WEBVTT

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[MUSIC PLAYING]

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MIKE SHORT: Instead
of saying, analyze

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this theoretical problem, I
said, analyze your toenails.

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Tell me how much arsenic and
gold you've got in your body.

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All we study at MIT is the
natural world and things

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we make out of it, so everything
is reducible to practice.

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Everything can be real,
if you put in the effort.

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SARAH HANSEN: Today
on the podcast,

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we're talking about
ionizing radiation

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and nuclear engineering.

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How do you make these
things real and tangible?

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MIKE SHORT: Matter
is a form of energy.

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And once that
clicked, everything

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seemed to make
sense-- radioactive

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decay, nuclear reactions,
all these things.

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I remember that aha
moment in this class

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that I teach as a second-year
student back in 2002.

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And it's those kind
of moments that

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made me want to stay in it,
because I feel like, wow, I

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really know this field now.

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SARAH HANSEN: Welcome
to Chalk Radio,

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a podcast about inspired
teaching at MIT.

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I'm your host, Sarah Hansen
from MIT OpenCourseWare.

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The Nuclear Engineering and
Ionizing Radiation course

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at MIT take students from
understanding basic physics

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to grappling with the core
concepts of Einstein's E equals

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mc squared.

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In this episode,
we're going to delve

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into how this is
possible, and what

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it takes to make a class that's
not only hands-on, but also

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capable of evolving daily.

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My guest is one of the main
people that makes this happen,

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Professor Mike Short.

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MIKE SHORT: This course
is all about radiation,

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both its origins and its uses.

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So this is the first course on
its intro to everything nuclear

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that any student
at MIT would take.

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And a lot of times for students,
it's their first modern physics

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course.

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The physics courses that
first-year students take

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are often things that we've
known for 100 to 300 years.

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And the field of nuclear
physics is still evolving.

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We're still using
nuclear radiation spectra

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to detect the presence of
water on Mars or the moon.

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We're still confirming
our knowledge

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of which particles do
and don't exist and why.

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So this is also intro
to modern physics.

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SARAH HANSEN: So nuclear science
and radiation in particular

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are emotionally charged
topics, you know?

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You read on the internet claims
like, cell phones cause cancer,

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things like that.

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How are you preparing students
to debunk pseudoscience

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and to really serve the public?

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MIKE SHORT: We actually
spent two weeks

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at the end of the class
looking at studies

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that are false or have
exaggerated claims

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and teaching students
what to look for.

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So the first 11
weeks of the class,

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we teach the students
the fundamentals

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of nuclear science.

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And then we turn to published
articles, and blogs,

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and other things in the field.

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And we debunk myths
like cell phones

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cause cancer due to
ionizing radiation.

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Cell phones don't emit
ionizing radiation.

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We debunk myths like,
the tiniest little bit

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of irradiation can harm
you, when in truth, we

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don't have the data for that.

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But a lot of misinformation in
radiation and nuclear science

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is incorporated into
culture, into our sort

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of collective
consciousness, and even

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in what's called the linear no
threshold model, which says,

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every little bit of
radiation does harm.

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We don't know that
to be true or false,

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and it's a good thing we don't.

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Because we would need to
have exposed tens of millions

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of people to low
levels of radiation

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in a controlled study,
which is not something

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I think is ethically
correct to do.

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It's also not ethically
correct to say

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that all radiation causes
harm, because we don't know.

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And I want students to both
recognize false science

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in the field, and
recognize when we

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don't know enough information
to say something confidently,

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and be comfortable with
that lack of knowledge.

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It means there's
something new to explore.

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But if you don't have
something to conclude,

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don't draw a conclusion.

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SARAH HANSEN: Uh-huh.

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How does this connect
to the irradiated fruit

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party that have in the class?

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What is that?

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MIKE SHORT: Yeah.

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The last day of class, we often
have an irradiated fruit party,

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where I bring in
fruit that could only

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be brought into the US
because it's irradiated.

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So there are many
fruits that are--

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there many different
types of produce,

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including fruits,
that are irradiated,

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and it's the only known way to
kill all of the insect, viral,

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and bacterial pathogens that
can wreak havoc on either people

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or on our crops.

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An interesting point
of information, Hawaii

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and Puerto Rico, despite
being part of the US,

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are agriculturally
distinct areas,

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and you are not
allowed to simply

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import produce from those.

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I had an apple confiscated
from the airport in Puerto Rico

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when I learned that
to be the case.

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However, if you
irradiate foods, like,

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this is why we can get a lot
of pineapples from Costa Rica.

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We've started
getting mangosteens

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in from Thailand, where I
didn't know what that fruit was

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until a few years
ago and now, you

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can find them at H
Mart in Cambridge.

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A lot of this is because
we can kill the pests,

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and it doesn't harm the food.

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It doesn't make the
food radioactive.

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But a lot of this is to
personalize the science.

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So when students eat
food that they may or may

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not known have been
irradiated, they taste good.

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They seem safe.

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And it's one of those things
where once it's personalized,

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it's not as scary.

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When you learn the knowledge and
then you see it for yourselves,

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it becomes a lot
more acceptable.

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SARAH HANSEN: Yeah,
learning through experience

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is very powerful.

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What does it mean
to you for students

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to develop fluency
in this field?

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MIKE SHORT: It's important
to be fluent in this field

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because a cursory knowledge
of radiation science

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is not enough.

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I'd say there are a lot of
self-proclaimed experts--

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I call them armchair PhDs--

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who have learned a bit of
genuine knowledge, but then

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extrapolate it too far.

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And that combined
with all the things

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we've heard in pop
culture, unfortunately

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sometimes from celebrities
spouting falsehoods

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about radiation, or
vaccines, or other things

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that they don't understand,
people listen to other people,

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and people listen to role models
and folks that they look up to.

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But it's important to be
fluent and well-grounded

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in the fundamentals so that you
can sort out fact from fiction.

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And I want every student
that leaves my class

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to be able to recognize
something that's incorrect,

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even if it's told to them by a
celebrity, an expert, a parent,

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a friend, anyone--

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that they know what the reality
is, and it shouldn't depend

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on the source it comes from.

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They should be able to tell
whether it's real or not

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and verify if the
source is genuine.

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SARAH HANSEN: Uh-huh.

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And how do you help students
develop this fluency?

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MIKE SHORT: So it starts
off with the fundamentals

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of radiation science.

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So like any class, we
teach all the fundamentals

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from well-established theory.

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But along the way every week, we
have labs and personalisation.

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Like, for example, the
first day of class,

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I ask students to bring in
their toenail clippings.

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[MUSIC PLAYING]

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And they usually say,
that's disgusting.

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What are we doing?

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And I say, you'll see.

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We're going to put
them in the reactor.

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And we irradiate their
toenail clippings.

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And because to some degree,
you are what you eat,

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some of the elements which
we eat and we don't want to,

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things like arsenic,
or selenium,

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or chromium, some of which
can be good in small amounts,

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bad in large amounts--

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others like arsenic,
I'm not sure

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if there's a good use of it--

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get incorporated
into our toenails.

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So we activate those toenails
by putting them in the reactor.

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They absorb neutrons and give
off characteristic gamma rays,

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giving away how many
atoms of arsenic,

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and selenium, and such are
incorporated into the toenails

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with striking precision.

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And so we're able to tell
where students come from based

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on analysis of their toenails.

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We had one student who had a
lot of gold in their toenails.

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And I said, I thought I asked
you guys to clean these off,

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remove any polish.

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And the student
said, yeah, I did.

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But I live near a gold mining
town, and it's in the water.

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SARAH HANSEN: Wow,
that's so interesting.

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MIKE SHORT: So that's
what I mean by personal,

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is they discover
things about themselves

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through nuclear science.

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In the problem sense,
instead of saying,

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analyze this theoretical
problem, I said,

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analyze your toenails.

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Tell me how much arsenic and
gold you've got in your body.

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SARAH HANSEN: Right, right.

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So in the course,
you make a point

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of saying that the
method of instruction

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is often context first, theory
second, and then context again.

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How does that relate to
that method of instruction?

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MIKE SHORT: This is an example
of that method of instruction.

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I like to start by
opening knowledge gaps

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rather than spouting
theory that someone.

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It doesn't usually stick if I
just say, here are some facts.

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Learn them.

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That's usually in one
ear, out the other,

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if they're listening at all.

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But when you show someone
something surprising,

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they're fully engaged.

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They're always
multi-sensory engaged.

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They're listening.

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In a lot of cases, they're
touching, in some cases,

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even smelling.

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Taste is the sense
that we don't tend

00:08:37.010 --> 00:08:39.620 align:middle line:84%
to engage in nuclear
science, with good reason.

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[CHUCKLES]

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But you can sense, and
feel, and hear a lot

00:08:43.610 --> 00:08:44.960 align:middle line:90%
of things in nuclear science.

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Like yesterday, I was with
one of my graduate students.

00:08:49.400 --> 00:08:52.160 align:middle line:84%
We were looking at some
highly irradiated materials

00:08:52.160 --> 00:08:55.010 align:middle line:84%
for a reactor in Idaho, and
we heard this little faint

00:08:55.010 --> 00:08:57.630 align:middle line:84%
buzzing noise in
the Geiger counter.

00:08:57.630 --> 00:08:59.630 align:middle line:84%
And if you put your ear
up to the Geiger counter

00:08:59.630 --> 00:09:01.400 align:middle line:84%
near the radiation
source, you can hear

00:09:01.400 --> 00:09:02.900 align:middle line:90%
tiny electrical discharges.

00:09:02.900 --> 00:09:04.940 align:middle line:84%
You can hear the
detector working.

00:09:04.940 --> 00:09:08.210 align:middle line:84%
And then I want the student
to say, why is that?

00:09:08.210 --> 00:09:10.820 align:middle line:84%
Why do I hear this fuzzy
noise near the detector

00:09:10.820 --> 00:09:11.990 align:middle line:90%
when it's working?

00:09:11.990 --> 00:09:15.380 align:middle line:84%
Then when you explain why,
students tend to remember.

00:09:15.380 --> 00:09:17.870 align:middle line:84%
Not too many people learn
well by being lectured at,

00:09:17.870 --> 00:09:20.660 align:middle line:84%
but everyone learns well
by opening knowledge gaps.

00:09:20.660 --> 00:09:24.890 align:middle line:84%
And you're effectively pulling
the information in rather

00:09:24.890 --> 00:09:26.815 align:middle line:84%
than us pushing it
to the students.

00:09:26.815 --> 00:09:28.190 align:middle line:84%
Something I learned
from a mentor

00:09:28.190 --> 00:09:30.400 align:middle line:90%
here is you can't push a string.

00:09:30.400 --> 00:09:32.150 align:middle line:84%
You want knowledge
into a student's brain,

00:09:32.150 --> 00:09:33.108 align:middle line:90%
they've got to pull it.

00:09:33.108 --> 00:09:35.126 align:middle line:90%
You can't push it.

00:09:35.126 --> 00:09:38.560 align:middle line:84%
SARAH HANSEN: You made a choice
in this iteration of the course

00:09:38.560 --> 00:09:43.070 align:middle line:84%
to offer students the ability
to do analytical homework

00:09:43.070 --> 00:09:45.650 align:middle line:90%
or take-home, hands-on labs.

00:09:45.650 --> 00:09:46.598 align:middle line:90%
How did that work out?

00:09:46.598 --> 00:09:48.140 align:middle line:84%
What does that look
like in practice?

00:09:48.140 --> 00:09:50.390 align:middle line:84%
MIKE SHORT: Interestingly,
I spent all this time

00:09:50.390 --> 00:09:52.460 align:middle line:90%
making these optional labs.

00:09:52.460 --> 00:09:54.330 align:middle line:90%
Nobody did them.

00:09:54.330 --> 00:09:56.270 align:middle line:84%
So the next couple
of years, I simply

00:09:56.270 --> 00:09:58.130 align:middle line:90%
made everything mandatory.

00:09:58.130 --> 00:10:00.067 align:middle line:84%
The students said they
loved the flexibility.

00:10:00.067 --> 00:10:02.150 align:middle line:84%
They're really psyched
that I put in all this time

00:10:02.150 --> 00:10:03.500 align:middle line:90%
to do the labs.

00:10:03.500 --> 00:10:05.550 align:middle line:84%
But it wasn't for a grade,
so they didn't do it.

00:10:05.550 --> 00:10:06.350 align:middle line:90%
And so that's when I learned.

00:10:06.350 --> 00:10:08.450 align:middle line:84%
If it's not graded, it's
not going to get done.

00:10:08.450 --> 00:10:10.250 align:middle line:84%
So I made all the
labs mandatory.

00:10:10.250 --> 00:10:12.320 align:middle line:84%
I cut out a little
bit of the analytics

00:10:12.320 --> 00:10:15.740 align:middle line:84%
in favor of adding context
before and after the theory,

00:10:15.740 --> 00:10:17.720 align:middle line:90%
and retention went up.

00:10:17.720 --> 00:10:19.550 align:middle line:90%
Grades went up, on average.

00:10:19.550 --> 00:10:21.680 align:middle line:84%
And the course
evaluations went up, too.

00:10:21.680 --> 00:10:24.520 align:middle line:84%
So anything numerical
we can get improved--

00:10:24.520 --> 00:10:26.740 align:middle line:84%
and in my subjective
opinion, so did

00:10:26.740 --> 00:10:29.750 align:middle line:84%
the students' knowledge
of what's happening.

00:10:29.750 --> 00:10:31.270 align:middle line:84%
And that, I get
from my colleagues,

00:10:31.270 --> 00:10:34.690 align:middle line:84%
because I track these students
as they progress through MIT,

00:10:34.690 --> 00:10:35.950 align:middle line:90%
through our department.

00:10:35.950 --> 00:10:38.590 align:middle line:84%
And my colleagues who
teach further-on courses,

00:10:38.590 --> 00:10:40.810 align:middle line:84%
the more advanced ones,
can tell me whether or not

00:10:40.810 --> 00:10:42.518 align:middle line:84%
the students really
know the fundamentals

00:10:42.518 --> 00:10:43.750 align:middle line:90%
that they're depending on.

00:10:43.750 --> 00:10:45.417 align:middle line:84%
So far, things have
been getting better,

00:10:45.417 --> 00:10:47.135 align:middle line:90%
but it requires planning.

00:10:47.135 --> 00:10:48.760 align:middle line:84%
And it also requires
a lot of thinking,

00:10:48.760 --> 00:10:50.620 align:middle line:84%
where I'll look
through my syllabus,

00:10:50.620 --> 00:10:53.613 align:middle line:84%
and I have an empty column
where the user doesn't

00:10:53.613 --> 00:10:55.780 align:middle line:84%
exist in most syllabi, which
is, what is this week's

00:10:55.780 --> 00:10:56.980 align:middle line:90%
hands-on instruction?

00:10:56.980 --> 00:10:58.780 align:middle line:84%
And I try to make
sure that's full.

00:10:58.780 --> 00:11:01.580 align:middle line:84%
So another example is
if you want to know,

00:11:01.580 --> 00:11:03.580 align:middle line:90%
do you have real diamond rings?

00:11:03.580 --> 00:11:05.860 align:middle line:84%
When we get to reading
electron spectra

00:11:05.860 --> 00:11:07.702 align:middle line:84%
and characteristic
X-ray spectra,

00:11:07.702 --> 00:11:09.910 align:middle line:84%
I could either give them a
problem from theory, which

00:11:09.910 --> 00:11:12.970 align:middle line:84%
is boring, or I can run
some standard for them,

00:11:12.970 --> 00:11:14.650 align:middle line:90%
where they know what to expect.

00:11:14.650 --> 00:11:16.630 align:middle line:84%
Or I can say, that's
a nice diamond ring.

00:11:16.630 --> 00:11:18.680 align:middle line:84%
Do you want to
know if it's real?

00:11:18.680 --> 00:11:20.797 align:middle line:84%
And the student invariably
says, absolutely, I

00:11:20.797 --> 00:11:21.880 align:middle line:90%
want to know if it's real.

00:11:21.880 --> 00:11:22.660 align:middle line:90%
SARAH HANSEN: Right.

00:11:22.660 --> 00:11:24.077 align:middle line:84%
MIKE SHORT: So we
have the student

00:11:24.077 --> 00:11:26.320 align:middle line:84%
take the controls of
the electron microscope

00:11:26.320 --> 00:11:30.770 align:middle line:84%
and analyze it to see, does that
diamond emit zirconium x-rays?

00:11:30.770 --> 00:11:33.160 align:middle line:84%
Because if it does,
it's cubic zirconia.

00:11:33.160 --> 00:11:36.580 align:middle line:84%
If it emits silicon x-rays, it's
moissanite or silicon carbide.

00:11:36.580 --> 00:11:39.340 align:middle line:84%
My favorite one was
this day happened

00:11:39.340 --> 00:11:40.750 align:middle line:90%
to fall on parents' weekend.

00:11:40.750 --> 00:11:43.180 align:middle line:84%
So I asked the students, does
anybody have a diamond ring?

00:11:43.180 --> 00:11:45.180 align:middle line:84%
And one of the students'
mothers said, oh, yeah.

00:11:45.180 --> 00:11:46.930 align:middle line:90%
Let's check my engagement ring.

00:11:46.930 --> 00:11:49.302 align:middle line:84%
And her husband
was just, oh, gosh.

00:11:49.302 --> 00:11:50.260 align:middle line:90%
What's going to happen?

00:11:50.260 --> 00:11:51.218 align:middle line:90%
What's going to happen?

00:11:51.218 --> 00:11:52.765 align:middle line:84%
He thinks he bought
a genuine ring.

00:11:52.765 --> 00:11:53.902 align:middle line:90%
It turned out to be real.

00:11:53.902 --> 00:11:54.610 align:middle line:90%
We had the proof.

00:11:54.610 --> 00:11:55.860 align:middle line:90%
SARAH HANSEN: OK, that's good.

00:11:55.860 --> 00:11:57.385 align:middle line:90%
[MUSIC PLAYING]

00:11:57.385 --> 00:11:58.255 align:middle line:90%


00:11:58.255 --> 00:12:02.380 align:middle line:84%
Mike, can you tell us about
the radioactive scavenger hunt?

00:12:02.380 --> 00:12:03.700 align:middle line:90%
MIKE SHORT: Sure.

00:12:03.700 --> 00:12:06.370 align:middle line:84%
I challenge the students to
find the most radioactive place

00:12:06.370 --> 00:12:07.590 align:middle line:90%
in Boston.

00:12:07.590 --> 00:12:09.688 align:middle line:84%
And each of them had
to go in teams of two

00:12:09.688 --> 00:12:11.980 align:middle line:84%
and pick a place that they
thought would be radioactive

00:12:11.980 --> 00:12:15.370 align:middle line:84%
based on what we'd learned
about where you find radiation.

00:12:15.370 --> 00:12:18.610 align:middle line:84%
So radiation, a lot of
it comes from space,

00:12:18.610 --> 00:12:21.100 align:middle line:84%
from cosmic protons
that hit the atmosphere.

00:12:21.100 --> 00:12:23.810 align:middle line:84%
So some students thought, I'll
go to the tallest building,

00:12:23.810 --> 00:12:25.810 align:middle line:84%
and I'll probably
get more radiation.

00:12:25.810 --> 00:12:28.060 align:middle line:84%
Others had read about
radon underground,

00:12:28.060 --> 00:12:31.905 align:middle line:84%
because there are isotopes
of radium emitting radon gas.

00:12:31.905 --> 00:12:34.030 align:middle line:84%
And so they thought, we'll
go down into the subway,

00:12:34.030 --> 00:12:35.620 align:middle line:90%
get as low as we can go.

00:12:35.620 --> 00:12:38.320 align:middle line:84%
Other students looked at the
relative amount of radiation

00:12:38.320 --> 00:12:41.800 align:middle line:84%
in different building materials,
like wood, clay, marble,

00:12:41.800 --> 00:12:45.970 align:middle line:84%
granite, and they went to the
most granite-dense locations

00:12:45.970 --> 00:12:48.610 align:middle line:84%
they could find, or the
ones with the most marble.

00:12:48.610 --> 00:12:50.488 align:middle line:84%
And those are the
students that won.

00:12:50.488 --> 00:12:52.030 align:middle line:84%
There were places
in Boston that have

00:12:52.030 --> 00:12:55.252 align:middle line:84%
six times the normal
radiation background,

00:12:55.252 --> 00:12:57.460 align:middle line:84%
simply because they're made
out of marble or granite.

00:12:57.460 --> 00:12:59.168 align:middle line:84%
These include things
like the state house

00:12:59.168 --> 00:13:01.150 align:middle line:84%
and some fancy
fountains around town.

00:13:01.150 --> 00:13:02.660 align:middle line:84%
Did not know about
the fountains,

00:13:02.660 --> 00:13:05.650 align:middle line:84%
but they just thought, let's
find giant chunks of stone,

00:13:05.650 --> 00:13:06.670 align:middle line:90%
and they were right.

00:13:06.670 --> 00:13:11.440 align:middle line:90%


00:13:11.440 --> 00:13:13.420 align:middle line:84%
SARAH HANSEN: The
hands-on experiences

00:13:13.420 --> 00:13:15.880 align:middle line:84%
that Mike creates for
students of his course

00:13:15.880 --> 00:13:17.770 align:middle line:90%
are pretty unique.

00:13:17.770 --> 00:13:19.810 align:middle line:84%
He told me that when
he took this course

00:13:19.810 --> 00:13:22.300 align:middle line:84%
as an undergraduate
student at MIT,

00:13:22.300 --> 00:13:24.730 align:middle line:90%
it wasn't typically hands-on.

00:13:24.730 --> 00:13:26.830 align:middle line:84%
So I wanted to know
what it's like to teach

00:13:26.830 --> 00:13:29.410 align:middle line:84%
in a way that's so different
from his own personal

00:13:29.410 --> 00:13:30.650 align:middle line:90%
experience.

00:13:30.650 --> 00:13:34.300 align:middle line:84%
What does it take to create such
fascinating labs and lessons

00:13:34.300 --> 00:13:37.750 align:middle line:84%
without a clear model from one's
own educational background?

00:13:37.750 --> 00:13:39.280 align:middle line:90%
MIKE SHORT: It's natural.

00:13:39.280 --> 00:13:42.280 align:middle line:84%
I teach the way that I
learn, because I thought back

00:13:42.280 --> 00:13:45.100 align:middle line:84%
on all my experiences and I
thought, from which courses

00:13:45.100 --> 00:13:47.860 align:middle line:90%
did I really remember a lot?

00:13:47.860 --> 00:13:50.290 align:middle line:84%
And these were things like
hands-on blacksmithing

00:13:50.290 --> 00:13:52.540 align:middle line:90%
or laboratory courses.

00:13:52.540 --> 00:13:55.210 align:middle line:84%
We did have a lab class where
we counted a lot of radiation,

00:13:55.210 --> 00:13:57.470 align:middle line:84%
and I remember those
labs very well.

00:13:57.470 --> 00:14:00.920 align:middle line:84%
And I think back to my
neutronics problem sets.

00:14:00.920 --> 00:14:02.890 align:middle line:84%
I remember the theory
OK, but I don't

00:14:02.890 --> 00:14:06.280 align:middle line:84%
remember very many visual
instances of that class.

00:14:06.280 --> 00:14:07.610 align:middle line:90%
It just kind of happened.

00:14:07.610 --> 00:14:09.360 align:middle line:84%
The knowledge is maybe
in there somewhere.

00:14:09.360 --> 00:14:09.970 align:middle line:90%
I don't know.

00:14:09.970 --> 00:14:11.650 align:middle line:84%
But I know where
I was when I did

00:14:11.650 --> 00:14:13.670 align:middle line:90%
most of the hands-on exercises.

00:14:13.670 --> 00:14:16.570 align:middle line:84%
And in the end, you can
make anything hands-on, even

00:14:16.570 --> 00:14:18.620 align:middle line:90%
neutronics that I mentioned.

00:14:18.620 --> 00:14:21.310 align:middle line:84%
So I at some point
went skulking around

00:14:21.310 --> 00:14:23.710 align:middle line:84%
places I oughtn't, like
around in the reactor

00:14:23.710 --> 00:14:28.060 align:middle line:84%
once I got access, and found
an eight-foot pile of graphite

00:14:28.060 --> 00:14:29.840 align:middle line:84%
that was behind a
bunch of equipment.

00:14:29.840 --> 00:14:30.610 align:middle line:90%
It wasn't hidden.

00:14:30.610 --> 00:14:32.598 align:middle line:90%
It was just covered with junk.

00:14:32.598 --> 00:14:33.640 align:middle line:90%
And I asked, what's that?

00:14:33.640 --> 00:14:35.950 align:middle line:84%
They just said, oh, that's our
subcritical graphite reactor

00:14:35.950 --> 00:14:36.460 align:middle line:90%
pile.

00:14:36.460 --> 00:14:38.290 align:middle line:84%
We're going to get
rid of that next year.

00:14:38.290 --> 00:14:41.260 align:middle line:84%
So I sounded the alarm and
said, you cannot get rid of this

00:14:41.260 --> 00:14:42.460 align:middle line:90%
graphite pile.

00:14:42.460 --> 00:14:44.710 align:middle line:84%
And then our neutronics
professors Ben Forget and Kord

00:14:44.710 --> 00:14:45.580 align:middle line:90%
Smith said, yeah, you're right.

00:14:45.580 --> 00:14:46.330 align:middle line:90%
We can't.

00:14:46.330 --> 00:14:48.787 align:middle line:84%
So they spent a whole
winter restoring it

00:14:48.787 --> 00:14:49.870 align:middle line:90%
with a couple of students.

00:14:49.870 --> 00:14:52.000 align:middle line:84%
And now, it's one of the
central labs in my class

00:14:52.000 --> 00:14:53.330 align:middle line:90%
and in their class.

00:14:53.330 --> 00:14:55.690 align:middle line:84%
So we've taken the most
theory-heavy, dry, and boring

00:14:55.690 --> 00:14:58.390 align:middle line:84%
class and turned it
experimental because you can.

00:14:58.390 --> 00:15:01.000 align:middle line:84%
You're always studying
the natural world, right?

00:15:01.000 --> 00:15:03.940 align:middle line:84%
All we study at MIT is the
natural world and things

00:15:03.940 --> 00:15:07.210 align:middle line:84%
we make out of it, so everything
is reducible to practice.

00:15:07.210 --> 00:15:11.686 align:middle line:84%
Everything can be real,
if you put in the effort.

00:15:11.686 --> 00:15:14.470 align:middle line:84%
SARAH HANSEN: Part of what's
so special about this class is

00:15:14.470 --> 00:15:16.450 align:middle line:84%
the dedication that
Mike and his colleagues

00:15:16.450 --> 00:15:19.300 align:middle line:84%
have to constantly improving
it through real-time student

00:15:19.300 --> 00:15:20.360 align:middle line:90%
feedback.

00:15:20.360 --> 00:15:22.480 align:middle line:84%
And I don't mean fixing
pieces to implement

00:15:22.480 --> 00:15:23.950 align:middle line:90%
for the next semester.

00:15:23.950 --> 00:15:26.080 align:middle line:84%
I'm talking about
next-day transformations

00:15:26.080 --> 00:15:27.760 align:middle line:90%
of class procedures.

00:15:27.760 --> 00:15:32.555 align:middle line:84%
To accomplish this, Mike created
the aptly titled Rants Page.

00:15:32.555 --> 00:15:35.800 align:middle line:84%
MIKE SHORT: The Rant Page is an
anonymous, simple, PHP comment

00:15:35.800 --> 00:15:39.220 align:middle line:84%
form that I wrote, where I
want students to tell me things

00:15:39.220 --> 00:15:41.140 align:middle line:90%
that they want changed.

00:15:41.140 --> 00:15:44.950 align:middle line:84%
Because I try my best to
collect in-person feedback

00:15:44.950 --> 00:15:47.993 align:middle line:84%
from the students both
one-on-one and in class.

00:15:47.993 --> 00:15:49.660 align:middle line:84%
But some students
don't feel comfortable

00:15:49.660 --> 00:15:52.400 align:middle line:84%
telling a professor, I don't
like what you're doing.

00:15:52.400 --> 00:15:55.660 align:middle line:84%
So I give them a place to do
so completely anonymously.

00:15:55.660 --> 00:15:57.520 align:middle line:84%
It ended up being
20 lines of code.

00:15:57.520 --> 00:15:58.850 align:middle line:90%
It wasn't hard.

00:15:58.850 --> 00:16:02.440 align:middle line:84%
And what I started getting
was real-time feedback about,

00:16:02.440 --> 00:16:03.880 align:middle line:90%
I can't read your writing.

00:16:03.880 --> 00:16:06.130 align:middle line:90%
So then I know to slow it down.

00:16:06.130 --> 00:16:08.860 align:middle line:84%
Or, I really wish you
wouldn't slow the class down

00:16:08.860 --> 00:16:11.380 align:middle line:84%
for this one student's
incessant questions,

00:16:11.380 --> 00:16:13.690 align:middle line:84%
so I know to limit each
student to a few questions

00:16:13.690 --> 00:16:15.580 align:middle line:90%
if it gets to be too much.

00:16:15.580 --> 00:16:17.110 align:middle line:84%
And I would address
them in class

00:16:17.110 --> 00:16:19.630 align:middle line:84%
to say, it's safe to address
this, because it's anonymous.

00:16:19.630 --> 00:16:21.710 align:middle line:84%
I have literally
no way of knowing.

00:16:21.710 --> 00:16:24.010 align:middle line:84%
But if one person wrote
it, probably a lot of you

00:16:24.010 --> 00:16:25.300 align:middle line:90%
are thinking it.

00:16:25.300 --> 00:16:27.190 align:middle line:84%
And the students responded
positively to say,

00:16:27.190 --> 00:16:28.898 align:middle line:84%
wow, it was really
nice to know that we'd

00:16:28.898 --> 00:16:30.947 align:middle line:84%
make a suggestion at
2:00 in the morning,

00:16:30.947 --> 00:16:33.280 align:middle line:84%
and then by 10:00 in the
morning, it would be addressed.

00:16:33.280 --> 00:16:34.570 align:middle line:84%
The class would
change in real time,

00:16:34.570 --> 00:16:37.240 align:middle line:84%
and they knew they had the power
to shape their own learning.

00:16:37.240 --> 00:16:40.060 align:middle line:90%
[MUSIC PLAYING]

00:16:40.060 --> 00:16:43.350 align:middle line:90%


00:16:43.350 --> 00:16:45.490 align:middle line:84%
SARAH HANSEN: With all the
buzz around this course,

00:16:45.490 --> 00:16:48.180 align:middle line:84%
we had a ton of great questions
come in from educators

00:16:48.180 --> 00:16:49.720 align:middle line:90%
and students alike.

00:16:49.720 --> 00:16:51.390 align:middle line:84%
So we picked out
some of our favorites

00:16:51.390 --> 00:16:53.770 align:middle line:90%
and posed them to Mike.

00:16:53.770 --> 00:16:59.542 align:middle line:84%
Number one, what math do I
need to understand this field?

00:16:59.542 --> 00:17:01.000 align:middle line:84%
MIKE SHORT: That's
a good question.

00:17:01.000 --> 00:17:04.000 align:middle line:84%
It depends on how deeply you
want to understand the field.

00:17:04.000 --> 00:17:05.500 align:middle line:84%
If you want to pass
my class, if you

00:17:05.500 --> 00:17:07.839 align:middle line:84%
want a get an A in my
class, you don't really

00:17:07.839 --> 00:17:10.599 align:middle line:84%
need much math beyond
single-variable calculus.

00:17:10.599 --> 00:17:13.250 align:middle line:84%
And even then,
it's not very much.

00:17:13.250 --> 00:17:14.680 align:middle line:90%
I think we use--

00:17:14.680 --> 00:17:17.470 align:middle line:84%
we have one or two lectures with
integrals and a few lectures

00:17:17.470 --> 00:17:20.470 align:middle line:84%
with differential equations,
but linear first order things

00:17:20.470 --> 00:17:22.927 align:middle line:90%
that you solve in calculus one.

00:17:22.927 --> 00:17:26.140 align:middle line:84%
SARAH HANSEN: Number two,
when you were a student,

00:17:26.140 --> 00:17:28.750 align:middle line:84%
how did you deal
with courses that

00:17:28.750 --> 00:17:33.032 align:middle line:84%
didn't seem interesting to
you, but that you had to study?

00:17:33.032 --> 00:17:34.490 align:middle line:84%
MIKE SHORT: That's
a good question.

00:17:34.490 --> 00:17:35.990 align:middle line:90%
I have a few answers to that.

00:17:35.990 --> 00:17:38.800 align:middle line:84%
So for courses that
didn't seem interesting

00:17:38.800 --> 00:17:41.740 align:middle line:84%
that I had to study, if I
knew why I had to study it,

00:17:41.740 --> 00:17:46.430 align:middle line:84%
there was at least a
practical reason to do well.

00:17:46.430 --> 00:17:48.760 align:middle line:84%
For example, for me,
it was neutronics.

00:17:48.760 --> 00:17:50.380 align:middle line:84%
Neutron transport
is one of the things

00:17:50.380 --> 00:17:52.870 align:middle line:84%
that makes nuclear
engineers what they are.

00:17:52.870 --> 00:17:57.820 align:middle line:84%
I found it to be dry
and not very real-world,

00:17:57.820 --> 00:18:00.730 align:middle line:84%
because I knew I was never
going to be a reactor designer.

00:18:00.730 --> 00:18:03.940 align:middle line:84%
But I felt I would need to
understand neutron transport

00:18:03.940 --> 00:18:06.640 align:middle line:84%
and power levels in order to be
an effective nuclear material

00:18:06.640 --> 00:18:07.510 align:middle line:90%
scientist.

00:18:07.510 --> 00:18:08.873 align:middle line:90%
Luckily, I was right.

00:18:08.873 --> 00:18:11.290 align:middle line:84%
For the classes which I just
had to take because they were

00:18:11.290 --> 00:18:15.220 align:middle line:84%
requirements, and I had no
reason to want to take them,

00:18:15.220 --> 00:18:16.750 align:middle line:90%
I got a little sneaky.

00:18:16.750 --> 00:18:20.110 align:middle line:84%
I ended up double majoring
with material science

00:18:20.110 --> 00:18:23.350 align:middle line:84%
and wrote a petition to get
out of this one medical imaging

00:18:23.350 --> 00:18:25.600 align:middle line:84%
class and replace
it with 12 others

00:18:25.600 --> 00:18:27.318 align:middle line:90%
in order to make a second major.

00:18:27.318 --> 00:18:28.610 align:middle line:90%
And that petition was approved.

00:18:28.610 --> 00:18:32.320 align:middle line:84%
So I actually did get to simply
drop a departmental requirement

00:18:32.320 --> 00:18:35.822 align:middle line:84%
by articulating why I wanted
to study something else.

00:18:35.822 --> 00:18:37.780 align:middle line:84%
Not all students realize
that they can do this,

00:18:37.780 --> 00:18:39.370 align:middle line:90%
but they can do this.

00:18:39.370 --> 00:18:42.130 align:middle line:84%
With a very good
intellectual justification,

00:18:42.130 --> 00:18:44.540 align:middle line:90%
rules can be bent or broken.

00:18:44.540 --> 00:18:47.150 align:middle line:90%
SARAH HANSEN: OK, number three.

00:18:47.150 --> 00:18:50.770 align:middle line:84%
Why can't we just send
nuclear waste to space?

00:18:50.770 --> 00:18:53.290 align:middle line:84%
MIKE SHORT: We could just
send nuclear waste to space

00:18:53.290 --> 00:18:55.180 align:middle line:90%
and get it out of our hair.

00:18:55.180 --> 00:18:56.660 align:middle line:90%
It would be expensive.

00:18:56.660 --> 00:18:59.440 align:middle line:84%
It costs a lot of money
per gram to get something

00:18:59.440 --> 00:19:00.850 align:middle line:90%
off the planet.

00:19:00.850 --> 00:19:03.130 align:middle line:84%
Someone has to
agree to pay for it.

00:19:03.130 --> 00:19:06.040 align:middle line:84%
And what worries me most is,
what if one of those missions

00:19:06.040 --> 00:19:07.310 align:middle line:90%
goes wrong?

00:19:07.310 --> 00:19:09.790 align:middle line:84%
What if you're launching a
rocket full of the world's

00:19:09.790 --> 00:19:12.190 align:middle line:84%
worst nuclear
waste, and something

00:19:12.190 --> 00:19:15.700 align:middle line:84%
goes wrong at the launch, and
then it comes back down, along

00:19:15.700 --> 00:19:16.900 align:middle line:90%
with the rocket explosion?

00:19:16.900 --> 00:19:19.780 align:middle line:84%
Then you have
contaminated the planet.

00:19:19.780 --> 00:19:23.230 align:middle line:84%
So I personally believe in
containing nuclear waste where

00:19:23.230 --> 00:19:26.170 align:middle line:84%
we can see it rather
than blasting it off

00:19:26.170 --> 00:19:28.720 align:middle line:84%
into space and
contaminating space,

00:19:28.720 --> 00:19:32.643 align:middle line:84%
unless we know where it's going,
and that nothing will go wrong.

00:19:32.643 --> 00:19:34.060 align:middle line:84%
Because a lot of
folks are worried

00:19:34.060 --> 00:19:35.810 align:middle line:84%
about the dangers
of radiation, how

00:19:35.810 --> 00:19:37.750 align:middle line:84%
we're going to deal
with nuclear waste.

00:19:37.750 --> 00:19:40.540 align:middle line:84%
And I don't fear
nuclear waste, but I've

00:19:40.540 --> 00:19:42.550 align:middle line:84%
got a healthy respect
for it in that whatever

00:19:42.550 --> 00:19:46.060 align:middle line:84%
we do with it has to have the
lowest probability of getting

00:19:46.060 --> 00:19:47.980 align:middle line:90%
out and contaminating anything.

00:19:47.980 --> 00:19:50.350 align:middle line:84%
I think it's a necessary
thing to make in order

00:19:50.350 --> 00:19:52.250 align:middle line:90%
to make nuclear power.

00:19:52.250 --> 00:19:56.292 align:middle line:84%
So if we want to make almost
unlimited carbon-free power,

00:19:56.292 --> 00:19:58.000 align:middle line:84%
we're going to make
waste in the process.

00:19:58.000 --> 00:19:59.292 align:middle line:90%
You can't fight thermodynamics.

00:19:59.292 --> 00:20:01.833 align:middle line:84%
You're always going to have some
waste of energy or something

00:20:01.833 --> 00:20:02.450 align:middle line:90%
else.

00:20:02.450 --> 00:20:03.460 align:middle line:84%
But then what you
do with it has to be

00:20:03.460 --> 00:20:04.940 align:middle line:90%
very carefully considered.

00:20:04.940 --> 00:20:07.100 align:middle line:84%
And it sounds simple
to blast it into space,

00:20:07.100 --> 00:20:09.100 align:middle line:84%
but then you have to
think, what could go wrong,

00:20:09.100 --> 00:20:11.590 align:middle line:84%
and who could I hurt
if it goes wrong?

00:20:11.590 --> 00:20:13.780 align:middle line:84%
SARAH HANSEN:
Number four, what do

00:20:13.780 --> 00:20:16.240 align:middle line:84%
you think about the
cultural and political idea

00:20:16.240 --> 00:20:17.980 align:middle line:90%
against nuclear power?

00:20:17.980 --> 00:20:21.370 align:middle line:84%
MIKE SHORT: To me, the current
cultural and political idea

00:20:21.370 --> 00:20:24.220 align:middle line:84%
against nuclear power
is not grounded in fact.

00:20:24.220 --> 00:20:25.762 align:middle line:90%
It's grounded in emotion.

00:20:25.762 --> 00:20:27.220 align:middle line:84%
And I've talked
with a lot of folks

00:20:27.220 --> 00:20:30.010 align:middle line:84%
who either know very
little or very much

00:20:30.010 --> 00:20:33.520 align:middle line:84%
about the physics and
engineering of nuclear power.

00:20:33.520 --> 00:20:35.080 align:middle line:84%
But I find more
often than not, it's

00:20:35.080 --> 00:20:38.050 align:middle line:84%
an issue designed
to rally a base.

00:20:38.050 --> 00:20:41.230 align:middle line:84%
Strangely, I've never
really understood this.

00:20:41.230 --> 00:20:45.445 align:middle line:84%
So many environmentalists
are against nuclear power.

00:20:45.445 --> 00:20:46.820 align:middle line:84%
And I'm an
environmentalist, too,

00:20:46.820 --> 00:20:48.820 align:middle line:84%
which is why I'm
for nuclear power.

00:20:48.820 --> 00:20:51.070 align:middle line:84%
So I find the
anti-nuclear sentiment

00:20:51.070 --> 00:20:55.570 align:middle line:84%
to be so strongly democratic
and the pro-nuclear sentiment

00:20:55.570 --> 00:20:58.930 align:middle line:84%
to be so strongly
Republican, neither of which

00:20:58.930 --> 00:21:02.380 align:middle line:84%
is for reasons which
I'm willing to accept.

00:21:02.380 --> 00:21:08.230 align:middle line:84%
They seem to be more about
political tribalism than fact.

00:21:08.230 --> 00:21:11.230 align:middle line:84%
And it's interesting now that
for the first time since we've

00:21:11.230 --> 00:21:14.023 align:middle line:84%
had Chernobyl
disasters and such,

00:21:14.023 --> 00:21:15.940 align:middle line:84%
more and more environmentalists
are coming out

00:21:15.940 --> 00:21:18.880 align:middle line:84%
in favor of nuclear
power, not because they're

00:21:18.880 --> 00:21:21.560 align:middle line:84%
in favor of radiation,
and waste, and such.

00:21:21.560 --> 00:21:24.970 align:middle line:84%
But the goal is to
prevent climate change.

00:21:24.970 --> 00:21:28.330 align:middle line:84%
I would much sooner
take a risk of something

00:21:28.330 --> 00:21:31.240 align:middle line:84%
going wrong with nuclear
power than definitely lose

00:21:31.240 --> 00:21:33.160 align:middle line:90%
the battle to climate change.

00:21:33.160 --> 00:21:37.630 align:middle line:84%
Everything to me comes out to
minimizing risk to human life

00:21:37.630 --> 00:21:40.820 align:middle line:90%
and maximizing quality of life.

00:21:40.820 --> 00:21:43.420 align:middle line:84%
So to me, the risk
of nuclear power

00:21:43.420 --> 00:21:46.370 align:middle line:84%
is that if we can go all
carbon-free for energy,

00:21:46.370 --> 00:21:48.670 align:middle line:90%
we can reverse climate change.

00:21:48.670 --> 00:21:51.520 align:middle line:84%
If we're afraid of using
nuclear power for fear

00:21:51.520 --> 00:21:55.150 align:middle line:84%
of the waste getting out,
or the risk, or the weapons,

00:21:55.150 --> 00:21:58.550 align:middle line:84%
then we're automatically
losing the war,

00:21:58.550 --> 00:22:01.120 align:middle line:84%
and we're going to have an
uninhabitable planet anyway.

00:22:01.120 --> 00:22:02.662 align:middle line:84%
And we can't get
off this planet yet,

00:22:02.662 --> 00:22:04.578 align:middle line:84%
and then we'll go make
the same mistakes there

00:22:04.578 --> 00:22:05.530 align:middle line:90%
as we would here.

00:22:05.530 --> 00:22:07.720 align:middle line:84%
For example, I came into
this department wanting

00:22:07.720 --> 00:22:10.870 align:middle line:84%
to study fusion, felt it
wasn't ready yet, so I spent

00:22:10.870 --> 00:22:12.700 align:middle line:84%
a lot of my time on
fission, thinking,

00:22:12.700 --> 00:22:14.740 align:middle line:84%
this is going to be
the bridge to fusion.

00:22:14.740 --> 00:22:17.860 align:middle line:84%
Because fusion promises
more carbon-free power

00:22:17.860 --> 00:22:20.700 align:middle line:84%
with far less radioactive
waste, but not none.

00:22:20.700 --> 00:22:22.605 align:middle line:84%
And I'm willing to accept
the some, so as not

00:22:22.605 --> 00:22:24.730 align:middle line:84%
to lose the climate change
battle, which is already

00:22:24.730 --> 00:22:26.350 align:middle line:90%
on our doorstep.

00:22:26.350 --> 00:22:28.240 align:middle line:84%
I do worry that many
environmentalists

00:22:28.240 --> 00:22:32.650 align:middle line:84%
lose sight of the real goal,
which is protecting the planet.

00:22:32.650 --> 00:22:36.250 align:middle line:84%
And to me, protecting the
planet doesn't mean, do no harm.

00:22:36.250 --> 00:22:38.800 align:middle line:84%
It means, do as little harm
as possible while preserving

00:22:38.800 --> 00:22:41.368 align:middle line:90%
our quality of life.

00:22:41.368 --> 00:22:45.670 align:middle line:84%
SARAH HANSEN: Number five, while
learning, occasionally, you

00:22:45.670 --> 00:22:48.360 align:middle line:84%
will have these moments where
all of the sudden, the dots

00:22:48.360 --> 00:22:51.390 align:middle line:84%
suddenly connect, and a
previously challenging topic

00:22:51.390 --> 00:22:54.120 align:middle line:84%
becomes seemingly
perfectly clear to you.

00:22:54.120 --> 00:22:57.906 align:middle line:84%
Could you share with us
one of your brain blasts?

00:22:57.906 --> 00:22:58.870 align:middle line:90%
MIKE SHORT: Let's see.

00:22:58.870 --> 00:23:01.630 align:middle line:84%
For me, it's the same one
that most students get

00:23:01.630 --> 00:23:04.660 align:middle line:84%
at about the one-month
mark in my class,

00:23:04.660 --> 00:23:10.090 align:middle line:84%
and that's energy is matter,
that E equals mc squared.

00:23:10.090 --> 00:23:12.130 align:middle line:84%
You see it on
shirts all over MIT.

00:23:12.130 --> 00:23:16.150 align:middle line:84%
It's probably the one equation
that everyone in America knows,

00:23:16.150 --> 00:23:18.910 align:middle line:84%
but not a lot of people
really understand

00:23:18.910 --> 00:23:22.240 align:middle line:84%
that the conversion
of matter into energy

00:23:22.240 --> 00:23:26.080 align:middle line:84%
through ionizing radiation
is the movement of energy

00:23:26.080 --> 00:23:27.130 align:middle line:90%
from one form to another.

00:23:27.130 --> 00:23:29.060 align:middle line:90%
Matter is a form of energy.

00:23:29.060 --> 00:23:30.850 align:middle line:84%
And once that
clicked, everything

00:23:30.850 --> 00:23:32.500 align:middle line:84%
seemed to make
sense-- radioactive

00:23:32.500 --> 00:23:35.020 align:middle line:84%
decay, nuclear reactions,
all these things.

00:23:35.020 --> 00:23:38.500 align:middle line:84%
I remember that aha
moment in this class

00:23:38.500 --> 00:23:42.610 align:middle line:84%
that I teach as a second-year
student back in 2002.

00:23:42.610 --> 00:23:44.230 align:middle line:84%
And it's those kind
of moments that

00:23:44.230 --> 00:23:46.350 align:middle line:84%
made me want to stay in it,
because I feel like, wow, I

00:23:46.350 --> 00:23:47.475 align:middle line:90%
really know this field now.

00:23:47.475 --> 00:23:50.266 align:middle line:90%
[MUSIC PLAYING]

00:23:50.266 --> 00:23:56.775 align:middle line:90%


00:23:56.775 --> 00:23:58.900 align:middle line:84%
SARAH HANSEN: If you're
interested in learning more

00:23:58.900 --> 00:24:02.410 align:middle line:84%
about ionizing radiation,
we've got all of Mike's course

00:24:02.410 --> 00:24:04.120 align:middle line:90%
materials on our site.

00:24:04.120 --> 00:24:08.500 align:middle line:90%
You can find us at ocw.mit.edu.

00:24:08.500 --> 00:24:10.900 align:middle line:84%
You can also read more of
his instructor insights

00:24:10.900 --> 00:24:15.040 align:middle line:84%
on his OCW course page made
especially for educators.

00:24:15.040 --> 00:24:17.810 align:middle line:84%
You can find all sorts of
different instructor insights

00:24:17.810 --> 00:24:24.520 align:middle line:84%
on our educator portal
at ocw.mit.edu/educator.

00:24:24.520 --> 00:24:29.880 align:middle line:84%
Until next time, I'm Sarah
Hansen from MIT OpenCourseWare.

00:24:29.880 --> 00:24:37.000 align:middle line:90%