WEBVTT

1
00:00:03.399 --> 00:00:07.719
<v Speaker 1>Welcome to Bedtime Astronomy. Explore the wonders of the cosmos

2
00:00:07.759 --> 00:00:12.279
<v Speaker 1>with our soothing Bedtime Astronomie podcast. Each episode offers a

3
00:00:12.359 --> 00:00:16.320
<v Speaker 1>gentle journey through the stars, planets, and beyond, perfect for

4
00:00:16.399 --> 00:00:20.239
<v Speaker 1>unwinding after a long day. Let's travel through the mysteries

5
00:00:20.239 --> 00:00:22.440
<v Speaker 1>of the universe as you drift off into a peaceful

6
00:00:22.480 --> 00:00:26.879
<v Speaker 1>slumber under the night sky.

7
00:00:26.960 --> 00:00:29.640
<v Speaker 2>If you look up at the Little Dipper tonight, you

8
00:00:29.679 --> 00:00:32.840
<v Speaker 2>aren't just seeing a familiar pattern of stars, right.

9
00:00:32.840 --> 00:00:35.640
<v Speaker 3>It's so easy to just see it as this static,

10
00:00:36.520 --> 00:00:37.600
<v Speaker 3>you know, beautiful canopy.

11
00:00:37.759 --> 00:00:41.000
<v Speaker 2>Yeah exactly, But you are actually looking at the very

12
00:00:41.159 --> 00:00:44.359
<v Speaker 2>edge of the largest and honestly the most impossible map

13
00:00:44.479 --> 00:00:46.320
<v Speaker 2>ever constructed by human beings.

14
00:00:46.399 --> 00:00:48.799
<v Speaker 3>It really does shatter your entire sense of scale.

15
00:00:48.880 --> 00:00:51.960
<v Speaker 2>It does, because we're talking about a three dimensional model

16
00:00:52.000 --> 00:00:55.799
<v Speaker 2>of the universe that is so vast and like so

17
00:00:56.079 --> 00:00:59.000
<v Speaker 2>detailed that the data pouring out of it right now

18
00:00:59.079 --> 00:01:01.520
<v Speaker 2>might actually prove that the fundamental laws of physics are

19
00:01:01.600 --> 00:01:03.560
<v Speaker 2>actively changing right over our heads.

20
00:01:03.679 --> 00:01:07.159
<v Speaker 3>And that specific patch of the cosmos near the Little

21
00:01:07.159 --> 00:01:11.439
<v Speaker 3>Dipper that actually served as the final observation target for

22
00:01:11.560 --> 00:01:13.040
<v Speaker 3>this monumental.

23
00:01:12.480 --> 00:01:15.359
<v Speaker 2>Project, which is just wild. We are talking about mapping

24
00:01:15.400 --> 00:01:19.159
<v Speaker 2>structures that stretch across eleven billion years of history.

25
00:01:19.239 --> 00:01:22.480
<v Speaker 3>Eleven billion. Yes, it's a number that is almost impossible

26
00:01:22.959 --> 00:01:25.920
<v Speaker 3>for the human brain to truly internalize.

27
00:01:25.280 --> 00:01:27.079
<v Speaker 2>And to put that into context for you listening. We

28
00:01:27.120 --> 00:01:29.319
<v Speaker 2>aren't talking about a map that helps us, you know,

29
00:01:29.439 --> 00:01:32.040
<v Speaker 2>find nearby planets or plot a Corset alfasentory.

30
00:01:32.560 --> 00:01:34.439
<v Speaker 3>No, the scale is entirely different, right.

31
00:01:34.920 --> 00:01:39.480
<v Speaker 2>The Dark Energy Spectroscopic Instrument, or DAI as it's called,

32
00:01:40.000 --> 00:01:43.480
<v Speaker 2>has just wrapped up its primary run and it delivered

33
00:01:43.480 --> 00:01:46.760
<v Speaker 2>the highest resolution, most comprehensive three D map of the

34
00:01:46.840 --> 00:01:47.920
<v Speaker 2>universe in existence.

35
00:01:48.000 --> 00:01:51.439
<v Speaker 3>So the map itself, interestingly enough, is almost a byproduct.

36
00:01:51.959 --> 00:01:54.359
<v Speaker 2>Yeah, the map wasn't the actual goal.

37
00:01:54.280 --> 00:01:56.920
<v Speaker 3>Was it not at all. It's a tool built for

38
00:01:56.959 --> 00:02:02.159
<v Speaker 3>a very specific, incredibly high stakes. The goal was never

39
00:02:02.359 --> 00:02:05.159
<v Speaker 3>just cartography for the sake of having a nice atlas

40
00:02:05.159 --> 00:02:06.040
<v Speaker 3>of the cosmos.

41
00:02:06.200 --> 00:02:08.400
<v Speaker 2>So they didn't just want to hang a shiny map.

42
00:02:08.159 --> 00:02:11.960
<v Speaker 3>On the wall exactly. The purpose of mapping millions upon

43
00:02:12.080 --> 00:02:15.840
<v Speaker 3>millions of distant galaxies is to track down and understand

44
00:02:15.879 --> 00:02:16.439
<v Speaker 3>a phantom.

45
00:02:16.599 --> 00:02:18.159
<v Speaker 2>A phantom I love that description.

46
00:02:18.479 --> 00:02:22.199
<v Speaker 3>Well, we're dealing with dark energy, the invisible repulsive force

47
00:02:22.240 --> 00:02:24.599
<v Speaker 3>that currently makes up roughly seventy percent of everything in

48
00:02:24.639 --> 00:02:25.120
<v Speaker 3>the universe.

49
00:02:25.199 --> 00:02:28.599
<v Speaker 2>Seventy percent that is, I mean everything we can see, touch,

50
00:02:28.719 --> 00:02:31.439
<v Speaker 2>or interact with is basically a rounding error compared to

51
00:02:31.479 --> 00:02:31.960
<v Speaker 2>this force.

52
00:02:32.080 --> 00:02:33.439
<v Speaker 3>It's all just a tiny fraction of.

53
00:02:33.400 --> 00:02:37.280
<v Speaker 2>Reality, which sets the stakes at an existential level. If

54
00:02:37.400 --> 00:02:40.680
<v Speaker 2>seventy percent of reality is driven by something we can't see,

55
00:02:40.840 --> 00:02:43.719
<v Speaker 2>and this new map is suddenly suggesting that our basic

56
00:02:43.719 --> 00:02:46.800
<v Speaker 2>assumptions about how that force operates are wrong.

57
00:02:46.919 --> 00:02:48.800
<v Speaker 3>Then we're looking at a paradigm.

58
00:02:48.439 --> 00:02:51.800
<v Speaker 2>Shift, a total paradigm shift that rewrites the fate of

59
00:02:51.840 --> 00:02:55.479
<v Speaker 2>the universe. Okay, let's unpack this because before we get

60
00:02:55.520 --> 00:02:58.680
<v Speaker 2>to the physics breaking anomaly they found, I want to

61
00:02:58.719 --> 00:03:01.639
<v Speaker 2>ground this in the far physical reality of how you

62
00:03:01.719 --> 00:03:02.439
<v Speaker 2>even build a.

63
00:03:02.400 --> 00:03:06.039
<v Speaker 3>Map like this. The sheer engineering is staggering, it really is.

64
00:03:06.080 --> 00:03:08.719
<v Speaker 2>This entire operation is based in Arizona, right, Yeah.

65
00:03:08.520 --> 00:03:11.479
<v Speaker 3>At the kit Peak National Observatory, which is managed by

66
00:03:11.479 --> 00:03:14.759
<v Speaker 3>the US Department of Energies Lawrence Berkeley National Laboratory. Okay,

67
00:03:15.159 --> 00:03:17.919
<v Speaker 3>And it is vital to understand that DSi is not

68
00:03:18.120 --> 00:03:19.560
<v Speaker 3>a space telescope.

69
00:03:19.159 --> 00:03:22.400
<v Speaker 2>Oh right, because we always hear about James Web or

70
00:03:22.479 --> 00:03:23.479
<v Speaker 2>Hubble exactly.

71
00:03:23.639 --> 00:03:26.560
<v Speaker 3>It is not floating out in the vacuum, free from interference.

72
00:03:26.960 --> 00:03:30.639
<v Speaker 3>It is a ground based instrument retrofitted onto an existing

73
00:03:30.680 --> 00:03:32.479
<v Speaker 3>telescope structure on a mountain.

74
00:03:32.240 --> 00:03:35.919
<v Speaker 2>Peak, which makes it sound almost I don't know, quoint,

75
00:03:36.360 --> 00:03:38.159
<v Speaker 2>but the instrumentation is anything but quaint.

76
00:03:38.280 --> 00:03:40.000
<v Speaker 3>It's a marvel of modern engineering.

77
00:03:40.319 --> 00:03:42.400
<v Speaker 2>Because when I think of a telescope, I think of

78
00:03:43.120 --> 00:03:46.520
<v Speaker 2>like a giant mirror or a massive glass lens pointed

79
00:03:46.560 --> 00:03:47.639
<v Speaker 2>at a patch of sky.

80
00:03:47.879 --> 00:03:49.879
<v Speaker 3>Right, the traditional galileo setup.

81
00:03:50.000 --> 00:03:53.840
<v Speaker 2>Yeah, but the DSi instrument operates on a completely different

82
00:03:53.840 --> 00:03:57.960
<v Speaker 2>mechanical level. The focal plane is packed with five thousand

83
00:03:58.039 --> 00:03:59.960
<v Speaker 2>individual fiber optic sensors.

84
00:04:00.199 --> 00:04:02.319
<v Speaker 3>Let's examine the mechanics of that, because it is an

85
00:04:02.360 --> 00:04:05.360
<v Speaker 3>astonishing feat of miniaturization and robotics.

86
00:04:05.400 --> 00:04:07.199
<v Speaker 2>Please, because I can barely visualize it.

87
00:04:07.319 --> 00:04:10.680
<v Speaker 3>So you have a circular plane, and embedded into it

88
00:04:10.759 --> 00:04:14.599
<v Speaker 3>are these five thousand robotic positioners, Okay, and each one

89
00:04:14.639 --> 00:04:17.839
<v Speaker 3>holds a tiny fiber optic cable. In the space of

90
00:04:17.920 --> 00:04:21.680
<v Speaker 3>just a few seconds, all five thousand robots can simultaneously

91
00:04:21.720 --> 00:04:23.680
<v Speaker 3>pivot and adjust their positions.

92
00:04:23.319 --> 00:04:24.519
<v Speaker 2>Wait all at the same time.

93
00:04:24.600 --> 00:04:27.240
<v Speaker 3>All at the same time, they align perfectly with the

94
00:04:27.279 --> 00:04:32.160
<v Speaker 3>incoming light from five thousand completely different, highly specific distant galaxies.

95
00:04:32.199 --> 00:04:35.120
<v Speaker 2>That's insant. Wait, how do they move that fast without colliding?

96
00:04:35.279 --> 00:04:37.399
<v Speaker 2>That is a big question, because if you have five

97
00:04:37.399 --> 00:04:40.920
<v Speaker 2>thousand robotic arms packed onto a single plate, all swarming

98
00:04:41.000 --> 00:04:43.560
<v Speaker 2>to find new targets for the next exposure, I mean

99
00:04:43.560 --> 00:04:45.600
<v Speaker 2>the collision algorithms alone must be a nightmare.

100
00:04:45.720 --> 00:04:50.040
<v Speaker 3>The choreography is entirely automated and highly highly complex. They

101
00:04:50.079 --> 00:04:52.560
<v Speaker 3>operate in this tightly packed honeycomb structure.

102
00:04:52.680 --> 00:04:54.240
<v Speaker 2>Oh, a honeycomb, that makes sense.

103
00:04:54.360 --> 00:04:58.279
<v Speaker 3>Yeah, And the targeting software calculates the optimal orientation for

104
00:04:58.439 --> 00:05:02.240
<v Speaker 3>every single positioner. It maximizes the number of galaxies captured

105
00:05:02.279 --> 00:05:06.319
<v Speaker 3>in a single exposure without any fibers, crossing paths or jamming.

106
00:05:06.319 --> 00:05:06.480
<v Speaker 2>Oh.

107
00:05:07.079 --> 00:05:09.560
<v Speaker 3>Once they lock into place, they captured the light, feed

108
00:05:09.600 --> 00:05:12.920
<v Speaker 3>it down into the spectrographs, and then instantly realign for

109
00:05:12.959 --> 00:05:13.920
<v Speaker 3>the next patch of sky.

110
00:05:14.120 --> 00:05:17.399
<v Speaker 2>So it is just an absolute observing machine, completely relentless,

111
00:05:17.480 --> 00:05:20.160
<v Speaker 2>and the numbers back that up. When the projects spun

112
00:05:20.279 --> 00:05:22.959
<v Speaker 2>up in May of twenty twenty one, I read that

113
00:05:23.000 --> 00:05:25.920
<v Speaker 2>the stated goal was to capture light from about thirty

114
00:05:25.920 --> 00:05:29.120
<v Speaker 2>four million galaxies and quasars.

115
00:05:28.680 --> 00:05:30.160
<v Speaker 3>Which alone would have been historic.

116
00:05:30.360 --> 00:05:32.639
<v Speaker 2>Right, thirty four million is a massive number.

117
00:05:32.720 --> 00:05:35.800
<v Speaker 3>It would have completely redefined the field of cosmology, but.

118
00:05:35.759 --> 00:05:38.759
<v Speaker 2>The efficiency of the instrument and the clarity of those

119
00:05:38.800 --> 00:05:42.720
<v Speaker 2>targeting protocols allowed them to vastly outpace their own projection

120
00:05:42.879 --> 00:05:44.920
<v Speaker 2>by a huge market. Yeah, by the time they took

121
00:05:45.000 --> 00:05:48.120
<v Speaker 2>that final scheduled shot near the Little Dipper, they hadn't

122
00:05:48.160 --> 00:05:49.839
<v Speaker 2>just hit thirty four million.

123
00:05:49.800 --> 00:05:50.480
<v Speaker 3>Not even close.

124
00:05:50.600 --> 00:05:55.279
<v Speaker 2>They captured over forty seven million galaxies and quasars.

125
00:05:54.879 --> 00:05:58.800
<v Speaker 3>Plus another twenty million stars just for the sake of completeness, just.

126
00:05:58.800 --> 00:06:01.560
<v Speaker 2>Threw them in there. That is data set containing information

127
00:06:01.680 --> 00:06:05.120
<v Speaker 2>from six times as many galaxies and quasars as every

128
00:06:05.240 --> 00:06:08.759
<v Speaker 2>single previous cosmic survey ever conducted combined.

129
00:06:09.000 --> 00:06:12.600
<v Speaker 3>The jumpin scale is it's honestly difficult to process.

130
00:06:12.759 --> 00:06:15.279
<v Speaker 2>It's like we spent decades trying to map a continent

131
00:06:15.360 --> 00:06:18.879
<v Speaker 2>by looking through a foggy keyhole, and suddenly someone handed

132
00:06:18.959 --> 00:06:21.160
<v Speaker 2>us a four k drone flying overhead.

133
00:06:21.519 --> 00:06:23.759
<v Speaker 3>That's a great way to put it. It's the difference

134
00:06:23.800 --> 00:06:27.079
<v Speaker 3>between mapping a coastline by walking along it with a

135
00:06:27.160 --> 00:06:30.720
<v Speaker 3>yardstick versus deploying a fleet of light our equipped satellites.

136
00:06:30.839 --> 00:06:33.079
<v Speaker 2>Yeah, the density of the data is just unprecedented.

137
00:06:33.199 --> 00:06:36.399
<v Speaker 3>Exactly we are no longer looking at broad, blurry estimates

138
00:06:36.399 --> 00:06:39.480
<v Speaker 3>of where galaxies tend to gather. We're seeing the intricate,

139
00:06:39.839 --> 00:06:42.759
<v Speaker 3>thread like structures of the costic web in high definition.

140
00:06:42.959 --> 00:06:45.319
<v Speaker 2>So let's talk about the visual reality of that three

141
00:06:45.399 --> 00:06:47.399
<v Speaker 2>D map, because if you sit down and look at

142
00:06:47.439 --> 00:06:49.600
<v Speaker 2>the rendering of this data, it doesn't look like a

143
00:06:49.639 --> 00:06:50.879
<v Speaker 2>solid sphere of stars.

144
00:06:50.959 --> 00:06:52.920
<v Speaker 3>No, it has a very specific geometry.

145
00:06:53.040 --> 00:06:55.680
<v Speaker 2>Right. It looks like a massive series of wedges, or

146
00:06:56.000 --> 00:06:59.720
<v Speaker 2>like slices of a pie, radiating out from a central point,

147
00:07:00.240 --> 00:07:02.839
<v Speaker 2>and Earth is sitting right at the very tip of

148
00:07:02.879 --> 00:07:03.519
<v Speaker 2>those wedges.

149
00:07:03.839 --> 00:07:07.399
<v Speaker 3>The wedge shape is an artifact of our vantage point.

150
00:07:07.639 --> 00:07:11.560
<v Speaker 3>We are observing from a fixed location inside a spiral galaxy,

151
00:07:11.800 --> 00:07:15.399
<v Speaker 3>the Milky Way. Exactly. We cannot just peel away our

152
00:07:15.439 --> 00:07:19.160
<v Speaker 3>own galactic environment to get a perfect, unobstructed three hundred

153
00:07:19.160 --> 00:07:21.879
<v Speaker 3>and sixty degree view of the deeper universe.

154
00:07:21.639 --> 00:07:24.639
<v Speaker 2>Which explains the most glaring feature of the visual map.

155
00:07:24.639 --> 00:07:27.560
<v Speaker 2>When you look at it, there is this massive, empty

156
00:07:27.639 --> 00:07:30.759
<v Speaker 2>black gap cutting right through the middle of the wedges.

157
00:07:30.879 --> 00:07:31.920
<v Speaker 3>It looks like a blind spot.

158
00:07:32.000 --> 00:07:34.240
<v Speaker 2>Yeah, it is exactly a blind spot. Why is that there?

159
00:07:34.360 --> 00:07:37.199
<v Speaker 3>We refer to it as the zone of avoidance because

160
00:07:37.199 --> 00:07:39.399
<v Speaker 3>our solar system is embedded within the disc of the

161
00:07:39.399 --> 00:07:42.319
<v Speaker 3>Milky Way. When we aim our telescopes along the plane

162
00:07:42.360 --> 00:07:44.800
<v Speaker 3>of that disk, we are attempting to look through tens

163
00:07:44.839 --> 00:07:47.600
<v Speaker 3>of thousands of light years of our own galactic material.

164
00:07:47.879 --> 00:07:52.240
<v Speaker 2>Oh so it's just blocked gas dust nearby stars. All

165
00:07:52.279 --> 00:07:54.279
<v Speaker 2>of it is in the way. It's like trying to

166
00:07:54.319 --> 00:07:56.879
<v Speaker 2>spot a firefly a mile away while someone is shining

167
00:07:56.879 --> 00:07:59.839
<v Speaker 2>a high beam flashlight directly into your eyes through a

168
00:07:59.839 --> 00:08:00.680
<v Speaker 2>cloud of smoke.

169
00:08:00.879 --> 00:08:04.040
<v Speaker 3>That's exactly it. The extinction of light is severe in

170
00:08:04.040 --> 00:08:08.360
<v Speaker 3>that direction. The interstellar dust absorbs and scatters the faint

171
00:08:08.399 --> 00:08:12.319
<v Speaker 3>optical light from ancient galaxies, rendering them virtually invisible to

172
00:08:12.399 --> 00:08:13.480
<v Speaker 3>dii's sensors.

173
00:08:13.639 --> 00:08:14.240
<v Speaker 2>Wow.

174
00:08:14.279 --> 00:08:18.079
<v Speaker 3>So the mapping naturally carves out these sweeping wedges above

175
00:08:18.120 --> 00:08:21.079
<v Speaker 3>and below the galactic plane, where the view out into

176
00:08:21.120 --> 00:08:23.079
<v Speaker 3>the deep cosmos is relatively clear.

177
00:08:23.199 --> 00:08:26.480
<v Speaker 2>Okay, so that covers horizontal and vertical spread of the map.

178
00:08:26.519 --> 00:08:29.959
<v Speaker 2>But a map of the universe is useless if it's flat. True,

179
00:08:30.040 --> 00:08:33.320
<v Speaker 2>The true triumph here is the third dimension depth. How

180
00:08:33.360 --> 00:08:36.720
<v Speaker 2>do five thousand robotic fibers in Arizona actually plot the

181
00:08:36.759 --> 00:08:39.600
<v Speaker 2>depth of a galaxy that is billions of light years away.

182
00:08:39.639 --> 00:08:41.840
<v Speaker 2>I mean they aren't bouncing radar off these things.

183
00:08:41.879 --> 00:08:45.639
<v Speaker 3>No, no radar. The third dimension is derived through spectroscopy,

184
00:08:45.960 --> 00:08:48.639
<v Speaker 3>which is where the true power of the instrument lies.

185
00:08:48.720 --> 00:08:49.879
<v Speaker 2>Okay, break that down for me.

186
00:08:50.120 --> 00:08:52.879
<v Speaker 3>So the instrument isn't just taking a picture of a galaxy.

187
00:08:53.399 --> 00:08:56.600
<v Speaker 3>It is taking the light from that galaxy and breaking

188
00:08:56.639 --> 00:09:01.200
<v Speaker 3>it apart into its constituent colors, its spectrums, exactly like

189
00:09:01.200 --> 00:09:02.559
<v Speaker 3>a prism. And this is where we have to talk

190
00:09:02.600 --> 00:09:06.639
<v Speaker 3>about redshift. Because the universe is expanding, everything is moving

191
00:09:06.639 --> 00:09:07.759
<v Speaker 3>away from us, right.

192
00:09:08.120 --> 00:09:10.360
<v Speaker 2>I always hear this compared to the Doppler effect with

193
00:09:10.840 --> 00:09:13.600
<v Speaker 2>sound like a police siren dropping in pitch as its

194
00:09:13.639 --> 00:09:14.600
<v Speaker 2>speeds past you.

195
00:09:15.039 --> 00:09:17.679
<v Speaker 3>It is the optical equivalent of that exact effect. As

196
00:09:17.720 --> 00:09:19.879
<v Speaker 3>a distant galaxy is carried away from us by the

197
00:09:19.879 --> 00:09:23.600
<v Speaker 3>expansion of space, the light waves it emitted are physically

198
00:09:23.639 --> 00:09:24.399
<v Speaker 3>stretched out.

199
00:09:24.240 --> 00:09:26.559
<v Speaker 2>Over their journey, and longer waves mean red light.

200
00:09:26.960 --> 00:09:29.840
<v Speaker 3>Correct. Longer light waves shift toward the red end of

201
00:09:29.879 --> 00:09:31.320
<v Speaker 3>the electromagnetic spectrum.

202
00:09:31.360 --> 00:09:34.000
<v Speaker 2>So the faster it's moving away from us, the redder

203
00:09:34.039 --> 00:09:36.279
<v Speaker 2>the light appears by the time it hits the sensor at.

204
00:09:36.279 --> 00:09:39.759
<v Speaker 3>Kitpeak precisely mm hm. And because we know the expansion

205
00:09:39.799 --> 00:09:42.919
<v Speaker 3>rate of the universe. That red shift acts as a

206
00:09:43.000 --> 00:09:46.799
<v Speaker 3>direct proxy for distance. The more the light is shifted

207
00:09:46.799 --> 00:09:49.200
<v Speaker 3>to the red, the further way the galaxy is.

208
00:09:49.240 --> 00:09:50.399
<v Speaker 2>That is so elegant.

209
00:09:50.600 --> 00:09:54.559
<v Speaker 3>What's fascinating here is the crucial realization about time. The

210
00:09:54.600 --> 00:09:57.080
<v Speaker 3>thing that elevates this from just a map of space

211
00:09:57.159 --> 00:10:00.000
<v Speaker 3>to a map of time is the finite speed of light.

212
00:10:00.279 --> 00:10:03.080
<v Speaker 2>Right. I want to clarify how this translates to time

213
00:10:03.120 --> 00:10:07.159
<v Speaker 2>travel for our listeners, because if DSi locks onto a

214
00:10:07.200 --> 00:10:10.039
<v Speaker 2>galaxy and measures a red shift that tells us it

215
00:10:10.080 --> 00:10:13.000
<v Speaker 2>is five billion light years away.

216
00:10:12.840 --> 00:10:14.840
<v Speaker 3>We aren't seeing where that galaxy.

217
00:10:14.399 --> 00:10:17.039
<v Speaker 2>Is right now exactly. We are seeing the light that

218
00:10:17.200 --> 00:10:20.000
<v Speaker 2>left that galaxy five billion years ago.

219
00:10:20.320 --> 00:10:24.240
<v Speaker 3>You are observing the universe exactly as it existed at

220
00:10:24.240 --> 00:10:26.399
<v Speaker 3>that precise moment in cosmic history.

221
00:10:26.120 --> 00:10:28.360
<v Speaker 2>Which just blows my mind every time I think about it.

222
00:10:28.360 --> 00:10:31.840
<v Speaker 3>It's incredible. When DISI pushes its sensors to the absolute limit,

223
00:10:32.159 --> 00:10:35.039
<v Speaker 3>capturing the faintest targets, it is looking at light that

224
00:10:35.080 --> 00:10:37.480
<v Speaker 3>has been traveling for eleven billion years.

225
00:10:37.200 --> 00:10:41.000
<v Speaker 2>Which means those wedges radiating out from Earth are literal timelines,

226
00:10:41.039 --> 00:10:43.480
<v Speaker 2>little timelines. Yes, the tip of the wedge is us

227
00:10:43.559 --> 00:10:45.759
<v Speaker 2>right now, and as you travel outward along the wedge,

228
00:10:45.759 --> 00:10:48.240
<v Speaker 2>you are moving backward through the epochs of the universe,

229
00:10:48.279 --> 00:10:52.039
<v Speaker 2>slice by slice, tracing the history of reality back eleven

230
00:10:52.240 --> 00:10:53.440
<v Speaker 2>billion years.

231
00:10:53.480 --> 00:10:56.639
<v Speaker 3>A point underscored by d side director doctor Michael Levi,

232
00:10:57.200 --> 00:11:00.159
<v Speaker 3>who noted how the instrument performed beyond the wildest to

233
00:11:00.200 --> 00:11:02.879
<v Speaker 3>expectations of the team that built it. I can imagine

234
00:11:03.000 --> 00:11:06.960
<v Speaker 3>pushing the boundaries of spectroscopy to capture these incredibly faint

235
00:11:07.080 --> 00:11:11.399
<v Speaker 3>ancient signals requires a level of precision that is honestly

236
00:11:11.440 --> 00:11:12.600
<v Speaker 3>difficult to overstate.

237
00:11:12.799 --> 00:11:16.000
<v Speaker 2>And they needed that precision because, as we established earlier,

238
00:11:16.080 --> 00:11:17.080
<v Speaker 2>they were hunting.

239
00:11:16.840 --> 00:11:18.720
<v Speaker 3>A ghost, the biggest ghost of all.

240
00:11:18.879 --> 00:11:22.240
<v Speaker 2>Yeah. They didn't build a time traveling three D map

241
00:11:22.399 --> 00:11:25.559
<v Speaker 2>just to account galaxies. They built it to watch how seventy

242
00:11:25.600 --> 00:11:28.799
<v Speaker 2>percent of the universe behaves over time. Let's pivot to

243
00:11:28.879 --> 00:11:29.440
<v Speaker 2>dark energy.

244
00:11:29.559 --> 00:11:30.039
<v Speaker 3>Let's do it.

245
00:11:30.240 --> 00:11:33.360
<v Speaker 2>What exactly was the prevailing assumption about this force before

246
00:11:33.639 --> 00:11:35.399
<v Speaker 2>DSi started churning out data.

247
00:11:35.679 --> 00:11:38.080
<v Speaker 3>Well, to frame dark energy correctly, you have to look

248
00:11:38.120 --> 00:11:41.039
<v Speaker 3>at the fundamental conflict governing the universe. It is a

249
00:11:41.159 --> 00:11:44.519
<v Speaker 3>cosmic tug of war. Okay, on one side, you have matter,

250
00:11:44.759 --> 00:11:49.039
<v Speaker 3>This includes stars, planets, gas clouds, and dark matter. All

251
00:11:49.080 --> 00:11:53.279
<v Speaker 3>of this matter possesses mass, and therefore it exerts gravity.

252
00:11:52.919 --> 00:11:54.519
<v Speaker 2>And gravity pulls things together.

253
00:11:54.840 --> 00:11:59.159
<v Speaker 3>Right, Gravity is an attractive force. Its inherent tendency is

254
00:11:59.200 --> 00:12:02.240
<v Speaker 3>to pull things together, to cause the universe to contract

255
00:12:02.320 --> 00:12:02.919
<v Speaker 3>and clump.

256
00:12:03.039 --> 00:12:06.240
<v Speaker 2>So logically, if gravity is the only player on the field,

257
00:12:06.720 --> 00:12:09.639
<v Speaker 2>the universe should be pulling itself back inward after the

258
00:12:09.679 --> 00:12:12.519
<v Speaker 2>initial explosion of the Big Bang, like the expansion should

259
00:12:12.559 --> 00:12:13.360
<v Speaker 2>be slowing down.

260
00:12:13.639 --> 00:12:18.120
<v Speaker 3>That was the widely held cosmological consensus for decades. Really, yes,

261
00:12:18.679 --> 00:12:22.559
<v Speaker 3>everyone assumed the expansion must be decelerating due to the

262
00:12:22.600 --> 00:12:25.799
<v Speaker 3>collective gravitational drag of all the matter in existence.

263
00:12:25.919 --> 00:12:27.200
<v Speaker 2>But then something changed.

264
00:12:27.519 --> 00:12:31.480
<v Speaker 3>Observations in the late nineteen nineties absolutely shattered that model.

265
00:12:31.639 --> 00:12:35.519
<v Speaker 3>Oh wow, instead of slowing down, astronomers realize the expansion

266
00:12:35.559 --> 00:12:39.440
<v Speaker 3>of the universe is accelerating. Distant galaxies are flying apart

267
00:12:39.559 --> 00:12:41.720
<v Speaker 3>at an ever increasing velocity.

268
00:12:41.360 --> 00:12:43.679
<v Speaker 2>Which just defies common sense. I mean, if you throw

269
00:12:43.679 --> 00:12:46.320
<v Speaker 2>a ball straight up into the air, gravity slows it down,

270
00:12:46.360 --> 00:12:49.200
<v Speaker 2>it doesn't suddenly accelerate upward into the stratosphere.

271
00:12:49.240 --> 00:12:52.399
<v Speaker 3>Exactly. For the universe to accelerate its expansion, there must

272
00:12:52.480 --> 00:12:56.000
<v Speaker 3>be a repulsive force overpowering the attractive force of gravity

273
00:12:56.279 --> 00:12:58.039
<v Speaker 3>on a macroscopic.

274
00:12:57.360 --> 00:12:58.600
<v Speaker 2>Scale, and that's the ghost.

275
00:12:58.879 --> 00:13:02.559
<v Speaker 3>That's the ghost. This invisible pressure driving the fabric of

276
00:13:02.600 --> 00:13:05.799
<v Speaker 3>space apart is what we term dark energy.

277
00:13:05.720 --> 00:13:08.919
<v Speaker 2>And because it is responsible for the accelerating expansion of

278
00:13:08.960 --> 00:13:12.759
<v Speaker 2>the entirety of space, mathematical models dictate that it must

279
00:13:12.799 --> 00:13:16.159
<v Speaker 2>account for roughly seventy percent of the total energy density

280
00:13:16.200 --> 00:13:19.480
<v Speaker 2>of the universe. That's right, Okay, so we knew dark

281
00:13:19.559 --> 00:13:22.080
<v Speaker 2>energy existed, or at least we knew something was pushing

282
00:13:22.080 --> 00:13:25.720
<v Speaker 2>the universe apart. But how did physicists define it mathematically?

283
00:13:25.799 --> 00:13:28.000
<v Speaker 2>Because this is where the D sign map throws a

284
00:13:28.120 --> 00:13:29.879
<v Speaker 2>massive wrench into the machine.

285
00:13:30.000 --> 00:13:33.799
<v Speaker 3>Right, So the most elegant and widely accepted mathematical explanation

286
00:13:34.600 --> 00:13:38.279
<v Speaker 3>was to treat dark energy as a cosmological.

287
00:13:37.519 --> 00:13:40.559
<v Speaker 2>Constant, the operative word being constant.

288
00:13:40.080 --> 00:13:43.919
<v Speaker 3>Exactly constant. The assumption was that this repulsive energy is

289
00:13:43.919 --> 00:13:47.080
<v Speaker 3>an intrinsic property of the vacuum of space itself. It's

290
00:13:47.240 --> 00:13:50.919
<v Speaker 3>uniform everywhere, okay, and crucially, its density never changes.

291
00:13:50.639 --> 00:13:52.159
<v Speaker 2>Over time, so it's always the same.

292
00:13:52.320 --> 00:13:55.519
<v Speaker 3>Yes. As the universe expands, it creates more empty space

293
00:13:55.559 --> 00:13:58.840
<v Speaker 3>and therefore more total dark energy. But the inherent strength

294
00:13:58.879 --> 00:14:02.720
<v Speaker 3>of that repulsive push per cubic meter remains absolutely rigid

295
00:14:02.759 --> 00:14:04.879
<v Speaker 3>and unchanging across eternity.

296
00:14:05.159 --> 00:14:07.519
<v Speaker 2>It's a static rule of the game, a fixed value

297
00:14:07.519 --> 00:14:10.320
<v Speaker 2>that you just plug into your equations exactly. But the

298
00:14:10.360 --> 00:14:13.440
<v Speaker 2>bombshell from DSI's early data, and this is just the

299
00:14:13.480 --> 00:14:17.120
<v Speaker 2>initial three year data set, is that this foundational assumption

300
00:14:17.639 --> 00:14:19.000
<v Speaker 2>might be entirely wrong.

301
00:14:19.120 --> 00:14:21.679
<v Speaker 3>It's a massive shock to the community because.

302
00:14:21.360 --> 00:14:24.519
<v Speaker 2>The data is heavily implying that dark energy is not

303
00:14:24.639 --> 00:14:28.600
<v Speaker 2>a constant. It suggests that this repulsive force is actually evolving.

304
00:14:28.759 --> 00:14:32.080
<v Speaker 3>The implications of that word evolving are monumental in the

305
00:14:32.120 --> 00:14:33.200
<v Speaker 3>field of cosmology.

306
00:14:33.240 --> 00:14:34.879
<v Speaker 2>I mean, it sounds like it breaks everything.

307
00:14:35.080 --> 00:14:38.519
<v Speaker 3>It really does. If dark energy is dynamic, if its

308
00:14:38.559 --> 00:14:42.240
<v Speaker 3>strength fluctuates or changes character as the universe ages, then

309
00:14:42.240 --> 00:14:44.960
<v Speaker 3>the cosmological constant is a flawed model.

310
00:14:45.039 --> 00:14:46.639
<v Speaker 2>So what does that mean? It actually is?

311
00:14:47.080 --> 00:14:49.799
<v Speaker 3>It suggests dark energy might not be a simple property

312
00:14:49.840 --> 00:14:53.720
<v Speaker 3>of empty space, but rather some kind of dynamic shifting field,

313
00:14:54.679 --> 00:14:58.240
<v Speaker 3>or even more radically, perhaps an indication that our underlying

314
00:14:58.279 --> 00:15:02.919
<v Speaker 3>theory of gravity is fundamentally incomplete on cosmic scales.

315
00:15:03.039 --> 00:15:04.799
<v Speaker 2>Let me stop you there, because here's where it gets

316
00:15:04.840 --> 00:15:08.200
<v Speaker 2>really interesting. If we throw out the constant part of

317
00:15:08.240 --> 00:15:10.679
<v Speaker 2>the cosmological constant, what does that.

318
00:15:10.639 --> 00:15:12.879
<v Speaker 3>Actually leave us with a lot of uncertainty?

319
00:15:13.000 --> 00:15:17.799
<v Speaker 2>Doesn't a dynamic shifting dark energy completely obliterate our ability

320
00:15:17.840 --> 00:15:21.200
<v Speaker 2>to predict how the universe ends? Because the ultimate fate

321
00:15:21.240 --> 00:15:24.639
<v Speaker 2>of reality relies entirely on who wins that cosmic tug

322
00:15:24.679 --> 00:15:27.279
<v Speaker 2>of war between gravity and dark energy.

323
00:15:27.440 --> 00:15:29.919
<v Speaker 3>You hit the nail on the head. It entirely rewrites

324
00:15:30.000 --> 00:15:34.039
<v Speaker 3>the predictive models. Wow. Under the assumption of a cosmological constant,

325
00:15:34.240 --> 00:15:37.799
<v Speaker 3>the fate of the universe is a slow, relentless expansion.

326
00:15:38.519 --> 00:15:41.440
<v Speaker 3>It is a scenario often called the Big Freeze or

327
00:15:41.440 --> 00:15:42.000
<v Speaker 3>heat death.

328
00:15:42.120 --> 00:15:44.799
<v Speaker 2>The Big Freeze sounds cozy.

329
00:15:44.559 --> 00:15:48.600
<v Speaker 3>Not quite. The acceleration continues steadily forever, pushing galaxies so

330
00:15:48.720 --> 00:15:52.080
<v Speaker 3>far apart that they become isolated islands, Stars burn out,

331
00:15:52.080 --> 00:15:55.480
<v Speaker 3>matter decays, and the universe drifts into a cold, dark,

332
00:15:55.600 --> 00:15:56.639
<v Speaker 3>infinite emptiness.

333
00:15:56.799 --> 00:15:57.159
<v Speaker 2>Bleak.

334
00:15:57.320 --> 00:16:00.879
<v Speaker 3>But you know, predictable, very predictable. But if the strength

335
00:16:00.879 --> 00:16:04.120
<v Speaker 3>of dark energy is actively changing, then what if the

336
00:16:04.159 --> 00:16:07.840
<v Speaker 3>force is dynamic? The future becomes wildly uncertain. If dark

337
00:16:07.960 --> 00:16:12.200
<v Speaker 3>energy is gradually weakening over time, gravity could eventually reclaim dominance.

338
00:16:12.320 --> 00:16:15.039
<v Speaker 2>Oh, so it could pull everything back together exactly.

339
00:16:15.200 --> 00:16:19.279
<v Speaker 3>The expansion could halt, reverse and pull all matter back

340
00:16:19.320 --> 00:16:22.480
<v Speaker 3>together in a catastrophic collapse, A big crunch, A big crunch.

341
00:16:23.000 --> 00:16:24.679
<v Speaker 2>Okay, And what if it goes the other way? What

342
00:16:24.799 --> 00:16:26.159
<v Speaker 2>if the push gets stronger?

343
00:16:26.480 --> 00:16:30.519
<v Speaker 3>Conversely, if the repulsive strength of dark energy is increasing,

344
00:16:30.840 --> 00:16:34.919
<v Speaker 3>the acceleration could become so violently intense that it eventually

345
00:16:34.960 --> 00:16:39.639
<v Speaker 3>overpowers the gravitational forces holding galaxy clusters together. Oh no,

346
00:16:40.320 --> 00:16:44.639
<v Speaker 3>then stellar systems, then planets, and ultimately the atomic bonds

347
00:16:44.639 --> 00:16:45.320
<v Speaker 3>of matter.

348
00:16:45.080 --> 00:16:48.840
<v Speaker 2>Itself, literally tearing the actual fabric of reality to shreds.

349
00:16:49.000 --> 00:16:51.440
<v Speaker 3>Yes, that scenario is known as the big rip.

350
00:16:51.639 --> 00:16:53.879
<v Speaker 2>The big rip. Okay, I need a minute. That's terrifying.

351
00:16:54.120 --> 00:16:57.919
<v Speaker 3>It's traumatic, certainly. Doctor Suhadri Natzer, who is an associate

352
00:16:57.919 --> 00:17:00.399
<v Speaker 3>professor at the University of Portsmouth and co chair of

353
00:17:00.440 --> 00:17:03.720
<v Speaker 3>the Clustering Working Group for DE and I frame this perfectly.

354
00:17:03.799 --> 00:17:04.400
<v Speaker 2>What did he say?

355
00:17:04.559 --> 00:17:06.960
<v Speaker 3>He pointed out that the mere possibility of dark energy

356
00:17:07.000 --> 00:17:10.440
<v Speaker 3>evolving with time is revolutionary on its own. It demands

357
00:17:10.440 --> 00:17:13.039
<v Speaker 3>a foundational reassessment of the math we use to describe

358
00:17:13.079 --> 00:17:13.839
<v Speaker 3>the cosmos.

359
00:17:14.079 --> 00:17:16.839
<v Speaker 2>But that creates a massive logical problem. In my head.

360
00:17:17.119 --> 00:17:20.599
<v Speaker 2>We've established that dark energy is totally invisible. We can't

361
00:17:20.599 --> 00:17:23.119
<v Speaker 2>put it in a jar, we can't directly measure its

362
00:17:23.119 --> 00:17:26.480
<v Speaker 2>temperature or its mass. So how on earth are these

363
00:17:26.559 --> 00:17:30.799
<v Speaker 2>researchers using a map of visible tangible galaxies to prove

364
00:17:30.880 --> 00:17:34.880
<v Speaker 2>that an invisible phantom force is changing its behavior over

365
00:17:34.920 --> 00:17:35.960
<v Speaker 2>billions of years.

366
00:17:36.160 --> 00:17:38.319
<v Speaker 3>It's a great question. They do it by tracking the

367
00:17:38.359 --> 00:17:42.279
<v Speaker 3>physical consequences of that cosmic tug of war over eleven

368
00:17:42.359 --> 00:17:43.079
<v Speaker 3>billion years.

369
00:17:43.200 --> 00:17:43.799
<v Speaker 2>Okay, go on.

370
00:17:44.119 --> 00:17:47.759
<v Speaker 3>Dark energy is invisible, but gravity is not, and the

371
00:17:47.759 --> 00:17:51.960
<v Speaker 3>way gravity pulls visible matter together leads a structural footprint

372
00:17:51.960 --> 00:17:52.920
<v Speaker 3>that we can actually measure.

373
00:17:53.000 --> 00:17:56.359
<v Speaker 2>You're talking about cosmic clustering, specifically.

374
00:17:55.759 --> 00:17:59.480
<v Speaker 3>Buryon acoustic oscillations, but the broader concept is clustering.

375
00:17:59.640 --> 00:17:59.880
<v Speaker 2>Right.

376
00:18:00.160 --> 00:18:04.000
<v Speaker 3>To trace dark energy DSi isn't just looking at individual galaxies.

377
00:18:04.319 --> 00:18:07.559
<v Speaker 3>It is analyzing the spatial relationships between them. It is

378
00:18:07.599 --> 00:18:11.559
<v Speaker 3>measuring exactly how galaxies group together at different points in

379
00:18:11.599 --> 00:18:12.359
<v Speaker 3>cosmic history.

380
00:18:12.400 --> 00:18:14.839
<v Speaker 2>I need a physical analogy for this, because measuring the

381
00:18:14.880 --> 00:18:18.200
<v Speaker 2>distance between dots on a map to track an invisible

382
00:18:18.200 --> 00:18:19.440
<v Speaker 2>force is a leap for me.

383
00:18:19.559 --> 00:18:20.039
<v Speaker 3>Let's hear it.

384
00:18:20.240 --> 00:18:23.359
<v Speaker 2>Okay, imagine looking at a crowd of people dispersing after

385
00:18:23.400 --> 00:18:26.880
<v Speaker 2>a concert from a helicopter. By tracking how the clusters

386
00:18:26.880 --> 00:18:29.640
<v Speaker 2>of people spread out over an hour, you could deduce

387
00:18:29.720 --> 00:18:32.240
<v Speaker 2>if there was like a sudden rainstorm pushing them to

388
00:18:32.319 --> 00:18:32.880
<v Speaker 2>run faster.

389
00:18:33.279 --> 00:18:35.279
<v Speaker 3>That's a good start. Let's make it a bit more

390
00:18:35.359 --> 00:18:39.160
<v Speaker 3>physical though. Imagine a giant rubber band stretched across a table.

391
00:18:39.359 --> 00:18:40.759
<v Speaker 2>Okay, a rubber band.

392
00:18:40.960 --> 00:18:44.039
<v Speaker 3>You have two heavy iron weights resting on it, pulling

393
00:18:44.079 --> 00:18:47.599
<v Speaker 3>the rubber band slightly toward each other. The tension of

394
00:18:47.640 --> 00:18:50.160
<v Speaker 3>the weights pulling together represents gravity.

395
00:18:50.279 --> 00:18:50.680
<v Speaker 2>Got it.

396
00:18:51.359 --> 00:18:54.720
<v Speaker 3>Now, the rubber band itself being slowly pulled from the

397
00:18:54.839 --> 00:18:57.640
<v Speaker 3>edges of the table. That is dark energy.

398
00:18:57.720 --> 00:19:00.880
<v Speaker 2>Oh, that is a highly functional analogy. So the weights

399
00:19:00.960 --> 00:19:03.599
<v Speaker 2>naturally want to slide toward each other and clump together,

400
00:19:03.960 --> 00:19:06.599
<v Speaker 2>but the surface they are resting on is actively being

401
00:19:06.640 --> 00:19:07.960
<v Speaker 2>stretched in the oposite direction.

402
00:19:08.160 --> 00:19:11.000
<v Speaker 3>Precisely so, if you want to know if the stretching

403
00:19:11.079 --> 00:19:14.680
<v Speaker 3>force the dark energy is constant or changing, you don't

404
00:19:14.720 --> 00:19:17.359
<v Speaker 3>look at the rubber band because you can't see it, right.

405
00:19:17.400 --> 00:19:19.480
<v Speaker 3>You just measure the distance between the two iron weights

406
00:19:19.519 --> 00:19:20.240
<v Speaker 3>at different times.

407
00:19:20.440 --> 00:19:24.440
<v Speaker 2>Oh, if the weights are pulling together fast, gravity is winning.

408
00:19:24.720 --> 00:19:27.599
<v Speaker 2>If they are suddenly being pulled apart, faster than before,

409
00:19:27.920 --> 00:19:30.119
<v Speaker 2>the stretching force must be ramping up.

410
00:19:30.079 --> 00:19:33.440
<v Speaker 3>Exactly, and in the context of the universe, those weights

411
00:19:33.640 --> 00:19:36.839
<v Speaker 3>are the massive clusters of galaxies. Right in the early

412
00:19:36.880 --> 00:19:40.680
<v Speaker 3>epochs of the universe, matter was much denser, Galaxies were

413
00:19:40.680 --> 00:19:44.079
<v Speaker 3>closer together, which meant the gravitational pull between them was

414
00:19:44.079 --> 00:19:48.400
<v Speaker 3>incredibly strong. Gravity was effectively dominating the tug of war,

415
00:19:48.839 --> 00:19:53.680
<v Speaker 3>actively pulling material together into these massive, intricate cosmic webs.

416
00:19:53.839 --> 00:19:55.640
<v Speaker 2>So the weights were tightly grouped.

417
00:19:55.880 --> 00:19:59.200
<v Speaker 3>But as the universe expanded, driven by dark energy, the

418
00:19:59.279 --> 00:20:00.160
<v Speaker 3>overall dense.

419
00:20:00.279 --> 00:20:02.119
<v Speaker 2>Matter dropped, the stretching continued.

420
00:20:02.240 --> 00:20:05.960
<v Speaker 3>Yes, galaxies were pushed further apart, which inevitably weakened the

421
00:20:05.960 --> 00:20:10.640
<v Speaker 3>gravitational attraction between them. As gravity's grip loosened on massive scales,

422
00:20:11.000 --> 00:20:13.519
<v Speaker 3>dark energy began to dictate the structural evolution.

423
00:20:14.039 --> 00:20:18.279
<v Speaker 2>So the map DSi built allows researchers to literally look

424
00:20:18.359 --> 00:20:21.799
<v Speaker 2>back at the tightly clumped weights eleven billion years ago

425
00:20:21.880 --> 00:20:25.720
<v Speaker 2>and then measure how that clumping pattern changes epoch by

426
00:20:25.799 --> 00:20:28.319
<v Speaker 2>epoch as you move closer to the present day.

427
00:20:28.720 --> 00:20:31.680
<v Speaker 3>They are essentially reading the historical record of the expansion

428
00:20:31.839 --> 00:20:35.720
<v Speaker 3>by taking incredibly precise measurements of ancient galaxy clusters and

429
00:20:35.799 --> 00:20:38.839
<v Speaker 3>comparing their distribution to clusters closer to us. In time,

430
00:20:39.519 --> 00:20:42.799
<v Speaker 3>they map the exact influence of dark energy at every

431
00:20:42.839 --> 00:20:45.240
<v Speaker 3>stage of the universe's life, but wait.

432
00:20:45.240 --> 00:20:48.960
<v Speaker 2>To get those measurements from eleven billion years ago. They

433
00:20:48.960 --> 00:20:52.039
<v Speaker 2>can't just look at regular galaxies, right, because the light

434
00:20:52.079 --> 00:20:54.400
<v Speaker 2>from a standard galaxy that far away would be way

435
00:20:54.440 --> 00:20:57.240
<v Speaker 2>too faint for even the five thousand fiber optic robots

436
00:20:57.240 --> 00:20:57.759
<v Speaker 2>to pick up.

437
00:20:57.880 --> 00:21:00.839
<v Speaker 3>You're absolutely right, which is why as significant portion of

438
00:21:00.880 --> 00:21:05.119
<v Speaker 3>dii's targeting relies on quasars quasars. To map the deepest

439
00:21:05.240 --> 00:21:08.880
<v Speaker 3>edges of the visible universe, you need a beacon. Quasars

440
00:21:08.920 --> 00:21:10.599
<v Speaker 3>serve as those distant lighthouses.

441
00:21:10.960 --> 00:21:12.799
<v Speaker 2>For those who might not be familiar with the sheer

442
00:21:12.880 --> 00:21:15.759
<v Speaker 2>violence of a quasar, we are talking about an active

443
00:21:15.799 --> 00:21:19.880
<v Speaker 2>galactic nucleus. It's a supermassive black hole at the center

444
00:21:19.920 --> 00:21:23.519
<v Speaker 2>of a distant galaxy that is actively feeding on astronomical

445
00:21:23.519 --> 00:21:25.000
<v Speaker 2>amounts of gas and dust.

446
00:21:25.160 --> 00:21:28.000
<v Speaker 3>The gravitational friction of that material spiraling into the black

447
00:21:28.000 --> 00:21:31.279
<v Speaker 3>hole heats to such extreme temperatures that it in miss

448
00:21:31.440 --> 00:21:36.240
<v Speaker 3>radiation across the entire electromagnetic spectrum. It's so bright unbelievably bright.

449
00:21:36.960 --> 00:21:40.799
<v Speaker 3>A single quasar can easily outshine the combined light of

450
00:21:40.880 --> 00:21:43.440
<v Speaker 3>every single star in its host galaxy.

451
00:21:43.480 --> 00:21:46.079
<v Speaker 2>They are practically screaming across the universe.

452
00:21:46.119 --> 00:21:51.119
<v Speaker 3>Their extreme luminosity allows disized spectrographs to capture their light

453
00:21:51.759 --> 00:21:55.799
<v Speaker 3>even from eleven billion light years away. Amazing, But the

454
00:21:55.839 --> 00:21:58.559
<v Speaker 3>quasars are doing more than just marking a point on

455
00:21:58.599 --> 00:22:02.200
<v Speaker 3>a map their light. It actually illuminates the invisible material

456
00:22:02.279 --> 00:22:04.039
<v Speaker 3>lying between them and Earth.

457
00:22:04.440 --> 00:22:07.359
<v Speaker 2>Like shining a flashlight through a foggy forest. You might

458
00:22:07.400 --> 00:22:09.680
<v Speaker 2>not see the individual trees in the dark, but the

459
00:22:09.720 --> 00:22:12.599
<v Speaker 2>beam of the flashlight catches the mist and the branches

460
00:22:12.640 --> 00:22:14.200
<v Speaker 2>between you and the light source.

461
00:22:14.480 --> 00:22:17.359
<v Speaker 3>That is an incredibly accurate description of what we call

462
00:22:17.400 --> 00:22:19.640
<v Speaker 3>the Liman alpha forest technique.

463
00:22:19.200 --> 00:22:21.440
<v Speaker 2>Oh Lyman alpha forest cool name.

464
00:22:21.559 --> 00:22:24.519
<v Speaker 3>It is as the brilliant light from a distant quasar

465
00:22:24.559 --> 00:22:28.000
<v Speaker 3>travels eleven billion light years to reach DSi, it passes

466
00:22:28.079 --> 00:22:33.119
<v Speaker 3>through massive invisible clouds of intergalactic hydrogen gas. Those gas

467
00:22:33.160 --> 00:22:37.960
<v Speaker 3>clouds absorb specific tiny slivers of the quasar's light spectrum.

468
00:22:37.480 --> 00:22:40.960
<v Speaker 2>Leaving dark bands, or like fingerprints, in the light wave

469
00:22:41.000 --> 00:22:43.559
<v Speaker 2>that DISI eventually captures an Arizona.

470
00:22:43.200 --> 00:22:47.920
<v Speaker 3>Exactly by analyzing those absorption bands, researchers can map the

471
00:22:47.960 --> 00:22:52.720
<v Speaker 3>density and distribution of invisible hydrogen gas spanning billions of

472
00:22:52.799 --> 00:22:53.279
<v Speaker 3>light years.

473
00:22:53.359 --> 00:22:54.319
<v Speaker 2>That is genius.

474
00:22:54.480 --> 00:22:56.440
<v Speaker 3>So they aren't just mapping the bright points of light.

475
00:22:56.839 --> 00:22:59.759
<v Speaker 3>They are mapping the invisible structure of the cosmic web itself.

476
00:23:00.519 --> 00:23:05.640
<v Speaker 3>And it is this comprehensive, multi layered mapping of visible galaxies,

477
00:23:05.920 --> 00:23:10.160
<v Speaker 3>brilliant quasars, and invisible gas clouds that provided the clustering data.

478
00:23:10.240 --> 00:23:12.039
<v Speaker 2>And when they finally ran the math on all of

479
00:23:12.039 --> 00:23:15.640
<v Speaker 2>that data, tracing the tug of war across eleven billion years,

480
00:23:16.000 --> 00:23:18.920
<v Speaker 2>the results pointed to an evolving dark energy.

481
00:23:19.079 --> 00:23:20.440
<v Speaker 3>The strength of the push varied.

482
00:23:20.680 --> 00:23:23.599
<v Speaker 2>It is an astonishing realization. And you know what strikes

483
00:23:23.640 --> 00:23:26.640
<v Speaker 2>me is the sheer human capital required to even process

484
00:23:26.640 --> 00:23:28.920
<v Speaker 2>a thought on this scale. I mean, the instrument is

485
00:23:28.960 --> 00:23:31.319
<v Speaker 2>a marvel, but the human machinery behind it is just

486
00:23:31.400 --> 00:23:32.000
<v Speaker 2>as vast.

487
00:23:32.359 --> 00:23:36.160
<v Speaker 3>The scale of collaboration is a defining characteristic of modern astrophysics.

488
00:23:36.599 --> 00:23:40.680
<v Speaker 3>You simply cannot process forty seven million spectroscopic measurements with a.

489
00:23:40.599 --> 00:23:42.680
<v Speaker 2>Small team in the basement, right, It takes an army.

490
00:23:42.960 --> 00:23:46.960
<v Speaker 3>The DTI collaboration involves over nine hundred researchers spanning more

491
00:23:46.960 --> 00:23:49.680
<v Speaker 3>than seventy institutions across the globe.

492
00:23:49.400 --> 00:23:53.400
<v Speaker 2>Nine hundred and I saw that a third of those researchers,

493
00:23:53.680 --> 00:23:56.599
<v Speaker 2>about three hundred of them, are PhD students. The next

494
00:23:56.640 --> 00:23:59.759
<v Speaker 2>generation of cosmologists are basically cutting their teeth on a

495
00:23:59.839 --> 00:24:03.160
<v Speaker 2>day data set that is actively dismantling the models their

496
00:24:03.200 --> 00:24:04.279
<v Speaker 2>textbooks were based on.

497
00:24:04.839 --> 00:24:08.480
<v Speaker 3>It represents a massive transfer of institutional knowledge. The project

498
00:24:08.519 --> 00:24:11.200
<v Speaker 3>is managed by the US Department of Energy at Berkeley Lab,

499
00:24:11.720 --> 00:24:14.039
<v Speaker 3>but the intellectual lifting is heavily distributed.

500
00:24:14.119 --> 00:24:15.920
<v Speaker 2>It's a global village, very much so.

501
00:24:16.279 --> 00:24:19.480
<v Speaker 3>You have major hubs of analysis in the UK, for example,

502
00:24:19.759 --> 00:24:23.559
<v Speaker 3>with deep involvement from the University of Portsmouth, University College London,

503
00:24:23.799 --> 00:24:24.880
<v Speaker 3>and Durham University.

504
00:24:25.000 --> 00:24:27.720
<v Speaker 2>And these teams are currently locked in what they describe

505
00:24:27.759 --> 00:24:31.720
<v Speaker 2>as churning through the data because the five year survey

506
00:24:31.799 --> 00:24:35.279
<v Speaker 2>is complete, right, the physical observations for this massive map

507
00:24:35.359 --> 00:24:36.680
<v Speaker 2>are done and in the camp.

508
00:24:36.759 --> 00:24:40.519
<v Speaker 3>Yes, the tantalizing evidence for evolving dark energy came from

509
00:24:40.559 --> 00:24:42.440
<v Speaker 3>the initial three year data release.

510
00:24:42.559 --> 00:24:43.880
<v Speaker 2>Okay, so what about the rest of it.

511
00:24:44.079 --> 00:24:48.160
<v Speaker 3>The definitive, highly rigorous cosmological constraints that will emerge from

512
00:24:48.240 --> 00:24:51.400
<v Speaker 3>the complete five year data set are expected in twenty twenty.

513
00:24:51.160 --> 00:24:54.920
<v Speaker 2>Seven twenty twenty seven, so the entire physics community is

514
00:24:55.039 --> 00:24:57.400
<v Speaker 2>essentially holding its breath for the next few years to

515
00:24:57.400 --> 00:25:00.000
<v Speaker 2>see if the cosmological constant officially died.

516
00:25:00.319 --> 00:25:00.839
<v Speaker 3>Pretty much.

517
00:25:00.920 --> 00:25:03.279
<v Speaker 2>But wait, while they are churning through the data for

518
00:25:03.400 --> 00:25:06.799
<v Speaker 2>dark energy, they've realized this map is so dense and

519
00:25:06.880 --> 00:25:10.319
<v Speaker 2>so precise that they can use it for completely different

520
00:25:10.400 --> 00:25:12.200
<v Speaker 2>scientific inquiries.

521
00:25:11.680 --> 00:25:13.079
<v Speaker 3>The bonus science.

522
00:25:12.880 --> 00:25:15.720
<v Speaker 2>The side quests. They are using the macrostructure of the

523
00:25:15.799 --> 00:25:19.599
<v Speaker 2>universe to study the most elusive subatomic particles in existence.

524
00:25:20.000 --> 00:25:24.440
<v Speaker 3>Yes, they're using the clustering data to calculate the mass

525
00:25:24.440 --> 00:25:25.200
<v Speaker 3>of neutrinos.

526
00:25:25.480 --> 00:25:27.920
<v Speaker 2>Okay, I genuinely struggle to wrap my head around this.

527
00:25:28.119 --> 00:25:31.480
<v Speaker 2>So what does this all mean? Neutrinos are the lightest,

528
00:25:31.640 --> 00:25:35.680
<v Speaker 2>most ghostlike fundamental particles we know of, right correct, Trillions

529
00:25:35.720 --> 00:25:37.799
<v Speaker 2>of them are passing through my body right now without

530
00:25:37.799 --> 00:25:40.960
<v Speaker 2>interacting with anything. How on earth does a giant map

531
00:25:41.000 --> 00:25:44.319
<v Speaker 2>of massive galaxies help us weigh the tiniest, lightest particles

532
00:25:44.359 --> 00:25:44.960
<v Speaker 2>in existence.

533
00:25:45.119 --> 00:25:48.039
<v Speaker 3>If we connect this to the bigger picture, it requires

534
00:25:48.160 --> 00:25:52.119
<v Speaker 3>linking the microscopic world of quantum mechanics to the macroscopic

535
00:25:52.160 --> 00:25:53.440
<v Speaker 3>evolution of the cosmos.

536
00:25:53.519 --> 00:25:54.440
<v Speaker 2>Okay, I'm with you.

537
00:25:54.519 --> 00:25:59.000
<v Speaker 3>Neutrinos are indeed incredibly elusive. They have virtually zero mass,

538
00:25:59.400 --> 00:26:02.079
<v Speaker 3>and they travel near the speed of light because they

539
00:26:02.119 --> 00:26:06.079
<v Speaker 3>interact so weakly with normal matter. Building a laboratory instrument

540
00:26:06.119 --> 00:26:08.279
<v Speaker 3>to waveh them directly is incredibly difficult.

541
00:26:08.400 --> 00:26:10.319
<v Speaker 2>That they do have a mass, it's not zero.

542
00:26:10.599 --> 00:26:13.880
<v Speaker 3>It is not zero, And while an individual neutrino's mass

543
00:26:13.920 --> 00:26:18.079
<v Speaker 3>is infinitesimally small, they are among the most abundant particles

544
00:26:18.079 --> 00:26:20.920
<v Speaker 3>in the universe. Right when you aggregate the mass of

545
00:26:21.039 --> 00:26:25.480
<v Speaker 3>every neutrino in existence, it constitutes a substantial amount of material,

546
00:26:26.079 --> 00:26:29.119
<v Speaker 3>and anything with mass exerts a gravitational influence.

547
00:26:29.359 --> 00:26:31.799
<v Speaker 2>Okay, so how does that influence show up on a

548
00:26:31.799 --> 00:26:32.880
<v Speaker 2>map of galaxies.

549
00:26:33.039 --> 00:26:35.160
<v Speaker 3>You have to look back at the early universe when

550
00:26:35.200 --> 00:26:38.119
<v Speaker 3>those massive galaxy clusters were just beginning to form.

551
00:26:38.240 --> 00:26:39.960
<v Speaker 2>Back to the weights on the rubber band.

552
00:26:39.880 --> 00:26:43.400
<v Speaker 3>Exactly, gravity was trying to pull dark matter in standard

553
00:26:43.400 --> 00:26:47.759
<v Speaker 3>matter together into dense structures. But because neutrinos are so hot,

554
00:26:47.920 --> 00:26:50.599
<v Speaker 3>meaning they move at velocities incredibly close to the speed

555
00:26:50.640 --> 00:26:53.400
<v Speaker 3>of light, they refuse to be bound by those early

556
00:26:53.759 --> 00:26:55.759
<v Speaker 3>relatively weak gravitational wells.

557
00:26:55.839 --> 00:26:57.880
<v Speaker 2>Oh they are moving too fast to be trapped by

558
00:26:57.880 --> 00:26:59.039
<v Speaker 2>the clumping matter.

559
00:26:59.079 --> 00:27:03.359
<v Speaker 3>Exactly right through these forming structures, and because they carry

560
00:27:03.400 --> 00:27:06.880
<v Speaker 3>mass with them as they stream outward, they effectively drag

561
00:27:06.920 --> 00:27:11.279
<v Speaker 3>a tiny amount of gravitational influence with them. Wow. This process,

562
00:27:11.480 --> 00:27:14.720
<v Speaker 3>known as free streaming, has a subtle but undeniable effect

563
00:27:14.720 --> 00:27:18.160
<v Speaker 3>on the formation of the cosmic web. It physically smears

564
00:27:18.160 --> 00:27:19.480
<v Speaker 3>out the distribution of matter.

565
00:27:19.680 --> 00:27:22.319
<v Speaker 2>It blurs the sharp edges of the galaxy clusters.

566
00:27:22.400 --> 00:27:25.279
<v Speaker 3>It suppresses the clumping of matter on certain specific scales.

567
00:27:25.799 --> 00:27:28.759
<v Speaker 3>Because Dehi's map of where galaxies are positioned is so

568
00:27:28.960 --> 00:27:33.440
<v Speaker 3>outrageously precise, researchers can scan the data looking for that

569
00:27:33.559 --> 00:27:35.640
<v Speaker 3>exact statistical smearing effect.

570
00:27:35.680 --> 00:27:36.640
<v Speaker 2>That is incredible.

571
00:27:36.720 --> 00:27:39.079
<v Speaker 3>The degree to which the cosmic web has been smoothed

572
00:27:39.079 --> 00:27:42.279
<v Speaker 3>out serves as a direct measurement of how much mass

573
00:27:42.319 --> 00:27:43.480
<v Speaker 3>the neutrinos were carrying.

574
00:27:43.519 --> 00:27:47.119
<v Speaker 2>That is profound. You are using the gravitational architecture of

575
00:27:47.160 --> 00:27:50.519
<v Speaker 2>the entire observable universe as a scale to weigh a

576
00:27:50.559 --> 00:27:51.720
<v Speaker 2>subatomic particle.

577
00:27:51.960 --> 00:27:54.920
<v Speaker 3>It highlights how deeply interconnected the physics of the vacuum

578
00:27:54.920 --> 00:27:57.960
<v Speaker 3>are with the physics of the very large It really does.

579
00:27:58.160 --> 00:28:01.160
<v Speaker 2>Doctor Natither mentioned that we have barely scratch the surface

580
00:28:01.160 --> 00:28:03.680
<v Speaker 2>of what this data set can do, and this neutrino

581
00:28:03.759 --> 00:28:06.160
<v Speaker 2>weighing is the perfect example, and it is.

582
00:28:06.160 --> 00:28:11.920
<v Speaker 3>Exactly that multidisciplinary utility that justifies extending the instrument's operational life.

583
00:28:11.960 --> 00:28:13.200
<v Speaker 2>Wait, they're keeping it going.

584
00:28:13.440 --> 00:28:16.759
<v Speaker 3>Oh, yes, the initial five year parameters have been fulfilled.

585
00:28:17.200 --> 00:28:21.599
<v Speaker 3>The primary map is complete, but the hardware is functioning flawlessly.

586
00:28:21.200 --> 00:28:24.400
<v Speaker 2>So they aren't turning the robots off. They are pushing

587
00:28:24.559 --> 00:28:26.000
<v Speaker 2>directly into the unknown.

588
00:28:26.240 --> 00:28:30.000
<v Speaker 3>From twenty twenty four through twenty twenty eight, DSi is

589
00:28:30.079 --> 00:28:31.839
<v Speaker 3>officially expanding its mission.

590
00:28:31.960 --> 00:28:35.640
<v Speaker 2>I love that they hit forty seven million targets blue

591
00:28:35.680 --> 00:28:39.640
<v Speaker 2>past their goals and immediately decided to map the absolute hardest,

592
00:28:39.680 --> 00:28:42.240
<v Speaker 2>most frustrating parts of the sky just to see what

593
00:28:42.240 --> 00:28:43.039
<v Speaker 2>they can extract.

594
00:28:43.240 --> 00:28:46.319
<v Speaker 3>The expansion of the survey area is significant. They are

595
00:28:46.319 --> 00:28:49.680
<v Speaker 3>increasing the maps coverage by roughly twenty percent, growing the

596
00:28:49.680 --> 00:28:53.960
<v Speaker 3>observed footprint from fourteen thousand square degrees to seventeen thousand

597
00:28:53.960 --> 00:28:54.599
<v Speaker 3>square degrees.

598
00:28:54.720 --> 00:28:57.359
<v Speaker 2>Let's contextualize a square degree because it's not a metric

599
00:28:57.400 --> 00:28:59.400
<v Speaker 2>you use at the grocery store. It's not if you

600
00:28:59.480 --> 00:29:02.680
<v Speaker 2>go outside and look at a full moon. The surface

601
00:29:02.720 --> 00:29:05.119
<v Speaker 2>area that the moon occupies in your field of vision

602
00:29:05.319 --> 00:29:07.680
<v Speaker 2>is about zero point two square degrees.

603
00:29:08.079 --> 00:29:08.359
<v Speaker 3>Right.

604
00:29:08.599 --> 00:29:11.839
<v Speaker 2>The entire sphere of the sky surrounding the Earth is

605
00:29:11.880 --> 00:29:14.960
<v Speaker 2>a bit over forty one thousand square degrees, So an

606
00:29:15.039 --> 00:29:18.119
<v Speaker 2>expansion of three thousand square degrees is the equivalent of

607
00:29:18.160 --> 00:29:21.039
<v Speaker 2>adding a swathe of the sky roughly the size of

608
00:29:21.119 --> 00:29:22.720
<v Speaker 2>fifteen thousand full moons.

609
00:29:23.000 --> 00:29:26.599
<v Speaker 3>It is a massive undertaking, particularly because they are actively

610
00:29:26.640 --> 00:29:31.839
<v Speaker 3>targeting regions that were previously deemed too difficult or inefficient.

611
00:29:31.319 --> 00:29:34.119
<v Speaker 2>To map, which brings us back to that massive black

612
00:29:34.160 --> 00:29:37.799
<v Speaker 2>blind spot we discussed earlier, the plane of the Milky Way.

613
00:29:38.039 --> 00:29:40.119
<v Speaker 3>They are attempting to thread the needle through the zone

614
00:29:40.119 --> 00:29:40.759
<v Speaker 3>of avoidance.

615
00:29:40.960 --> 00:29:43.680
<v Speaker 2>But how we talked about how the dust and stellar

616
00:29:43.759 --> 00:29:46.440
<v Speaker 2>crowding of our own galaxy obscure the faint light from

617
00:29:46.480 --> 00:29:47.400
<v Speaker 2>the distant universe.

618
00:29:47.480 --> 00:29:51.160
<v Speaker 3>We did, But the instrumentation on DSi is sensitive enough

619
00:29:51.279 --> 00:29:54.759
<v Speaker 3>and the background algorithms have become sophisticated enough that they

620
00:29:54.759 --> 00:29:57.839
<v Speaker 3>believe they can extract viable spectroscopic data from some of

621
00:29:57.839 --> 00:29:59.240
<v Speaker 3>those highly obscured regions.

622
00:29:59.319 --> 00:30:02.240
<v Speaker 2>They are literally staring straight into the high beam headlights

623
00:30:02.279 --> 00:30:04.160
<v Speaker 2>to find the fireflies.

624
00:30:03.759 --> 00:30:06.640
<v Speaker 3>They really are. But that's only one of the challenging regions.

625
00:30:06.680 --> 00:30:09.160
<v Speaker 3>What's the other The second area they are expanding into

626
00:30:09.519 --> 00:30:12.400
<v Speaker 3>pushes further to the south, and the obstacle there isn't

627
00:30:12.400 --> 00:30:16.160
<v Speaker 3>interstellar dust. It's our own planet's atmosphere.

628
00:30:16.200 --> 00:30:18.960
<v Speaker 2>Oh, because kit Peak is in Arizona exactly.

629
00:30:19.279 --> 00:30:23.440
<v Speaker 3>Operating a ground based telescope involves constantly fighting the Earth's atmosphere.

630
00:30:23.799 --> 00:30:27.839
<v Speaker 3>To observe targets further south, the telescope must angle lower

631
00:30:27.920 --> 00:30:29.319
<v Speaker 3>toward the horizon, so you.

632
00:30:29.319 --> 00:30:32.160
<v Speaker 2>Are no longer looking straight up through the thinnest part

633
00:30:32.200 --> 00:30:35.039
<v Speaker 2>of the atmosphere. You are looking at a sharp angle

634
00:30:35.480 --> 00:30:37.519
<v Speaker 2>through a massive cross section of air.

635
00:30:37.880 --> 00:30:41.119
<v Speaker 3>The term is air mass. When you look toward the horizon,

636
00:30:41.559 --> 00:30:44.160
<v Speaker 3>the light from a distant galaxy has to travel through

637
00:30:44.160 --> 00:30:48.799
<v Speaker 3>a much thicker layer of turbulent, shifting atmospheric gases before

638
00:30:48.839 --> 00:30:50.279
<v Speaker 3>it hits the primary.

639
00:30:49.839 --> 00:30:52.240
<v Speaker 2>Mirror, which causes distortion.

640
00:30:52.000 --> 00:30:56.559
<v Speaker 3>Massive distortion. It causes atmospheric refraction and significant scattering of

641
00:30:56.599 --> 00:30:57.359
<v Speaker 3>the optical light.

642
00:30:57.640 --> 00:31:01.160
<v Speaker 2>It's why stars twinkle violently when they're low on the horizon,

643
00:31:01.319 --> 00:31:03.960
<v Speaker 2>but look steady when they are straight overhead.

644
00:31:03.680 --> 00:31:08.039
<v Speaker 3>Exactly, And for an instrument relying on the precise separation

645
00:31:08.160 --> 00:31:12.440
<v Speaker 3>of light frequencies to measure microscopic ridshifts. That atmosphere twinkling

646
00:31:12.599 --> 00:31:16.559
<v Speaker 3>is incredibly destructive. The data becomes noisy.

647
00:31:16.400 --> 00:31:17.799
<v Speaker 2>But they're going for it anyway.

648
00:31:18.119 --> 00:31:20.839
<v Speaker 3>But again, the analytical pipelines have improved to the point

649
00:31:20.880 --> 00:31:24.000
<v Speaker 3>where researchers are confident they can clean that noisy data

650
00:31:24.279 --> 00:31:27.440
<v Speaker 3>and push the map further south than initially thought possible.

651
00:31:27.720 --> 00:31:30.440
<v Speaker 2>And it's not just about pushing the borders outward, is it.

652
00:31:30.559 --> 00:31:34.480
<v Speaker 2>They are also turning the instrument back inward, revisiting patches

653
00:31:34.480 --> 00:31:36.200
<v Speaker 2>of the sky they've already mapped.

654
00:31:36.039 --> 00:31:40.640
<v Speaker 3>Because the initial sweep naturally prioritized the most prominent, easily

655
00:31:40.680 --> 00:31:44.240
<v Speaker 3>identifiable targets to build the structural foundation of the map.

656
00:31:44.599 --> 00:31:47.559
<v Speaker 3>Now they are hunting for a specific class of object

657
00:31:47.680 --> 00:31:49.480
<v Speaker 3>to increase the density of the data.

658
00:31:49.519 --> 00:31:51.559
<v Speaker 2>They are looking for luminous red galaxies.

659
00:31:51.559 --> 00:31:56.119
<v Speaker 3>They're massive, incredibly ancient elliptical galaxies. They have exhausted their

660
00:31:56.160 --> 00:31:59.799
<v Speaker 3>star forming gas, meaning they are populated by older.

661
00:31:59.480 --> 00:32:01.319
<v Speaker 2>Redders, which makes them hard to see.

662
00:32:01.319 --> 00:32:04.240
<v Speaker 3>It very faint and difficult to isolate, but they serve

663
00:32:04.279 --> 00:32:07.039
<v Speaker 3>as excellent tracers for the mass of dark matter halos

664
00:32:07.319 --> 00:32:10.799
<v Speaker 3>that dictate the structure of the cosmic web by layering

665
00:32:10.799 --> 00:32:14.480
<v Speaker 3>the locations of these elusive red galaxies into the existing data.

666
00:32:14.599 --> 00:32:18.119
<v Speaker 3>They are essentially upgrading the resolution of the map, taking.

667
00:32:17.759 --> 00:32:21.160
<v Speaker 2>A four K map and cramming even more pixels into it. Exactly,

668
00:32:21.160 --> 00:32:23.839
<v Speaker 2>but practically speaking, how do you manage that you have

669
00:32:23.880 --> 00:32:26.920
<v Speaker 2>a telescope that needs to execute its primary tracking, but

670
00:32:27.000 --> 00:32:29.000
<v Speaker 2>now you are asking it to fight the milky ways,

671
00:32:29.039 --> 00:32:32.640
<v Speaker 2>glare peer through miles of turbulent atmosphere on the horizon,

672
00:32:33.160 --> 00:32:36.640
<v Speaker 2>and go hunting for faint red ghosts and previously mapped areas.

673
00:32:37.359 --> 00:32:40.480
<v Speaker 3>This raises an important question about efficiency. How do we

674
00:32:40.599 --> 00:32:44.240
<v Speaker 3>ensure it all works? It requires seamless logistical integration.

675
00:32:44.440 --> 00:32:46.079
<v Speaker 2>The software must be working overtime.

676
00:32:46.200 --> 00:32:49.200
<v Speaker 3>The expanded mission doesn't operate in a vacuum. These new,

677
00:32:49.279 --> 00:32:52.880
<v Speaker 3>incredibly challenging observations are being interwoven directly into the ongoing

678
00:32:52.920 --> 00:32:57.599
<v Speaker 3>observational program. The scheduling software constantly calculates the optimal sequence

679
00:32:57.640 --> 00:33:00.319
<v Speaker 3>of targets to ensure that the five thousand Rouws body

680
00:33:00.400 --> 00:33:04.839
<v Speaker 3>positioners are never idle. It is relentless optimization of telescope time.

681
00:33:05.000 --> 00:33:08.599
<v Speaker 2>It really stands as a monument to human curiosity. We

682
00:33:08.720 --> 00:33:13.240
<v Speaker 2>built a machine of unprecedented power, finished the largest cartography

683
00:33:13.279 --> 00:33:16.599
<v Speaker 2>project in history early and the immediate reaction wasn't to

684
00:33:16.640 --> 00:33:17.680
<v Speaker 2>celebrate and go home.

685
00:33:17.839 --> 00:33:19.519
<v Speaker 3>No, the reaction was to dig deeper.

686
00:33:19.759 --> 00:33:23.200
<v Speaker 2>It was to push the machine harder into the darkest,

687
00:33:23.319 --> 00:33:25.920
<v Speaker 2>dirtiest parts of the sky, just to see what the

688
00:33:25.920 --> 00:33:27.480
<v Speaker 2>ghost is doing in the shadows.

689
00:33:27.599 --> 00:33:31.200
<v Speaker 3>It reflects the urgency of the questions being asked. When

690
00:33:31.200 --> 00:33:34.680
<v Speaker 3>the foundational rules of your field are suddenly called into question,

691
00:33:35.079 --> 00:33:37.960
<v Speaker 3>you don't turn off the instrument. You collect more data.

692
00:33:38.079 --> 00:33:41.559
<v Speaker 2>Which brings this entire journey full circle. We started this

693
00:33:41.640 --> 00:33:44.200
<v Speaker 2>discussion standing on a dark night looking up at the

694
00:33:44.200 --> 00:33:47.119
<v Speaker 2>Little Dipper, but intellectually we've traveled from a mountain peak

695
00:33:47.160 --> 00:33:50.759
<v Speaker 2>in Arizona to the edge of the observable universe. Tracing

696
00:33:50.799 --> 00:33:55.319
<v Speaker 2>the ancient light of forty seven million galaxies across eleven billion.

697
00:33:55.079 --> 00:33:58.799
<v Speaker 3>Years, we have watched the most comprehensive measurement of the

698
00:33:58.839 --> 00:34:02.319
<v Speaker 3>cosmic dug of war ever recorded. We've seen how tracking

699
00:34:02.400 --> 00:34:04.920
<v Speaker 3>the structural evolution of the universe from the tightly bound

700
00:34:04.960 --> 00:34:08.679
<v Speaker 3>early Epex to the vastly expanded modern era has revealed

701
00:34:08.679 --> 00:34:10.360
<v Speaker 3>a fundamental anomaly.

702
00:34:10.199 --> 00:34:14.039
<v Speaker 2>An anomaly suggesting that dark energy, the dominant force of reality,

703
00:34:14.519 --> 00:34:18.800
<v Speaker 2>might not be an unwavering mathematical constant, but an actively

704
00:34:18.920 --> 00:34:22.079
<v Speaker 2>evolving pressure. And that is where I want to leave you.

705
00:34:22.159 --> 00:34:24.719
<v Speaker 2>That's a lot to process, it really is. When we

706
00:34:24.719 --> 00:34:27.000
<v Speaker 2>think about the laws of physics, we tend to conceptualize

707
00:34:27.039 --> 00:34:29.440
<v Speaker 2>them as a rigid rule book, a set of mathematical

708
00:34:29.480 --> 00:34:31.800
<v Speaker 2>constants that were etched into stone at the exact moment

709
00:34:31.840 --> 00:34:34.360
<v Speaker 2>of the Big Bang, governing everything from the speed of

710
00:34:34.400 --> 00:34:37.280
<v Speaker 2>light to the pull of gravity. Our job, as we

711
00:34:37.360 --> 00:34:39.920
<v Speaker 2>understood it, was simply to build better machines to read

712
00:34:39.960 --> 00:34:43.679
<v Speaker 2>those static rules. But if seventy percent of the universe

713
00:34:43.760 --> 00:34:46.320
<v Speaker 2>is driven by a force that shifts and changes as

714
00:34:46.360 --> 00:34:50.320
<v Speaker 2>time passes, it forces a deeply provocative question. If the

715
00:34:50.360 --> 00:34:52.960
<v Speaker 2>constants of the universe are capable of evolving along with

716
00:34:53.000 --> 00:34:55.920
<v Speaker 2>the universe itself, perhaps we aren't trying to decipher a

717
00:34:55.960 --> 00:34:59.159
<v Speaker 2>finished static rulebook at all. Perhaps the universe is still

718
00:34:59.159 --> 00:35:02.280
<v Speaker 2>actively writing it. Keep that flexibility of reality in mind

719
00:35:02.320 --> 00:35:03.800
<v Speaker 2>the next time you look up at the night sky.
