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]