WEBVTT

0
00:00:00.400 --> 00:00:03.400
Avery: Welcome to Astronomy Daily, the podcast that

1
00:00:03.400 --> 00:00:06.000
brings you the universe one story at a time.

2
00:00:06.320 --> 00:00:07.280
I'm Avery.

3
00:00:07.360 --> 00:00:09.920
Anna: And I'm Anna. It's great to have you with us

4
00:00:10.240 --> 00:00:12.240
today. We've got stories that range from

5
00:00:12.240 --> 00:00:14.920
NASA's next great observatory to a stunning

6
00:00:14.920 --> 00:00:16.680
new image from the James Webb Space

7
00:00:16.680 --> 00:00:19.000
Telescope. We'll also be looking at some

8
00:00:19.000 --> 00:00:21.720
trouble on a Kazakhstani launch pad and why

9
00:00:21.720 --> 00:00:23.840
Earth is so geologically unique.

10
00:00:24.240 --> 00:00:26.760
Avery: Let's not wait. Anna, why don't you start us

11
00:00:26.760 --> 00:00:27.840
off with our first story?

12
00:00:27.920 --> 00:00:30.040
It sounds like there's a new powerhouse

13
00:00:30.040 --> 00:00:31.910
telescope getting ready for the cosmic st.

14
00:00:32.460 --> 00:00:33.500
That's right, Avery.

15
00:00:33.660 --> 00:00:36.020
Anna: NASA has just completed the assembly of the

16
00:00:36.020 --> 00:00:38.380
Nancy Grace Roman Space Telescope.

17
00:00:38.540 --> 00:00:40.780
Technicians at, ah, the Goddard Space Flight

18
00:00:40.780 --> 00:00:43.020
center join the inner and outer portions of

19
00:00:43.020 --> 00:00:45.420
the spacecraft, which is a major milestone.

20
00:00:45.660 --> 00:00:47.780
Avery: So it's fully built now. When do we get to

21
00:00:47.780 --> 00:00:48.540
see it in action?

22
00:00:49.100 --> 00:00:51.540
Anna: After some final testing, it's slated to

23
00:00:51.540 --> 00:00:54.420
launch by May 2027. Although the team

24
00:00:54.420 --> 00:00:56.420
says they're on track for a potential launch

25
00:00:56.420 --> 00:00:59.140
as early as fall 2026. A

26
00:00:59.140 --> 00:01:01.300
SpaceX Falcon Heavy will carry it to its

27
00:01:01.300 --> 00:01:03.180
destination. A million miles.

28
00:01:04.110 --> 00:01:06.470
Avery: A million miles. Same neighborhood as the

29
00:01:06.470 --> 00:01:08.910
Webb Telescope. Then what's the mission for

30
00:01:08.910 --> 00:01:11.190
Roman? What mysteries is it designed to

31
00:01:11.190 --> 00:01:11.550
solve?

32
00:01:12.110 --> 00:01:14.910
Anna: Its scope is just immense. The primary

33
00:01:14.910 --> 00:01:17.830
Instrument is a 288 megapixel

34
00:01:17.830 --> 00:01:20.150
wide field camera. To put that in

35
00:01:20.150 --> 00:01:22.750
perspective, Roman is expected to gather data

36
00:01:22.910 --> 00:01:25.230
hundreds of times faster than the Hubble

37
00:01:25.230 --> 00:01:26.110
Space Telescope.

38
00:01:26.350 --> 00:01:28.430
Avery: Wow. Hundreds of times faster.

39
00:01:28.830 --> 00:01:31.750
Anna: Exactly. In its first five years alone, the

40
00:01:31.750 --> 00:01:33.670
mission is projected to unveil more than

41
00:01:33.670 --> 00:01:36.490
100,000 new exoplane, hundreds of

42
00:01:36.490 --> 00:01:39.130
millions of stars, and billions of galaxies.

43
00:01:39.370 --> 00:01:42.050
It's also testing a new technology called a

44
00:01:42.050 --> 00:01:44.610
coronagraph instrument. This is designed to

45
00:01:44.610 --> 00:01:46.730
block out the overwhelming light from a star,

46
00:01:46.890 --> 00:01:49.330
allowing astronomers to directly image the

47
00:01:49.330 --> 00:01:52.250
much fainter planets orbiting it. It's a huge

48
00:01:52.250 --> 00:01:54.370
leap forward in our ability to survey the

49
00:01:54.370 --> 00:01:54.890
cosmos.

50
00:01:55.130 --> 00:01:57.930
Avery: That's incredible. From one powerful machine

51
00:01:57.930 --> 00:01:58.490
to another.

52
00:01:58.730 --> 00:02:00.970
Our next story is a bit more down to Earth,

53
00:02:00.970 --> 00:02:03.770
and unfortunately it involves some damage.

54
00:02:04.330 --> 00:02:06.250
Anna: Damage is the polite way of putting it.

55
00:02:06.250 --> 00:02:08.450
Though it's not as catastrophic as some would

56
00:02:08.450 --> 00:02:08.970
have you believe.

57
00:02:09.290 --> 00:02:12.050
Avery: On November 27, a Russian

58
00:02:12.050 --> 00:02:14.370
Soyuz rocket successfully launched three

59
00:02:14.370 --> 00:02:16.690
astronauts to the International Space Station

60
00:02:16.690 --> 00:02:19.330
from the Baikonur Cosmodrome. The launch

61
00:02:19.330 --> 00:02:21.210
itself went off without a hitch.

62
00:02:21.850 --> 00:02:24.010
Anna: Okay, so what's the problem?

63
00:02:24.730 --> 00:02:27.650
Avery: The issue was discovered during routine

64
00:02:27.650 --> 00:02:30.600
post launch inspections. Officials from

65
00:02:30.600 --> 00:02:33.320
Roscosmos, Russia space agency

66
00:02:33.720 --> 00:02:36.520
reported finding damage to several launch

67
00:02:36.520 --> 00:02:37.560
pad components.

68
00:02:38.360 --> 00:02:40.920
Anna: That doesn't sound good. Do they know what

69
00:02:40.920 --> 00:02:43.320
caused it? Roscosmos is still assessing the

70
00:02:43.320 --> 00:02:45.600
situation, but they've said all the necessary

71
00:02:45.600 --> 00:02:47.880
spare parts are available for a quick repair.

72
00:02:48.360 --> 00:02:50.840
However, one expert, Brian Harvey, has

73
00:02:50.840 --> 00:02:53.720
suggested a possible cause. He believes a

74
00:02:53.720 --> 00:02:56.080
combination of the intense vibration and heat

75
00:02:56.080 --> 00:02:58.590
from the launch, along with some improperly

76
00:02:58.590 --> 00:03:00.790
installed roller pins, may have caused a

77
00:03:00.790 --> 00:03:03.110
service tower to topple over after the rocket

78
00:03:03.110 --> 00:03:06.110
had cleared the pad. Right. A service tower

79
00:03:06.110 --> 00:03:08.750
falling over would certainly count as damage.

80
00:03:09.310 --> 00:03:11.390
What does this mean for future launches?

81
00:03:11.790 --> 00:03:13.630
Avery: Harvey, uh, estimates it could take about

82
00:03:13.630 --> 00:03:16.110
three months to repair, likely scavenging

83
00:03:16.110 --> 00:03:18.670
parts from other launch pads. The good news

84
00:03:18.670 --> 00:03:21.230
is that the next crew handover at the ISS

85
00:03:21.310 --> 00:03:23.870
isn't scheduled until July, and the next

86
00:03:23.870 --> 00:03:26.590
astronaut mission from US soil is a

87
00:03:26.590 --> 00:03:29.250
SpaceX flight in February, so no

88
00:03:29.250 --> 00:03:31.730
astronauts are stranded. However, the next

89
00:03:31.730 --> 00:03:34.490
Russian Progress supply ship delivery to the

90
00:03:34.490 --> 00:03:37.250
spaceship will be delayed. We'll be keeping

91
00:03:37.250 --> 00:03:39.610
an eye on how quickly those repairs progress,

92
00:03:39.930 --> 00:03:42.370
but please note, there is no panic. And it

93
00:03:42.370 --> 00:03:44.570
isn't the end of the Russian space program.

94
00:03:44.730 --> 00:03:46.530
As has been reported in some of the more

95
00:03:46.530 --> 00:03:49.410
sensationalist media, it will be repaired

96
00:03:49.410 --> 00:03:50.410
and back in business.

97
00:03:51.050 --> 00:03:54.010
Anna: From problems on the ground to problems

98
00:03:54.010 --> 00:03:56.970
in orbit. Avery, we often talk about light

99
00:03:56.970 --> 00:03:59.860
pollution for ground based telescopes, but a,

100
00:03:59.860 --> 00:04:02.390
uh, new forecast reveals that even our eyes

101
00:04:02.390 --> 00:04:04.150
in space are not safe.

102
00:04:04.310 --> 00:04:06.510
Avery: You're talking about satellite mega

103
00:04:06.510 --> 00:04:08.870
constellations, right? I've seen some

104
00:04:08.870 --> 00:04:11.870
startling images of bright streaks ruining

105
00:04:11.870 --> 00:04:13.190
astronomical photos.

106
00:04:13.830 --> 00:04:16.710
Anna: Exactly, and it's getting worse. If the

107
00:04:16.710 --> 00:04:19.510
current industry proposals for about half a

108
00:04:19.510 --> 00:04:22.070
million new satellites become a reality,

109
00:04:22.230 --> 00:04:24.550
the problem will escalate dramatically.

110
00:04:24.950 --> 00:04:27.304
Projections show that by the2030s,

111
00:04:27.516 --> 00:04:30.430
1/3 of all images from the Hubble

112
00:04:30.430 --> 00:04:33.210
Space Telescope will be contamina with

113
00:04:33.210 --> 00:04:34.290
satellite trails.

114
00:04:34.930 --> 00:04:37.810
Avery: One third? That's a massive loss of data

115
00:04:37.810 --> 00:04:39.970
and time. For one of our most important

116
00:04:40.130 --> 00:04:42.450
scientific instruments, it is.

117
00:04:42.450 --> 00:04:45.290
Anna: And for some newer telescopes, it's even

118
00:04:45.290 --> 00:04:48.050
more dire. The Chinese space station

119
00:04:48.050 --> 00:04:50.970
telescope Sentient is projected to be

120
00:04:50.970 --> 00:04:53.690
the worst affected. Some studies predict

121
00:04:53.690 --> 00:04:56.530
contamination and more than 96%

122
00:04:56.610 --> 00:04:59.210
of its observations. With an average of

123
00:04:59.210 --> 00:05:02.210
92 satellite trails per exposure.

124
00:05:03.180 --> 00:05:06.020
Avery: 96%. At that point, the

125
00:05:06.020 --> 00:05:08.900
telescope is almost unusable for its intended

126
00:05:08.900 --> 00:05:11.500
purpose, it seems unsustainable.

127
00:05:12.140 --> 00:05:14.300
Are there any solutions being discussed?

128
00:05:14.780 --> 00:05:17.260
Anna: There are. Mitigation strategies are

129
00:05:17.260 --> 00:05:19.940
actively being developed. They include better

130
00:05:19.940 --> 00:05:22.580
orbital tracking to help astronomers avoid

131
00:05:22.580 --> 00:05:24.620
pointing at satellites, international

132
00:05:24.860 --> 00:05:26.940
coordination on satellite brightness

133
00:05:26.940 --> 00:05:29.340
standards, and perhaps most importantly,

134
00:05:29.580 --> 00:05:31.900
restricting the altitudes of these large

135
00:05:31.900 --> 00:05:33.420
constellations to below

136
00:05:34.520 --> 00:05:36.520
kilometers, which would reduce their

137
00:05:36.520 --> 00:05:39.200
visibility. It's a critical issue for the

138
00:05:39.200 --> 00:05:40.280
future of astronomy.

139
00:05:40.760 --> 00:05:43.480
Avery: It's a stark reminder of how crowded our

140
00:05:43.480 --> 00:05:44.920
orbital space is becoming.

141
00:05:45.560 --> 00:05:48.520
Okay, from our near space environment to our

142
00:05:48.520 --> 00:05:51.320
planetary neighbors, let's talk about Venus.

143
00:05:51.640 --> 00:05:54.280
We often call it Earth's twin. But new

144
00:05:54.280 --> 00:05:56.640
research is helping us understand one of the

145
00:05:56.640 --> 00:05:59.120
biggest differences between them. Plate

146
00:05:59.120 --> 00:05:59.680
tectonics.

147
00:05:59.680 --> 00:06:02.070
Anna: Plate. Right. Earth has this

148
00:06:02.070 --> 00:06:04.950
active moving crust, while Venus is often

149
00:06:04.950 --> 00:06:07.510
described as having a, uh, stagnant single

150
00:06:07.510 --> 00:06:09.590
plate surface. Why is that?

151
00:06:10.070 --> 00:06:12.390
Avery: An international team has developed a new

152
00:06:12.390 --> 00:06:15.030
framework for understanding how planets work

153
00:06:15.110 --> 00:06:17.670
geologically. Using numerical

154
00:06:17.670 --> 00:06:19.910
models, they identified six

155
00:06:20.070 --> 00:06:22.750
distinct regimes for planetary

156
00:06:22.750 --> 00:06:25.670
tectonics. Earth exists in what they

157
00:06:25.670 --> 00:06:28.510
call the mobile lid regime, which is

158
00:06:28.510 --> 00:06:30.510
crucial for our planet's long term

159
00:06:30.510 --> 00:06:33.170
habitability as it regulates climate by

160
00:06:33.170 --> 00:06:34.290
cycling carbon.

161
00:06:34.850 --> 00:06:37.810
Anna: The mobile lid. I like that. So

162
00:06:37.810 --> 00:06:39.650
what kind of lid does Venus have?

163
00:06:40.130 --> 00:06:42.530
Avery: The studies suggest Venus operates under

164
00:06:42.530 --> 00:06:45.330
what's called a plutonic squishy lid

165
00:06:45.490 --> 00:06:48.290
or an episodic squishy lid regime.

166
00:06:48.530 --> 00:06:51.330
In this model, the lithosphere, the planet's

167
00:06:51.330 --> 00:06:54.250
outer shell, is too hot and weak to

168
00:06:54.250 --> 00:06:56.850
break into distinct plates like Earth's.

169
00:06:57.090 --> 00:06:59.650
Instead, rising magma from the mantle

170
00:06:59.650 --> 00:07:01.330
weakens the crust from below.

171
00:07:02.370 --> 00:07:04.930
Anna: A squishy lid. So it doesn't move

172
00:07:04.930 --> 00:07:07.570
globally, but it's not totally inactive

173
00:07:07.570 --> 00:07:07.970
either.

174
00:07:08.530 --> 00:07:11.170
Avery: Precisely. This leads to regional

175
00:07:11.330 --> 00:07:14.050
intermittent volcanism rather than the global

176
00:07:14.050 --> 00:07:17.010
tectonics we see here. And this model

177
00:07:17.010 --> 00:07:19.010
actually helps explain some other recent

178
00:07:19.010 --> 00:07:21.650
discoveries. We've seen findings suggesting

179
00:07:21.650 --> 00:07:24.450
there are active volcanoes on Venus, which

180
00:07:24.530 --> 00:07:27.170
seemed puzzling without plate tectonics.

181
00:07:27.490 --> 00:07:30.410
This squishy lid idea provides a mechanism

182
00:07:30.410 --> 00:07:32.290
for that volcanism to occur.

183
00:07:33.230 --> 00:07:36.030
Anna: Speaking of spectacular space phenomena,

184
00:07:36.190 --> 00:07:38.350
let's turn back to the James Webb Space

185
00:07:38.350 --> 00:07:40.750
Telescope. It has captured another

186
00:07:40.830 --> 00:07:43.630
breathtaking image, this time of a close

187
00:07:43.630 --> 00:07:46.190
encounter between two dwarf galaxies.

188
00:07:46.830 --> 00:07:49.390
Avery: Oh, I saw this one. The image is just

189
00:07:49.390 --> 00:07:52.030
stunning. It's the pair NGC

190
00:07:52.110 --> 00:07:54.590
4490 and NGC

191
00:07:54.590 --> 00:07:56.190
4485. Right.

192
00:07:56.750 --> 00:07:59.390
Anna: That's them. They're about 24 million

193
00:07:59.470 --> 00:08:01.550
light years away, and they're in the process

194
00:08:01.550 --> 00:08:03.870
of colliding. The Webb image

195
00:08:04.650 --> 00:08:07.490
detailed it reveals a glowing bridge of gas

196
00:08:07.490 --> 00:08:10.090
and streams of newborn stars

197
00:08:10.170 --> 00:08:12.290
connecting the two galaxies. The

198
00:08:12.290 --> 00:08:14.450
gravitational interaction between them has

199
00:08:14.450 --> 00:08:16.770
spurred a massive burst of new star

200
00:08:16.770 --> 00:08:17.370
formation.

201
00:08:18.330 --> 00:08:20.690
Avery: So they're creating new stars as, ah, they

202
00:08:20.690 --> 00:08:23.370
pull each other apart. That's poetic.

203
00:08:23.770 --> 00:08:26.170
Can we tell how this interaction unfolded?

204
00:08:26.330 --> 00:08:28.810
Anna: We can. By analyzing the different

205
00:08:28.810 --> 00:08:31.770
populations of stars, researchers have been

206
00:08:31.770 --> 00:08:34.490
able to trace the timeline to. They suggest

207
00:08:34.570 --> 00:08:37.290
the two galaxies first swept past each

208
00:08:37.290 --> 00:08:39.850
other about 200 million years ago.

209
00:08:40.330 --> 00:08:43.050
During that pass, the larger galaxy,

210
00:08:43.130 --> 00:08:45.050
NGC4490

211
00:08:45.690 --> 00:08:48.330
began siphoning gas from its smaller

212
00:08:48.330 --> 00:08:50.970
partner, NGC4485.

213
00:08:51.530 --> 00:08:54.490
That stolen gas is now fueling the starburst

214
00:08:54.490 --> 00:08:56.410
we see in that glowing bridge.

215
00:08:57.210 --> 00:08:59.850
Avery: Incredible. It's like cosmic

216
00:08:59.850 --> 00:09:02.840
archaeology. A fantastic image with a

217
00:09:02.840 --> 00:09:04.440
fascinating story behind it.

218
00:09:05.080 --> 00:09:07.960
Now for our final story, we're coming

219
00:09:07.960 --> 00:09:10.680
much closer to home, to our very

220
00:09:10.680 --> 00:09:13.280
own star. In early November,

221
00:09:13.280 --> 00:09:16.040
astronomers captured some extremely rare

222
00:09:16.120 --> 00:09:18.960
high definition images of sunspots in

223
00:09:18.960 --> 00:09:21.600
an active region designated NOAA

224
00:09:21.600 --> 00:09:23.080
14,274.

225
00:09:24.040 --> 00:09:26.200
Anna: And what makes these images so special?

226
00:09:27.090 --> 00:09:29.930
Avery: The timing. The images were taken by

227
00:09:29.930 --> 00:09:32.610
the Gregor solar telescope in Spain

228
00:09:32.930 --> 00:09:35.730
just 30 minutes before those same sunspots

229
00:09:35.730 --> 00:09:38.210
erupted, emitting a powerful

230
00:09:38.210 --> 00:09:40.770
X1.2 class solar flare.

231
00:09:41.970 --> 00:09:44.810
Anna: Wow. That's like having a camera pointed at a

232
00:09:44.810 --> 00:09:47.650
volcano right before it blows. Capturing

233
00:09:47.650 --> 00:09:49.930
that with a ground based telescope must be

234
00:09:49.930 --> 00:09:51.250
incredibly difficult.

235
00:09:51.730 --> 00:09:54.630
Avery: It is. You have to be looking at the

236
00:09:54.630 --> 00:09:57.110
right spot at the right time, and you need

237
00:09:57.110 --> 00:09:59.750
clear weather. It's a rare trifecta.

238
00:10:00.070 --> 00:10:03.030
The images are remarkable. They show what

239
00:10:03.030 --> 00:10:05.870
are called penumbral fibrils. These are

240
00:10:05.870 --> 00:10:08.549
the filaments extending from the dark center

241
00:10:08.549 --> 00:10:11.430
of the sunspot that are strongly curved and

242
00:10:11.430 --> 00:10:12.310
braided together.

243
00:10:13.670 --> 00:10:15.750
Anna: And what does that braiding tell us?

244
00:10:16.150 --> 00:10:18.870
Avery: It's a clear visual indicator of a highly

245
00:10:18.870 --> 00:10:21.790
stressed and tangled magnetic field. Think

246
00:10:21.790 --> 00:10:24.790
of it like a tightly wound rubber band.

247
00:10:25.190 --> 00:10:27.670
That immense stored energy is a direct

248
00:10:27.750 --> 00:10:30.550
precursor to an explosive release, which

249
00:10:30.550 --> 00:10:32.790
is exactly what happened 30 minutes later

250
00:10:32.790 --> 00:10:35.630
with the solar flare. And this is just the

251
00:10:35.630 --> 00:10:37.590
beginning. Researchers are currently

252
00:10:37.670 --> 00:10:40.510
processing nearly 40,000 more data sets from

253
00:10:40.510 --> 00:10:42.990
the telescope, which could revolutionize how

254
00:10:42.990 --> 00:10:45.430
we predict these powerful solar events.

255
00:10:46.800 --> 00:10:49.200
Anna: And better prediction is crucial.

256
00:10:49.520 --> 00:10:52.080
These powerful solar events can disrupt

257
00:10:52.160 --> 00:10:55.000
satellites, power grids, and even pose a

258
00:10:55.000 --> 00:10:57.760
risk to astronauts. Understanding their

259
00:10:57.760 --> 00:11:00.440
warning signs is vital for our technological

260
00:11:00.440 --> 00:11:03.320
infrastructure. And that brings us to

261
00:11:03.320 --> 00:11:06.080
the end of our news roundup for today. It's

262
00:11:06.080 --> 00:11:08.160
been another busy day in the cosmos.

263
00:11:08.560 --> 00:11:11.400
Avery: It certainly has. Thanks for joining us on

264
00:11:11.400 --> 00:11:13.910
Astronomy Daily. We'll be back again tomorrow

265
00:11:13.910 --> 00:11:16.110
with another look at the latest news from

266
00:11:16.110 --> 00:11:18.830
across the universe. Until then, I'm Avery

267
00:11:19.070 --> 00:11:20.030
and I'm Anna.

268
00:11:20.030 --> 00:11:22.030
Anna: Reminding you to keep looking up

269
00:11:22.190 --> 00:11:23.470
Astronomy Day.

270
00:11:24.990 --> 00:11:26.430
Avery: The stories we told.

271
00:11:32.990 --> 00:11:34.350
The stories the to.
