1 00:00:00,010 --> 00:00:04,050 [ Kathleen McIntyre ] The GOES satellites are really a national treasure. 2 00:00:04,070 --> 00:00:08,110 [ Andre Dress ] These satellites are providing a huge service and they provide the safety net 3 00:00:08,130 --> 00:00:12,140 for people so that they get out of harms way. When I think of GOES, 4 00:00:12,160 --> 00:00:14,210 it’s not just a weather satellite. 5 00:00:14,230 --> 00:00:18,260 [ Dr. Howard J. Singer ] The GOES satellites provide us very critical data for space weather. 6 00:00:18,280 --> 00:00:22,300 [ Paul Richards ] That’s very critical and very important for astronauts because 7 00:00:22,320 --> 00:00:26,340 we are not protected from Earth’s atmosphere from the space weather. 8 00:00:26,360 --> 00:00:28,400 [ Andre Dress ] One of the big things is Search and Rescue. 9 00:00:28,420 --> 00:00:32,450 [ Mickey Fitzmaurice ] The GOES satellites save lives not just through search and rescue 10 00:00:32,470 --> 00:00:38,540 distress alert but with real-time monitoring of severe weather events. 11 00:00:38,560 --> 00:00:46,560 [ dramatic music ] 12 00:00:46,580 --> 00:00:48,600 [ Andre Dress ] Well, GOES-P is the last in the series. 13 00:00:48,620 --> 00:00:52,640 [ Kathleen McIntyre ] We want to make sure that we have the capability on orbit 14 00:00:52,660 --> 00:00:55,660 for continuous weather monitoring for this country. 15 00:00:55,680 --> 00:00:58,720 [ Andre Dress ] So GOES-P will be important to be a spare satellite. 16 00:01:00,830 --> 00:01:04,870 [ Kathleen McIntyre ] The first GOES satellite was launched in 1975 17 00:01:04,890 --> 00:01:08,930 and it was called GOES-A. It was the first time we actually saw an image 18 00:01:08,950 --> 00:01:11,960 of what the weather was creating on Earth. 19 00:01:11,980 --> 00:01:16,000 [ Andre Dress ] They were satellites we called spinners. The instrument that was on it actually rotated 20 00:01:16,020 --> 00:01:21,020 with the satellite so it took a long time to actually get the images from the Earth. 21 00:01:22,070 --> 00:01:26,070 [ Tom Fields ] The next generation, which was the previous one to the current generation, I through M, 22 00:01:26,090 --> 00:01:30,090 was the first series that was 3-axis stabilized, which meant it actually 23 00:01:30,110 --> 00:01:35,100 sat and pointed at the Earth as supposed to spinning and having to take images while it’s spinning. 24 00:01:35,120 --> 00:01:37,130 [ Kathleen McIntyre ] So we were able to continuously monitor weather. 25 00:01:40,160 --> 00:01:41,160 [ music ] 26 00:01:41,180 --> 00:01:45,170 [ Andre Dress ] We jumped to a 3-axis stabilized spacecraft. 27 00:01:45,190 --> 00:01:48,220 [ Mickey Fitzmaurice ] The next generation is always better than the previous generation. 28 00:01:48,240 --> 00:01:50,220 GOES-P will be the best of the lot. 29 00:01:50,240 --> 00:01:54,290 [ Andre Dress ] The spacecraft has the ability to be very very stable. 30 00:01:54,310 --> 00:01:56,320 [ Tom Fields ] Our images; our data is used real-time. 31 00:01:56,340 --> 00:02:00,340 Real-time we have to be able to calibrate and know that when we look at that . 32 00:02:00,360 --> 00:02:03,390 image, where exactly is that point on the Earth’s surface. 33 00:02:03,410 --> 00:02:07,450 [ Andre Dress ] When we have a huge hurricane, we want to have an accurate prediction. If it’s off by 34 00:02:07,470 --> 00:02:11,480 kilometers or miles, you’ve got people in harms way that you 35 00:02:11,500 --> 00:02:13,530 didn’t think were going to be in harms way. 36 00:02:13,550 --> 00:02:17,560 [ Jolyn Russell ] So when the spacecraft is sitting in space, it’s looking down at the Earth and it stays 37 00:02:17,580 --> 00:02:21,590 stationary like this but this solar array out here moves and tracks 38 00:02:21,610 --> 00:02:26,620 the sun so that way it’s always looking at the sun and can take a scan every minute. 39 00:02:26,640 --> 00:02:30,630 [ Paul Richards ] Different phenomenon from the sun is constantly 40 00:02:30,650 --> 00:02:34,750 bombarding the Earth. Although you might not know it, the solar weather affects you 41 00:02:34,770 --> 00:02:39,820 every day down here as well, not only just astronauts, it affects people on Earth. 42 00:02:39,840 --> 00:02:44,880 [ Janet Green ] Space weather can affect the power grid. It can affect communication with planes, it can cause errors 43 00:02:44,900 --> 00:02:47,920 in GPS, it can damage satellites. 44 00:02:47,940 --> 00:02:51,960 [ Dr. Howard J. Singer ] That whole series of satellites, GOES N-O-P, 45 00:02:51,980 --> 00:02:56,000 has some new capabilities for us in space weather. This is data that arrives 46 00:02:56,020 --> 00:03:00,060 almost instantaneously and therefore allows us 47 00:03:00,080 --> 00:03:03,120 to provide very timely alerts and warnings. 48 00:03:03,140 --> 00:03:07,160 [ Mickey Fitzmaurice ] The search and rescue system is another valuable tool for these satellites. 49 00:03:07,180 --> 00:03:11,180 In many cases one or two bursts from a beacon 50 00:03:11,200 --> 00:03:13,210 saves a person’s life. 51 00:03:13,230 --> 00:03:17,250 [ Paul Richards ] GOES satellites are operational satellites, meaning 52 00:03:17,270 --> 00:03:21,260 they are not experimental, they are constantly up there so it is 53 00:03:21,280 --> 00:03:25,280 constantly giving us data with no gaps in 54 00:03:25,300 --> 00:03:27,330 the data coming to us. 55 00:03:27,350 --> 00:03:29,430 [ Andre Dress ] In the future, we are going to get better resolution 56 00:03:29,450 --> 00:03:31,470 and not only that but faster images. 57 00:03:31,490 --> 00:03:36,510 We can start getting images on the order of 5 minutes as supposed to 26 minutes it takes