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