WEBVTT FILE 1 00:00:00.766 --> 00:00:05.250 Narrator: Today, Mars is a cold desert surrounded by a thin wisp of air, 2 00:00:05.600 --> 00:00:09.683 but its dry lakebeds and empty river channels point to a warmer, 3 00:00:09.683 --> 00:00:12.900 wetter past maintained by a thicker atmosphere. 4 00:00:13.583 --> 00:00:15.533 Where did the ancient atmosphere go? 5 00:00:15.533 --> 00:00:18.500 And with it the water? 6 00:00:18.500 --> 00:00:21.233 To answer that question, NASA's MAVEN orbiter 7 00:00:21.233 --> 00:00:24.950 has been studying the upper atmosphere of Mars since 2014. 8 00:00:25.516 --> 00:00:27.916 Now, it has witnessed a rare phenomenon 9 00:00:27.983 --> 00:00:30.983 that was last seen more than two decades ago at Earth. 10 00:00:32.216 --> 00:00:36.750 Among MAVEN’s suite of science instruments is the Solar Wind Ion Analyzer, 11 00:00:36.750 --> 00:00:41.366 which measures electrically charged particles or ions surrounding Mars. 12 00:00:42.800 --> 00:00:46.283 In this data visualization, yellow spikes indicate the velocity 13 00:00:46.283 --> 00:00:50.483 of charged particles encountered by MAVEN along one of its orbital tracks. 14 00:00:51.233 --> 00:00:55.133 The largest source of charged particles in the solar system is the Sun, 15 00:00:55.200 --> 00:00:59.866 which constantly bombards the planets with a stream of electrons and hydrogen ions. 16 00:01:00.616 --> 00:01:03.533 When this solar wind reaches Mars, it interacts 17 00:01:03.533 --> 00:01:06.316 with heavier ions in the planet's upper atmosphere. 18 00:01:06.716 --> 00:01:10.166 This creates a global magnetic field, or magnetosphere, 19 00:01:10.166 --> 00:01:13.400 that deflects the solar wind around Mars in a bow shock. 20 00:01:13.483 --> 00:01:18.800 MAVEN’s science orbit is designed to probe these distinct regions in situ. 21 00:01:19.350 --> 00:01:23.633 With each pass, it crosses through the magnetosphere, bow shock, and upstream 22 00:01:23.633 --> 00:01:28.166 solar wind, measuring changes in ion velocity and density along the way. 23 00:01:28.883 --> 00:01:31.766 On December 25th, 2022, MAVEN 24 00:01:31.766 --> 00:01:35.633 encountered a sudden and dramatic decrease in solar wind density. 25 00:01:35.633 --> 00:01:39.600 As the pressure of the solar wind dropped, the Martian magnetosphere 26 00:01:39.600 --> 00:01:43.383 and bow shock ballooned outward, engulfing MAVEN's orbit. 27 00:01:43.383 --> 00:01:46.516 From the spacecraft's perspective, shielded beneath 28 00:01:46.516 --> 00:01:49.800 the bow shock, the solar wind had disappeared. 29 00:01:49.800 --> 00:01:55.716 In 1999, NASA's ACE satellite observed the same phenomenon at Earth. 30 00:01:55.800 --> 00:02:00.300 The solar wind density dropped by more than 98%, causing our planet's 31 00:02:00.300 --> 00:02:04.250 magnetosphere to expand to over five times its normal size. 32 00:02:05.066 --> 00:02:08.266 These rare events occur when a fast-moving region of the solar 33 00:02:08.266 --> 00:02:13.350 wind overtakes a slower moving region, leaving a low-density void in its wake. 34 00:02:13.350 --> 00:02:16.566 As quickly as the solar wind had disappeared from Mars, 35 00:02:16.583 --> 00:02:20.750 it returned on December 27th and squeezed the magnetosphere and the bow 36 00:02:20.766 --> 00:02:23.033 shock back to their usual proportions. 37 00:02:23.116 --> 00:02:28.166 MAVEN could once again feel the solar wind blowing across its instruments, 38 00:02:28.433 --> 00:02:31.916 and it could continue to study how Mars had evolved from a wet, 39 00:02:32.116 --> 00:02:36.016 hospitable planet into the cold, dry world we see today. 40 00:02:36.016 --> 00:02:45.666 [Music]