1 00:00:03,680 --> 00:00:07,520 We're taking a deep dive into the  world of moon rocks and the mind-blowing   2 00:00:07,520 --> 00:00:13,200 technology that NASA uses to study these  remarkable rocks from space... next, on Real World. 3 00:00:13,200 --> 00:00:21,417 [Music] 4 00:00:21,417 --> 00:00:27,160 The Moon, our closest celestial neighbor, has fascinated humans for centuries. Thanks to   5 00:00:27,160 --> 00:00:32,360 NASA's Apollo missions, we have been able to bring  back rock samples from the Moon and study them in   6 00:00:32,360 --> 00:00:38,440 detail. But, how many samples were collected and  what do we know about them? Across the six Apollo   7 00:00:38,440 --> 00:00:43,680 missions they collected 2,196 individually  numbered samples. There are so many different   8 00:00:43,680 --> 00:00:47,960 types of sample that they brought back. The biggest  division is rocks versus soil, so they brought back   9 00:00:47,960 --> 00:00:52,880 about 2/3 rock and about 1/3 soil. Within each  of those divisions you have different types   10 00:00:52,880 --> 00:00:56,880 of rocks. You have rocks that are what we call  igneous - they form from molten lava. And then we   11 00:00:56,880 --> 00:01:01,560 have rocks that are sedimentary that form through  impact processes and so each of those answers   12 00:01:01,560 --> 00:01:05,560 different questions about the Moon and then with  the soils we brought back surface soils and deep   13 00:01:05,560 --> 00:01:10,840 soils and deep, deep soils and each of those tells  us something different about solar system and   14 00:01:10,840 --> 00:01:15,560 lunar history. When we talk about soil on the  Moon, it's really what we call regolith and the   15 00:01:15,560 --> 00:01:21,680 difference is soil involves a chemical process.  So soil on Earth has worms in it, it has water   16 00:01:21,680 --> 00:01:26,480 there's a chemical breakdown of the material into  soil. Moon doesn't have any of that. The Moon is   17 00:01:26,480 --> 00:01:31,720 entirely a physical process and so we call that a  regolith but most people think of it as soil. Math   18 00:01:31,720 --> 00:01:37,080 is used every day at every level when we curate  the samples and when people study the samples. At   19 00:01:37,080 --> 00:01:42,200 the most basic we have to keep track of the mass  so we have to be able to add and subtract as we   20 00:01:42,200 --> 00:01:47,400 we started with a kilogram of sample and then we  subtracted off 100 milligrams to send to you now   21 00:01:47,400 --> 00:01:51,560 how much do we have left so that's very basic  but it's very important because it's what lets   22 00:01:51,560 --> 00:01:56,120 us know how much we have left. We've also used  math to calculate the density of a rock and so   23 00:01:56,120 --> 00:02:00,640 so density equals the mass of something divided by  the volume of that of the material you're weighing.   24 00:02:00,640 --> 00:02:04,760 So if you know how much it weighs and you know how  big it is then you can figure out the density. So   25 00:02:04,760 --> 00:02:10,000 the normal way to calculate the density of a rock  is to actually just to weigh it and then you need   26 00:02:10,000 --> 00:02:14,560 to figure out the volume of the rock and you  could figure out the volume of a rock by using   27 00:02:14,560 --> 00:02:19,160 um a laser 3D scanner and in fact this is done  quite commonly on terrestrial samples uh where   28 00:02:19,160 --> 00:02:22,880 you put the rock and you scan it with a laser  and it gives you a very precise volume and then   29 00:02:22,880 --> 00:02:26,840 you weigh it and then the density is relatively  straightforward to figure out after that you just   30 00:02:26,840 --> 00:02:31,520 divide the mass by the volume and there's your  density. Once the scientists get the samples they   31 00:02:31,520 --> 00:02:37,360 use math in everything they do. Whoa! There are so  many different types of samples available for   32 00:02:37,360 --> 00:02:42,360 researchers to study and so many different ways  for them to study them, but how do we protect   33 00:02:42,360 --> 00:02:47,600 these samples and how do we make sure that they  are not contaminated with particles from Earth?   34 00:02:47,600 --> 00:02:54,280 We're working in a clean room for the fact that we  need to keep the samples that came from the Moon   35 00:02:54,280 --> 00:02:59,520 in the same pristine state that they were in when  they were collected. It's important to use a clean   36 00:02:59,520 --> 00:03:06,120 room because we want to make sure that what's  being analyzed is actually from the Moon versus   37 00:03:06,120 --> 00:03:12,760 analyzing what's actually on Earth. There were six  missions that the astronauts brought back 842 lbs   38 00:03:12,760 --> 00:03:20,960 of rocks, 382 kg of rocks, are processed in nitrogen-filled cabinets in the Lunar Lab. And we process them   39 00:03:20,960 --> 00:03:29,200 in that environment so that we're not contaminating.  The Lunar Lab is actually a ISO 6 lab; we have a   40 00:03:29,200 --> 00:03:36,320 Return Processing Lab that's actually ISO 7. Those  ISO numbers, or government numbers, saying the   41 00:03:36,320 --> 00:03:42,160 cleanliness of laboratories. There's procedures  step by step in order to enter the laboratory.   42 00:03:42,160 --> 00:03:50,280 We actually don uh hat, booties, gloves, bunny suit. These rooms are all pressurized so that the clean   43 00:03:50,280 --> 00:03:56,040 air is flowing outward and dirty air doesn't go  in. Who ever would have thought that a rock would   44 00:03:56,040 --> 00:04:01,800 need to be so clean? Now that we know about the  different types of Moon rocks that we have and   45 00:04:01,800 --> 00:04:07,120 how we protect them from contamination, what kind  of math is used to help curate and process these   46 00:04:07,120 --> 00:04:13,680 lunar artifacts? When a sample is processed,  the database has the original weight that   47 00:04:13,680 --> 00:04:20,240 was given when the sample came back, so that mass  is recorded in the database. So once we weigh the   48 00:04:20,240 --> 00:04:26,480 sample it has to be within the balance tolerance.  That's where our math is involved. NASA waited   49 00:04:26,480 --> 00:04:33,640 50 years to open up the samples that they had on  reserve until someone would put in a request that was   50 00:04:33,640 --> 00:04:41,640 different using updated and different technology  because technology definitely has changed from the   51 00:04:41,640 --> 00:04:49,520 70s to now. With the CT scanning, you can look at a  sample and you will actually see what's inside of   52 00:04:49,520 --> 00:04:55,840 a sample. If it's a large class if they're small  classes before you even decide I want to break   53 00:04:55,840 --> 00:05:02,840 this rock, you know what's inside of the rock. These  rocks are out of this world! Seriously, they're   54 00:05:02,840 --> 00:05:10,560 from the Moon. It truly is amazing that we can  learn so much from an object as simple as a rock.   55 00:05:10,560 --> 00:05:16,880 And thanks to the work from rock stars like Ryan  and Andrea, we are one step closer to understanding   56 00:05:16,880 --> 00:05:24,240 and appreciating the wonders of our universe.  And that is rock solid! See you next time on Real 57 00:05:24,240 --> 00:05:25,459 World.