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Short Wave

The Woman Behind A Mystery That Changed Astronomy

Short Wave

NPR

Daily News, Nature, Life Sciences, Astronomy, Science, News

4.76K Ratings

🗓️ 29 December 2022

⏱️ 13 minutes

🧾️ Download transcript

Summary

In 1967, Jocelyn Bell Burnell made a discovery that revolutionized astronomy. She detected the radio signals emitted by certain dying stars called pulsars. Today, Jocelyn's story. Scientist-in-residence Regina G. Barber talks to Jocelyn about her winding career, her discovery and how pulsars continue to push the field of astronomy today. (encore)

Transcript

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0:00.0

Hey there folks, editor Giselle Grayson here. In today's episode, NPR's astrophysicist Regina

0:05.7

G. Barbara talks to astrophysicist Jocelyn Bell Bernal about her discovery of pulsars

0:11.2

and about the twists and turns in her career. So as I spend my last week as shortwave

0:16.2

senior supervising editor, I want to reflect on and thank some of the people who have made

0:20.8

this last chapter in my career a complete joy. The core shortwave team, Emily Kwong, Rebecca

0:27.3

Ramirez, Berli McCoy, Aaron Scott, Regina Barber, Gabriel Spitzer, Thomas Liu,

0:32.4

Britt Hansen, Margaret Serino, and Brendan Crump. Many others came through shortwave's doors

0:37.4

in 2022, Chloe Weiner, Devon Schwartz, Stephanie O'Neill, Catherine Cipher, Eva Tessfy, Rachel

0:43.2

Carlson, Abilavine, and thanks to all our NPR reporters, engineers, bosses, and colleagues

0:50.0

for all the support you've shown shortwave. A wonderful group of people brings you

0:54.4

our listener, this podcast, and NPR every day. At the end of this episode, Bernal says there's

1:00.4

plenty more unexpected things to trip over if you keep your eyes open. That sounds to me like the

1:05.2

perfect thought to ring in the new year. Happy 2023 from me to the incredible shortwave team,

1:11.3

and to all y'all our listeners. Thank you so much. Happy new year.

1:15.3

You're listening to shortwave from NPR.

1:23.2

Jocelyn Bell Bernal knows that in space, just as in life, nothing lasts forever.

1:28.3

Bigger stars are at the end of their life, explored dramatically. They hugely brighten up,

1:35.5

they kick out a whole lot of gas and stuff into space, and the core gets kicked against,

1:42.5

gets compressed, gets shrunk right down. Massive stars more than 20 times bigger than our son

1:48.8

eventually collapse into black holes. Infinitely small points of immense mass that we can't directly see.

1:56.2

Then there are smaller stars, still bigger than our son, that don't fully collapse into black holes.

2:02.6

They're known as neutron stars, because they're largely composed of one of the fundamental

...

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