Jan. 28, 2026

Solar Sentinel Reaches L1, Challenger's 40-Year Legacy, and AI's Hubble Discoveries

Solar Sentinel Reaches L1, Challenger's 40-Year Legacy, and AI's Hubble Discoveries

## Today's Headlines: 🛰️ **NOAA Solar Observatory Reaches L1** NOAA's Space Weather Follow-On satellite successfully arrived at Lagrange point 1 on January 21st, establishing the first component of a future constellation designed to provide early...

## Today's Headlines:
🛰️ **NOAA Solar Observatory Reaches L1**  
NOAA's Space Weather Follow-On satellite successfully arrived at Lagrange point 1 on January 21st, establishing the first component of a future constellation designed to provide early warning of solar storms and coronal mass ejections. The satellite offers 15-60 minutes advance notice of space weather events that could impact Earth's infrastructure.
🚀 **Challenger Disaster: 40 Years Later**  
Marking four decades since the Space Shuttle Challenger tragedy, we examine how unseasonably cold weather and O-ring failures led to the loss of seven crew members. The disaster fundamentally changed NASA's safety culture and decision-making processes, lessons that continue to influence spaceflight today.
🤖 **AI Uncovers Cosmic Treasures in Hubble Archive**  
Advanced artificial intelligence algorithms have identified hundreds of previously undetected gravitational lenses in Hubble Space Telescope data. These discoveries include rare Einstein rings and exotic lensing configurations that provide windows into the early universe and dark matter distribution.
☄️ **Venus's Potential Meteor Shower**  
Astronomers predict Venus may experience a significant meteor shower in July 2026 from debris of asteroid 2002 VT37. The event offers a rare opportunity to study how meteor showers interact with Venus's dense carbon dioxide atmosphere.
🌌 **Stellar Fireworks at the Galactic Center**  
New observations reveal intense stellar activity near Sagittarius A*, our galaxy's supermassive black hole, including star formation, supernovae, and tidal disruption events in one of the most extreme environments in the Milky Way.
📡 **Watch Artemis 2 Rocket Live**  
NASA has launched a 24-hour livestream of the Artemis 2 Space Launch System rocket on Launch Pad 39B as crews prepare for the first crewed lunar mission since 1972, currently targeting April 2026.  https://www.youtube.com/watch?v=nrVnsO_rdew
#### Resources & Links:
- Story Sources: SpaceNews, Spectrum Local News, NASA Science, Space.com, Universe Today
- Website: astronomydaily.io
- Social Media: @AstroDailyPod (all platforms)

Become a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-space-news-updates--5648921/support.

Sponsor Details:
Ensure your online privacy by using NordVPN. To get our special listener deal and save a lot of money, visit www.bitesz.com/nordvpn. You'll be glad you did!

Become a supporter of Astronomy Daily by joining our Supporters Club. Commercial free episodes daily are only a click way... Click Here

This episode includes AI-generated content.

WEBVTT

0
00:00:00.320 --> 00:00:03.080
Anna: Welcome to Astronomy Daily, your source for

1
00:00:03.080 --> 00:00:06.080
the latest space and astronomy news. I'm

2
00:00:06.080 --> 00:00:06.640
Anna.

3
00:00:06.800 --> 00:00:09.360
Avery: And I'm Avery. Today is Wednesday, January

4
00:00:09.520 --> 00:00:12.040
28, 2026, and we've got a

5
00:00:12.040 --> 00:00:14.000
fantastic lineup of storeys for you.

6
00:00:14.160 --> 00:00:16.560
Anna: We certainly do. We'll be covering

7
00:00:16.560 --> 00:00:19.360
NOAA's new solar observatory reaching its

8
00:00:19.360 --> 00:00:21.880
destination, looking back at how weather

9
00:00:21.880 --> 00:00:24.640
played a tragic role in the Talinger disaster

10
00:00:24.720 --> 00:00:27.240
40 years ago, and discovering how

11
00:00:27.240 --> 00:00:30.000
AI is uncovering hidden cosmic

12
00:00:30.000 --> 00:00:32.580
treasures in Hubble's AR Plus,

13
00:00:32.580 --> 00:00:33.380
Venus might be.

14
00:00:33.380 --> 00:00:35.980
Avery: In for a spectacular meteor shower this July.

15
00:00:36.380 --> 00:00:38.580
We'll explore stellar fireworks at the heart

16
00:00:38.580 --> 00:00:41.140
of our galaxy. And NASA is giving us a live

17
00:00:41.140 --> 00:00:43.460
view of the Artemis 2 moon rocket on the

18
00:00:43.460 --> 00:00:44.060
launch pad.

19
00:00:44.300 --> 00:00:45.420
Anna: Let's dive right in.

20
00:00:45.740 --> 00:00:47.980
Avery: Our top storey today takes us about a million

21
00:00:48.060 --> 00:00:50.391
miles from Earth, where NOAA's Space Weather

22
00:00:50.469 --> 00:00:53.380
Follow on Lagrange 1 Observatory has just

23
00:00:53.380 --> 00:00:55.860
arrived at its permanent home. Anna, uh, this

24
00:00:55.860 --> 00:00:58.060
is a pretty significant milestone for space

25
00:00:58.060 --> 00:00:59.500
weather monitoring, isn't it?

26
00:00:59.860 --> 00:01:02.580
Anna: Absolutely, Avery. This observatory reached

27
00:01:02.580 --> 00:01:05.500
Lagrange Point 1, or L1, on

28
00:01:05.500 --> 00:01:08.260
January 21, after launching back in

29
00:01:08.260 --> 00:01:11.180
June 2024. Now, uh, for our listeners

30
00:01:11.180 --> 00:01:13.980
who might not be familiar, L1 is this

31
00:01:13.980 --> 00:01:16.580
special gravitational sweet spot between

32
00:01:16.660 --> 00:01:19.460
Earth and the sun, about 1.5

33
00:01:19.460 --> 00:01:21.380
million kilometres from our planet.

34
00:01:21.620 --> 00:01:24.340
Avery: And what makes this location so ideal for

35
00:01:24.340 --> 00:01:25.140
watching the Sun?

36
00:01:25.550 --> 00:01:28.510
Anna: Well, at L1, the observatory maintains a

37
00:01:28.510 --> 00:01:31.430
constant view of the sun while orbiting in

38
00:01:31.430 --> 00:01:34.350
sync with Earth. It's like having a cosmic

39
00:01:34.350 --> 00:01:36.870
early warning system. The satellite can

40
00:01:36.870 --> 00:01:39.270
detect solar storms and coronal mass

41
00:01:39.270 --> 00:01:41.870
ejections headed our way, giving us that

42
00:01:41.870 --> 00:01:44.430
crucial advance notice, typically about

43
00:01:44.510 --> 00:01:47.510
15 to 60 minutes before these events

44
00:01:47.510 --> 00:01:48.350
impact Earth.

45
00:01:48.590 --> 00:01:50.750
Avery: That advance warning time is critical, isn't

46
00:01:50.750 --> 00:01:52.750
it? I mean, we're talking about protecting

47
00:01:52.750 --> 00:01:55.230
everything from power grids to satellites.

48
00:01:55.630 --> 00:01:57.830
Anna: Exactly right. And here's what's really

49
00:01:57.830 --> 00:02:00.510
exciting. It's not just one observatory,

50
00:02:00.670 --> 00:02:03.390
it's a constellation. NOAA is planning

51
00:02:03.390 --> 00:02:05.990
four more satellites for L1, plus

52
00:02:05.990 --> 00:02:08.270
additional ones at, uh, Lagrange point five.

53
00:02:08.750 --> 00:02:11.150
Together, they'll create this comprehensive

54
00:02:11.309 --> 00:02:13.510
solar monitoring network. The second

55
00:02:13.510 --> 00:02:15.950
satellite is already scheduled to launch in

56
00:02:15.950 --> 00:02:16.910
2027.

57
00:02:17.310 --> 00:02:19.790
Avery: So we're looking at a much more robust space

58
00:02:19.790 --> 00:02:21.790
weather forecasting capability in the near

59
00:02:21.790 --> 00:02:22.110
future.

60
00:02:22.670 --> 00:02:25.010
Anna: Precisely. And given how dependent our, uh,

61
00:02:25.070 --> 00:02:27.510
modern infrastructure is on satellites and

62
00:02:27.510 --> 00:02:30.270
power grids, this kind of monitoring becomes

63
00:02:30.270 --> 00:02:33.150
more important every year. The observatory

64
00:02:33.150 --> 00:02:36.030
is now beginning what NOAA calls an extended

65
00:02:36.030 --> 00:02:38.469
checkout period before it becomes fully

66
00:02:38.469 --> 00:02:39.070
operational.

67
00:02:39.630 --> 00:02:42.030
Avery: Moving to a More sombre note, January

68
00:02:42.110 --> 00:02:44.790
28th marks 40 years since the space Shuttle

69
00:02:44.790 --> 00:02:47.390
Challenger disaster. Anna, uh, there's been

70
00:02:47.390 --> 00:02:49.830
renewed focus on how weather and engineering

71
00:02:49.830 --> 00:02:51.630
decisions played into that tragedy.

72
00:02:51.950 --> 00:02:54.670
Anna: Yes. And it's a powerful reminder of how

73
00:02:54.670 --> 00:02:56.990
critical environmental factors are in

74
00:02:56.990 --> 00:02:59.310
spaceflight. You know, Avery, the night

75
00:02:59.310 --> 00:03:01.910
before that launch, temperatures at Kennedy

76
00:03:01.910 --> 00:03:04.630
Space Centre dropped to just 28 degrees

77
00:03:04.630 --> 00:03:07.390
Fahrenheit. That's minus 2 Celsius

78
00:03:07.630 --> 00:03:10.030
for Florida. That was exceptionally cold.

79
00:03:10.350 --> 00:03:12.070
Avery: And, um, those cold temperatures were at the

80
00:03:12.070 --> 00:03:13.470
heart of the problem, weren't they?

81
00:03:13.550 --> 00:03:16.390
Anna: They were. Engineers from Morton Thykol,

82
00:03:16.390 --> 00:03:18.390
the company that built the solid rocket

83
00:03:18.390 --> 00:03:21.030
boosters, were deeply concerned about the O

84
00:03:21.030 --> 00:03:23.430
rings, these critical rubber seals in the

85
00:03:23.430 --> 00:03:26.090
boost joints. They'd never been tested below

86
00:03:26.170 --> 00:03:28.930
53 degrees Fahrenheit, and the engineers

87
00:03:28.930 --> 00:03:31.090
warned that the cold could make them too

88
00:03:31.090 --> 00:03:32.650
stiff to seal properly.

89
00:03:32.810 --> 00:03:34.490
Avery: But the launch went ahead anyway.

90
00:03:34.570 --> 00:03:37.370
Anna: It did. Despite the engineering concerns,

91
00:03:37.450 --> 00:03:39.850
there was enormous pressure to maintain the

92
00:03:39.850 --> 00:03:42.730
launch schedule. NASA had already postponed

93
00:03:42.730 --> 00:03:45.210
the mission several times, and there was this

94
00:03:45.210 --> 00:03:47.450
institutional momentum to proceed.

95
00:03:47.930 --> 00:03:50.570
73 seconds after liftoff, hot

96
00:03:50.570 --> 00:03:53.170
gases escaped through a failed O ring

97
00:03:53.170 --> 00:03:56.130
seal, leading to the catastrophic breakup of

98
00:03:56.130 --> 00:03:56.850
Challenger.

99
00:03:57.010 --> 00:03:59.810
Avery: It's heartbreaking. Seven crew members lost,

100
00:03:59.890 --> 00:04:01.930
including Christa McAuliffe, who would have

101
00:04:01.930 --> 00:04:03.330
been the first teacher in space.

102
00:04:03.810 --> 00:04:06.529
Anna: The tragedy fundamentally changed how

103
00:04:06.529 --> 00:04:09.490
NASA approached decision making. The Rogers

104
00:04:09.490 --> 00:04:11.610
Commission investigation that followed was

105
00:04:11.610 --> 00:04:14.290
incredibly thorough, and it led to major

106
00:04:14.370 --> 00:04:17.170
reforms in safety, culture and communication.

107
00:04:18.010 --> 00:04:20.330
One of the key findings was that engineering

108
00:04:20.330 --> 00:04:22.970
concerns need to override schedule

109
00:04:22.970 --> 00:04:24.090
pressures. Always.

110
00:04:24.810 --> 00:04:27.130
Avery: And those lessons still resonate today, don't

111
00:04:27.130 --> 00:04:29.810
they? I mean, we see NASA taking extra time

112
00:04:29.810 --> 00:04:32.330
with Artemis missions being very methodical.

113
00:04:32.810 --> 00:04:35.810
Anna: Absolutely. The Challenger disaster taught

114
00:04:35.810 --> 00:04:38.650
us that in spaceflight, there's no such thing

115
00:04:38.650 --> 00:04:41.450
as a routine launch. Every mission

116
00:04:41.450 --> 00:04:44.090
requires the same level of scrutiny and

117
00:04:44.090 --> 00:04:46.760
respect for engineering limits. It's a

118
00:04:46.760 --> 00:04:49.720
lesson paid for with seven lives and one

119
00:04:49.720 --> 00:04:51.040
we must never forget.

120
00:04:51.280 --> 00:04:53.600
Avery: On a brighter note, let's talk about some

121
00:04:53.600 --> 00:04:56.160
exciting discoveries from the Hubble Space

122
00:04:56.160 --> 00:04:58.680
Telescope. Anna? Uh, artificial

123
00:04:58.680 --> 00:05:01.400
intelligence has just helped astronomers

124
00:05:01.400 --> 00:05:03.800
uncover hundreds of previously

125
00:05:03.800 --> 00:05:06.760
undetected cosmic objects in Hubble's

126
00:05:06.760 --> 00:05:07.760
vast archives.

127
00:05:08.080 --> 00:05:11.040
Anna: This is fascinating stuff, Avery. So

128
00:05:11.040 --> 00:05:13.920
researchers have developed this AI algorithm

129
00:05:13.920 --> 00:05:16.240
that can sift through decades of Hubble

130
00:05:16.240 --> 00:05:18.580
observations. And it's finding things that

131
00:05:18.580 --> 00:05:20.140
human astronomers missed.

132
00:05:20.540 --> 00:05:23.340
Avery: Exactly. The algorithm focuses on

133
00:05:23.340 --> 00:05:25.700
something called gravitational lensing. When

134
00:05:25.700 --> 00:05:28.300
a massive object like a galaxy cluster

135
00:05:28.460 --> 00:05:30.820
bends light from more distant objects behind

136
00:05:30.820 --> 00:05:33.820
it. Einstein predicted this effect. And it's

137
00:05:33.820 --> 00:05:36.220
like having a natural cosmic magnifier.

138
00:05:36.620 --> 00:05:39.180
Anna: And these lensed objects can tell us a lot

139
00:05:39.180 --> 00:05:40.860
about the early universe, right?

140
00:05:41.340 --> 00:05:43.900
Avery: They can. The AI has identified

141
00:05:43.980 --> 00:05:46.460
hundreds of gravitational lens candidates,

142
00:05:46.890 --> 00:05:49.330
including some exceptionally distant galaxies

143
00:05:49.330 --> 00:05:52.050
from when the universe was very young. What's

144
00:05:52.050 --> 00:05:53.970
really clever about this approach is that the

145
00:05:53.970 --> 00:05:56.610
algorithm was trained on existing verified

146
00:05:56.610 --> 00:05:59.330
gravitational lenses. So it knows what to

147
00:05:59.330 --> 00:05:59.770
look for.

148
00:06:00.330 --> 00:06:02.570
Anna: So it's not just finding more of the same,

149
00:06:02.810 --> 00:06:05.490
it's finding rare and unusual examples

150
00:06:05.490 --> 00:06:05.850
too.

151
00:06:06.490 --> 00:06:09.410
Avery: That's what makes this so exciting. The AI is

152
00:06:09.410 --> 00:06:12.130
uncovering exotic lensing configurations that

153
00:06:12.130 --> 00:06:14.610
would be extremely time consuming for humans

154
00:06:14.610 --> 00:06:17.480
to find manually. We're talking about complex

155
00:06:17.640 --> 00:06:20.600
multi image systems arc like structures,

156
00:06:20.840 --> 00:06:23.160
even Einstein rings where the background

157
00:06:23.160 --> 00:06:24.920
object is perfectly aligned.

158
00:06:25.240 --> 00:06:27.880
Anna: And Hubble has been collecting data for over

159
00:06:27.880 --> 00:06:30.720
30 years now. So there's this enormous

160
00:06:30.720 --> 00:06:31.800
archive to mine.

161
00:06:32.280 --> 00:06:34.560
Avery: Right. It's like having a treasure trove that

162
00:06:34.560 --> 00:06:36.560
we're only now learning how to properly

163
00:06:36.560 --> 00:06:39.040
search. These discoveries will help us

164
00:06:39.040 --> 00:06:41.680
understand dark matter distribution in galaxy

165
00:06:41.680 --> 00:06:44.600
clusters, study extremely distant galaxies

166
00:06:44.600 --> 00:06:46.760
that would otherwise be too faint to detect

167
00:06:47.160 --> 00:06:49.880
and refine our models of cosmic evolution.

168
00:06:50.440 --> 00:06:52.840
Anna: It really shows how AI and human

169
00:06:52.840 --> 00:06:55.760
astronomers can work together. The AI does

170
00:06:55.760 --> 00:06:57.680
the heavy lifting of searching through

171
00:06:57.680 --> 00:07:00.360
millions of images and then human experts

172
00:07:00.360 --> 00:07:02.640
verify and study the most interesting

173
00:07:02.640 --> 00:07:03.240
candidates.

174
00:07:03.720 --> 00:07:05.960
Avery: Exactly. It's not replacing

175
00:07:05.960 --> 00:07:08.200
astronomers, it's amplifying what they can

176
00:07:08.200 --> 00:07:10.660
achieve. And as these AI tools get more

177
00:07:10.660 --> 00:07:13.140
sophisticated, who knows what other cosmic

178
00:07:13.140 --> 00:07:15.340
secrets might be hiding in plain sight in our

179
00:07:15.340 --> 00:07:15.860
archives.

180
00:07:16.500 --> 00:07:18.820
Anna: Now for something you don't hear every

181
00:07:19.380 --> 00:07:22.180
Venus might be getting a meteor shower.

182
00:07:22.340 --> 00:07:25.219
Avery, tell us about this cosmic event coming

183
00:07:25.220 --> 00:07:25.860
this July.

184
00:07:26.260 --> 00:07:28.690
Avery: This is a really cool storey, Anna. Uh,

185
00:07:28.690 --> 00:07:31.060
astronomers had determined that Venus could

186
00:07:31.060 --> 00:07:33.860
experience a significant meteor shower in

187
00:07:33.860 --> 00:07:36.740
July 2026. And it uh, all traces

188
00:07:36.740 --> 00:07:39.140
back to an asteroid breakup that happened

189
00:07:39.140 --> 00:07:42.060
long ago. We're talking about debris from

190
00:07:42.060 --> 00:07:44.072
asteroid 2002

191
00:07:44.368 --> 00:07:45.700
VT37.

192
00:07:46.260 --> 00:07:49.260
Anna: Though an asteroid broke apart and now its

193
00:07:49.260 --> 00:07:51.220
debris is going to hit Venus?

194
00:07:51.779 --> 00:07:54.420
Avery: Essentially, yes. When asteroids

195
00:07:54.420 --> 00:07:57.340
collide or break apart, they create streams

196
00:07:57.340 --> 00:07:59.460
of debris that continue orbiting the Sun.

197
00:07:59.940 --> 00:08:02.300
Earth regularly passes through these debris

198
00:08:02.300 --> 00:08:04.260
streams. That's what causes our meteor

199
00:08:04.260 --> 00:08:06.660
showers like the Perseids or the Geminites.

200
00:08:07.150 --> 00:08:09.110
Anna: But we don't usually think about other

201
00:08:09.110 --> 00:08:10.830
planets having meteor showers.

202
00:08:11.150 --> 00:08:13.870
Avery: We don't, and that's partly because we can't

203
00:08:13.870 --> 00:08:16.070
observe them as easily. But

204
00:08:16.070 --> 00:08:18.510
mathematical modelling shows that Venus's

205
00:08:18.510 --> 00:08:20.350
orbit will take it through this particular

206
00:08:20.510 --> 00:08:23.390
debris stream in July. The timing and

207
00:08:23.390 --> 00:08:26.230
geometry appear to line up for a genuine

208
00:08:26.230 --> 00:08:27.470
meteor shower event.

209
00:08:27.870 --> 00:08:30.430
Anna: What would that look like? I mean, Venus has

210
00:08:30.430 --> 00:08:32.750
that incredibly thick atmosphere, right?

211
00:08:33.210 --> 00:08:36.170
Avery: It does. Venus's atmosphere is about 90

212
00:08:36.250 --> 00:08:38.930
times denser than Earth's and is mostly

213
00:08:38.930 --> 00:08:41.930
carbon dioxide. Any meteors entering that

214
00:08:41.930 --> 00:08:43.970
atmosphere would experience tremendous

215
00:08:43.970 --> 00:08:46.730
heating and friction. They'd likely burn up

216
00:08:46.730 --> 00:08:49.010
at, uh, much higher altitudes than meteors do

217
00:08:49.010 --> 00:08:51.650
on Earth, creating bright streaks across the

218
00:08:51.650 --> 00:08:52.730
Venusian sky.

219
00:08:52.890 --> 00:08:55.250
Anna: Though I suppose nobody's going to be on the

220
00:08:55.250 --> 00:08:56.810
surface watching this Light show?

221
00:08:57.130 --> 00:08:59.810
Avery: No. Surface conditions on Venus are pretty

222
00:08:59.810 --> 00:09:02.610
inhospitable. We're talking temperatures hot

223
00:09:02.610 --> 00:09:05.010
enough to melt lead and crushing

224
00:09:05.010 --> 00:09:08.010
atmospheric pressure. But spacecraft in orbit

225
00:09:08.010 --> 00:09:10.090
around Venus, or even Earth based

226
00:09:10.090 --> 00:09:12.890
observations with certain wavelength might be

227
00:09:12.890 --> 00:09:15.090
able to detect evidence of the meteor shower.

228
00:09:15.250 --> 00:09:17.370
Anna: Could this tell us anything scientifically

229
00:09:17.370 --> 00:09:17.890
valuable?

230
00:09:18.290 --> 00:09:21.010
Avery: Absolutely. Studying how meteor

231
00:09:21.010 --> 00:09:23.210
showers interact with Venus's unique

232
00:09:23.210 --> 00:09:25.370
atmosphere could give us insights into

233
00:09:25.370 --> 00:09:27.490
atmosphere chemistry and dynamics.

234
00:09:28.140 --> 00:09:30.340
Plus it helps us understand the distribution

235
00:09:30.340 --> 00:09:32.620
of debris throughout the inner solar system.

236
00:09:33.100 --> 00:09:35.740
And it's just a reminder that these dramatic

237
00:09:35.740 --> 00:09:38.380
cosmic events aren't exclusive to Earth.

238
00:09:38.700 --> 00:09:41.300
Anna: Speaking of dramatic cosmic events, let's

239
00:09:41.300 --> 00:09:44.100
head to the centre of our own galaxy. Avery.

240
00:09:44.100 --> 00:09:45.780
Astronomers have been observing what they're

241
00:09:45.780 --> 00:09:48.220
calling stellar fireworks at the heart of the

242
00:09:48.220 --> 00:09:48.860
Milky Way.

243
00:09:49.180 --> 00:09:52.100
Avery: The galactic centre is such a wild place,

244
00:09:52.100 --> 00:09:55.020
isn't it? I mean, we've got that supermassive

245
00:09:55.020 --> 00:09:57.780
black hole, Sagittarius A, and

246
00:09:57.780 --> 00:10:00.280
all sorts of extreme phys going on there.

247
00:10:00.360 --> 00:10:03.320
Anna: It really is cosmic chaos in the best way

248
00:10:03.320 --> 00:10:06.120
possible. The region around Sagittarius A

249
00:10:06.280 --> 00:10:09.200
is incredibly dense with stars, gas and

250
00:10:09.200 --> 00:10:11.760
dust. And what astronomers are seeing is a

251
00:10:11.760 --> 00:10:14.200
spectacular display of stellar activity.

252
00:10:14.600 --> 00:10:17.440
Massive stars being born, living out their

253
00:10:17.440 --> 00:10:20.040
brief but brilliant lives and dying in

254
00:10:20.040 --> 00:10:21.400
supernova explosions.

255
00:10:21.640 --> 00:10:23.630
Avery: And all of this is happening in a, uh,

256
00:10:23.680 --> 00:10:25.880
relatively small region of space, right?

257
00:10:26.350 --> 00:10:29.230
Anna: Exactly. The galactic centre is an incredibly

258
00:10:29.230 --> 00:10:31.670
compact environment. You've got stellar

259
00:10:31.670 --> 00:10:33.630
densities that are millions of times higher

260
00:10:33.630 --> 00:10:35.630
than what we see in our solar neighbourhood.

261
00:10:35.950 --> 00:10:38.070
Stars are packed so tightly that

262
00:10:38.070 --> 00:10:40.550
gravitational interactions are common and the

263
00:10:40.550 --> 00:10:42.509
radiation environment is intense.

264
00:10:42.910 --> 00:10:45.350
Avery: What kind of observations are revealing these

265
00:10:45.350 --> 00:10:46.110
fireworks?

266
00:10:46.350 --> 00:10:48.710
Anna: Astronomers are using multiple wavelengths,

267
00:10:48.710 --> 00:10:51.310
infrared x ray and radio observations

268
00:10:51.550 --> 00:10:53.450
to peer through the thick dust that obscures,

269
00:10:53.450 --> 00:10:55.710
um, the galactic centre in visible light.

270
00:10:56.180 --> 00:10:58.500
What they're seeing are energetic outbursts,

271
00:10:58.740 --> 00:11:01.260
shock waves from supernova remnants, and

272
00:11:01.260 --> 00:11:04.140
evidence of stars being torn apart by intense

273
00:11:04.140 --> 00:11:06.340
tidal forces near the black hole.

274
00:11:06.580 --> 00:11:09.540
Avery: That sounds pretty dramatic, stars

275
00:11:09.540 --> 00:11:10.580
being torn apart.

276
00:11:10.820 --> 00:11:13.340
Anna: Yes. There's this phenomenon called tidal

277
00:11:13.340 --> 00:11:15.780
disruption, where a star that ventures too

278
00:11:15.780 --> 00:11:18.740
close to Sagittarius A gets stretched by

279
00:11:18.740 --> 00:11:21.420
gravitational forces, sort of like cosmic

280
00:11:21.420 --> 00:11:24.350
spaghettification. The star literally gets

281
00:11:24.350 --> 00:11:26.910
pulled apart and some of that material falls

282
00:11:26.910 --> 00:11:29.350
into the black hole while the rest is ejected

283
00:11:29.350 --> 00:11:30.750
at tremendous speeds.

284
00:11:30.990 --> 00:11:33.550
Avery: And, um, we're also seeing new stars forming

285
00:11:33.550 --> 00:11:35.070
in this extreme environment.

286
00:11:35.630 --> 00:11:38.070
Anna: You're. Despite the harsh conditions, or

287
00:11:38.070 --> 00:11:40.470
perhaps because of them, there are regions of

288
00:11:40.470 --> 00:11:42.990
intense star formation. The gravitational

289
00:11:42.990 --> 00:11:45.590
compression from all that mass can trigger

290
00:11:45.590 --> 00:11:48.030
the collapse of gas clouds, leading to new

291
00:11:48.030 --> 00:11:50.360
stellar births. These tend to be very

292
00:11:50.440 --> 00:11:53.240
massive, hot stars that burn bright and

293
00:11:53.240 --> 00:11:53.880
die young.

294
00:11:54.200 --> 00:11:57.000
Avery: It's almost like the galactic centre is this

295
00:11:57.000 --> 00:11:59.560
constant cycle of creation and destruction.

296
00:11:59.800 --> 00:12:02.160
Anna: That's a perfect way to describe it. And

297
00:12:02.160 --> 00:12:04.360
study in this region helps us understand how

298
00:12:04.360 --> 00:12:07.360
galaxies evolve, how supermassive black holes

299
00:12:07.360 --> 00:12:09.240
influence their surroundings, and what

300
00:12:09.240 --> 00:12:11.240
conditions were like in the early universe

301
00:12:11.240 --> 00:12:13.560
when star formation was much more vigorous

302
00:12:13.560 --> 00:12:14.120
everywhere.

303
00:12:14.440 --> 00:12:17.000
Avery: For our final storey, let's come back closer

304
00:12:17.000 --> 00:12:19.950
to home. NASA has launched a 24

305
00:12:19.950 --> 00:12:22.510
hour livestream showing the Artemis II moon

306
00:12:22.510 --> 00:12:24.790
rocket on the launch pad at Kennedy Space

307
00:12:24.790 --> 00:12:25.230
Centre.

308
00:12:25.630 --> 00:12:27.350
Anna: This is pretty exciting for space

309
00:12:27.350 --> 00:12:30.070
enthusiasts. Avery. The Space Launch System

310
00:12:30.070 --> 00:12:32.550
rocket with the Orion spacecraft is now

311
00:12:32.550 --> 00:12:35.470
stacked and standing on launch pad, um, 39B.

312
00:12:35.710 --> 00:12:38.110
And anyone can watch it live whenever they

313
00:12:38.110 --> 00:12:38.430
want.

314
00:12:38.990 --> 00:12:41.230
Avery: This is the mission that will send astronauts

315
00:12:41.230 --> 00:12:43.430
around the moon, right? The first crewed

316
00:12:43.430 --> 00:12:45.150
lunar mission since Apollo 17.

317
00:12:45.950 --> 00:12:48.470
Anna: That's right. Artemis II will carry four

318
00:12:48.470 --> 00:12:51.470
astronauts, NASA astronauts Reid Wiseman,

319
00:12:51.470 --> 00:12:54.430
Victor Glover, Christina Koch and CSA

320
00:12:54.430 --> 00:12:57.150
astronaut Jeremy Hansen, on a journey around

321
00:12:57.230 --> 00:12:59.510
the moon. They won't land, but they'll

322
00:12:59.510 --> 00:13:01.749
perform a lunar flyby before returning to

323
00:13:01.749 --> 00:13:02.110
Earth.

324
00:13:02.510 --> 00:13:05.230
Avery: And having the rocket on the pad now. That

325
00:13:05.230 --> 00:13:06.750
means we're getting close to launch.

326
00:13:07.470 --> 00:13:10.030
Anna: Well, the current target is no earlier than

327
00:13:10.030 --> 00:13:12.770
April 2026. Though space missions

328
00:13:12.770 --> 00:13:15.410
often face schedule adjustments, right now

329
00:13:15.410 --> 00:13:17.490
the rocket is on the pad for integrated

330
00:13:17.490 --> 00:13:20.130
testing, making sure all the systems work

331
00:13:20.130 --> 00:13:22.250
together properly before committing to a

332
00:13:22.250 --> 00:13:22.890
launch attempt.

333
00:13:23.450 --> 00:13:25.130
Avery: What kind of testing are they doing?

334
00:13:25.530 --> 00:13:27.370
Anna: They're running through what's called a wet

335
00:13:27.370 --> 00:13:29.730
dress rehearsal, which involves loading the

336
00:13:29.730 --> 00:13:31.890
rocket with propellants and going through the

337
00:13:31.890 --> 00:13:34.450
countdown sequence, stopping just short of

338
00:13:34.450 --> 00:13:37.130
ignition. It's essentially a, ah, full launch

339
00:13:37.130 --> 00:13:39.770
simulation to verify that all systems,

340
00:13:39.850 --> 00:13:42.010
ground, equipment and procedures work as

341
00:13:42.010 --> 00:13:42.490
planned.

342
00:13:43.000 --> 00:13:45.400
Avery: And the livestream lets us watch all this

343
00:13:45.400 --> 00:13:46.760
happening in real time?

344
00:13:47.320 --> 00:13:50.320
Anna: Exactly. It's a continuous feed, so you can

345
00:13:50.320 --> 00:13:53.240
cheque in at any time, day or night, and

346
00:13:53.240 --> 00:13:55.480
see the rockets standing there on the pad.

347
00:13:55.800 --> 00:13:57.880
Sometimes you'll catch technicians working,

348
00:13:58.360 --> 00:14:00.200
other times you might see weather rolling

349
00:14:00.200 --> 00:14:02.880
through. It's a unique behind the scenes look

350
00:14:02.880 --> 00:14:05.400
at the preparation for this historic mission.

351
00:14:05.880 --> 00:14:08.760
Avery: I have to say there's something awe inspiring

352
00:14:08.760 --> 00:14:10.760
about seeing that massive rocket just

353
00:14:10.760 --> 00:14:13.470
standing there, ready to take humans beyond

354
00:14:13.470 --> 00:14:16.030
Earth orbit for the first time in over 50

355
00:14:16.110 --> 00:14:16.510
years.

356
00:14:17.150 --> 00:14:19.990
Anna: There really is, and it represents years

357
00:14:19.990 --> 00:14:22.670
of work by thousands of people. After

358
00:14:22.670 --> 00:14:25.670
Artemis 2's lunar flyby, Artemis 3 will

359
00:14:25.670 --> 00:14:28.190
attempt the first crewed lunar landing since

360
00:14:28.190 --> 00:14:30.990
1972, including landing the

361
00:14:30.990 --> 00:14:33.350
first woman and first person of colour on the

362
00:14:33.350 --> 00:14:33.710
moon.

363
00:14:34.030 --> 00:14:36.750
Avery: It's a new chapter in lunar exploration and

364
00:14:36.750 --> 00:14:39.070
we're watching it unfold in real time,

365
00:14:39.150 --> 00:14:41.640
literally. We'll put a link in the show notes

366
00:14:41.640 --> 00:14:42.720
if you'd like to cheque it out.

367
00:14:43.120 --> 00:14:45.080
Anna: And that wraps up today's episode of

368
00:14:45.080 --> 00:14:46.080
Astronomy Daily.

369
00:14:46.400 --> 00:14:48.560
From solar observatories reaching their

370
00:14:48.560 --> 00:14:51.400
cosmic outposts to remembering hard learned

371
00:14:51.400 --> 00:14:54.280
lessons from AI discoveries in telescope

372
00:14:54.280 --> 00:14:56.760
archives to potential meteor showers on

373
00:14:56.760 --> 00:14:59.520
Venus, stellar fireworks at our galactic

374
00:14:59.520 --> 00:15:02.160
centre, and moon rockets on the launch pad,

375
00:15:02.240 --> 00:15:04.320
it's been quite a journey through the cosmos

376
00:15:04.320 --> 00:15:04.640
today.

377
00:15:05.040 --> 00:15:07.690
Avery: It certainly has. If you want to stay up to

378
00:15:07.690 --> 00:15:09.810
date with all the latest space and astronomy

379
00:15:09.810 --> 00:15:11.650
news, make sure you're subscribed to

380
00:15:11.650 --> 00:15:14.010
Astronomy Daily. You can find us on your

381
00:15:14.010 --> 00:15:15.410
favourite podcast platform.

382
00:15:15.890 --> 00:15:17.810
Anna: And don't forget to visit our website at

383
00:15:17.810 --> 00:15:20.610
astronomydaily IO for additional

384
00:15:20.610 --> 00:15:22.890
content, show notes and links to all the

385
00:15:22.890 --> 00:15:24.050
storeys we covered today.

386
00:15:24.370 --> 00:15:26.370
Avery: You can also connect with us on social media

387
00:15:26.610 --> 00:15:29.090
astrodaily Pod across all major

388
00:15:29.090 --> 00:15:29.810
platforms.

389
00:15:30.130 --> 00:15:32.760
Anna: Until next time, keep looking up Clear

390
00:15:32.760 --> 00:15:33.640
skies, everyone.