WEBVTT FILE 1 00:00:00.650 --> 00:00:05.759 My name is David Choi, and I study the weather on giant planets. When we look at 2 00:00:05.759 --> 00:00:09.030 Jupiter we're seeing the top of its atmosphere and its weather layer, and its 3 00:00:09.030 --> 00:00:12.000 weather layer contains a lot of interesting features such as jet streams, 4 00:00:12.000 --> 00:00:17.039 vortices, storms, and these particular features called hot spots. 5 00:00:17.039 --> 00:00:20.939 So hot spots are like holes in the clouds because they appear very dark when observed 6 00:00:20.939 --> 00:00:24.689 in visible light, but in near infrared light they appear very bright, and this 7 00:00:24.689 --> 00:00:28.890 indicates that we're seeing deeper down into warmer layers of the atmosphere. Hot 8 00:00:28.890 --> 00:00:33.630 spots have been previously studied by the Galileo atmospheric probe. In 1995 9 00:00:33.630 --> 00:00:36.950 the spacecraft released a probe that descended into Jupiter's atmosphere 10 00:00:36.950 --> 00:00:41.520 specifically at a hot spot, and this probe made the first in situ 11 00:00:41.520 --> 00:00:44.430 measurements and the only in situ measurements of Jupiter that exist today. 12 00:00:44.430 --> 00:00:48.510 So it's very important to understand how hot spot meteorology works, in order to 13 00:00:48.510 --> 00:00:51.899 place these in situ measurements from the Galileo probe in its proper 14 00:00:51.899 --> 00:00:56.969 In 2000 the Cassini spacecraft flew past Jupiter and created a series 15 00:00:56.969 --> 00:01:00.870 of still images that we compiled into time-lapse movies of Jupiter's 16 00:01:00.870 --> 00:01:04.500 atmosphere. Using these movies, we observed Rossby waves that caused 17 00:01:04.500 --> 00:01:09.270 north-south meanders in a jet stream south of the equator. With new movies we 18 00:01:09.270 --> 00:01:13.439 instead focused on hot spots. Hot spots are unique because we believe that there 19 00:01:13.439 --> 00:01:17.070 is a Rossby wave similar to what we previously detected, but instead of this 20 00:01:17.070 --> 00:01:21.390 Rossby wave moving north-south, it primarily moves up and down in the 21 00:01:21.390 --> 00:01:25.590 atmosphere. The downward portion of the wave pushes air down into warmer layers 22 00:01:25.590 --> 00:01:29.340 of the atmosphere. This causes any clouds that are embedded within the wave to 23 00:01:29.340 --> 00:01:33.509 evaporate and prevents further clouds from forming. So at any given time there 24 00:01:33.509 --> 00:01:37.560 are approximately eight to ten hot spots in Jupiter's atmosphere that are spaced 25 00:01:37.560 --> 00:01:41.490 roughly evenly apart from one another. We believe that each of the downward 26 00:01:41.490 --> 00:01:45.530 portions of this Rossby wave corresponds to the hot spots that we see on Jupiter. 27 00:01:45.530 --> 00:01:49.470 This new finding is exciting because it will allow us to re-examine the Galileo 28 00:01:49.470 --> 00:01:53.340 probe data, and allow us to better understand it and better place it in the 29 00:01:53.340 --> 00:01:56.330 context of Jupiter's overall global climate and atmosphere. 30 00:01:56.330 --> 00:01:59.680 Music 31 00:01:59.680 --> 00:02:05.400 Beep, Beep, Beep