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 --> 00:00:23.800
<v Speaker 1>slumber under the night sky.

7
00:00:26.920 --> 00:00:29.440
<v Speaker 2>You know, when you think about uncovering the past on Earth,

8
00:00:30.640 --> 00:00:34.280
<v Speaker 2>whether you are looking at like a core sample of

9
00:00:34.280 --> 00:00:38.320
<v Speaker 2>glacial ice or the rings of an ancient bristle comb pine,

10
00:00:38.799 --> 00:00:43.079
<v Speaker 2>there is this fundamental expectation of structural layering. Time basically

11
00:00:43.200 --> 00:00:46.399
<v Speaker 2>leaves a physical tactile mark. You dig down past the

12
00:00:46.439 --> 00:00:49.079
<v Speaker 2>top soil, you hit a layer of limestone from the

13
00:00:49.159 --> 00:00:53.320
<v Speaker 2>Jurassic period, and you have this, well, you have a

14
00:00:53.479 --> 00:00:57.960
<v Speaker 2>chronological anchor. Time is buried in a specific measurable order.

15
00:00:58.119 --> 00:01:01.920
<v Speaker 3>Yeah, exactly. The Earth act as a physical ledger. We

16
00:01:01.960 --> 00:01:05.000
<v Speaker 3>rely really heavily on that spatial representation of time because

17
00:01:05.079 --> 00:01:08.480
<v Speaker 3>you know, it grounds our understanding of history. We intuitively

18
00:01:08.519 --> 00:01:12.200
<v Speaker 3>grasp that deeper usually means older, and we can test

19
00:01:12.239 --> 00:01:15.120
<v Speaker 3>the material at each stratum to build a reliable timeline

20
00:01:15.159 --> 00:01:16.359
<v Speaker 3>of planetary evolution.

21
00:01:16.640 --> 00:01:18.359
<v Speaker 2>But the moment that you point a telescope at the

22
00:01:18.439 --> 00:01:22.439
<v Speaker 2>night sky, that comforting geological layer cake just well, it

23
00:01:22.480 --> 00:01:25.040
<v Speaker 2>completely vanishes, it really does. We're suddenly looking at a

24
00:01:25.079 --> 00:01:27.480
<v Speaker 2>cosmic landscape that is, to the naked eye, and even

25
00:01:27.519 --> 00:01:31.200
<v Speaker 2>to our most powerful traditional instruments, completely temporally flat.

26
00:01:31.280 --> 00:01:32.480
<v Speaker 3>Right, it's completely flattened out.

27
00:01:32.640 --> 00:01:35.439
<v Speaker 2>You look up and everything appears to be happening right now,

28
00:01:35.680 --> 00:01:38.879
<v Speaker 2>all at once projected onto the inside of a sphere.

29
00:01:39.000 --> 00:01:42.959
<v Speaker 3>It is the ultimate temporal illusion. Really, when we observe

30
00:01:43.079 --> 00:01:46.920
<v Speaker 3>a starfield, we are bombarded by photons that left their

31
00:01:46.959 --> 00:01:50.519
<v Speaker 3>sources at wildly different times. Yeah, I mean, we might

32
00:01:50.560 --> 00:01:53.040
<v Speaker 3>see a star that just ignited a million years ago

33
00:01:53.159 --> 00:01:55.680
<v Speaker 3>right next to a dying red giant that has been

34
00:01:55.719 --> 00:02:00.519
<v Speaker 3>burning for ten billion years, and to us they are

35
00:02:00.560 --> 00:02:05.079
<v Speaker 3>just two adjacent pinpricks of light on a flattened canvas, right.

36
00:02:05.120 --> 00:02:07.439
<v Speaker 2>Because we lack that physical z axis of.

37
00:02:07.400 --> 00:02:09.919
<v Speaker 3>Time exactly, we don't have depth when it comes to

38
00:02:10.000 --> 00:02:11.039
<v Speaker 3>time in the sky.

39
00:02:11.159 --> 00:02:14.840
<v Speaker 2>Which means in astronomy, the absolute hardest thing to figure

40
00:02:14.879 --> 00:02:17.000
<v Speaker 2>out isn't what an object is, but when it is.

41
00:02:17.159 --> 00:02:20.840
<v Speaker 3>Yes, age is the ultimate hidden variable in space and.

42
00:02:20.840 --> 00:02:24.560
<v Speaker 2>Without knowing the age of a celestial object. You were

43
00:02:24.639 --> 00:02:27.319
<v Speaker 2>essentially looking at a photograph of a stranger and trying

44
00:02:27.319 --> 00:02:29.960
<v Speaker 2>to deduce their entire life story, right way to put it,

45
00:02:30.039 --> 00:02:33.680
<v Speaker 2>like their internal biology, their future. Just from a single snapshot.

46
00:02:33.919 --> 00:02:36.680
<v Speaker 2>You don't know the internal processes that are currently dominating

47
00:02:36.680 --> 00:02:37.360
<v Speaker 2>their existence.

48
00:02:37.800 --> 00:02:42.800
<v Speaker 3>Because age dictates nearly every physical characteristic of a celestial body.

49
00:02:43.319 --> 00:02:47.759
<v Speaker 3>It dictates the internal structure, the temperature, the atmosphere, chemistry,

50
00:02:47.800 --> 00:02:50.199
<v Speaker 3>and the evolutionary trajectory.

51
00:02:50.280 --> 00:02:50.879
<v Speaker 2>Wow.

52
00:02:50.919 --> 00:02:54.879
<v Speaker 3>Without an age, you cannot accurately model the physics of

53
00:02:54.919 --> 00:02:58.000
<v Speaker 3>what you are actually looking at. You are simply cataloging

54
00:02:58.080 --> 00:03:02.879
<v Speaker 3>static properties without understanding the dynamic timeline that produces them.

55
00:03:03.120 --> 00:03:07.199
<v Speaker 2>So today we are going to explore a massive recent

56
00:03:07.319 --> 00:03:12.680
<v Speaker 2>breakthrough where astrophysicists finally managed to crack this cosmic clock.

57
00:03:12.800 --> 00:03:15.599
<v Speaker 2>And it's an incredible breakthrough, it really is, and they

58
00:03:15.639 --> 00:03:17.879
<v Speaker 2>managed to do it on one of the most highly elusive,

59
00:03:18.400 --> 00:03:21.840
<v Speaker 2>incredibly frustrating types of celestial objects in the universe.

60
00:03:21.919 --> 00:03:23.280
<v Speaker 3>Oh, absolutely frustrating.

61
00:03:23.400 --> 00:03:26.800
<v Speaker 2>We're going to explore the strange boundary between stars and planets,

62
00:03:27.120 --> 00:03:30.879
<v Speaker 2>will learn how the physics of acoustic resonance literally starquakes

63
00:03:30.960 --> 00:03:32.840
<v Speaker 2>solved a multi decade mystery.

64
00:03:32.560 --> 00:03:34.560
<v Speaker 3>Which sounds like science fiction, but it's real.

65
00:03:34.599 --> 00:03:37.960
<v Speaker 2>Right, and we will discover how one single finding is

66
00:03:38.080 --> 00:03:42.280
<v Speaker 2>rewriting our understanding of cosmic time and evolution. Okay, let's

67
00:03:42.319 --> 00:03:46.199
<v Speaker 2>unpack this sound, starting with the troublemakers themselves, the boundary

68
00:03:46.280 --> 00:03:49.240
<v Speaker 2>dwellers brown dwarfs.

69
00:03:49.039 --> 00:03:55.039
<v Speaker 3>Ah, brown dwarfs. They occupy a highly ambiguous mass range.

70
00:03:55.080 --> 00:03:58.639
<v Speaker 3>They exist in this transitional void between the heaviest gas

71
00:03:58.680 --> 00:04:01.360
<v Speaker 3>giant planets and the light main sequence.

72
00:04:00.960 --> 00:04:03.879
<v Speaker 2>Stars, so they're stuck in the middle exactly.

73
00:04:04.199 --> 00:04:07.280
<v Speaker 3>Generally, we classify them as objects with a mass between

74
00:04:07.520 --> 00:04:10.800
<v Speaker 3>roughly thirteen and eighty times the mass of Jupiter.

75
00:04:10.960 --> 00:04:13.599
<v Speaker 2>Okay, So, as you know, for a celestial body to

76
00:04:13.639 --> 00:04:17.839
<v Speaker 2>become a true star, it has to achieve hydrostatic equilibrium. Right.

77
00:04:17.879 --> 00:04:20.759
<v Speaker 2>You have a collapsing cloud of molecular gas. Gravity is

78
00:04:20.800 --> 00:04:24.160
<v Speaker 2>crushing that mass inward, and the core pressure and temperature

79
00:04:24.240 --> 00:04:24.959
<v Speaker 2>just skyrock.

80
00:04:25.040 --> 00:04:26.519
<v Speaker 3>Yeah, it gets incredibly hot.

81
00:04:26.759 --> 00:04:29.720
<v Speaker 2>And if that object has enough mass, specifically, if it

82
00:04:29.759 --> 00:04:33.399
<v Speaker 2>crosses that threshold of about eighty Jupiter masses, the core

83
00:04:33.439 --> 00:04:37.600
<v Speaker 2>temperature reaches millions of degrees and sustained hydrogen one fusion ignites.

84
00:04:37.720 --> 00:04:41.160
<v Speaker 3>And that is the key that outward radiation pressure perfectly

85
00:04:41.240 --> 00:04:42.839
<v Speaker 3>balances the inward pull of gravity.

86
00:04:42.920 --> 00:04:44.199
<v Speaker 2>Right, they balance out that.

87
00:04:44.279 --> 00:04:48.240
<v Speaker 3>Sustained hydrogen fusion is the defining characteristic of a main

88
00:04:48.319 --> 00:04:53.439
<v Speaker 3>sequence star. It provides a constant, massive internal heat source

89
00:04:53.839 --> 00:04:57.519
<v Speaker 3>that allows the star to shine steadily for billions of years.

90
00:04:57.879 --> 00:05:00.759
<v Speaker 2>But a brown dwarf simply fails to reach that critical

91
00:05:00.759 --> 00:05:01.439
<v Speaker 2>mass threshold.

92
00:05:01.519 --> 00:05:04.120
<v Speaker 3>Right, Yeah, it just misses the mark. It forms from

93
00:05:04.160 --> 00:05:08.199
<v Speaker 3>the same collapsing molecular clouds as stars do. It gathers mass,

94
00:05:08.439 --> 00:05:11.600
<v Speaker 3>and its core heats up significantly under the crushing weight

95
00:05:11.639 --> 00:05:13.120
<v Speaker 3>of its own gravity.

96
00:05:12.839 --> 00:05:14.480
<v Speaker 2>Because there's still a lot of mass there.

97
00:05:14.399 --> 00:05:17.000
<v Speaker 3>A lot of mass. Yeah. But before the core can

98
00:05:17.040 --> 00:05:20.240
<v Speaker 3>get hot enough and dense enough to ignite stable hydrogen fusion,

99
00:05:20.399 --> 00:05:22.680
<v Speaker 3>the collapse is halted by quantum mechanics.

100
00:05:22.720 --> 00:05:26.600
<v Speaker 2>Wait, halted by quantum mechanics, You mean electron degeneracy pressure exactly.

101
00:05:26.959 --> 00:05:29.480
<v Speaker 3>The electrons and the core get packed so tightly together

102
00:05:29.519 --> 00:05:31.480
<v Speaker 3>that the poly exclusion principle kicks in.

103
00:05:31.680 --> 00:05:34.319
<v Speaker 2>Right, They refuse to occupy the same quantum state, yes.

104
00:05:34.319 --> 00:05:38.000
<v Speaker 3>Which creates an outward physical pressure that completely halts any

105
00:05:38.040 --> 00:05:39.480
<v Speaker 3>further gravitational collapse.

106
00:05:39.560 --> 00:05:41.160
<v Speaker 2>So the core becomes degenerate.

107
00:05:41.439 --> 00:05:44.040
<v Speaker 3>It does, it locks the brown dwarf into a state

108
00:05:44.079 --> 00:05:46.800
<v Speaker 3>where it can never achieve the core conditions required for

109
00:05:46.959 --> 00:05:48.519
<v Speaker 3>main sequence hydrogen fusion.

110
00:05:48.879 --> 00:05:50.759
<v Speaker 2>That's fascinating. So it's just stuck.

111
00:05:51.399 --> 00:05:53.879
<v Speaker 3>Yeah, I mean some of the more massive brown dwarfs

112
00:05:53.959 --> 00:05:58.160
<v Speaker 3>might briefly fuse deuterium, which is a heavier isotope of hydrogen,

113
00:05:58.920 --> 00:06:03.680
<v Speaker 3>or even lithium. Okay, but those fuel sources are incredibly sparse,

114
00:06:03.800 --> 00:06:07.439
<v Speaker 3>and they burn out very quickly in astronomical.

115
00:06:06.800 --> 00:06:08.120
<v Speaker 2>Terms, like a flash in the pan.

116
00:06:08.399 --> 00:06:12.199
<v Speaker 3>Precisely once that initial burst is over, the brown dwarf

117
00:06:12.319 --> 00:06:13.519
<v Speaker 3>never truly turns on.

118
00:06:13.800 --> 00:06:16.759
<v Speaker 2>It's essentially a cosmic engine that flooded before it could

119
00:06:16.800 --> 00:06:17.240
<v Speaker 2>turn over.

120
00:06:17.519 --> 00:06:19.040
<v Speaker 3>That is a perfect analogy.

121
00:06:19.199 --> 00:06:22.040
<v Speaker 2>So because they lack that internal nuclear furnace to maintain

122
00:06:22.079 --> 00:06:26.279
<v Speaker 2>this steady temperature, they spend their entire existence slowly fading

123
00:06:26.879 --> 00:06:29.800
<v Speaker 2>like they are born hot from the primordial energy of

124
00:06:29.839 --> 00:06:34.279
<v Speaker 2>their gravitational collapse, and then they spend billions of years

125
00:06:34.319 --> 00:06:36.959
<v Speaker 2>just radiating that heat away into the vacuum space.

126
00:06:37.040 --> 00:06:40.800
<v Speaker 3>Yeah, they just get colder and darker forever.

127
00:06:40.560 --> 00:06:42.160
<v Speaker 2>Which sounds incredibly depressing.

128
00:06:42.279 --> 00:06:45.360
<v Speaker 3>It's a lonely existence, but from a scientific standpoint, that

129
00:06:45.399 --> 00:06:49.000
<v Speaker 3>continuous cooling curve is precisely what creates the massive headache

130
00:06:49.040 --> 00:06:50.879
<v Speaker 3>for astrophysicists trying to study them.

131
00:06:51.079 --> 00:06:51.680
<v Speaker 2>Why is that?

132
00:06:51.959 --> 00:06:55.279
<v Speaker 3>Well, with a main sequence star like oursun the sustained

133
00:06:55.360 --> 00:06:59.680
<v Speaker 3>fusion keeps the stars luminosity and temperature relatively stable for

134
00:07:00.160 --> 00:07:03.439
<v Speaker 3>billions of years. We can plot it on a diagram

135
00:07:03.439 --> 00:07:04.720
<v Speaker 3>and understand its life cycle.

136
00:07:04.839 --> 00:07:05.600
<v Speaker 2>Oh, I see, But.

137
00:07:05.639 --> 00:07:09.319
<v Speaker 3>A brown dwarf is constantly changing because its temperature and

138
00:07:09.399 --> 00:07:12.879
<v Speaker 3>luminosity are always dropping. You cannot simply look at its

139
00:07:12.920 --> 00:07:16.680
<v Speaker 3>current thermal emission and instantly know its evolutionary state.

140
00:07:16.879 --> 00:07:19.360
<v Speaker 2>Wait, let me push back on that logic for a second. Sure,

141
00:07:19.519 --> 00:07:22.519
<v Speaker 2>if a brown dwarf is literally just radiating its initial

142
00:07:22.560 --> 00:07:26.519
<v Speaker 2>heat over time, we have incredibly sensitive thermal cameras, right

143
00:07:26.639 --> 00:07:30.439
<v Speaker 2>we do. We use infrared observatories like JWST to measure

144
00:07:30.480 --> 00:07:34.680
<v Speaker 2>thermal signatures across the galaxy all the time. Can't we

145
00:07:34.800 --> 00:07:37.879
<v Speaker 2>just measure the exact infrared heat signature of the brown dwarf,

146
00:07:38.480 --> 00:07:41.879
<v Speaker 2>calculate its physical volume, and backtrack the thermo dynamics to

147
00:07:41.920 --> 00:07:42.399
<v Speaker 2>minute one?

148
00:07:42.639 --> 00:07:44.959
<v Speaker 3>It seems like we should be able to Yeah, Like.

149
00:07:44.879 --> 00:07:47.600
<v Speaker 2>Why can't we just take its temperature and derive the age?

150
00:07:47.720 --> 00:07:50.439
<v Speaker 3>You could calculate the H that way, provided every single

151
00:07:50.480 --> 00:07:53.399
<v Speaker 3>brown dwarf started its life with the exact same initial

152
00:07:53.439 --> 00:07:56.759
<v Speaker 3>mass and the exact same reservoir of thermal energy.

153
00:07:56.680 --> 00:07:58.279
<v Speaker 2>H And I'm guessing they don't.

154
00:07:58.480 --> 00:08:01.439
<v Speaker 3>They absolutely don't. And this is where that electron degeneracy

155
00:08:01.480 --> 00:08:06.439
<v Speaker 3>pressure creates an observational nightmare. How So, because a brown

156
00:08:06.519 --> 00:08:10.560
<v Speaker 3>dwarf is supported by quantum degeneracy rather than thermal expansion,

157
00:08:10.959 --> 00:08:14.439
<v Speaker 3>its physical radius is largely independent of its mass.

158
00:08:14.519 --> 00:08:16.800
<v Speaker 2>Wait wait, wait, are you saying a lightweight brown dwarf

159
00:08:16.839 --> 00:08:20.040
<v Speaker 2>and a massive brown dwarf or the exact same size.

160
00:08:19.800 --> 00:08:21.560
<v Speaker 3>Roughly the same physical volume.

161
00:08:21.639 --> 00:08:23.160
<v Speaker 2>Yes, that is wild.

162
00:08:23.480 --> 00:08:26.720
<v Speaker 3>It really is counterintuitive. A brown dwarf at fifteen Jupiter

163
00:08:26.759 --> 00:08:29.800
<v Speaker 3>masses has approximately the same radius as a brown dwarf

164
00:08:29.839 --> 00:08:31.639
<v Speaker 3>at seventy five jupiter.

165
00:08:31.279 --> 00:08:33.360
<v Speaker 2>Masses, So if I'm looking at it through a telescope,

166
00:08:33.399 --> 00:08:35.000
<v Speaker 2>I can't tell the difference just based.

167
00:08:34.720 --> 00:08:38.559
<v Speaker 3>On size exactly. So imagine you observe a brown dwarf

168
00:08:38.600 --> 00:08:42.240
<v Speaker 3>with a measured surface temperature of five hundred kelvin. Because

169
00:08:42.240 --> 00:08:45.080
<v Speaker 3>you can't determine its mass just by looking at its size,

170
00:08:45.480 --> 00:08:47.879
<v Speaker 3>you are instantly faced with a paradox.

171
00:08:48.200 --> 00:08:51.120
<v Speaker 2>I see the problem you just don't know the starting conditions, right.

172
00:08:51.519 --> 00:08:54.919
<v Speaker 3>Is this a very lightweight fifteen jupiter mass brown dwarf

173
00:08:54.960 --> 00:08:59.200
<v Speaker 3>that formed relatively recently, say, a few hundred million years ago,

174
00:08:59.360 --> 00:09:01.840
<v Speaker 3>and hasn't had much time to cool down? Or is

175
00:09:01.919 --> 00:09:06.039
<v Speaker 3>this a massive seventy jupiter mass brown dwarf that formed

176
00:09:06.240 --> 00:09:09.720
<v Speaker 3>ten billion years ago, started with a massive reservoir of

177
00:09:09.759 --> 00:09:13.200
<v Speaker 3>thermal energy and has been cooling down for an eternity

178
00:09:13.360 --> 00:09:16.080
<v Speaker 3>to finally reach that same five hundred kelvin mark.

179
00:09:16.480 --> 00:09:19.000
<v Speaker 2>Wow, So the low mass young object and the high

180
00:09:19.039 --> 00:09:23.000
<v Speaker 2>mass ancient object look identical to our photometric instrument.

181
00:09:23.120 --> 00:09:26.080
<v Speaker 3>You look exactly the same. That is a severe degeneracy problem.

182
00:09:26.120 --> 00:09:27.559
<v Speaker 2>It's an absolute catch twenty two.

183
00:09:27.759 --> 00:09:28.360
<v Speaker 3>It really is.

184
00:09:28.639 --> 00:09:32.080
<v Speaker 2>To understand how a brown dwarf evolves. To map its

185
00:09:32.120 --> 00:09:35.840
<v Speaker 2>specific cooling rate and figure out its mass, you absolutely

186
00:09:35.879 --> 00:09:39.279
<v Speaker 2>need to know its precise age, yes, but to determine

187
00:09:39.320 --> 00:09:42.399
<v Speaker 2>its exact age from its current temperature, you already need

188
00:09:42.440 --> 00:09:46.240
<v Speaker 2>to know its mass and its specific evolutionary cooling track exactly.

189
00:09:46.279 --> 00:09:49.039
<v Speaker 3>You need the age to solve the evolution, but you

190
00:09:49.080 --> 00:09:51.559
<v Speaker 3>need the evolution to solve the age. It's an impossible

191
00:09:51.600 --> 00:09:52.279
<v Speaker 3>loop that.

192
00:09:52.159 --> 00:09:54.240
<v Speaker 2>Sounds incredibly frustrating. For astronomers.

193
00:09:54.440 --> 00:09:57.960
<v Speaker 3>It is the defining frustration of substellar astrophysics. I mean,

194
00:09:58.039 --> 00:10:00.840
<v Speaker 3>the object itself is locked in an ambiguit state, its

195
00:10:01.080 --> 00:10:04.639
<v Speaker 3>luminosity and temperature are changing, its radius tells you nothing

196
00:10:04.639 --> 00:10:07.840
<v Speaker 3>about its mass, and it simply refuses to provide any

197
00:10:07.879 --> 00:10:10.360
<v Speaker 3>independent metric that reveals its age.

198
00:10:10.600 --> 00:10:11.480
<v Speaker 2>So what did theorists do?

199
00:10:12.440 --> 00:10:17.360
<v Speaker 3>Just guess Well, they spent decades building complex computational models

200
00:10:17.360 --> 00:10:21.000
<v Speaker 3>predicting how these objects should cool based on various masses

201
00:10:21.080 --> 00:10:22.519
<v Speaker 3>and atmospheric composition.

202
00:10:22.639 --> 00:10:23.919
<v Speaker 2>But it couldn't prove it right.

203
00:10:24.000 --> 00:10:27.480
<v Speaker 3>They had no way to definitively calibrate those models against reality.

204
00:10:27.720 --> 00:10:31.559
<v Speaker 2>So because they couldn't interrogate the Brown dwarf directly, astronomers

205
00:10:31.559 --> 00:10:33.759
<v Speaker 2>realized they had to find a loophole. They had to

206
00:10:33.799 --> 00:10:37.039
<v Speaker 2>stop looking at isolated Brown dwarfs floating alone in the

207
00:10:37.039 --> 00:10:40.600
<v Speaker 2>interstellar medium. They needed a twin. Yes, they needed a

208
00:10:40.600 --> 00:10:43.200
<v Speaker 2>Brown dwarf gravitationally tethered to something that would give up

209
00:10:43.200 --> 00:10:46.360
<v Speaker 2>its postestificate. And they found one of the constellation Pegasus

210
00:10:46.639 --> 00:10:49.000
<v Speaker 2>in the Hr seven six to seventy two system.

211
00:10:48.759 --> 00:10:51.879
<v Speaker 3>Ah yes Hr seven sixty seven two. It is a

212
00:10:51.919 --> 00:10:55.679
<v Speaker 3>binary system located about fifty eight light years away. It

213
00:10:55.720 --> 00:10:59.279
<v Speaker 3>consists of a primary solar type main sequence star and

214
00:10:59.360 --> 00:11:02.240
<v Speaker 3>a faint sub stellar companion, the brown dwarf, yes, a

215
00:11:02.279 --> 00:11:05.399
<v Speaker 3>brown dwarf in orbit around it, and this specific pairing

216
00:11:05.840 --> 00:11:08.480
<v Speaker 3>is the key to breaking the entire catch twenty two

217
00:11:08.639 --> 00:11:10.519
<v Speaker 3>of brown dwarf evolution.

218
00:11:10.320 --> 00:11:14.000
<v Speaker 2>Because they coalesced from the exact same collapsing molecular cloud

219
00:11:14.039 --> 00:11:14.799
<v Speaker 2>of gas and dust.

220
00:11:15.000 --> 00:11:18.559
<v Speaker 3>Exactly, they share the same primordial origin. They formed at

221
00:11:18.559 --> 00:11:21.200
<v Speaker 3>the exact same time from the same material, sharing the

222
00:11:21.240 --> 00:11:25.279
<v Speaker 3>same initial metallicity. Right, even though one gathered enough mass

223
00:11:25.360 --> 00:11:28.240
<v Speaker 3>to ignite hydrogen fusion and become a true star and

224
00:11:28.279 --> 00:11:30.960
<v Speaker 3>the others stalled out as a brown dwarf, they are

225
00:11:31.039 --> 00:11:34.600
<v Speaker 3>fundamentally siblings born in the same cosmic event.

226
00:11:34.559 --> 00:11:38.840
<v Speaker 2>Which means therefore whatever age the primary main sequence star is,

227
00:11:39.080 --> 00:11:41.759
<v Speaker 2>the brown dwarf companion must be the exact same age.

228
00:11:41.840 --> 00:11:43.159
<v Speaker 3>That's the loophole, so the.

229
00:11:43.120 --> 00:11:46.279
<v Speaker 2>Star becomes the proxy. If you could date the primary star,

230
00:11:46.720 --> 00:11:50.120
<v Speaker 2>you immediately unlock the age of the brown dwarf. But wait,

231
00:11:50.240 --> 00:11:51.879
<v Speaker 2>doesn't that just move the goalposts?

232
00:11:52.240 --> 00:11:52.600
<v Speaker 3>Wow?

233
00:11:52.720 --> 00:11:55.600
<v Speaker 2>Because means he can. Stars are famously difficult to date

234
00:11:55.639 --> 00:11:58.799
<v Speaker 2>precisely once they settle into their mature phase. Right. Their

235
00:11:58.799 --> 00:12:02.759
<v Speaker 2>surface temperatures and limit venosities don't change drastically for billions

236
00:12:02.799 --> 00:12:05.679
<v Speaker 2>of years, So how did they force the primary star

237
00:12:05.840 --> 00:12:07.000
<v Speaker 2>to reveal its age?

238
00:12:07.120 --> 00:12:10.000
<v Speaker 3>This is where the methodology shifts from standard photometry to

239
00:12:10.200 --> 00:12:15.360
<v Speaker 3>incredibly advanced high resolution spectroscopy. The researchers utilize the WM

240
00:12:15.480 --> 00:12:19.879
<v Speaker 3>Keck Observatory in Hawaii. Specifically, they leveraged an instrument called

241
00:12:19.879 --> 00:12:22.799
<v Speaker 3>the Kech planet Finder, and they didn't just measure the

242
00:12:22.840 --> 00:12:28.480
<v Speaker 3>star's total light output. They employed astro seismology. Astroismology, yes,

243
00:12:28.519 --> 00:12:31.480
<v Speaker 3>they study the internal acoustic waves of the star itself.

244
00:12:31.639 --> 00:12:34.039
<v Speaker 2>What's fascinating here is that we tend to think of

245
00:12:34.039 --> 00:12:38.480
<v Speaker 2>stars as these silent, static, glowing orbs. They do, but internally,

246
00:12:39.240 --> 00:12:42.879
<v Speaker 2>a solar type star is a violently turbulent environment.

247
00:12:43.000 --> 00:12:43.639
<v Speaker 3>It's chaotic.

248
00:12:43.799 --> 00:12:46.000
<v Speaker 2>In the outer envelope of a star like Hr seven

249
00:12:46.120 --> 00:12:50.279
<v Speaker 2>six seven to two, you have massive convection zones, huge

250
00:12:50.320 --> 00:12:53.720
<v Speaker 2>plumes of superheated plasma are constantly boiling to the surface,

251
00:12:53.759 --> 00:12:57.759
<v Speaker 2>cooling and sinking back down. And this violent, continuous churning

252
00:12:58.200 --> 00:13:00.000
<v Speaker 2>generates broadband acoustic noise.

253
00:13:00.519 --> 00:13:03.480
<v Speaker 3>It is an environment of unimaginable acoustic energy. I mean

254
00:13:03.519 --> 00:13:06.879
<v Speaker 3>the turbulence in the convective envelope continuously excites millions of

255
00:13:06.879 --> 00:13:07.840
<v Speaker 3>different sound waves.

256
00:13:07.879 --> 00:13:08.960
<v Speaker 2>Sound waves in a star.

257
00:13:08.960 --> 00:13:12.320
<v Speaker 3>Yeah, these are pressure waves or p modes. And because

258
00:13:12.440 --> 00:13:16.320
<v Speaker 3>the star is a bounded sphere of dense plasma, it

259
00:13:16.399 --> 00:13:18.919
<v Speaker 3>acts as a three dimensional resonant cavity.

260
00:13:19.159 --> 00:13:21.480
<v Speaker 2>So the star literally rings like a bell.

261
00:13:21.759 --> 00:13:22.759
<v Speaker 3>It literally does.

262
00:13:22.960 --> 00:13:25.840
<v Speaker 2>The physics of this are just incredible. These acoustic waves

263
00:13:26.120 --> 00:13:29.879
<v Speaker 2>travel downward from the surface into the dense interior of

264
00:13:29.919 --> 00:13:32.399
<v Speaker 2>the star. Right, But the speed of sound in a

265
00:13:32.440 --> 00:13:36.440
<v Speaker 2>plasma depends heavily on the temperature and the mean molecular

266
00:13:36.440 --> 00:13:37.320
<v Speaker 2>weight of that plasma.

267
00:13:37.399 --> 00:13:39.159
<v Speaker 3>Right, Yes, those are the key variable.

268
00:13:39.279 --> 00:13:41.559
<v Speaker 2>So as the sound waves dive deeper toward the core,

269
00:13:42.000 --> 00:13:45.919
<v Speaker 2>the temperature and density increase dramatically, which causes the sound

270
00:13:45.919 --> 00:13:50.000
<v Speaker 2>waves to refract. They curve back upward towards the surface.

271
00:13:49.720 --> 00:13:52.360
<v Speaker 3>And when those refracted sound waves hit the surface of

272
00:13:52.399 --> 00:13:55.320
<v Speaker 3>the star from the inside, they cause the star's outer

273
00:13:55.440 --> 00:14:00.879
<v Speaker 3>layers to physically expand and contract. Wow, the entire starstantly pulsating,

274
00:14:00.960 --> 00:14:04.559
<v Speaker 3>driven by this internal acoustic resonance. But the crucial part

275
00:14:04.600 --> 00:14:07.600
<v Speaker 3>of astro seismology, the mechanism that actually allows us to

276
00:14:07.679 --> 00:14:11.080
<v Speaker 3>date the star, lies in how that internal sound speed

277
00:14:11.440 --> 00:14:12.399
<v Speaker 3>changes over time.

278
00:14:12.559 --> 00:14:15.080
<v Speaker 2>Right, Because the core composition of the star is not static.

279
00:14:15.559 --> 00:14:19.759
<v Speaker 2>As the star ages, it fuses hydrogen into helium.

280
00:14:19.399 --> 00:14:22.840
<v Speaker 3>And helium is denser and heavier than hydrogen. Okay, So

281
00:14:22.879 --> 00:14:26.279
<v Speaker 3>as the star burns through its main sequence life, helium

282
00:14:26.320 --> 00:14:28.360
<v Speaker 3>ash slowly accumulates in the core.

283
00:14:28.960 --> 00:14:29.679
<v Speaker 2>That makes sense.

284
00:14:29.840 --> 00:14:33.720
<v Speaker 3>This gradually increases the mean molecular weight of the star's interior.

285
00:14:34.039 --> 00:14:37.039
<v Speaker 3>And because the speed of sound is inversely proportional to

286
00:14:37.080 --> 00:14:39.759
<v Speaker 3>the square root of the mean molecular weight, the build

287
00:14:39.840 --> 00:14:43.039
<v Speaker 3>up of helium physically alters the sound speed profile of

288
00:14:43.080 --> 00:14:43.919
<v Speaker 3>the entire star.

289
00:14:44.600 --> 00:14:47.879
<v Speaker 2>I see. So, as the star ages, the internal acoustic

290
00:14:47.919 --> 00:14:51.440
<v Speaker 2>cavity changes its properties, which means the specific frequencies at

291
00:14:51.440 --> 00:14:54.600
<v Speaker 2>which the star resonates the pitch of the starquakes shifts

292
00:14:54.639 --> 00:14:55.159
<v Speaker 2>over time.

293
00:14:55.279 --> 00:14:58.639
<v Speaker 3>You've got it. By meticulously measuring the frequencies of those

294
00:14:58.679 --> 00:15:03.720
<v Speaker 3>surface pulsations, astrophysicists can essentially perform an ultrasound on the star.

295
00:15:03.919 --> 00:15:07.120
<v Speaker 2>An ultrasound on a star that is wild.

296
00:15:06.799 --> 00:15:10.039
<v Speaker 3>It's amazing. They map the internal density profile, They determine

297
00:15:10.080 --> 00:15:12.600
<v Speaker 3>exactly how much helium has accumulated in the core, and

298
00:15:12.639 --> 00:15:15.639
<v Speaker 3>from that mass, fraction of helium ash. They can calculate

299
00:15:15.679 --> 00:15:18.000
<v Speaker 3>the star's age with astonishing precision.

300
00:15:18.159 --> 00:15:20.320
<v Speaker 2>But I mean, this scale of this measurement is what

301
00:15:20.399 --> 00:15:21.559
<v Speaker 2>truly blows my mind.

302
00:15:21.720 --> 00:15:23.080
<v Speaker 3>It's hard to wrap your head around.

303
00:15:23.240 --> 00:15:26.720
<v Speaker 2>We are talking about acoustic waves causing a star to

304
00:15:26.799 --> 00:15:30.240
<v Speaker 2>expand and contract by a few meters on an object

305
00:15:30.279 --> 00:15:33.879
<v Speaker 2>that is millions of kilometers across, located fifty eight light

306
00:15:33.960 --> 00:15:37.679
<v Speaker 2>years away. Yeah, how is an instrument on Earth measuring

307
00:15:37.720 --> 00:15:38.879
<v Speaker 2>that physical pulsation?

308
00:15:39.039 --> 00:15:41.639
<v Speaker 3>Well? As the surface of the star heaves out well

309
00:15:41.759 --> 00:15:45.440
<v Speaker 3>toward Earth and then contracts inward away from Earth, the

310
00:15:45.559 --> 00:15:50.360
<v Speaker 3>light emitted from that surface undergoes a microscopic Doppler shift.

311
00:15:50.600 --> 00:15:51.919
<v Speaker 2>Ah, the Doppler effect.

312
00:15:52.000 --> 00:15:55.000
<v Speaker 3>Right, when the surface moves toward us, the light waves

313
00:15:55.000 --> 00:15:58.720
<v Speaker 3>are compressed, shifting slightly toward the blue end of the spectrum. Okay,

314
00:15:58.759 --> 00:16:01.759
<v Speaker 3>and when it moves away, the light stretches, shifting toward

315
00:16:01.840 --> 00:16:02.200
<v Speaker 3>the red.

316
00:16:02.399 --> 00:16:05.720
<v Speaker 2>So the Keck planet finder isn't taking pictures. No, it's

317
00:16:05.759 --> 00:16:09.559
<v Speaker 2>a high resolution a shell spectrograph breaking the starlight apart

318
00:16:09.639 --> 00:16:13.360
<v Speaker 2>and looking for these minuscule rhythmic shifts in the absorption lines.

319
00:16:13.679 --> 00:16:17.360
<v Speaker 3>And the precision required is just staggering. We are looking

320
00:16:17.360 --> 00:16:21.200
<v Speaker 3>for radial velocity shifts on the order of centimeters per second.

321
00:16:21.240 --> 00:16:23.240
<v Speaker 2>Centimeters per second, that's barely a walking pace.

322
00:16:23.440 --> 00:16:28.000
<v Speaker 3>It's incredibly slow. The Keck planet finder uses advanced technology

323
00:16:28.240 --> 00:16:33.480
<v Speaker 3>like laser frequency combs to create an absolute calibration grid.

324
00:16:33.600 --> 00:16:33.919
<v Speaker 2>Okay.

325
00:16:34.159 --> 00:16:37.279
<v Speaker 3>This ensures that any shift they measure is genuinely coming

326
00:16:37.320 --> 00:16:41.480
<v Speaker 3>from the star and not from microscopic temperature fluctuations in

327
00:16:41.559 --> 00:16:45.000
<v Speaker 3>the instrument itself. They are measuring variations in the starlight

328
00:16:45.080 --> 00:16:47.639
<v Speaker 3>occurring on time scales of mere minutes.

329
00:16:47.960 --> 00:16:49.960
<v Speaker 2>It's like trying to measure the ripples in a cup

330
00:16:50.000 --> 00:16:52.919
<v Speaker 2>of coffee from a mile away by watching how the

331
00:16:52.960 --> 00:16:55.399
<v Speaker 2>glare of the sun bounces off the surface of the

332
00:16:55.440 --> 00:16:58.799
<v Speaker 2>liquid while staring through the turbulent atmosphere of the Earth.

333
00:16:58.879 --> 00:17:02.039
<v Speaker 3>That is a very accurate, if slightly terrifying way to

334
00:17:02.039 --> 00:17:04.799
<v Speaker 3>describe the engineering challenge. Yes, it's bordering on magic, but

335
00:17:04.839 --> 00:17:05.440
<v Speaker 3>they did it.

336
00:17:05.559 --> 00:17:08.920
<v Speaker 2>They isolated the acoustic modes of HR seven six seventy two,

337
00:17:09.400 --> 00:17:11.680
<v Speaker 2>They mapped the helium density of the core, and they

338
00:17:11.720 --> 00:17:13.680
<v Speaker 2>derived a precise independent age.

339
00:17:13.720 --> 00:17:16.279
<v Speaker 3>They did the astra seismic data confirmed that the Hr

340
00:17:16.319 --> 00:17:18.799
<v Speaker 3>seven sixty seven to two system is exactly two point

341
00:17:18.839 --> 00:17:20.240
<v Speaker 3>three billion years old.

342
00:17:20.079 --> 00:17:23.240
<v Speaker 2>Two point three billion years, which instantly assigns that exact

343
00:17:23.279 --> 00:17:25.039
<v Speaker 2>same age to the brown dwarf companion.

344
00:17:25.759 --> 00:17:26.599
<v Speaker 3>Mystery solved.

345
00:17:26.799 --> 00:17:30.480
<v Speaker 2>They finally bypassed the degeneracy problem and forced a brown

346
00:17:30.559 --> 00:17:32.079
<v Speaker 2>dwarf to hand over its birth certify.

347
00:17:32.200 --> 00:17:33.680
<v Speaker 3>Yes, they finally got the timestamp.

348
00:17:34.039 --> 00:17:39.279
<v Speaker 2>But I want to explore why the astrophysics community views

349
00:17:39.400 --> 00:17:42.720
<v Speaker 2>this specific system as such a massive breakthrough.

350
00:17:42.839 --> 00:17:43.920
<v Speaker 3>Okay, let's get into it.

351
00:17:43.880 --> 00:17:47.720
<v Speaker 2>Because surely we have found other brown dwarfs orbiting stars before.

352
00:17:48.640 --> 00:17:50.359
<v Speaker 2>Why does this one change the game.

353
00:17:51.000 --> 00:17:54.240
<v Speaker 3>Well, while we have detected other brown dwarfs and binary systems,

354
00:17:54.279 --> 00:17:57.880
<v Speaker 3>the specific orbital architecture of HR seventy six seven to

355
00:17:57.960 --> 00:18:01.640
<v Speaker 3>two is exceedingly rare. Oh so, this brown dwarf is

356
00:18:01.799 --> 00:18:05.119
<v Speaker 3>orbiting relatively close to its host star. Okay, when you

357
00:18:05.160 --> 00:18:09.759
<v Speaker 3>analyze the statistical distribution of substellar companions orbiting solar type

358
00:18:09.799 --> 00:18:13.279
<v Speaker 3>stars at these close to intermediate distances we're talking roughly

359
00:18:13.319 --> 00:18:18.039
<v Speaker 3>within five astronomical units, you find a glaring statistical anomaly.

360
00:18:17.640 --> 00:18:18.519
<v Speaker 2>Well kind of anomaly.

361
00:18:18.559 --> 00:18:20.759
<v Speaker 3>Astrophysicists call it the Brown dwarf desert.

362
00:18:20.839 --> 00:18:23.720
<v Speaker 2>A desert, a zone where these objects simply do not exist.

363
00:18:23.799 --> 00:18:26.960
<v Speaker 2>We find terrestrial planets close to stars, we find gas

364
00:18:26.960 --> 00:18:30.640
<v Speaker 2>giants like Jupiter slightly further out, but in that specific

365
00:18:30.759 --> 00:18:34.319
<v Speaker 2>mass range of thirteen to eighty jupiter masses, the data

366
00:18:34.359 --> 00:18:35.720
<v Speaker 2>suddenly drops off a cliff.

367
00:18:35.920 --> 00:18:38.640
<v Speaker 3>It is a profound accents and it points to the

368
00:18:38.640 --> 00:18:42.839
<v Speaker 3>fundamental mechanics of how different objects form in a protoplanetary disk.

369
00:18:42.920 --> 00:18:43.559
<v Speaker 2>How do they form?

370
00:18:43.920 --> 00:18:47.960
<v Speaker 3>Well? Planets form through core recretion. Dust grains stick together,

371
00:18:48.119 --> 00:18:51.920
<v Speaker 3>form pebbles, then planetesimals, and eventually, if a rocky core

372
00:18:51.960 --> 00:18:55.720
<v Speaker 3>gets massive enough, it rapidly sweeps up surrounding gas to

373
00:18:55.759 --> 00:18:59.319
<v Speaker 3>become a giant planet like Jupiter. Right, But that process

374
00:18:59.359 --> 00:19:02.039
<v Speaker 3>seems to hit a hard upper limit, well below the

375
00:19:02.079 --> 00:19:04.000
<v Speaker 3>mass of a brown dwarf.

376
00:19:03.880 --> 00:19:05.920
<v Speaker 2>Because by the time a core could accrete forty or

377
00:19:05.920 --> 00:19:09.400
<v Speaker 2>fifty jupiter masses of gas, the primordial disc has either

378
00:19:09.440 --> 00:19:12.559
<v Speaker 2>dissipated or the growing planet has carved such a massive

379
00:19:12.599 --> 00:19:15.680
<v Speaker 2>gap in the disc that it starves itself a further material.

380
00:19:15.759 --> 00:19:18.559
<v Speaker 3>Precisely, you just run out of raw material. Brown dwarfs,

381
00:19:18.559 --> 00:19:20.920
<v Speaker 3>on the other hand, likely form through the same mechanism

382
00:19:20.920 --> 00:19:24.079
<v Speaker 3>as stars, the racket gravitational fragmentation and collapse of a

383
00:19:24.119 --> 00:19:25.000
<v Speaker 3>molecular cloud.

384
00:19:25.240 --> 00:19:26.359
<v Speaker 2>So they form like stars.

385
00:19:26.799 --> 00:19:30.680
<v Speaker 3>Yes, but forming a star and a brown dwarf simultaneously

386
00:19:31.200 --> 00:19:35.920
<v Speaker 3>in such close proximity creates an incredibly unstable dynamic environment.

387
00:19:36.000 --> 00:19:36.920
<v Speaker 2>Oh I could imagine.

388
00:19:36.960 --> 00:19:40.880
<v Speaker 3>In most cases, the complex multibody gravitational interactions during the

389
00:19:40.880 --> 00:19:44.519
<v Speaker 3>formation phase either eject the lighter brown dwarf out of

390
00:19:44.519 --> 00:19:48.200
<v Speaker 3>the system entirely or force it to spiral inward and

391
00:19:48.319 --> 00:19:49.720
<v Speaker 3>merge with the primary star.

392
00:19:49.920 --> 00:19:52.440
<v Speaker 2>So the environment is just too violent for the brown

393
00:19:52.480 --> 00:19:55.119
<v Speaker 2>dwarf to survive in that orbit. Yes, so finding the

394
00:19:55.319 --> 00:19:58.960
<v Speaker 2>Hr seven six seven to two brown dwarf sitting perfectly

395
00:19:58.960 --> 00:20:01.720
<v Speaker 2>intact right in the middle of this desert is an

396
00:20:01.759 --> 00:20:02.799
<v Speaker 2>extreme anomaly.

397
00:20:03.039 --> 00:20:07.200
<v Speaker 3>It's incredibly lucky it survived the chaotic formation process, and.

398
00:20:07.079 --> 00:20:10.200
<v Speaker 2>Its survival in that specific orbit is what makes it

399
00:20:10.319 --> 00:20:11.519
<v Speaker 2>scientifically invaluable.

400
00:20:11.640 --> 00:20:15.799
<v Speaker 3>Exactly when theorists attempt to test complex physics models like

401
00:20:15.839 --> 00:20:19.279
<v Speaker 3>the atmospheric evolution of substellar objects over billions of years,

402
00:20:19.319 --> 00:20:22.559
<v Speaker 3>they require the cleanest possible empirical data. Makes sense if

403
00:20:22.599 --> 00:20:25.079
<v Speaker 3>you observe a brown dwarf in a dense young star cluster,

404
00:20:25.160 --> 00:20:28.799
<v Speaker 3>its evolution is constantly altered by the intense ultraviolet radiation

405
00:20:28.839 --> 00:20:32.240
<v Speaker 3>of nearby massive stars or by chaotic gravitational encounters.

406
00:20:32.359 --> 00:20:35.039
<v Speaker 2>Right, Or if you observe a brown dwarf in a

407
00:20:35.160 --> 00:20:38.599
<v Speaker 2>very wide binary orbit, the orbital dynamics are so loose

408
00:20:38.880 --> 00:20:42.119
<v Speaker 2>that galactic tidal forces or passing stars could disrupt the.

409
00:20:42.119 --> 00:20:44.079
<v Speaker 3>System exactly, it's too noisy.

410
00:20:44.200 --> 00:20:46.799
<v Speaker 2>So Hr seven sixty seven to two is a tightly bound,

411
00:20:46.960 --> 00:20:48.440
<v Speaker 2>dynamically stable system.

412
00:20:48.559 --> 00:20:52.759
<v Speaker 3>Yes, the brown dwarf is isolated from external galactic perturbations,

413
00:20:53.240 --> 00:20:55.759
<v Speaker 3>yet it is far enough from the primary star that

414
00:20:55.799 --> 00:20:58.920
<v Speaker 3>it isn't being completely irradiated or tidally shredded.

415
00:20:59.119 --> 00:21:02.240
<v Speaker 2>It exists in a state of pristine, undisturbed evolution.

416
00:21:02.480 --> 00:21:04.599
<v Speaker 3>It is a perfectly clean laboratory.

417
00:21:04.960 --> 00:21:06.440
<v Speaker 2>It is the ultimate control group.

418
00:21:06.559 --> 00:21:07.200
<v Speaker 3>It really is.

419
00:21:07.440 --> 00:21:10.319
<v Speaker 2>It's like trying to test the long term metabolic effects

420
00:21:10.640 --> 00:21:12.720
<v Speaker 2>of a specific nutritional regimen on someone.

421
00:21:12.799 --> 00:21:14.039
<v Speaker 3>Okay, I like this analogy.

422
00:21:14.279 --> 00:21:16.920
<v Speaker 2>If your test subject lives next to a noisy airport,

423
00:21:17.240 --> 00:21:20.680
<v Speaker 2>suffers from chronic stress, and occasionally binges at a buffet,

424
00:21:21.319 --> 00:21:25.960
<v Speaker 2>any metabolic data you extract is heavily contaminated by external variables.

425
00:21:26.279 --> 00:21:27.480
<v Speaker 3>You wouldn't know what caused what.

426
00:21:27.799 --> 00:21:30.640
<v Speaker 2>Right, you need a subject in a perfectly controlled, isolated

427
00:21:30.680 --> 00:21:33.799
<v Speaker 2>bubble where the only variable driving change is the internal

428
00:21:33.839 --> 00:21:34.839
<v Speaker 2>biology itself.

429
00:21:35.000 --> 00:21:38.000
<v Speaker 3>The isolation of Hr seven six seventy two provides that

430
00:21:38.079 --> 00:21:42.079
<v Speaker 3>exact bubble because the environment is chemically and dynamically clean,

431
00:21:42.200 --> 00:21:44.960
<v Speaker 3>and because we now possess a hype literally, and then

432
00:21:45.000 --> 00:21:47.960
<v Speaker 3>you transition down to the cooler T type dwarfs, where

433
00:21:48.000 --> 00:21:51.519
<v Speaker 3>methane dominates the spectrum and the silicate clouds sink below

434
00:21:51.519 --> 00:21:54.240
<v Speaker 3>the visible photosphere, and theorists.

435
00:21:53.839 --> 00:21:59.440
<v Speaker 2>Have spent decades writing incredibly dense computational models to simulate

436
00:21:59.480 --> 00:22:03.000
<v Speaker 2>these phase transition We've had to Yeah, they've built equations

437
00:22:03.000 --> 00:22:06.039
<v Speaker 2>to predict exactly how the opacity of those iron and

438
00:22:06.039 --> 00:22:10.000
<v Speaker 2>silicate clouds traps heat, how convection dredges up methane from

439
00:22:10.039 --> 00:22:13.519
<v Speaker 2>the interior, and how the luminosity should decline over time.

440
00:22:13.680 --> 00:22:19.440
<v Speaker 3>But without an independently dated object, those models were fundamentally uncalibrated.

441
00:22:18.720 --> 00:22:20.440
<v Speaker 2>Right, because you don't know the starting point.

442
00:22:20.599 --> 00:22:23.160
<v Speaker 3>Farris would predict that a brown dwarf of a certain

443
00:22:23.240 --> 00:22:26.480
<v Speaker 3>mass at two point three billion years should exhibit a

444
00:22:26.519 --> 00:22:31.920
<v Speaker 3>specific atmospheric chemistry, a specific temperature, and a specific luminosity,

445
00:22:32.039 --> 00:22:34.240
<v Speaker 3>but it was entirely theoretical until now.

446
00:22:34.400 --> 00:22:36.599
<v Speaker 2>Until now, with the Hr seven sixty seven to two

447
00:22:36.599 --> 00:22:41.119
<v Speaker 2>brown dwarf. Astrophysicists can perform the ultimate mechanical calibration. They

448
00:22:41.160 --> 00:22:45.079
<v Speaker 2>take the theoretical evolutionary track what the physics models predict

449
00:22:45.440 --> 00:22:48.640
<v Speaker 2>a two point three billion year old brown dwarf should

450
00:22:48.640 --> 00:22:51.319
<v Speaker 2>look like, and they compare it directly against the physical

451
00:22:51.400 --> 00:22:54.720
<v Speaker 2>reality of the Hr seven sixty seven to two observations.

452
00:22:55.240 --> 00:22:59.880
<v Speaker 3>They execute a direct comparison of the empirical bollometric luminosity

453
00:23:00.400 --> 00:23:04.119
<v Speaker 3>and the measured effective temperature against the isochrones generated by

454
00:23:04.119 --> 00:23:04.599
<v Speaker 3>the models.

455
00:23:04.640 --> 00:23:07.799
<v Speaker 2>And this is the definition of establishing a benchmark object.

456
00:23:07.880 --> 00:23:09.200
<v Speaker 3>Exactly, this is the benchmark.

457
00:23:09.319 --> 00:23:11.799
<v Speaker 2>Some mepose a scenario regarding that benchmark, just to play

458
00:23:11.799 --> 00:23:15.759
<v Speaker 2>Devil's advocate. What happens if the decades of theoretical modeling

459
00:23:16.079 --> 00:23:20.079
<v Speaker 2>turn out to be significantly misaligned with the empirical data. Okay,

460
00:23:20.279 --> 00:23:22.799
<v Speaker 2>let's say the observed luminosity of the HR seven six

461
00:23:22.799 --> 00:23:26.480
<v Speaker 2>seventy two dwarf is notably higher or lower than what

462
00:23:26.559 --> 00:23:28.759
<v Speaker 2>the models predicted for a two point three billion year

463
00:23:28.799 --> 00:23:32.920
<v Speaker 2>old object. Does that invalidate the entire field of subcellar physics.

464
00:23:33.119 --> 00:23:36.319
<v Speaker 3>No, No, it doesn't invalidate the field. It actually accelerates it.

465
00:23:36.519 --> 00:23:40.160
<v Speaker 3>How So, discrepancies between theory and a pristine benchmark are

466
00:23:40.200 --> 00:23:44.359
<v Speaker 3>exactly how science progresses. If the empirical luminosity deviates from

467
00:23:44.359 --> 00:23:46.960
<v Speaker 3>the model, it reveals that our understanding of the underlying

468
00:23:46.960 --> 00:23:48.000
<v Speaker 3>physics is incomplete.

469
00:23:48.319 --> 00:23:51.920
<v Speaker 2>Ah I see, perhaps the models miscalculated the grain size

470
00:23:52.160 --> 00:23:55.000
<v Speaker 2>of the silicate dust in the upper atmosphere, which would

471
00:23:55.079 --> 00:23:58.920
<v Speaker 2>alter the opacity and allow heat to escape faster than predicted. Right,

472
00:23:59.240 --> 00:24:02.599
<v Speaker 2>Or perhaps the internal equation of state governing the electron

473
00:24:02.640 --> 00:24:04.960
<v Speaker 2>degeneracy requires some refinement.

474
00:24:05.200 --> 00:24:08.200
<v Speaker 3>The single anchor point forces the theory to evolve to

475
00:24:08.240 --> 00:24:09.759
<v Speaker 3>match reality exactly.

476
00:24:10.079 --> 00:24:13.440
<v Speaker 2>You iteratively adjust the physics in the model, the opacities,

477
00:24:13.480 --> 00:24:17.839
<v Speaker 2>the chemical equilibrium equations, the convective boundary conditions, until the

478
00:24:17.880 --> 00:24:21.599
<v Speaker 2>model successfully reproduces the exact temperature and luminosity of the

479
00:24:21.759 --> 00:24:24.680
<v Speaker 2>Hr seven six seventy two dwarf at two point three

480
00:24:24.759 --> 00:24:29.000
<v Speaker 2>billion years. Once your model accurately predicts this benchmark, you

481
00:24:29.079 --> 00:24:31.599
<v Speaker 2>have successfully calibrated your computational tools.

482
00:24:31.759 --> 00:24:33.839
<v Speaker 3>And once the tool is calibrated, you can turn it

483
00:24:33.839 --> 00:24:36.039
<v Speaker 3>toward the rest of the galaxy. Yes, you can point

484
00:24:36.039 --> 00:24:39.440
<v Speaker 3>your telescope at an isolated brown dwarf floating alone in

485
00:24:39.440 --> 00:24:43.000
<v Speaker 3>interstellar space, one that doesn't have a convenient primary star

486
00:24:43.119 --> 00:24:46.079
<v Speaker 3>to data back, take its temperature, run it through the

487
00:24:46.079 --> 00:24:49.960
<v Speaker 3>calibrated model, and finally extract a reliable age and mass.

488
00:24:50.200 --> 00:24:54.039
<v Speaker 2>You've got it. We have broken the mass age luminosity degeneracy.

489
00:24:54.160 --> 00:24:56.799
<v Speaker 3>That is incredible if we connect this to the bigger picture,

490
00:24:57.240 --> 00:24:59.880
<v Speaker 3>the calibration achieved with Hr seven sixty seven to two

491
00:25:00.519 --> 00:25:04.720
<v Speaker 3>is really emblematic of a massive paradigm shift in modern astronomy.

492
00:25:05.160 --> 00:25:08.359
<v Speaker 3>For much of its history, astronomy was an observational science,

493
00:25:08.599 --> 00:25:13.720
<v Speaker 3>focused primarily on discovery and cataloging, building larger apertures to

494
00:25:13.720 --> 00:25:18.440
<v Speaker 3>capture fanter light, mapping the astrometry, classifying the spectral types.

495
00:25:18.519 --> 00:25:21.039
<v Speaker 2>It was essentially cosmic stamp collecting. We were just trying

496
00:25:21.039 --> 00:25:22.519
<v Speaker 2>to figure out what was out there in the dark.

497
00:25:22.759 --> 00:25:25.319
<v Speaker 3>That's a good way to describe it. But discovery is

498
00:25:25.359 --> 00:25:28.440
<v Speaker 3>no longer the sole frontier. The current era is defined

499
00:25:28.440 --> 00:25:32.480
<v Speaker 3>by precision, characterization, decision characterization. Yes, we are no longer

500
00:25:32.519 --> 00:25:35.839
<v Speaker 3>satisfied with simply identifying the presence of a celestial body.

501
00:25:36.400 --> 00:25:40.720
<v Speaker 3>The science demands that we extract deep, rigorous physical metrics

502
00:25:40.720 --> 00:25:42.680
<v Speaker 3>from the faintest possible signals.

503
00:25:42.799 --> 00:25:44.920
<v Speaker 2>We want to know how it takes exactly.

504
00:25:44.440 --> 00:25:47.839
<v Speaker 3>We want to know the internal structural density, the precise

505
00:25:47.920 --> 00:25:52.839
<v Speaker 3>chemical abundances, the atmospheric fluid dynamics, and most importantly, the

506
00:25:53.000 --> 00:25:55.319
<v Speaker 3>exact evolutionary timeline, which.

507
00:25:55.200 --> 00:25:58.359
<v Speaker 2>Is exactly what astra seismology delivers. We are moving from

508
00:25:58.400 --> 00:26:02.720
<v Speaker 2>taking static two dimensional pictures of the sky to executing

509
00:26:03.559 --> 00:26:08.640
<v Speaker 2>complex three dimensional physical analyzes of objects tens of light

510
00:26:08.720 --> 00:26:12.799
<v Speaker 2>years away. Yes, and we're doing it using microscopic Doppler

511
00:26:12.799 --> 00:26:13.799
<v Speaker 2>shifts in their light.

512
00:26:14.039 --> 00:26:15.559
<v Speaker 3>It's a huge leap forward.

513
00:26:15.880 --> 00:26:20.000
<v Speaker 2>And this specific calibration tool doesn't just apply to brown dwarfs. Right.

514
00:26:20.799 --> 00:26:25.119
<v Speaker 2>The ability to precisely date host stars ripples outward across

515
00:26:25.240 --> 00:26:26.519
<v Speaker 2>all of planetary science.

516
00:26:26.559 --> 00:26:31.400
<v Speaker 3>Oh. Absolutely, It dramatically impacts our study of exoplanets.

517
00:26:30.559 --> 00:26:32.200
<v Speaker 2>Like the ones found by Kepler and Tests.

518
00:26:32.359 --> 00:26:35.400
<v Speaker 3>Yes, through missions like Kepler and Tests, we have discovered

519
00:26:35.599 --> 00:26:39.559
<v Speaker 3>thousands of exoplanets orbiting other stars, thousands of them thousands.

520
00:26:39.880 --> 00:26:43.799
<v Speaker 3>We know their orbital periods, their radii, and sometimes their masses,

521
00:26:44.119 --> 00:26:47.359
<v Speaker 3>but we rarely know their ages with any meaningful precision.

522
00:26:47.440 --> 00:26:49.000
<v Speaker 2>Because if you don't know the age of the host star,

523
00:26:49.160 --> 00:26:51.640
<v Speaker 2>you don't know the age of the planetary system exactly.

524
00:26:51.680 --> 00:26:53.799
<v Speaker 3>We know they exist, but we don't know where they

525
00:26:53.799 --> 00:26:55.160
<v Speaker 3>are in their evolutionary life.

526
00:26:55.039 --> 00:26:58.039
<v Speaker 2>Cycle, and understanding the age of a planetary system is

527
00:26:58.119 --> 00:26:59.960
<v Speaker 2>critical to understanding planetary physics.

528
00:27:00.400 --> 00:27:04.720
<v Speaker 3>Without a doubt, if we observe a gas giant exoplanet

529
00:27:04.720 --> 00:27:08.559
<v Speaker 3>that is highly inflated, or a terrestrial planet that appears

530
00:27:08.599 --> 00:27:11.759
<v Speaker 3>to have lost its primary atmosphere, we need to know the.

531
00:27:11.720 --> 00:27:14.960
<v Speaker 2>Timeline right because if it just formed yesterday, that tells

532
00:27:14.960 --> 00:27:17.039
<v Speaker 2>you something very different than if it's been around for

533
00:27:17.079 --> 00:27:17.920
<v Speaker 2>ten billion years.

534
00:27:18.039 --> 00:27:21.720
<v Speaker 3>Exactly does a terrestrial planet lose its hydrogen envelope to

535
00:27:21.839 --> 00:27:25.359
<v Speaker 3>stellar wind shipping in fifty million years or five hundred

536
00:27:25.359 --> 00:27:26.000
<v Speaker 3>million years?

537
00:27:26.200 --> 00:27:27.839
<v Speaker 2>Big difference, Huge difference.

538
00:27:28.119 --> 00:27:32.640
<v Speaker 3>By applying astro seismology to the host stars of exoplanetary systems,

539
00:27:33.079 --> 00:27:36.759
<v Speaker 3>listening to the internal acoustic resonance and mapping the core

540
00:27:36.839 --> 00:27:41.000
<v Speaker 3>healium accumulation, we can establish precise ages for the planet's

541
00:27:41.079 --> 00:27:41.599
<v Speaker 3>orbiting them.

542
00:27:41.720 --> 00:27:45.119
<v Speaker 2>We can start to build an empirical chronological timeline of

543
00:27:45.200 --> 00:27:47.680
<v Speaker 2>planetary evolution across the entire Milky Way.

544
00:27:47.839 --> 00:27:51.279
<v Speaker 3>We can track how planetary orbits migrate over billions of years,

545
00:27:51.359 --> 00:27:55.000
<v Speaker 3>how atmospheric chemistry evolves, and how the internal cooling of

546
00:27:55.039 --> 00:27:57.599
<v Speaker 3>a planet drives its geological activity.

547
00:27:57.799 --> 00:28:01.279
<v Speaker 2>We are basically transitioning from estimating these processes based on

548
00:28:01.359 --> 00:28:07.559
<v Speaker 2>broad assumptions to testing them rigorously against precise empirical temporal benchmarks.

549
00:28:07.839 --> 00:28:10.519
<v Speaker 2>So what does this all mean for the future of astrophysics.

550
00:28:11.160 --> 00:28:14.759
<v Speaker 2>It means we are systematically removing the fuzziness from the universe.

551
00:28:14.920 --> 00:28:16.799
<v Speaker 3>I like that. Removing the fuzziness.

552
00:28:16.920 --> 00:28:20.519
<v Speaker 2>We are taking the vast complex physics of how celestial

553
00:28:20.559 --> 00:28:23.680
<v Speaker 2>bodies form, how they ignite, how they fail, and how

554
00:28:23.680 --> 00:28:25.960
<v Speaker 2>they cool down, and we are anchoring all of it

555
00:28:26.240 --> 00:28:28.880
<v Speaker 2>to undeniably measurable physical reality.

556
00:28:28.960 --> 00:28:34.039
<v Speaker 3>We are replacing estimated evolutionary tracks with calibrated cosmic time. Yes,

557
00:28:34.119 --> 00:28:37.839
<v Speaker 3>and that clarification allows us to understand not just isolated

558
00:28:38.240 --> 00:28:41.400
<v Speaker 3>anomalous objects like a brown dwarf in a desert, but

559
00:28:41.519 --> 00:28:47.279
<v Speaker 3>how entire stellar and planetary systems evolve as interconnected dynamic

560
00:28:47.519 --> 00:28:50.440
<v Speaker 3>units over the entire lifespan of the universe.

561
00:28:50.519 --> 00:28:53.000
<v Speaker 2>It puts the timeline back into the cosmos, it really does,

562
00:28:53.039 --> 00:28:56.000
<v Speaker 2>which brings us full circle. Space isn't a flat projection,

563
00:28:56.200 --> 00:28:58.559
<v Speaker 2>No it's not. It isn't a static photograph where everything

564
00:28:58.640 --> 00:29:02.000
<v Speaker 2>just exists in an unchanging present. Time is the hidden

565
00:29:02.039 --> 00:29:04.839
<v Speaker 2>dimension that drives every single physical process We observe.

566
00:29:04.960 --> 00:29:08.200
<v Speaker 3>This raises an important question about how we fundamentally perceive

567
00:29:08.279 --> 00:29:12.119
<v Speaker 3>the night sky. For centuries, our observational limits forced us

568
00:29:12.160 --> 00:29:15.359
<v Speaker 3>to treat the stars as fixed, unchanging points of light.

569
00:29:16.079 --> 00:29:19.640
<v Speaker 3>We analyze their light devoid of temporal context.

570
00:29:19.200 --> 00:29:20.799
<v Speaker 2>Because we had no other choice. Right.

571
00:29:21.240 --> 00:29:24.400
<v Speaker 3>But by capturing the acoustic resonance of Hr seven sixty

572
00:29:24.359 --> 00:29:27.640
<v Speaker 3>seven to two and establishing a precise two point three

573
00:29:27.799 --> 00:29:31.480
<v Speaker 3>billion year timestamp on its substellar companion, we are learning

574
00:29:31.480 --> 00:29:33.680
<v Speaker 3>how to read the dynamic history of the universe.

575
00:29:33.839 --> 00:29:36.400
<v Speaker 2>We're mapping the shifts in the landscape. Yes, we finally

576
00:29:36.440 --> 00:29:38.839
<v Speaker 2>figured out how to dig down into the starlight and

577
00:29:38.960 --> 00:29:42.359
<v Speaker 2>uncover the geological layers of the sky. We found the

578
00:29:42.400 --> 00:29:45.039
<v Speaker 2>two point three billion year mark hidden in the rhythmic

579
00:29:45.079 --> 00:29:48.440
<v Speaker 2>pulsations of a star. It's profound, it is, and it

580
00:29:48.519 --> 00:29:51.480
<v Speaker 2>leaves me with this one lingering, highly provocative thought. Feuure

581
00:29:51.519 --> 00:29:56.680
<v Speaker 2>justm all over if taking our modern spectrographs and measuring microscopic,

582
00:29:56.960 --> 00:30:00.000
<v Speaker 2>minute long Doppler shifts in a star's light can reveal

583
00:30:00.240 --> 00:30:03.839
<v Speaker 2>the exact multi billion year age of a completely different

584
00:30:03.880 --> 00:30:08.119
<v Speaker 2>object millions of miles away. Yeah, what other invisible ancient

585
00:30:08.119 --> 00:30:11.880
<v Speaker 2>physical stories are currently hidden? In the subtle, chaotic flickers

586
00:30:11.880 --> 00:30:14.240
<v Speaker 2>of the stars we casually look up at every single night.

587
00:30:14.480 --> 00:30:16.039
<v Speaker 3>There's so much left to find.

588
00:30:16.319 --> 00:30:18.559
<v Speaker 2>The sky is no longer a static painting. It's an

589
00:30:18.599 --> 00:30:21.559
<v Speaker 2>impossibly complex clock tigging in the dark, and we were

590
00:30:21.599 --> 00:30:23.039
<v Speaker 2>finally learning how to read the dial.
