out of mind. And
36:05
even though there may be smaller spills,
36:07
the impact of that spill, I
36:10
wish we knew more. And I'm surprised we still know
36:12
so little 15 years later. So
36:15
the Gulf is this wonderful place shared
36:17
with several countries that I
36:20
think deserves more attention. Dr.
36:23
Chakrabarti, thank you so much for your time. Thank
36:26
you for having me, and thanks for calling attention
36:28
to the spill. Dr. Prasanta
36:30
Chakrabarti is a Curator of
36:32
Fishes at Louisiana State University's
36:34
Museum of Natural Science. Let
36:51
me take you back to the Big Bang. The
36:54
universe explodes into existence
36:57
as an infinitely dense, infinitely
36:59
hot point, and immediately
37:01
starts to expand at a tremendous
37:03
rate. Almost
37:08
instantaneously matter evolves out of
37:10
pure energy, and the
37:13
tiny proto-universe is filled with
37:15
super-hot stuff. Then,
37:18
perhaps, something very strange
37:20
happens. So it's possible
37:23
that just white noise, little
37:25
fluctuations in the density of this huge
37:27
bath of matter in the early universe,
37:29
could have produced huge numbers of black
37:31
holes that could have had really any
37:33
range of masses. That's
37:35
physicist Matt Kaplan, and what he's
37:37
talking about is the theory of
37:39
primordial black holes. These
37:42
are black holes that have been around for 13.7 billion years
37:44
since the birth of our
37:47
universe. And if
37:49
researchers' suspicions are correct, they
37:51
could come in a range of sizes, from
37:54
the unimaginably tiny to the
37:57
supermassive, and the universe
37:59
might be full. of them. Invisible.
38:01
Largely undetectable. Some
38:04
of the smallest of these
38:07
primordial black holes might also
38:09
be a promising candidate to
38:11
explain another mystery. The coincidentally
38:13
invisible and so far undetectable
38:15
dark matter that astronomers say
38:18
makes up more than four-fifths of the mass
38:20
of the universe. Dr.
38:22
Kaplan. It's just a fact that most
38:24
of the matter in the universe doesn't
38:26
light up. It doesn't seem to interact
38:28
with light and it doesn't seem to
38:30
have electric charge. So this
38:33
puts real restrictions on what it could
38:35
be. It might be some new undiscovered
38:37
particle. But when I think of matter
38:39
that doesn't light up, black holes
38:41
really fit the bill perfectly, right? I mean, I'm
38:43
not crazy for thinking that. Well,
38:45
history will be the judge. But
38:47
if he's right that these primordial black
38:50
holes form shortly after the Big Bang,
38:52
the next natural question is, can
38:55
we find the ones that could be the solution
38:57
to the dark matter mystery? Well,
39:00
maybe. And maybe right
39:02
in our stellar neighborhood. Dr.
39:04
Kaplan is a professor of physics
39:07
at Illinois State University in Normal,
39:09
Illinois. Hello and welcome back to Quirks
39:11
and Quarks. Hey Bob, good to be back.
39:13
First of all, tell me what a primordial
39:15
black hole is. So
39:18
a primordial black hole is a
39:20
black hole. Let's start with that. A black
39:22
hole is just this overdense region of space
39:24
time that's collapsed on itself to produce a
39:26
singularity. The question then is what
39:28
makes a black hole primordial and that's when
39:30
it formed. It takes very dense matter to
39:32
make black holes. So the most obvious way
39:34
to do this is in a supernova and
39:36
that makes these order solar
39:38
mass black holes. But the early
39:41
universe was incredibly dense. So it's
39:43
possible that just white
39:45
noise, little fluctuations in the density of
39:47
this huge bath of matter in the
39:49
early universe could have produced huge numbers
39:51
of black holes that could have had
39:53
really any range of masses. Why
39:55
do you think primordial black holes may be
39:57
the answer to the dark matter problem? I
40:00
like primordial black holes as a
40:03
dark matter solution because it
40:05
doesn't require new physics
40:07
beyond what we already know. If
40:09
dark matter is a new undiscovered
40:11
particle, that would be really cool,
40:13
that would be really exciting but
40:15
that's also this massive theoretical garden
40:18
of how many millions of
40:20
different possible particles that we
40:22
could theoretically think up. And
40:25
that's a step away from
40:27
known physics. Black holes are not unknown physics,
40:29
they are very well known. We've seen plenty
40:31
of them, we've seen the merging LIGO black
40:34
holes. So I don't think it would be
40:36
too much of a stretch to think that
40:38
some large number could have been produced in
40:40
the early universe. It seems like it has
40:42
the fewest assumptions of any dark matter explanation
40:45
I've ever seen. Okay, so primordial black holes
40:47
are the answer to dark matter. There's a
40:49
lot of dark matter out there so what
40:51
does that mean for how common these little
40:53
black holes would be? It
40:56
depends on their exact mass, right? So
40:59
the less massive these black holes would
41:01
be, the more abundant they would be
41:03
by number. And so they could
41:05
be whizzing through the solar system even if
41:07
they're low enough mass. But if
41:10
dark matter is made of black holes and they're
41:12
passing through our solar system, wouldn't we notice that?
41:14
Because black holes do have a tendency, as you
41:16
say, to eat things and stuff
41:18
that falls into them lights up and all that.
41:21
Yes, they would be very easy
41:23
to miss. The amount of dark matter in the
41:25
solar system is comparable to a molten. So if
41:28
we said, well, what if that was all a
41:30
black hole? So what if there was roughly one
41:32
black hole, the mass of a mountain, passing through
41:34
the solar system at any given time? That
41:36
black hole would also be about the size of an atom.
41:39
So it would be very easy to miss. You're probably not
41:41
going to find it with a telescope. But
41:43
you're onto it, which is that
41:45
occasionally things will hit planets,
41:48
stars, moons. And when
41:50
that happens, then something exciting and observable
41:52
could happen. Wait a minute. A
41:54
black hole the size of an atom? Oh,
41:56
yeah. Yeah. Straightforward homework problem.
42:00
So it's the sort of asteroid mass black
42:02
holes that could potentially explain the dark matter
42:05
So what then would happen if
42:08
one of these atom-sized black holes was to hit
42:10
the earth? So people
42:12
have thought about this there are actual real
42:14
peer-reviewed Publications about what would happen if
42:16
one of these itty-bitty teeny tiny black holes hit
42:18
the earth if you can believe it or not
42:22
So a black hole of that
42:24
mass would be falling in at a very
42:26
high speed. It's coming from the galaxy So
42:29
it's going fast. It's falling towards the earth
42:31
and accelerated by Earth's gravity So it's going
42:33
to be fast So it's going significantly faster
42:35
than escape velocity when it enters the atmosphere
42:37
and it's so small It can
42:39
barely eat any mass while it's passing through
42:41
the planet So it's like a bullet through
42:44
cotton candy these things enter one side of
42:46
the planet They're out the other and then
42:48
they're off into space never to come back
42:50
again And it all happens in a few
42:52
seconds Wow So they're above the
42:54
atmosphere and they're invisible and then as soon as
42:56
you put matter around them that they can start
42:58
To pull in they're going to start
43:00
to get very hot and bright because matter falling
43:03
into a black hole is going very fast It
43:05
gets heated by friction colliding with other matter that's
43:07
falling in and what you get
43:09
are these really bright accretion discs These
43:11
are the pictures that you usually see
43:13
those orange bands around black holes. Those
43:15
are these accretion discs So you
43:17
have a black hole that's now entering the atmosphere
43:19
and it is lighting up like a fire as it
43:22
streaks through the sky Punches through the planet punches all
43:24
the way through to the other side and leaves like
43:26
a shooting star coming up from the ground Okay,
43:30
so if one passed through my house what I noticed
43:33
Yeah, you your house would probably be
43:35
on fire and It
43:38
depends on the mass of the black hole
43:40
because the masses have this huge range of
43:42
masses The smallest ones could potentially leave your
43:44
house intact and the biggest ones would probably
43:46
destroy your house and the neighbors Now
43:49
do we have any evidence that little black
43:51
holes have gone through the earth and he
43:53
scars any any holes through the planet? So
43:57
to the best of our knowledge we haven't found
43:59
any of these that doesn't mean they don't exist.
44:01
And that's because the Earth has surface
44:03
processes. It has rain, it has wind,
44:06
it has erosion, it has seasons. All
44:08
of these things tend to erase surface
44:11
impacts in craters. Only the
44:13
largest, biggest, beefiest craters in
44:15
deserts stick around for a
44:17
really long time. So
44:19
if you did wanna look for evidence
44:21
of primordial black holes hitting the Earth,
44:24
you should probably start with the moon because the
44:26
moon doesn't have those things that would
44:28
erase the evidence of those impacts. Okay,
44:32
so do we have any evidence on the
44:34
moon? I know it's covered in a lot
44:36
of craters. It's been hit a lot by
44:38
real asteroids, like actual asteroids. Any signs that
44:40
it's been hit by black holes? Indeed
44:43
it has. And so this is
44:45
a search that's ongoing. We have
44:47
done our first attempt and
44:50
the sizes of these black holes mean that
44:52
their craters are only a couple meters in
44:54
size. So think about the size of a
44:56
car. You could comfortably fill up one
44:59
of these craters just by standing in
45:01
it. And the highest resolution
45:03
surface scans that we have of the moon
45:06
are about a football field per pixel,
45:08
so like order 65 meters. And
45:11
as a result, the craters are too small to
45:14
even show up as one pixel if they exist.
45:16
So we've done a search for them as
45:18
a proof of concepts computationally through all of
45:21
these images. And we can't push
45:23
low enough to find them, but that doesn't mean they're
45:25
not there. What we hope is
45:27
that some future generation of satellite will
45:29
take surface images
45:31
that are 10 times higher in
45:34
resolution. And with that, we could
45:36
reasonably test this hypothesis. Well,
45:38
how could you tell the difference between a crater made
45:40
by a black hole and one made by an asteroid?
45:43
That is another fantastic question,
45:45
Bob. So a regular crater
45:47
is rock hitting rock. So that's like
45:50
a point explosion. That's like piling up
45:52
a bunch of TNT on the surface
45:54
and then detonating it. That's gonna make
45:56
those nice big round basin craters with
45:58
the ejecta blankets around it, sloping
46:00
anthill that sort of comes away from the
46:02
crater. A black hole doesn't do
46:05
that precisely because it goes
46:07
straight through the moon. The
46:09
black hole is a creating matter
46:11
creating this high
46:14
density, high pressure, high temperature volume
46:16
around it and it does this
46:18
as a big stripe. So
46:20
instead of having a point explosion like
46:22
the TNT on the surface or the
46:24
asteroid hitting it, you have a line
46:26
explosion. You could think it's the difference
46:28
between having all of your TNT and
46:30
a big pile on the surface versus
46:32
drilling a borehole and then filling that
46:34
with TNT and then detonating it. The
46:36
cratering dynamics and how it spreads matter
46:38
around the crater are going to be
46:40
different resulting in a different crater shape.
46:44
So would you have a hole right through the moon
46:46
and an exit crater on the other
46:48
side? You do get an exit
46:50
crater on the other side. So this is fortunate
46:52
for us. If a later asteroid comes and overwrites
46:54
one of them, you still have the other one
46:56
on the far side. So you don't have to
46:59
worry too much about that. The
47:01
hole through the moon, fortunately the moon's not
47:03
Swiss cheese. If you are deep
47:05
enough in the moon, the pressure is high
47:07
enough that the sort of sand and rock
47:09
will flow back and fill it in. So
47:11
you shouldn't think of it as like you're
47:14
gonna look through and see out the other
47:16
side. This is going to, on the surface,
47:18
look like a crater. It's just going to
47:20
have different dimensions than asteroid or impact made
47:22
craters. Okay, so we haven't seen
47:24
any black hole craters on the moon yet,
47:27
but possibly with instruments and better
47:29
resolution we might spot them. You
47:32
got it. Dr. Kaplan, thank
47:34
you so much for your time. Yep, so
47:36
good to be here. Thanks Bob. That
47:38
was Dr. Matt Kaplan, a professor of
47:40
physics from Illinois State University. Now
47:43
what's exciting is that if these
47:45
tiny primordial black holes are the
47:47
answers of the dark matter mystery,
47:49
we might already
47:51
have the observations we need to find
47:53
them. Theoretical physicists
47:55
from Belgium are proposing we
47:57
could find indirect evidence of
48:00
them from outside of our Milky
48:02
Way galaxy. All we
48:04
have to do is look for the
48:06
shadow of the shattered remains of stars
48:08
they've destroyed. Nicolas
48:10
Esser is the lead author of
48:12
the study and PhD candidate of
48:15
theoretical physics at the French pre-University
48:17
of Brussels. We caught up
48:19
with him in Montreal. Hello Mr.
48:21
Esser, welcome to Quarks and Quarks. Hello
48:23
Bob, thanks for having me. So where
48:25
do you think we might be able to
48:27
detect primordial black holes? Well
48:30
one possibility to study ultra-fine
48:32
dwarf galaxies. These galaxies
48:34
are small galaxies which are satellites of
48:36
our own galaxy, the Milky Way. Small
48:39
galaxies, now why these dwarf galaxies and
48:42
not our own Milky Way? So
48:46
in these galaxies we have seen for
48:48
observations of the motion of the stars
48:51
that there must be more dark matter
48:53
in there and hence potentially more black
48:56
holes. So if they
48:58
are the mass of an asteroid they would actually be
49:00
the size of an atom and
49:02
we wouldn't be able to see them which
49:04
is why we need some indirect
49:06
way of proving them. Okay,
49:09
since we can't see black holes what
49:12
are we going to see with the stars in their relationship
49:14
to the black holes? So one
49:17
possibility is that if primordial
49:20
black holes exist and are roughly of
49:22
the mass of an asteroid what
49:24
could happen is that when stars
49:26
form it actually starts from a
49:29
huge cloud of gas, a cloud which is
49:31
like tens of times the
49:33
size of our own solar system
49:36
and this cloud of gas when contracting
49:39
will carry with it the primordial
49:41
black holes that are moving around in
49:43
this cloud and these black holes would
49:46
be carried with the gas towards
49:48
the final product of this contraction which
49:50
is the star and
49:52
since this scenario works
49:54
better for heavier stars what
49:57
could happen is that this black hole would end up
49:59
well completely. stuck in the star
50:01
and would eat it. Oh
50:03
I see, so they would get caught up in
50:06
the big clouds of what just slow down by
50:08
friction because they're so small and end up inside
50:10
the star. So what happens from
50:12
that point? What has star with a black hole
50:14
in its center? What
50:17
happens from that point is that well we
50:19
know that black holes they basically
50:22
attract everything that's around them and once
50:25
you've entered a black hole you cannot get
50:27
out and what would happen is that
50:29
the matter in the star would slowly
50:31
get attracted inside the black hole
50:33
would be basically strongly eaten
50:36
with the technical term is accreted and
50:39
the black hole would slowly eat the particles of
50:41
the star and in a few million years what
50:43
could happen is that the stars would be completely
50:45
destroyed and there would be nothing
50:47
less apart from a remnant black hole which
50:50
would be roughly the mass of this initial
50:52
star. Holy smoke, talk
50:55
about indigestion, a star being
50:58
eaten from the inside out. Yeah that's
51:00
kind of the idea. Now you mentioned
51:02
that this would only happen to big
51:04
stars, why is that? Well
51:06
the reason is that if you have
51:08
a bigger star this means you
51:10
have a stronger gravitational attraction and
51:13
also you start with a bigger cloud
51:16
which means that you just have a
51:18
higher probability of capturing a black hole
51:20
and of getting an indigestion when
51:22
you have a bigger star. Okay
51:25
so then where will
51:27
the data come from when you're looking at
51:29
these dwarf galaxies that will tell you that
51:31
these primordial black holes are there that they've
51:33
eaten these stars? So
51:35
the observation we
51:37
could use is called the mass
51:40
function of the stars and this
51:42
basically is just the information of
51:44
how many stars you have for
51:46
a given star mass
51:49
right so this gives you the function of
51:52
the number of stars that functions their masses and
51:54
we can observe we can
51:57
measure this using our last telescopes such
51:59
as the the Hubble telescope, the James
52:01
Webb telescope, as well as the Euclid
52:03
telescope. These telescopes could allow us to
52:05
measure these mass functions, and if we
52:08
see that heavy stars
52:10
are missing, then this could
52:12
give us a hint that there is
52:14
primarily black holes in the 12th galaxy.
52:17
Oh, I see. So it's what you
52:19
don't see in these galaxies that tells you the
52:21
black holes are there if the big stars are
52:23
missing. Exactly. How
52:26
far along in this process are
52:28
you to count how
52:30
many big stars are missing out
52:32
of these galaxies? So actually,
52:36
there already exist measurements of
52:38
star counting in these galaxies.
52:40
These measurements exist. What
52:42
we are trying to do now is to
52:44
obtain these results, which are now in the
52:46
end of other astrophysicists, and try
52:49
to analyze the data with this idea
52:51
that high mass stars should be
52:53
missing. OK,
52:55
so if you do detect that
52:58
these big stars are missing
53:00
from these dwarf galaxies, and
53:03
that shows that there's probably black
53:05
holes there, what would
53:07
that say to you about the idea
53:10
that primordial black holes are going to
53:12
solve our dark matter mystery? I
53:15
wouldn't say it would be like a pure
53:17
confirmation that there is asteroid mass primordial
53:19
black hole in these galaxies, but it
53:21
would be a great hint towards this
53:24
idea. But of course, there could be
53:26
some other astrophysical explanations for missing high
53:28
mass stars in these galaxies. But it
53:30
would be a hint, and it would
53:32
motivate further study. How
53:35
much closer would your observations bring us
53:37
to the idea that these primordial black
53:39
holes even exist? It
53:42
cannot be approved, because it's still indirect,
53:45
so there can be other
53:47
explanations. But if
53:49
you combine different observations, among
53:52
which would be this observation of missing
53:54
high mass stars, then at some point
53:56
you would be convinced that, OK, that
53:59
it must be. these black holes
54:01
because we have three, four, maybe five
54:03
different observations. They all correlate. They all
54:05
say, okay, there should be
54:07
black holes. So it would
54:09
be a step among others to prove the
54:11
existence of these black holes. Mr.
54:14
Esser, thank you so much for your time. Well,
54:16
thanks for having me again. That was
54:19
Nicolas Esser, a PhD candidate at
54:21
the French Free University of Brussels.
54:25
And that's it for Quirks and Quarks this week. If
54:28
you'd like to get in touch
54:30
with us, our email is quirks
54:32
at cbc.ca or just go to
54:34
the contact link on our web
54:36
page at cbc.ca/quirks where you
54:39
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54:41
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54:43
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54:45
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54:50
and Quarks is produced by Livia
54:53
Diring, Olsi Sorokina, Amanda Buckowitz and
54:55
Sonja Biding. Our senior producer is
54:57
Jim Lemons. I'm Bob
54:59
McDonald. Thanks for listening. For
55:12
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