Stem Cells and Gene Therapy
The Naked Scientists Podcast
Dr Chris Smith
4.6 • 958 Ratings
🗓️ 17 April 2013
⏱️ 54 minutes
🧾️ Download transcript
Summary
Transcript
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| 0:00.0 | And the Hello, welcome to the naked scientist with me, Chris Smith and with Kate Lamble. |
| 0:20.0 | Hello and this week we track down potentially habitable planets, investigate nanosuits for insects |
| 0:26.2 | and find out why your hearing gets quieter after a concert. |
| 0:30.0 | Plus we report from the British Society for Gene and Cell Therapy's conference at Royal Holloway University in Surrey. |
| 0:37.0 | If you'd like to get in touch with us here at the Naked Scientist, email studio at the Naked Scientist.com, tweet at naked scientists or find us on |
| 0:44.8 | Facebook the naked scientists podcast is powered by UKfast dot code okk UK UK. with an update of this week's science news. |
| 1:03.0 | This week I am joined by Dan Cleary from Science magazine, Philip Broadwith from Chemistry |
| 1:07.7 | World and Peter Rogers from E-Life for a look at what's been making science headlines. |
| 1:12.1 | Dan, what have you got for us? |
| 1:14.0 | Well the story I've got this week is about exoplanets, planets around other stars. |
| 1:20.0 | There's an announcement this week that the Kepler satellite has discovered the best |
| 1:25.4 | candidate so far for a habitable planet around a distant sun-like star so So it could have oceans, it could have land, it could be |
| 1:36.3 | habitable by some sort of creature, but we don't know that much about it, only |
| 1:41.4 | that it's the right size, it's the right distance from its sun, and you know it looks a little bit like Earth. |
| 1:50.0 | So what are we looking for when we're looking for habitable planets rather than just |
| 1:55.4 | any old lump of rock or gas? What's the indicators? |
| 1:58.8 | Well all they can tell with this particular method that Kepler uses. Because planets are so small and so |
| 2:07.6 | dim compared to the star they're orbiting around, you can't see them directly, or's very very hard to see them directly so you |
| 2:14.3 | have to detect them by other methods. Kepler uses the method of transit so |
| 2:19.4 | it essentially looks at a star measures how bright it is, and keeps watching it, and if occasionally it |
| 2:26.0 | gets a very, very tiny bit dimmer, that means that a planet has passed in front of it. So the only information you get are about its orbit, so how long |
| 2:36.5 | it takes to orbit the star, and the size of the planet. so you can tell its radius. |
... |
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