1 00:00:00,066 --> 00:00:04,466 [ Music ] 2 00:00:04,466 --> 00:00:08,866 Enceladus is one of Saturn’s many moons, and it’s a very small moon 3 00:00:08,866 --> 00:00:11,033 that people tend to kind of ignore because it is so small 4 00:00:11,033 --> 00:00:12,900 about 500 kilometers in diameter. 5 00:00:12,900 --> 00:00:16,466 But decades ago, in the 1980's from ground-based observing, 6 00:00:16,466 --> 00:00:20,233 we found out that the location of Enceladus relative to Saturn 7 00:00:20,233 --> 00:00:23,533 happened to coincide nicely with Saturn’s E ring 8 00:00:23,533 --> 00:00:27,200 and so we were thinking that Enceladus had something to do with the E ring 9 00:00:27,200 --> 00:00:30,366 particulates, that icy material, but we weren’t sure. 10 00:00:30,366 --> 00:00:34,666 What we later find from Cassini was that we directly determined 11 00:00:34,666 --> 00:00:38,933 that there are indeed plumes jetting out of the south polar region from cracks 12 00:00:38,933 --> 00:00:41,400 in the south pole of Enceladus in the crust. 13 00:00:41,400 --> 00:00:45,200 And it’s dominantly water-rich material just jetting out into space. 14 00:00:45,200 --> 00:00:50,366 And so the way we saw it, Cassini happened to be located where Enceladus was backlit 15 00:00:50,366 --> 00:00:54,833 from the Sun, and so you saw this curtain of beautiful, diffuse material 16 00:00:54,833 --> 00:00:58,533 jetting out of the south polar region – quite breathtaking actually. 17 00:00:58,533 --> 00:01:01,533 Even more, we were able to use the different compliments of instruments 18 00:01:01,533 --> 00:01:05,800 onboard Cassini to go after the chemical composition of the plumes, 19 00:01:05,800 --> 00:01:11,000 and that’s where things got really interesting. So number one, that’s because of liquid water. 20 00:01:11,000 --> 00:01:16,466 There’s definitely a liquid water reservoir subsurface below the icy crust, but that is there. 21 00:01:16,466 --> 00:01:21,566 Number two, the chemical composition of the plumes told us that there is a lot of organics 22 00:01:21,566 --> 00:01:25,266 things that make up amino acids and things on life that are very interesting. 23 00:01:25,266 --> 00:01:29,733 And number three, what we were really looking for was a source of energy. 24 00:01:29,733 --> 00:01:33,933 On Enceladus, photons from the Sun aren’t going to work because you can’t penetrate 25 00:01:33,933 --> 00:01:38,733 the tens of kilometers of icy crust to get down to where the liquid water reservoir is. 26 00:01:38,733 --> 00:01:42,733 But, what Enceladus does have is hydrothermal vents. 27 00:01:42,733 --> 00:01:47,533 It’s very hot with the liquid water, that has a lot of analogies with the ocean floor 28 00:01:47,533 --> 00:01:53,133 where we have a form of releasing chemical energy via something called serpentinization. 29 00:01:53,133 --> 00:01:56,233 And so we think that Enceladus might have that potential 30 00:01:56,233 --> 00:02:00,533 to have an energy source being chemical, not sunlight. 31 00:02:00,533 --> 00:02:05,033 And so you put all that together and Enceladus has all the ingredients, 32 00:02:05,033 --> 00:02:07,700 or most of what we need for life. 33 00:02:07,700 --> 00:02:11,933 That makes it a very astrobiologically interesting object to study. 34 00:02:11,933 --> 00:02:20,166 [ Music ]