1 00:00:00,010 --> 00:00:04,110 [music, sound effects] 2 00:00:04,130 --> 00:00:08,230 Narrator: What happens if you have something like this, and you want to find out if something 3 00:00:12,440 --> 00:00:08,330 like this is inside? Obviously, you can 4 00:00:12,460 --> 00:00:16,510 but if you separate things out, the answer becomes 5 00:00:16,530 --> 00:00:20,580 clear. Scientists have the same problem. How do you know if there was 6 00:00:20,600 --> 00:00:24,640 once water on Mars...or, for that matter, life? Obviously 7 00:00:24,660 --> 00:00:28,670 you can't tell just by looking at pictures of Mars, but scientists think the answer may lie hidden in 8 00:00:28,690 --> 00:00:32,710 tiny molecules in Martian soil. So, how do you take apart 9 00:00:32,730 --> 00:00:36,730 a molecule to see what's inside? Luckily, scientists have a tool to do just 10 00:00:36,750 --> 00:00:40,750 that. It's called a mass spectrometer, and it lets us take an extremely close look 11 00:00:40,770 --> 00:00:44,900 at whatever we're studying. And even though Mars immediately comes to mind, mass 12 00:00:44,920 --> 00:00:49,020 spectrometers are used in multiple NASA missions. They're also used in labs for hundreds 13 00:00:49,040 --> 00:00:53,100 of scientific purposes. But the important question is: How does it work? 14 00:00:53,120 --> 00:00:57,190 Today, we'll be looking at a special kind of spectrometer called the quadrupole mass 15 00:00:57,210 --> 00:01:01,280 spectrometer. It's called this because of the four long poles that make up the center 16 00:01:01,300 --> 00:01:05,350 of the instrument. So say you have a sample that's been turned into a gas, and you want to 17 00:01:05,370 --> 00:01:09,400 find out if it contains certain things. The gas is sent into the mass spectrometer 18 00:01:09,420 --> 00:01:13,450 first hitting a piece called the ion source. Here, a stream of electrons 19 00:01:13,470 --> 00:01:17,490 hits the molecule, breaking it into fragments and giving each fragment a charge. 20 00:01:17,510 --> 00:01:21,510 Next, the fragments enter what's called the analyzer. Here, 21 00:01:21,530 --> 00:01:25,520 they're separated based on their mass, and the analyzer is tuned so that only 22 00:01:25,540 --> 00:01:29,630 the fragments we want to see make it through. Everything else flies off in a different 23 00:01:29,650 --> 00:01:33,710 direction. After this, the fragments hit what's called the detector, 24 00:01:33,730 --> 00:01:37,810 and scientists record the data. If you're looking for more than one kind, the analyzer 25 00:01:37,830 --> 00:01:41,910 can scan across a range of fragments, building up a record of not only what kind, 26 00:01:41,930 --> 00:01:46,010 but how many. Once you have these results, called a mass spectrum, 27 00:01:46,030 --> 00:01:50,080 you can verify that your sample in fact contains what you're looking for. And here, 28 00:01:50,100 --> 00:01:54,130 the real work begins. The mass spectrometer is a powerful tool, and 29 00:01:54,150 --> 00:01:58,170 by taking many samples, looking at the results, and studying what we find, 30 00:01:58,190 --> 00:02:02,200 scientists can work to discover not only the secrets of water and life on Mars, but 31 00:02:02,220 --> 00:02:06,210 also answers to bigger questions about the universe. And all by studying something 32 00:02:06,230 --> 00:02:10,280 as tiny as a molecule. 33 00:02:10,300 --> 00:02:14,390 [music, beeping] 34 00:02:14,410 --> 00:02:18,460 [beeping]