How to detect a supernova - Samantha Kuula
-
0:08 - 0:12Just now, somewhere in the universe,
a star exploded. -
0:12 - 0:15There goes another one.
-
0:15 - 0:21In fact, a supernova occurs every second
or so in the observable universe, -
0:21 - 0:24and there is one on average
every 25 to 50 years -
0:24 - 0:28in a galaxy the size
and age of the Milky Way. -
0:28 - 0:31Yet we've never actually been able
to watch one happen -
0:31 - 0:35from its first violent moments.
-
0:35 - 0:37Of course, how would we?
-
0:37 - 0:40There are hundreds of billions
of stars close enough -
0:40 - 0:42that we could watch
the supernova explosion -
0:42 - 0:44break through the surface of the star.
-
0:44 - 0:48But we'd have to have our best telescopes
focused on the right one -
0:48 - 0:52at precisely the right time
to get meaningful data. -
0:52 - 0:57Suffice it to say, the odds of that
happening are astronomically low. -
0:57 - 1:02But what if we could anticipate
a supernova before its light reached us? -
1:02 - 1:04That may seem impossible.
-
1:04 - 1:08After all, nothing travels faster
than the speed of light, right? -
1:08 - 1:10As far as we know, yes.
-
1:10 - 1:14But in a race, fast doesn't matter
if you take a detour -
1:14 - 1:17while someone else beelines it
for the finish line. -
1:17 - 1:19For exactly that reason,
-
1:19 - 1:22photons don't win
the supernova race to Earth. -
1:22 - 1:25Neutrinos do.
-
1:25 - 1:27Here's why.
-
1:27 - 1:29There are two types of supernova.
-
1:29 - 1:34Type 1 is when a star accumulates
so much matter from a neighboring star, -
1:34 - 1:41that a runaway nuclear reaction ignites
and causes it to explode. -
1:41 - 1:45In type 2, the star runs out
of nuclear fuel, -
1:45 - 1:47so the gravitational forces pulling in
-
1:47 - 1:52overwhelm the quantum mechanical
forces pushing out, -
1:52 - 1:58and the stellar core collapses under
its own weight in a hundredth of a second. -
1:58 - 2:02While the outer reaches of the star
are unaffected by the collapsed core, -
2:02 - 2:04the inner edges accelerate
through the void, -
2:04 - 2:10smash into the core,
and rebound to launch the explosion. -
2:10 - 2:12In both of these scenarios,
-
2:12 - 2:16the star expels an unparalleled
amount of energy, -
2:16 - 2:19as well as a great deal of matter.
-
2:19 - 2:24In fact, all atoms heavier than nickel,
including elements like gold and silver, -
2:24 - 2:29only form in supernova reactions.
-
2:29 - 2:30In type 2 supernovae,
-
2:30 - 2:33about 1% of the energy
consists of photons, -
2:33 - 2:35which we know of as light,
-
2:35 - 2:40while 99% radiates out as neutrinos,
-
2:40 - 2:45the elementary particles that are known
for rarely interacting with anything. -
2:45 - 2:47Starting from the center of the star,
-
2:47 - 2:51the exploding matter takes
tens of minutes, or even hours, -
2:51 - 2:58or in rare cases, several days, to reach
and break through the surface of the star. -
2:58 - 3:02However, the neutrinos,
thanks to their non-interactivity, -
3:02 - 3:04take a much more direct route.
-
3:04 - 3:08By the time there is any visible change
in the star's suface, -
3:08 - 3:13the neutrinos typically have a several
hour head start over the photons. -
3:13 - 3:15That's why astronomers and physicists
-
3:15 - 3:19have been able to set up a project
called SNEWS, -
3:19 - 3:22the Supernova Early Warning System.
-
3:22 - 3:26When detectors around the world
pick up bursts of neutrinos, -
3:26 - 3:30they send messages
to a central computer in New York. -
3:30 - 3:33If multiple detectors receive
similar signals within ten seconds, -
3:33 - 3:38SNEWS will trigger an alert warning
that a supernova is imminent. -
3:38 - 3:42Aided by some distance and direction
information from the neutrino detectors, -
3:42 - 3:45the amateur astronomers
and scientists alike -
3:45 - 3:47will scan the skies and share information
-
3:47 - 3:51to quickly identify
the new galactic supernova -
3:51 - 3:55and turn the world's major
telescopes in that direction. -
3:55 - 4:01The last supernova that sent detectable
neutrinos to Earth was in 1987 -
4:01 - 4:03on the edge of the Tarantula Nebula
-
4:03 - 4:07in the large Magellanic Cloud,
a nearby galaxy. -
4:07 - 4:13Its neutrinos reached Earth about
three hours ahead of the visible light. -
4:13 - 4:16We're due for another one any day now,
and when that happens, -
4:16 - 4:21SNEWS should give you the opportunity
to be among the first to witness something -
4:21 - 4:25that no human has ever seen before.
- Title:
- How to detect a supernova - Samantha Kuula
- Description:
-
View full lesson: http://ed.ted.com/lessons/how-to-detect-a-supernova-samantha-kuula
Just now, somewhere in the universe, a star exploded. In fact, a supernova occurs every second or so in the observable universe. Yet, we’ve never actually been able to watch a supernova in its first violent moments. Is early detection possible? Samantha Kuula details the science behind an early supernova warning system.
Lesson by Samantha Kuula, animation by Nick Hilditch.
- Video Language:
- English
- Team:
- closed TED
- Project:
- TED-Ed
- Duration:
- 04:42
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