1 00:00:05,240 --> 00:00:10,240 Hi, I'm Joel Hurowitz, a scientist with the surface sampling system team and this is your 2 00:00:10,240 --> 00:00:12,720 Curiosity rover report. 3 00:00:12,720 --> 00:00:17,460 This week the Curiosity science team released its initial findings from its first ever drilled 4 00:00:17,460 --> 00:00:19,210 sample on Mars. 5 00:00:19,210 --> 00:00:22,990 This sample was collected from the “John Klein” drill site, which is located about 6 00:00:22,990 --> 00:00:26,869 500 meters east of where we landed about 7 months ago. 7 00:00:26,869 --> 00:00:32,330 Curiosity obtained her first drill sample and passed that sample on to her onboard analytical 8 00:00:32,330 --> 00:00:34,950 lab instruments, called CheMin and SAM. 9 00:00:34,950 --> 00:00:39,160 These powerful instruments tell us about what minerals are present in these rocks and whether 10 00:00:39,160 --> 00:00:43,520 they contain the ingredients necessary to sustain life as we know it. 11 00:00:43,520 --> 00:00:47,020 What the Curiosity team has found is incredibly exciting. 12 00:00:47,020 --> 00:00:51,989 When we combine what we have learned from our remote sensing and contact science instruments 13 00:00:51,989 --> 00:00:57,820 with the data that’s coming in from CheMin and SAM, we get a picture of an ancient watery 14 00:00:57,820 --> 00:01:01,720 environment, which would have been habitable had life been present in it. 15 00:01:01,720 --> 00:01:05,260 As an example, the information that we’re getting from the CheMin instrument, tells 16 00:01:05,260 --> 00:01:10,030 us that the minerals that are present in this lakebed sedimentary rock at John Klein are 17 00:01:10,030 --> 00:01:14,100 very different from just about anything we’ve ever analyzed before on Mars. 18 00:01:14,100 --> 00:01:19,670 And they tell us that the John Klein rock was deposited in a fresh water environment. 19 00:01:19,670 --> 00:01:24,380 This is an important contrast with other sedimentary environments that we‘ve visited on Mars, 20 00:01:24,380 --> 00:01:28,580 like the Meridiani Planum landing site where the Mars Exploration Rover, Opportunity, has 21 00:01:28,580 --> 00:01:30,170 been operating since 2004. 22 00:01:30,170 --> 00:01:35,600 At that site, the sedimentary rocks record evidence of an environment that was only wet 23 00:01:35,600 --> 00:01:40,520 on a very intermittent basis, and when it was, the waters that were there were highly 24 00:01:40,520 --> 00:01:45,990 acidic, very salty, and not favorable for the survival of organic compounds. 25 00:01:45,990 --> 00:01:49,829 This is in direct contrast to the fresh water environment we’re seeing here at the John 26 00:01:49,829 --> 00:01:50,869 Klein Site. 27 00:01:50,869 --> 00:01:55,049 The SAM instrument is telling us that these rocks contained all of the ingredients necessary 28 00:01:55,049 --> 00:01:56,740 for a habitable environment. 29 00:01:56,740 --> 00:02:01,210 We found carbon, sulfur and oxygen, all present and a number of other elements in states that 30 00:02:01,210 --> 00:02:03,259 life could have taken advantage of. 31 00:02:03,259 --> 00:02:07,259 All in all, these few tablespoons of powder from a Martian rock have provided the Curiosity 32 00:02:07,259 --> 00:02:12,040 science team with an exciting new dataset that tells us that Gale Crater, and perhaps 33 00:02:12,040 --> 00:02:15,170 all of Mars, contained habitable environments. 34 00:02:15,170 --> 00:02:19,200 This is an incredible success for the Curiosity mission to Gale, and the science team is looking 35 00:02:19,200 --> 00:02:23,980 forward to digging deeper into Mars’ ancient watery past in the weeks, months, and years 36 00:02:23,980 --> 00:02:25,020 ahead.