WEBVTT FILE 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 ]