WEBVTT

00:00:03.133 --> 00:00:06.133
[rocket rumbling]

00:00:06.133 --> 00:00:12.133
[dramatic music]

00:00:17.968 --> 00:00:19.801
&gt;&gt; HEY, WELCOME
TO "NASA LAUNCHPAD."

00:00:19.801 --> 00:00:21.400
I'M YOUR HOST, AMBER WHALEN.

00:00:21.400 --> 00:00:25.133
WHAT DO RADIOS, MICROWAVES,
AND X-RAYS HAVE IN COMMON?

00:00:25.133 --> 00:00:26.767
WELL, RADIOS PLAY MUSIC,

00:00:26.767 --> 00:00:29.200
MICROWAVES ARE A FAST
AND EASY WAY TO COOK FOOD,

00:00:29.200 --> 00:00:31.167
AND X-RAYS ALLOW US
TO SEE OUR INSIDES

00:00:31.167 --> 00:00:32.667
FROM THE OUTSIDE.

00:00:32.667 --> 00:00:35.000
SO HOW DO THESE THREE THINGS
HAVE A COMMON LINK?

00:00:35.000 --> 00:00:37.067
THEY'RE ALL PART
OF A BROADER SPECTRUM,

00:00:37.067 --> 00:00:39.367
THE ELECTROMAGNETIC SPECTRUM,
TO BE EXACT.

00:00:39.367 --> 00:00:41.100
THIS IS THE NAME
THAT SCIENTISTS HAVE GIVEN

00:00:41.100 --> 00:00:42.667
TO ALL THE DIFFERENT TYPES
OF RADIATION

00:00:42.667 --> 00:00:44.067
THAT TRAVEL IN WAVES.

00:00:44.067 --> 00:00:45.934
SO WE CAN LISTEN TO OUR FAVORITE
MUSIC FOR FREE

00:00:45.934 --> 00:00:48.467
BECAUSE THE RADIO STATION
EMITS RADIO WAVES.

00:00:48.467 --> 00:00:50.901
BUT DID YOU KNOW
THAT STARS, PLANETS,

00:00:50.901 --> 00:00:53.801
AND EVEN GASES IN SPACE
EMIT RADIO WAVES TOO?

00:00:53.801 --> 00:00:59.801
[dramatic rock guitar music]

00:00:59.801 --> 00:01:01.868
EVEN OUR OWN SUN CREATES
RADIO WAVES.

00:01:05.200 --> 00:01:06.767
TAKE A LOOK AT THIS.

00:01:06.767 --> 00:01:09.601
THIS IS A SOLAR FLARE
ON OUR SUN.

00:01:09.601 --> 00:01:12.000
ON THE RIGHT,
YOU SEE RADIO WAVES.

00:01:12.000 --> 00:01:16.100
WHEN THE SUN FLARES,
SO DO THE RADIO SIGNALS.

00:01:16.100 --> 00:01:18.267
OKAY, SO, ENOUGH
WITH RADIO WAVES.

00:01:18.267 --> 00:01:21.033
THERE ARE EVEN MORE INTERESTING
TYPES OF RADIATION OUT THERE.

00:01:21.033 --> 00:01:24.267
LIKE I SAID, MANY DIFFERENT
TYPES OF RADIATION CAN BE FOUND

00:01:24.267 --> 00:01:25.801
ON THE ELECTROMAGNETIC SPECTRUM,

00:01:25.801 --> 00:01:28.133
FROM THE RADIO WAVES
WE TALKED ABOUT

00:01:28.133 --> 00:01:31.868
TO MICROWAVE,
INFRARED,

00:01:31.868 --> 00:01:33.667
AND VISIBLE--

00:01:33.667 --> 00:01:35.133
THAT'S THE PORTION
OF THE SPECTRUM

00:01:35.133 --> 00:01:37.067
THAT WE CAN SEE
WITH OUR OWN EYES--

00:01:37.067 --> 00:01:39.834
TO ULTRAVIOLET,

00:01:39.834 --> 00:01:42.601
X-RAYS,

00:01:42.601 --> 00:01:44.601
AND GAMMA RAYS.

00:01:49.734 --> 00:01:51.267
THE HIGHER YOU GO
ON THE SPECTRUM,

00:01:51.267 --> 00:01:52.734
THE HIGHER THE ENERGY GETS.

00:01:52.734 --> 00:01:54.767
SO RADIO WAVELENGTHS
ARE VERY LONG,

00:01:54.767 --> 00:01:57.868
WHEREAS GAMMA RAY WAVELENGTHS
ARE VERY SHORT.

00:01:57.868 --> 00:02:00.033
HERE'S OUR SUN AGAIN.

00:02:00.033 --> 00:02:02.567
EACH COLOR YOU SEE
REPRESENTS RADIATION

00:02:02.567 --> 00:02:05.300
FROM DIFFERENT PARTS
OF THE ELECTROMAGNETIC SPECTRUM.

00:02:05.300 --> 00:02:08.234
BY LOOKING AT THE SUN
IN DIFFERENT WAVELENGTHS,

00:02:08.234 --> 00:02:10.567
WE ARE ABLE TO NOTICE
DIFFERENT FEATURES.

00:02:10.567 --> 00:02:15.200
[percussive rock music]

00:02:15.200 --> 00:02:17.434
WHAT'S THE TERM "X-RAY"
MEAN TO YOU?

00:02:17.434 --> 00:02:19.467
BROKEN BONES
AT THE HOSPITAL, RIGHT?

00:02:19.467 --> 00:02:22.100
WELL, HIGH-ENERGY X-RAYS
ARE VERY USEFUL

00:02:22.100 --> 00:02:23.901
FOR MORE THAN LOOKING
INTO OUR BODIES.

00:02:23.901 --> 00:02:25.567
MANY DIFFERENT X-RAY TELESCOPES

00:02:25.567 --> 00:02:27.501
HAVE ENABLED US
TO EXPLORE THE UNIVERSE.

00:02:27.501 --> 00:02:29.033
WE HAVE LEARNED
ABOUT BLACK HOLES,

00:02:29.033 --> 00:02:32.367
NEUTRON STARS, AND SUPERNOVAS,
AMONG OTHER PHENOMENA.

00:02:32.367 --> 00:02:33.868
SO YOU MIGHT WONDER,

00:02:33.868 --> 00:02:35.667
WHY DO WE WANT
TO SEE GAMMA RAYS?

00:02:35.667 --> 00:02:37.567
WELL, SOME OF THE MOST
INTERESTING OBJECTS

00:02:37.567 --> 00:02:39.000
THROUGHOUT OUR UNIVERSE

00:02:39.000 --> 00:02:41.534
EMIT A GOOD PORTION
OF THEIR LIGHT AS GAMMA RAYS.

00:02:41.534 --> 00:02:45.801
HOWEVER, IT'S NOT VISIBLE
TO THE NAKED EYE.

00:02:45.801 --> 00:02:48.133
SO TO LEARN MORE, ENGINEERS
AND SCIENTISTS CREATED

00:02:48.133 --> 00:02:51.968
THE GAMMA RAY LARGE AREA
SPACE TELESCOPE, OR GLAST.

00:02:51.968 --> 00:02:53.567
LAUNCHED IN JUNE OF 2008,

00:02:53.567 --> 00:02:55.100
THE TELESCOPE
WAS RENAMED FERMI,

00:02:55.100 --> 00:02:56.934
AFTER PROFESSOR ENRICO FERMI,

00:02:56.934 --> 00:02:59.467
A PIONEER
IN HIGH-ENERGY PHYSICS.

00:02:59.467 --> 00:03:03.033
[upbeat rock music]

00:03:03.033 --> 00:03:04.634
FERMI NOW ORBITS EARTH

00:03:04.634 --> 00:03:06.601
AND CREATES IMAGES
OF OUR UNIVERSE.

00:03:10.567 --> 00:03:12.467
OKAY, SO MAYBE
I HAVEN'T BEEN CLEAR

00:03:12.467 --> 00:03:15.501
ON HOW INCREDIBLY POWERFUL
GAMMA RAYS ARE

00:03:15.501 --> 00:03:17.934
AND WHAT MAKES THEM
SO WORTHY OF STUDY.

00:03:17.934 --> 00:03:20.901
A SINGLE GAMMA RAY BURST,
LIKE FROM THE DEATH OF A STAR,

00:03:20.901 --> 00:03:23.534
IS SO FORCEFUL THAT
FOR A BRIEF MOMENT IN TIME,

00:03:23.534 --> 00:03:26.801
IT ACTUALLY OUTSHINES
THE ENTIRE UNIVERSE.

00:03:26.801 --> 00:03:29.434
THAT'S PRETTY POWERFUL
IF YOU ASK ME.

00:03:29.434 --> 00:03:31.701
HOW ABOUT ANOTHER POWERFUL
FORCE IN THE UNIVERSE?

00:03:31.701 --> 00:03:32.968
A BLACK HOLE.

00:03:32.968 --> 00:03:34.100
BUT GET THIS:

00:03:34.100 --> 00:03:36.067
EVEN A BLACK HOLE,
WHICH IS INFAMOUS

00:03:36.067 --> 00:03:37.701
FOR PULLING IN MATTER,
EVEN LIGHT,

00:03:37.701 --> 00:03:39.901
ACTUALLY PUSHES AWAY MATTER
IN JETS THAT MOVE

00:03:39.901 --> 00:03:42.467
AT OVER 99%
OF THE SPEED OF LIGHT.

00:03:42.467 --> 00:03:44.467
GUESS WHAT'S INSIDE THESE JETS.

00:03:44.467 --> 00:03:45.501
YOU GOT IT.

00:03:45.501 --> 00:03:47.734
GAMMA RAYS,
AND A WHOLE LOT OF THEM.

00:03:47.734 --> 00:03:50.033
FERMI WILL HELP SCIENTISTS
STUDY WHY THIS HAPPENS.

00:03:50.033 --> 00:03:51.267
TAKE A LOOK AT THIS.

00:03:51.267 --> 00:03:53.067
FERMI SENT THIS IMAGE
BACK TO EARTH.

00:03:53.067 --> 00:03:56.067
IT COMBINES 95 HOURS
OF IMAGES OF THE SKY

00:03:56.067 --> 00:03:57.634
AND GAMMA RAYS EMITTED.

00:03:57.634 --> 00:03:58.868
IF YOU LOOK CLOSE,

00:03:58.868 --> 00:04:01.167
YOU'LL SEE THAT'S
OUR OWN MILKY WAY GALAXY

00:04:01.167 --> 00:04:02.701
RIGHT IN THE CENTER.

00:04:02.701 --> 00:04:05.067
THERE ARE
IMMENSELY POWERFUL GAMMA RAYS

00:04:05.067 --> 00:04:07.567
COMING FROM
OUR OWN GALACTIC BACKYARD.

00:04:07.567 --> 00:04:09.667
IT KIND OF MAKES YOU REALIZE
HOW BIG THINGS REALLY ARE

00:04:09.667 --> 00:04:11.434
AND HOW MUCH WE STILL
NEED TO KNOW

00:04:11.434 --> 00:04:13.000
ABOUT WHAT'S GOING ON
OUT THERE.

00:04:13.000 --> 00:04:15.300
WELL, UNTIL NEXT TIME,
I'M AMBER WHALEN,

00:04:15.300 --> 00:04:17.000
AND THANKS FOR WATCHING
"NASA LAUNCHPAD."