How To Discover A New Planet (Science Out Loud S1 Ep1) - Free Educational videos for Students in K-12 | Lumos Learning

How To Discover A New Planet (Science Out Loud S1 Ep1) - Free Educational videos for Students in k-12


How To Discover A New Planet (Science Out Loud S1 Ep1) - By MITK12Videos



Transcript
00:00 25 years ago , most people would have told you
00:03 that there are only nine planets in the universe .
00:05 Since then we've lost one . Sorry , Pluto ,
00:09 but we've discovered thousands of others . So what happened
00:12 ? Did astronomers suddenly get a new pair of glasses
00:14 and now we're meeting all of our new neighbors ?
00:16 Well , no , it turns out we could have
00:18 seen these exit plants all along , but we only
00:20 recently figured out exactly where and how to look .
00:24 We call these new planets exoplanets or extrasolar plants .
00:29 These are plants outside our own solar system . Up
00:31 until a few decades ago , we only knew about
00:33 plants in our own solar system , like venus ,
00:36 mercury and Earth . But in the last 20 years
00:39 , we've discovered over 1000 confirmed plants outside our own
00:42 solar system and over 3000 candidates that are probably planets
00:46 . In fact , scientists think that there are quintillion
00:49 of planets in our universe that we just haven't seen
00:51 yet . We've known for the last 400 years about
00:56 our nine well ate plants in our solar system .
01:00 So how are we now just finding all of these
01:02 other planets ? The simple answer is we've built telescopes
01:05 that are made to find them and they use something
01:07 called the Transit method . Here's an easy way to
01:11 think about it . This light is a star and
01:15 I am a transiting exoplanet when I pass in front
01:18 of the star , you can't see my features ,
01:20 but you can see my outline and that's how ,
01:22 you know , I'm there and that's exactly how the
01:24 transiting method works . This is real space telescope data
01:29 . What scientists do is that they monitor the brightness
01:31 of a star over time when they look for are
01:34 these tiny dips in the overall light and that tells
01:37 you that there may be a planet around that star
01:40 . The Transit method needs planets that orbit their star
01:44 quickly so that we can get lots of transit and
01:47 get a good signal . This means that the plants
01:50 need to be close to their star now in our
01:53 own solar system . The plants that are closer to
01:55 the star are the small rocky planets like mercury ,
01:58 venus and earth . Because astronomers used to think that
02:01 every planetary system had to look like our own solar
02:04 system , they thought that the planets that were close
02:06 enough to the star to detect with the transit method
02:09 were too small to see what their old telescopes ,
02:11 so they didn't even bother looking Had they looked ,
02:15 scientists could have found a jupiter sized planet right next
02:19 to its host star . It turns out exoplanet systems
02:22 are nothing like our own solar system . In fact
02:25 , they're changing the way we see and study plant
02:28 formation in our universe . Not only have you been
02:32 able to find large planets next their stars , but
02:34 we built better telescopes that can find these small rocky
02:37 planets too . For example , Nasa's kepler telescope has
02:41 found thousands of exoplanets using only the transit method .
02:46 And now the next generation is coming . This is
02:49 tess the transiting Exoplanet survey satellite She's going to be
02:54 launched in 2017 is being built right now by Google
02:57 M . IT and NASA Test . His main job
03:00 is to look for exoplanets around the brightest and closest
03:03 stars to our own solar system . With any luck
03:06 , she'll find planets that are close enough that we
03:09 can follow them up with other space and ground based
03:11 telescopes to better understand their atmospheres and climates . It's
03:15 amazing that such a simple method can help us find
03:18 so many new planets . Just by looking for dips
03:20 in brightness , we might be able to find a
03:22 plant that can host life . All we had to
03:24 know was exactly how and where to look . Yeah
00:0-1 .
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