1 00:00:00,000 --> 00:00:00,734 [Music Plays] 2 00:00:00,734 --> 00:00:24,124 ERIN: Hi, Facebook. 3 00:00:24,124 --> 00:00:26,226 We're live from NASA Goddard's Space Flight Center. 4 00:00:26,226 --> 00:00:31,531 I'm Erin Kisliuk and you are live in 360 at the Hubble 5 00:00:31,531 --> 00:00:34,835 Space Telescope Operations Control Center. 6 00:00:34,835 --> 00:00:35,669 Take a look around. 7 00:00:35,669 --> 00:00:38,906 This place is the heart, soul, and the brains of the Hubble 8 00:00:38,906 --> 00:00:43,243 Space Telescope who launched 28 years ago today. 9 00:00:43,243 --> 00:00:47,080 Speaking of brains, we've got a couple of pretty smart 10 00:00:47,080 --> 00:00:50,250 folks here to answer your questions so send them all in to 11 00:00:50,250 --> 00:00:53,854 the comments section below so we can answer them during the show 12 00:00:53,854 --> 00:00:55,856 and even a few after it's ended. 13 00:00:55,856 --> 00:00:59,927 So without further ado, we've got Deputy Project Manager 14 00:00:59,927 --> 00:01:00,527 Jim Jeletic. 15 00:01:00,527 --> 00:01:01,595 JIM: Hi, Erin. 16 00:01:01,595 --> 00:01:02,529 ERIN: Hey, Jim. 17 00:01:02,529 --> 00:01:03,697 Thanks so much for being here. 18 00:01:03,697 --> 00:01:04,965 JIM: Thanks for having me. 19 00:01:04,965 --> 00:01:08,702 ERIN: So, Hubble is such an iconic, iconic mission 20 00:01:08,702 --> 00:01:10,304 but it's not so young anymore. 21 00:01:10,304 --> 00:01:11,004 How's Hubble doing? 22 00:01:11,004 --> 00:01:13,774 (1:09) JIM: Well, science-wise it is at the peak of its 23 00:01:13,774 --> 00:01:15,042 scientific capability. 24 00:01:15,042 --> 00:01:15,909 It's been doing great. 25 00:01:15,909 --> 00:01:19,279 In fact, this year we had more papers published on its 26 00:01:19,279 --> 00:01:21,882 discoveries than ever in its 28 year history. 27 00:01:21,882 --> 00:01:24,184 And as far as the spacecraft is concerned, you 28 00:01:24,184 --> 00:01:26,553 know, even with all those parts that are on it that have been 29 00:01:26,553 --> 00:01:30,590 flying in the harsh environment of space for 28 years, we still 30 00:01:30,590 --> 00:01:32,659 have redundancy in all of its critical systems. 31 00:01:32,659 --> 00:01:35,128 We're hopeful that we can continue to make these 32 00:01:35,128 --> 00:01:38,298 groundbreaking observations well into the next decade. 33 00:01:38,298 --> 00:01:39,800 ERIN: Into the next decade? 34 00:01:39,800 --> 00:01:44,004 So, when Hubble was launched it had a life expectancy of about 35 00:01:44,004 --> 00:01:45,339 15 years. 36 00:01:45,339 --> 00:01:47,074 How have we managed to double that? 37 00:01:47,074 --> 00:01:51,044 JIM: Well, you know we had 5 servicing missions that we 38 00:01:51,044 --> 00:01:53,680 went went up on a space shuttle with astronauts and they 39 00:01:53,680 --> 00:01:57,651 repaired, replaced, and upgraded its hardware over time. 40 00:01:57,651 --> 00:02:00,220 And it's kinda like your cell phone you know when you get a 41 00:02:00,220 --> 00:02:02,956 new cell phone you get a better camera on it a higher 42 00:02:02,956 --> 00:02:05,525 resolution, you can take even better pictures. 43 00:02:05,525 --> 00:02:07,461 Well, we did that with the instruments on Hubble. 44 00:02:07,461 --> 00:02:11,331 Because of that it's at its peak of its capability and we're 45 00:02:11,331 --> 00:02:13,834 hopeful that we can continually change our fundamental 46 00:02:13,834 --> 00:02:15,836 understanding of the universe for years to come with it. 47 00:02:15,836 --> 00:02:17,304 ERIN: That sounds great. 48 00:02:17,304 --> 00:02:19,606 I just want to remind anyone just tuning in that we are at 49 00:02:19,606 --> 00:02:22,175 NASA Goddard's Space Flight Center in Hubble Space 50 00:02:22,175 --> 00:02:24,011 Telescope's Operations Control Center. 51 00:02:24,011 --> 00:02:26,980 We're in 360 so take a look around while I introduce our 52 00:02:26,980 --> 00:02:29,850 next guest we have Senior Project Scientist 53 00:02:29,850 --> 00:02:31,284 Jennifer Wiseman joining us today. 54 00:02:31,284 --> 00:02:31,952 Hi! 55 00:02:31,952 --> 00:02:32,619 JENNIFER: Hi, Erin. 56 00:02:32,619 --> 00:02:34,421 ERIN: Thank you so much for being here. 57 00:02:34,421 --> 00:02:35,155 JENNIFER: My pleasure. 58 00:02:35,155 --> 00:02:39,259 ERIN: You've been on this mission for about 11 years. 59 00:02:39,259 --> 00:02:42,462 Does Hubble still do anything or show you anything that surprises 60 00:02:42,462 --> 00:02:43,130 you? 61 00:02:43,130 --> 00:02:46,066 JENNIFER: Oh my goodness, every year Hubble 62 00:02:46,066 --> 00:02:46,733 is surprising us. 63 00:02:46,733 --> 00:02:49,669 We're looking at things with Hubble now that we didn't even 64 00:02:49,669 --> 00:02:52,139 imagine that we would be observing when it was launched 65 00:02:52,139 --> 00:02:53,407 back in 1990. 66 00:02:53,407 --> 00:02:56,343 For example, we are studying the atmospheres of 67 00:02:56,343 --> 00:03:01,581 planets outside our solar system and we recently observed light 68 00:03:01,581 --> 00:03:04,718 coming from a merger of neutron stars. 69 00:03:04,718 --> 00:03:08,522 This event also created gravitational waves and these 70 00:03:08,522 --> 00:03:11,358 are the kind of phenomena we didn't even imagine decades 71 00:03:11,358 --> 00:03:11,525 ago. 72 00:03:11,558 --> 00:03:12,893 ERIN: That's amazing. 73 00:03:12,893 --> 00:03:16,763 And I hear Hubble sent us something amazing for its own 74 00:03:16,763 --> 00:03:17,664 anniversary. 75 00:03:17,664 --> 00:03:19,332 Can we talk about this image here? 76 00:03:19,332 --> 00:03:22,436 JENNIFER: We have this great image of the 77 00:03:22,436 --> 00:03:23,103 Lagoon Nebula. 78 00:03:23,103 --> 00:03:28,642 So this is a region of gas and dust that's being churned up by 79 00:03:28,642 --> 00:03:30,510 star formation. 80 00:03:30,510 --> 00:03:35,849 You can see a lot of features like pillars and clumps of gas. 81 00:03:35,849 --> 00:03:39,419 It's lit up because one of the stars that has recently formed 82 00:03:39,419 --> 00:03:40,954 is a monster star. 83 00:03:40,954 --> 00:03:43,590 It's about 200 thousand times brighter than our sun. 84 00:03:43,590 --> 00:03:48,061 And it's ionizing the gas, it's creating these structures, its 85 00:03:48,061 --> 00:03:52,566 winds and radiation are carving out these various pillars and 86 00:03:52,566 --> 00:03:56,069 globules and so we like to think of this as kind of a 87 00:03:56,069 --> 00:03:56,736 stellar nursery. 88 00:03:56,736 --> 00:03:58,305 ERIN: That's amazing. 89 00:03:58,305 --> 00:04:01,775 So are these two different like parts of the nebula? 90 00:04:01,775 --> 00:04:02,909 Why do they look so different? 91 00:04:02,909 --> 00:04:05,278 JENNIFER: So you see two images here, but they are 92 00:04:05,278 --> 00:04:06,980 actually the same place. 93 00:04:06,980 --> 00:04:11,318 They are both the same region of the Lagoon Nebula, but they are 94 00:04:11,318 --> 00:04:14,721 looking at it with different kinds of light so Hubble can see 95 00:04:14,721 --> 00:04:17,491 both visible light like our eyes can see and that's what we can 96 00:04:17,491 --> 00:04:21,661 see here on the left and also infrared light which is what you 97 00:04:21,661 --> 00:04:23,163 see here on the right. 98 00:04:23,163 --> 00:04:26,266 And so infrared light we can actually see through a lot of 99 00:04:26,266 --> 00:04:30,604 the dusty veil in front of and within the nebula. 100 00:04:30,604 --> 00:04:35,208 You can see a lot of stars behind it you can see 101 00:04:35,208 --> 00:04:36,943 some stars within the nebula. 102 00:04:36,943 --> 00:04:39,379 And you can see these very dark globules where new smaller stars 103 00:04:39,379 --> 00:04:42,916 are still incubating so it's wonderful to have Hubble's 104 00:04:42,916 --> 00:04:45,652 panchromatic view of all these different colors. 105 00:04:45,652 --> 00:04:47,287 It gives us different information. 106 00:04:47,287 --> 00:04:48,155 ERIN: That's amazing. 107 00:04:48,155 --> 00:04:50,123 And so how far away about is this? 108 00:04:50,123 --> 00:04:55,295 JENNIFER: So the nebula is about 4,000 lightyears away, that's a 109 00:04:55,295 --> 00:04:58,031 unit of distance that we use that basically means that the 110 00:04:58,031 --> 00:05:01,401 light started its journey to us about 4,000 years ago. 111 00:05:01,401 --> 00:05:03,737 Think about what was happening on Earth at that time and that's 112 00:05:03,737 --> 00:05:05,472 when the light started traveling to us. 113 00:05:05,472 --> 00:05:08,708 ERIN: That is extremely impressive. 114 00:05:08,708 --> 00:05:11,545 For our viewers at home we are at NASA Goddard Space Flight 115 00:05:11,545 --> 00:05:14,514 Center inside the Hubble Space Telescope Operations Control 116 00:05:14,514 --> 00:05:18,151 Center and now I'm going to jump over and ask someone really cool 117 00:05:18,151 --> 00:05:19,986 to speak with me if he has a second. 118 00:05:19,986 --> 00:05:22,255 We've got systems engineer Mike Wenz. 119 00:05:22,255 --> 00:05:23,123 Hi. 120 00:05:23,123 --> 00:05:24,624 Thank you so much for being here. 121 00:05:24,624 --> 00:05:26,560 MIKE: Hi, Erin. 122 00:05:26,560 --> 00:05:28,328 You are perfectly welcome. 123 00:05:28,328 --> 00:05:30,063 ERIN: So can you tell us a little bit about what goes on in 124 00:05:30,063 --> 00:05:30,764 this room? 125 00:05:30,764 --> 00:05:32,098 MIKE: Yeah, this is actually the room where we 126 00:05:32,098 --> 00:05:33,433 control the Hubble Space Telescope. 127 00:05:33,433 --> 00:05:35,936 We'll send commands up to it and we'll also receive telemetry 128 00:05:35,936 --> 00:05:38,305 down from it so we can actually see how the instruments are 129 00:05:38,305 --> 00:05:40,407 doing and how the telescope is doing. 130 00:05:40,407 --> 00:05:44,010 In this room right here, this is where the systems engineers will 131 00:05:44,010 --> 00:05:46,079 work for various circumstances. 132 00:05:46,079 --> 00:05:48,582 This is actually where we did support the servicing missions 133 00:05:48,582 --> 00:05:51,251 that Jim talked about where we were replacing the instruments 134 00:05:51,251 --> 00:05:54,421 on Hubble that was a lot of fun working with the astronauts. 135 00:05:54,421 --> 00:05:57,557 But we use this room now mainly for two reasons one of 136 00:05:57,557 --> 00:06:00,293 them is if we have some sort of anomaly on the spacecraft which 137 00:06:00,293 --> 00:06:02,229 is when the spacecraft does something we weren't quite 138 00:06:02,229 --> 00:06:05,732 expecting and so the system engineers here try to figure out 139 00:06:05,732 --> 00:06:08,835 what's going on and why it happened and what can we do to 140 00:06:08,835 --> 00:06:10,570 make it not happen again. 141 00:06:10,570 --> 00:06:13,106 We also use this room for testing if we are going to be 142 00:06:13,106 --> 00:06:16,276 sending up new software to the instruments or new software to 143 00:06:16,276 --> 00:06:16,943 the telescope. 144 00:06:16,943 --> 00:06:19,346 We gotta make sure we test it out on the ground beforehand 145 00:06:19,346 --> 00:06:21,314 because you don't want to be testing it out 146 00:06:21,314 --> 00:06:21,982 on the spacecraft itself. 147 00:06:21,982 --> 00:06:25,318 ERIN: Ok, so trick question! 148 00:06:25,318 --> 00:06:29,923 What is something that Hubble do that would fall under that 149 00:06:29,923 --> 00:06:31,191 unexpected category? 150 00:06:31,191 --> 00:06:35,295 MIKE: One of the small anomalies that we have fairly 151 00:06:35,295 --> 00:06:38,231 recently that we have once, maybe even twice a week is there 152 00:06:38,231 --> 00:06:40,700 is instruments on the Hubble that allow us to point the 153 00:06:40,700 --> 00:06:42,002 telescope very accurately. 154 00:06:42,002 --> 00:06:45,405 To be able to take the images that Jennifer was talking about 155 00:06:45,405 --> 00:06:48,341 have to be able to point and hold the telescope extremely 156 00:06:48,341 --> 00:06:50,810 accurately in fact we have to able to focus on essentially on 157 00:06:50,810 --> 00:06:53,546 the width of a human hair held at one mile distance. 158 00:06:53,546 --> 00:06:56,483 To be able to do that is instruments that we have fine 159 00:06:56,483 --> 00:06:57,817 guidance sensors. 160 00:06:57,817 --> 00:06:59,219 They lock up on stars. 161 00:06:59,219 --> 00:07:01,588 They actually find the stars and they lock and they hold it. 162 00:07:01,588 --> 00:07:04,391 But every once in a while they'll try to lock up on a star 163 00:07:04,391 --> 00:07:07,427 and they can't do it and they send information 164 00:07:07,427 --> 00:07:08,094 down saying we can't do it. 165 00:07:08,094 --> 00:07:12,932 So we have to come in here and we find that they are actually 166 00:07:12,932 --> 00:07:17,270 lock up on single stars and that they aren't single stars but we 167 00:07:17,270 --> 00:07:18,705 don't know about it on the ground yet. 168 00:07:18,705 --> 00:07:21,574 No one on the ground can tell that these are double stars or 169 00:07:21,574 --> 00:07:24,277 binary stars and Hubble makes these discoveries when it 170 00:07:24,277 --> 00:07:25,912 actually has these anomalies. 171 00:07:25,912 --> 00:07:29,049 ERIN: That's quite the silver lining. 172 00:07:29,049 --> 00:07:29,949 So how about you? 173 00:07:29,949 --> 00:07:31,384 What is your role? 174 00:07:31,384 --> 00:07:32,752 How long have you been working with Hubble? 175 00:07:32,752 --> 00:07:34,254 MIKE: I'm a systems engineer here. 176 00:07:34,254 --> 00:07:36,256 I've actually been on Hubble for 26 years. 177 00:07:36,256 --> 00:07:39,592 I'm one of the older guys around who've been 178 00:07:39,592 --> 00:07:40,493 around here for a lot of it. 179 00:07:40,493 --> 00:07:43,697 I'm actually in charge of those fine guidance sensors and those 180 00:07:43,697 --> 00:07:46,833 are actually the instruments that I have to take care of. 181 00:07:46,833 --> 00:07:48,902 I actually am the one who gets to come in here and find all the 182 00:07:48,902 --> 00:07:51,037 double stars and variable stars that Hubble has found because 183 00:07:51,037 --> 00:07:51,705 it's had trouble. 184 00:07:51,705 --> 00:07:53,540 ERIN: That's an amazing job. 185 00:07:53,540 --> 00:07:54,808 I'll let you get back to work. 186 00:07:54,808 --> 00:07:56,142 Thank you so much for your time. 187 00:07:56,142 --> 00:07:56,810 MIKE: Thank you. 188 00:07:56,810 --> 00:07:58,511 ERIN: Alright, so we are going to start taking some of 189 00:07:58,511 --> 00:07:59,479 your questions. 190 00:07:59,479 --> 00:08:00,647 Continue to send them in. 191 00:08:00,647 --> 00:08:04,084 We're going to be taking them here and also after the show is 192 00:08:04,084 --> 00:08:06,453 over we'll be answering them in the comments section below. 193 00:08:06,453 --> 00:08:09,322 Let's see what we've got here. 194 00:08:09,322 --> 00:08:13,693 So Tia from Twitter asks: how do you deal with damages made by 195 00:08:13,693 --> 00:08:17,063 impacts from space objects on Hubble? 196 00:08:17,063 --> 00:08:18,398 That's an interesting one, do you want to take that one Jim? 197 00:08:18,398 --> 00:08:19,065 JIM: Sure. 198 00:08:19,065 --> 00:08:20,400 It's a great question we actually look for major impacts 199 00:08:20,400 --> 00:08:21,768 so that we can actually turn the telescope to be as small of 200 00:08:21,768 --> 00:08:23,103 surface area as possible so they'll avoid us if we know 201 00:08:23,103 --> 00:08:24,437 one's coming or if it's big enough. 202 00:08:24,437 --> 00:08:25,772 But for the most part it gets hit and so far I think we've 203 00:08:25,772 --> 00:08:27,107 been really lucky in that nothing has hit us that has 204 00:08:27,107 --> 00:08:28,441 caused anything really to break. 205 00:08:28,441 --> 00:08:29,809 We are going to keep our fingers crossed here for the next 206 00:08:29,809 --> 00:08:30,477 however many years. 207 00:08:30,477 --> 00:08:31,144 ERIN: Long live Hubble. 208 00:08:31,144 --> 00:08:32,479 Alright, so Dan asks: what's the furthest point in lightyears 209 00:08:32,479 --> 00:08:33,146 that Hubble has seen? 210 00:08:33,146 --> 00:08:34,481 I'll leave that to you, Jennifer. 211 00:08:34,481 --> 00:08:35,849 JENNIFER: That's a very good question, so we're trying 212 00:08:35,849 --> 00:08:40,854 to see objects in space farther and farther out, the cameras on 213 00:08:43,056 --> 00:08:49,362 Hubble have improved over the years because of these astronaut 214 00:08:49,362 --> 00:08:54,367 servicing missions we've had more sensitivities. 215 00:09:14,587 --> 00:09:18,925 So right now we're seeing emission in galaxies in the very 216 00:09:18,925 --> 00:09:25,765 distant universe that are in the process of forming more than 13 217 00:09:25,765 --> 00:09:27,033 billion lightyears away. 218 00:09:27,033 --> 00:09:30,837 So we know the universe seems to be about 13.8 billion 219 00:09:30,837 --> 00:09:36,176 years old and we're seeing these baby galaxies form within the 220 00:09:36,176 --> 00:09:39,479 first point eight of these 13.8 billion years in fact within the 221 00:09:39,479 --> 00:09:42,315 first few hundred million years we are seeing these infant 222 00:09:42,315 --> 00:09:44,084 galaxies start to form. 223 00:09:44,084 --> 00:09:47,086 And the upcoming James Webb Space Telescope will be able to 224 00:09:47,086 --> 00:09:50,623 see even farther because it has infrared capabilities and will 225 00:09:50,623 --> 00:09:54,360 be able to see even farther back into time as light travels 226 00:09:54,360 --> 00:09:57,397 through this expanding universe and gets stretched into redder 227 00:09:57,397 --> 00:09:58,898 and redder wavelengths of light. 228 00:09:58,898 --> 00:10:00,133 ERIN: Thanks. 229 00:10:00,133 --> 00:10:02,469 Alright, let's see what we've got next. 230 00:10:02,469 --> 00:10:06,739 On that same note, what has Hubble found out about the 231 00:10:06,739 --> 00:10:08,274 beginning of the universe? 232 00:10:08,274 --> 00:10:11,878 JENNIFER: Well, Hubble cannot see all the way back to 233 00:10:11,878 --> 00:10:13,046 the beginning. 234 00:10:13,046 --> 00:10:18,151 There's a time before radiation could even escape for us to see. 235 00:10:18,151 --> 00:10:19,853 But we are able to see pretty close. 236 00:10:19,853 --> 00:10:24,190 Like I said, the first point eight of the 13.8 billion year 237 00:10:24,190 --> 00:10:27,894 history of the universe and what we've learned is that galaxies 238 00:10:27,894 --> 00:10:29,863 formed early on. 239 00:10:29,863 --> 00:10:33,333 Galaxies are collections of stars and gas and dark matter. 240 00:10:33,333 --> 00:10:37,537 Stars formed early on these gravitational collections 241 00:10:37,537 --> 00:10:41,407 of material grew over time and we can now see with Hubble by 242 00:10:41,407 --> 00:10:46,179 looking far out in space, which means looking back in time, that 243 00:10:46,179 --> 00:10:49,482 galaxies were once quite small and and irregular looking and 244 00:10:49,482 --> 00:10:53,553 they merged together many times to grow into the bigger type 245 00:10:53,553 --> 00:10:55,522 galaxies like the Milky Way. 246 00:10:55,522 --> 00:10:58,658 So we've been able to see with Hubble that galaxies began 247 00:10:58,658 --> 00:11:03,096 small, they grew over time, and now we have the privilege of 248 00:11:03,096 --> 00:11:08,434 several generations of stars, massive stars, that come and go 249 00:11:08,434 --> 00:11:11,671 and that gives us heavier elements like carbon and oxygen 250 00:11:11,671 --> 00:11:13,840 things we need for planets and life. 251 00:11:13,840 --> 00:11:15,842 ERIN: Thank you so much. 252 00:11:15,842 --> 00:11:18,678 Unfortunately, I think we're going to have to get out of here 253 00:11:18,678 --> 00:11:20,246 and let these folks get back to work. 254 00:11:20,246 --> 00:11:22,815 But I want to thank you all for joining us and please continue 255 00:11:22,815 --> 00:11:23,816 to send in your questions. 256 00:11:23,816 --> 00:11:26,386 We'll get to some of them in the comments section below. 257 00:11:26,386 --> 00:11:28,888 Take one last look at the room around us before you leave and 258 00:11:28,888 --> 00:11:31,257 if you want to know anything more about Hubble you can always 259 00:11:31,257 --> 00:11:35,695 find on nasa.gov/hubble or NASA Social Media @NASAHubble. 260 00:11:35,695 --> 00:11:37,063 Thank you both so much for being here. 261 00:11:37,063 --> 00:11:42,068 Let's get on out of here. 262 00:11:47,674 --> 00:11:52,845 Thanks, Mike! 263 00:11:52,845 --> 00:11:57,850 [Music Fades]