WEBVTT FILE 1 00:00:00.600 --> 00:00:03.020 Floating hundreds of miles from Earth, 2 00:00:03.040 --> 00:00:05.820 astronauts get a unique perspective of our planet. 3 00:00:05.840 --> 00:00:07.960 While they might recognize landmarks, 4 00:00:07.980 --> 00:00:13.110 space is the only place they can see the very edge of our planet’s atmosphere. 5 00:00:13.130 --> 00:00:14.950 From orbit particularly looking at the horizon, 6 00:00:14.970 --> 00:00:18.110 did bring to mind how thin the atmosphere is. 7 00:00:18.130 --> 00:00:21.510 It's like an onionskin around this great big ball of the earth. 8 00:00:21.530 --> 00:00:24.190 This uppermost layer of Earth’s atmosphere, 9 00:00:24.210 --> 00:00:28.830 the ionosphere, also overlaps with the very beginning of space. 10 00:00:28.850 --> 00:00:31.070 It’s the job of NASA’s new mission, GOLD - 11 00:00:31.090 --> 00:00:34.280 the Global-scale Observations of the Limb and Disk instrument - 12 00:00:34.300 --> 00:00:36.210 to study this region -- 13 00:00:36.230 --> 00:00:39.300 a region that isn’t just for astronauts to explore, 14 00:00:39.320 --> 00:00:42.800 but that affects humans every day down on the ground. 15 00:00:42.820 --> 00:00:46.390 For one thing, this layer of the upper atmosphere helps protect us 16 00:00:46.410 --> 00:00:50.420 from harmful radiation and energy emanating from the Sun. 17 00:00:50.440 --> 00:00:53.180 But in our modern society, it does so much more. 18 00:00:53.200 --> 00:00:55.630 It affects the smartphone that sits in your pocket 19 00:00:55.650 --> 00:00:59.170 and the radio waves that guide our airplanes. 20 00:00:59.190 --> 00:01:02.080 The ionosphere is a crucial layer of the atmosphere 21 00:01:02.100 --> 00:01:05.570 through which our communications and GPS signals travel. 22 00:01:05.590 --> 00:01:10.530 And when this region changes, it impacts those communications signals. 23 00:01:10.550 --> 00:01:14.430 Changes can occur above this region from the Sun’s activity, 24 00:01:14.450 --> 00:01:16.420 also known as space weather. 25 00:01:16.440 --> 00:01:22.080 Changes can also occur below from Earth’s weather such as hurricanes and wind patterns. 26 00:01:22.100 --> 00:01:26.350 GOLD connects the dots between how space weather and Earth’s weather 27 00:01:26.370 --> 00:01:28.780 shape the upper reaches of the atmosphere. 28 00:01:28.800 --> 00:01:31.030 But this region isn’t easy to study. 29 00:01:31.050 --> 00:01:35.320 The ionosphere spans roughly 60 to 400 miles from Earth’s surface, 30 00:01:35.340 --> 00:01:38.550 which is too high for aircraft and scientific balloons 31 00:01:38.570 --> 00:01:42.780 and the lower regions are too low to easily study with satellites. 32 00:01:42.800 --> 00:01:44.520 What are attainable, however, 33 00:01:44.540 --> 00:01:49.030 are the swathes of red and green light shining out from the upper atmosphere. 34 00:01:49.050 --> 00:01:51.960 Formed when the Sun’s rays hit atmospheric molecules, 35 00:01:51.980 --> 00:01:56.440 this light named “airglow”, comes from green and red bands of glowing gas. 36 00:01:56.460 --> 00:01:59.000 Some of the airglow is invisible to our eyes, 37 00:01:59.020 --> 00:02:01.480 shining in infrared and ultraviolet light, 38 00:02:01.500 --> 00:02:04.810 which can only be seen with scientific instrumentation. 39 00:02:04.830 --> 00:02:09.250 Taking advantage of our planet’s natural glow is GOLD. 40 00:02:09.270 --> 00:02:12.120 The GOLD instrument, which is about the size of a mini fridge, 41 00:02:12.140 --> 00:02:16.350 is hitching a ride on a commercial communications satellite, SES-14. 42 00:02:16.370 --> 00:02:20.420 The satellite’s orbit lies 22,000 miles above Earth 43 00:02:20.440 --> 00:02:26.020 where it can record images in ultraviolet light to monitor changes in airglow across the globe. 44 00:02:26.040 --> 00:02:32.660 These images give information on the temperature, density, and composition of particles in the upper atmosphere. 45 00:02:32.680 --> 00:02:36.890 GOLD collects these observations faster than any mission has ever done before. 46 00:02:36.910 --> 00:02:40.920 It captures an image of Earth’s entire disk every 30 minutes, 47 00:02:40.940 --> 00:02:45.340 allowing scientists to see how the upper atmosphere evolves throughout the day. 48 00:02:45.360 --> 00:02:49.280 GOLD joins a host of missions studying the very nature of space -- 49 00:02:49.300 --> 00:02:52.130 around Earth, the Sun, and planets. 50 00:02:52.150 --> 00:02:55.020 As NASA ventures farther and farther from home, 51 00:02:55.040 --> 00:02:57.150 knowing the nature of space itself 52 00:02:57.170 --> 00:03:01.860 is crucial for our journey to understand our solar system -- and beyond. 53 00:03:01.880 --> 00:03:13.240