WEBVTT FILE 1 00:00:00.100 --> 00:00:00.834 [ Music ] 2 00:00:00.834 --> 00:00:03.136 So when we look at Jupiter, we see a lot of 3 00:00:03.136 --> 00:00:05.806 structure that looks very similar to the Earth. 4 00:00:05.806 --> 00:00:10.577 We can see storms, we see cyclones, we see anticyclones, 5 00:00:10.577 --> 00:00:13.247 and these sort of storms and weather systems that we see on 6 00:00:13.247 --> 00:00:16.250 Earth are very similar and are happening on Jupiter. 7 00:00:16.250 --> 00:00:19.720 Fluid mechanics is hopefully the same everywhere in the universe, 8 00:00:19.720 --> 00:00:22.356 but Jupiter and Earth are very different. 9 00:00:22.356 --> 00:00:25.058 Jupiter is much bigger, it rotates a lot faster, they're 10 00:00:25.058 --> 00:00:28.528 made of different material, and Jupiter is much further away 11 00:00:28.528 --> 00:00:31.031 from the sun than the Earth is. 12 00:00:31.031 --> 00:00:34.668 The quasi-biennial oscillation, or the QBO, on Earth is an 13 00:00:34.668 --> 00:00:37.771 equatorial phenomenon in the stratosphere where the winds are 14 00:00:37.771 --> 00:00:40.507 changing direction approximately every two years. 15 00:00:40.507 --> 00:00:44.611 Depending on which phase the QBO is in, eastward or westward, the 16 00:00:44.611 --> 00:00:47.748 temperature signal corresponds to that, so it's warmer in the 17 00:00:47.748 --> 00:00:50.484 eastward phase and cooler in the westward phase. 18 00:00:50.484 --> 00:00:53.487 It's been shown that it can actually be a barrier to 19 00:00:53.487 --> 00:00:57.357 transport of aerosols across the equator, and has been linked to 20 00:00:57.357 --> 00:01:00.661 the frequency and the formation of hurricanes in the Atlantic 21 00:01:00.661 --> 00:01:02.296 and the Pacific Ocean. 22 00:01:02.296 --> 00:01:06.066 The long-term scales on Earth's climate is something that we're 23 00:01:06.066 --> 00:01:08.635 very interested in, and how that applies to other planets' 24 00:01:08.635 --> 00:01:13.140 atmospheres is really why we're studying Earth and Jupiter. 25 00:01:13.140 --> 00:01:15.208 The quasi-quadrennial oscillation in Jupiter's 26 00:01:15.208 --> 00:01:18.211 stratosphere is a temperature signal that we see in the 27 00:01:18.211 --> 00:01:21.448 equator, where we see the temperature get warmer and 28 00:01:21.448 --> 00:01:24.418 cooler approximately every four Earth years. 29 00:01:24.418 --> 00:01:27.321 We used a general circulation model, where we focused on 30 00:01:27.321 --> 00:01:30.123 simulating the effects of small-scale waves produced from 31 00:01:30.123 --> 00:01:33.827 convection in Jupiter's equatorial region to simulate 32 00:01:33.827 --> 00:01:34.928 the QQO. 33 00:01:34.928 --> 00:01:38.832 The waves propagate upwards from the clouds and force the winds 34 00:01:38.832 --> 00:01:42.035 in the stratosphere to change direction, going from eastward 35 00:01:42.035 --> 00:01:45.238 to westward approximately every four years. 36 00:01:45.238 --> 00:01:48.742 Our model was able to reproduce the behavior of the QQO, but was 37 00:01:48.742 --> 00:01:51.211 also able to reproduce temperatures from the 38 00:01:51.211 --> 00:01:54.348 observations, and both of those together give us a lot of 39 00:01:54.348 --> 00:01:57.351 confidence that our model is very accurate in what's driving 40 00:01:57.351 --> 00:01:58.652 the QQO. 41 00:01:59.419 --> 00:02:02.189 The outer planets serve as a laboratory for understanding 42 00:02:02.189 --> 00:02:05.792 atmospheric physics under very different conditions than are 43 00:02:05.792 --> 00:02:07.094 present on the Earth. 44 00:02:07.094 --> 00:02:09.896 Understanding how their atmospheres change and evolve 45 00:02:09.896 --> 00:02:11.999 and their climates can give us insight 46 00:02:11.999 --> 00:02:14.134 into any planetary atmosphere. 47 00:02:15.035 --> 00:02:23.543 [ Satellite beeping ]