Supernovae: Witnessing Cosmic Explosions Firsthand – Yvette Cendes
Watch on YouTubeVideo summary
The video explores the fascinating phenomenon of supernovae, beginning with an observation of familiar constellations like Orion. The speaker highlights Betelgeuse, a massive red star located in Orion's shoulder, which is currently believed to be nearing the end of its life and destined to explode as a supernova. This event serves as a prime example of how stars vastly differ in size and lifespan; while most stars like our Sun simply shed their outer layers quietly at the end of their lives, massive stars swell into giants before culminating in a catastrophic explosion. A supernova is described as the most powerful explosion known in astronomy, capable of outshining an entire galaxy for a brief period and remaining visible from billions of light-years away.
Historical records provide crucial evidence of these cosmic events, particularly the famous supernova of 1054 AD, which was observed by astronomers across China, Japan, Arabia, and Europe. This event was so luminous that it could be seen during the day for two years and allowed people to read by its light. Modern technology has allowed us to pinpoint the exact location of this ancient explosion in the sky, revealing a supernova remnant visible even through telescopes like Hubble. The speaker notes that such events are rare within our own galaxy, occurring roughly once every century, which is why the last one observed without aid was in 1604, and the most recent close one, Supernova 1987A, occurred in a neighboring satellite galaxy called the Large Magellanic Cloud rather than directly in our Milky Way.
For those interested in witnessing a supernova firsthand within our own galaxy, the video explains that we would receive an early warning system through neutrinos. These fundamental particles are produced in vast quantities during the core collapse of a star and can escape the exploding star hours before the visible light reaches Earth, as light must travel through the dense outer layers of the dying star. While gravitational waves have not yet been detected from supernovae, neutrino detectors around the world could theoretically alert observers to look up at the night sky for a new "guest star" appearing in hundreds of years. The speaker reassures viewers that there is no danger to Earth from such an explosion, as any supernova close enough to disrupt our atmosphere would need to be within a few hundred light-years, and current observations show no nearby stars are about to explode.
Read the full video transcript
[Applause]
[Music]
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Mars
in the winter I really like it because
we have a riot or riot very cool
constellation input I think he actually
looks like something unlike some other
constellations so first here we have
Orion's belt some of you guys might
notice the three bright stars here make
up a running belt part of the entire
constellation Orion is the constellation
here and Betelgeuse is bright star star
up here
Betelgeuse is very bright red star makes
up the left shoulder of Orion Rigel is
the star down here another bright star
in Orion and cool thing also about Orion
is if you follow the belt down you get
to the star Sirius that's the brightest
star in the night sky
Orion's also cool is near Logan here at
Betelgeuse this sort of reddish star the
left shoulder star in Orion that is a
star that genres think is at the end of
its life and is going to go supernova
someday so females remember about stars
and just as we see them in the night sky
doesn't mean they're all there you know
some are closer some are further they're
all vastly different sizes so if we're
looking at the stars that I was just
showing you in the night sky so here's
our Sun it is a very tiny star compared
to stars like Siri
okay definitely bigger Rigel is huge
Betelgeuse is the biggest of all the
reason this happens is if your star like
our Sun when you reach the end of your
life some 99% of stars you kind of swell
up and you poof out your outer layers
and then that is the end of your stellar
story if you are a star however big like
Betelgeuse what is going to happen if
you are going to swell up you're going
to be huge
absolutely giant and what is going to
happen though at the end of your stellar
like when you finally run out of fuel at
the center of your core as you are going
to end up in a supernova explosion
so what a supernova explosion happens
the stars basically run out of fuel at
the center of its core and basically the
outer layers come down a neutron star or
black hole is born in the center and we
have basically an explosion that is the
biggest explosion we really know of in
astronomy one supernova can be brighter
than the light of the rest of the galaxy
when you see a supernova occurs so these
things you could see them from even
billions of light-years away
particularly bright one nobody is we
actually know about them pretty well
okay so supernova the reason we know
about supernova is what they would
actually look like for us is we've
actually seen them we have them in the
historic record chinese astronomers in
particular we're very good about
recording the guest stars in the sky
that they saw so stars that suddenly
showed up that were suddenly bright and
you know see so of a 1054 ad is
particularly famous one and the reason
is it was a supernova the Chinese the
Japanese the Arabic astronomers
definitely saw it
we also think the European and
astronomers in Chaco Canyon so people
all around the world saw this object the
reason was it was so bright you could
read by the light of the star it was so
bright it was in the sky for two years
at the guest star and no idea of course
what was causing it but it turns out
because the chinese astronomers very
good at recording where these guest
stars are we can go today and see where
is that what exactly is in that location
No
so this is what you see at the point how
about I just tell you next slide this is
what you see that if you go at the
Hubble telescope to see this something
that's on the track every one so our
next slide please
so think about supernovae I know is
unless at 10:54 II we don't actually see
them that often and the reason is
because I said only one person of these
stars goes supernova so we end up having
effectively one supernova in a galaxy
our size from century so when that
happens the last time we saw one in our
own galaxy 1604 Galileo saw it he didn't
have his telescope yet so he couldn't
pointed but 1604 I just told you want
every century well we have a lot of dust
in our galaxy a lot of probably a few
supernovae have happened but we just
have not seen them because it doesn't we
doesn't it
so the closest supernova to us since the
invention of the telescope is this
object here called supernova 1987a and
the reason I like supernova 1987a is
it's actually one of the things I talked
about in my PhD thesis first whatever
you do my research on and it's also one
that tells you like when I tell you what
I love the information first it happened
not in our own galaxy it happened in a
galaxy it called the Large Magellanic
Cloud which is a satellite to auro it's
basically 170,000 light-years away but
you can look out at the Galactic plane
so that's why you can actually see a lot
of cool things happen seeing the Large
Magellanic Cloud and you could even
though it's so far away and you're in
the southern hemisphere really see it
for a few weeks with your naked eyes
so what I do if this a little bit fear
works yes so I basically study this
supernova when the shockwave happen the
shockwave goes out and interacts with
all the material that is surrounding
this region of 1987 day that the start
affected before it died so if you want
to know what happens in supernova it's a
bit more circular but normally but you
can basically see that some region light
up and you can see supernovae they
really also interact with the
surrounding galaxies around these
systems a lot of star formation gets
triggered as the supernova shockwaves go
out and then you get you know and this
stuff showing you that picture the
supernova this is all radio data by the
way oh this is very strong so to start
wrap up folks are like what would happen
it was supernova though happened closer
than the Large Magellanic Cloud you know
like let's get rid of this for a second
so first of all the first thing to
emphasize is
staying off them people worry about
whatever you talk about Johnny explosion
and we're not going to die if a
supernova happens in our galaxy why do I
say this so if the supernova is going to
disrupt their atmosphere and things like
that it has to be with it a few hundred
light years of the mania thousand like
your maximum these stars I mean
Betelgeuse that was a huge star you know
you can see that from very far away
we're pretty sure we know about the
immediate area around us and we don't
see any stars that are about to go to
explode that are going to really hurt us
so that's cool so next slide please
the next strike though is so okay what
kind of alert will we get it for these
supernovae some of you guys like save
nothing those questions we miss being up
late that's not a case of supernovae
there's a little technicality here
particles in the universe called
neutrinos and neutrinos are fundamental
particles or like electrons are in all
their other favorite friends like that
but they're a little different cuz
there's just a bunch of them so this is
an interactive astronomy on time
everybody give me a thumbs up hey okay
so when you do your homes up every
single second
about a billion neutrinos go into the
tip of your thumb so these are particles
they are just very weakly interacting
they don't really
interact with anything but when a
supernova happens and the neutron star
is created in the center of the
supernova basically enough neutrinos
come out it's about the number of atoms
there are in the Sun and what happened
for 1987 is detectors like this this is
a neutrino detector just for comparison
next slide please
sort of if you look that that's two
people in a pope for comparison and what
this neutrino detectors like in size and
the first time we ever detected
neutrinos from outside of our own galaxy
was expert from our own solar system
forgive me was actually during 1987a I
told you all these neutrinos get created
and they saw them like 20 and 3
observatories around the world it was
the coolest thing that ever happened so
but the trick is also you get the
neutrinos arrive a few hours before the
light because I just told you they don't
interact with anything the light has to
travel through the layers of the star
when the core of the star collapses so
you actually get the alert from you the
neutrinos treat several hours before the
actual supernova Venice scene you can
actually by the way go online online
there's a supernova supernova alert
Network neutrinos Network that you can
sign up for alerts it's because suddenly
all the neutrino detectors around the
world go up you can sign up to say ok
like I want to see what's gonna happen
and you know you just got what we all
received the alert tonight we're gonna
run outside we're going to
see this view here and so what's gonna
happen you're gonna stand there maybe
you're going to be the first person you
know over 400 years to see light from
the supernova in our own galaxy and
you're gonna wait wait love astronomy is
waiting and then look there we are and
then that is what it will be like
suddenly we'll have a guest star first
time in hundreds of years in our a night
sky
[Applause]
so the question was you all star
supernova No so all only 1% of stars are
massive enough to go supernova you have
to be roughly 8 times the mass of our
own Sun to go supernova so in the case
of supernova 1987a basically because
there was the supernova event and they
knew from theory that that's what caused
it and they literally never detected you
to turn support that was the main reason
for it but as I said it was also the
fact that was the
so the question was where is the picture
of the neutrino lab that was actually in
Japan so the deputies are very good at
neutrino astronomy did you use the
various neutrino detectors this kind of
triangulation as a big telescope to
point you at the supernovae so the
question was being used in neutrino
detectors at the telescope so the answer
is people can now like I mean of the
field said 30 years or so to evolve and
the field is now at the point where yes
you can they have actually within the
past and associate in the 19 you know
that would have it
the question was that's a good question
how do you evaluate data from a thousand
ad I think the fact that if you go and
then you see the supernova remnant there
is very telling and also the fact that
all of these records have been up there
in the same period of time
archeoastronomy is so supernova remnants
is literally just the remnants of the
star and the gas and everything
surrounding sorry so supernova remnants
on another clone field of astronomy and
yes okay so the question was good
question have we detected gravitational
waves from supernovae the answer is no
but my understanding is when the
supernova goes off in our own galaxy
like as would be expected I did actually
ask at one point for whatever basic
gravitational wave detectors there were
in 1987 quite stupid detected or not
apparently there is a
[Music]
[Applause]
so that was a good question or what is
better another star
that might go supernova other than
Betelgeuse actually the best candidate
in my opinion at the star called eater
Carina but it's in the southern
hemisphere so the talk is not as good
[Laughter]
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