Sept. 24, 2025
IMAP Launch Countdown, BION's Space Ark, and Hubble's Cosmic Oddities
- NASA and SpaceX Prepare for Major Launch: The countdown is on for the launch of NASA's Interstellar Mapping and Acceleration Probe (IMAP) from Cape Canaveral this Wednesday. Designed to study the heliosphere, IMAP aims to enhance our understanding of cosmic radiation and protect future astronauts on long-duration missions. Joining IMAP on the Falcon 9 rocket is NOAA's Space Weather Follow-on L1 satellite, crucial for monitoring solar activity, and the Carruthers Geo Corona Observatory, which will investigate Earth's extended atmosphere.
- Successful Return of Russian Biological Satellite: The BION-M M2 satellite has successfully returned to Earth, carrying a diverse array of life forms, including 75 mice and over 1500 fruit flies. This mission, dubbed a "Noah's Ark in space," provides vital insights into how organisms respond to microgravity and radiation, helping to address the risks of long-term space travel.
- NASA's Artemis Program Moves Forward: NASA is making strides with its Artemis program, aiming for the Artemis 2 mission to launch as early as February 2026. This mission will mark humanity's first return beyond low Earth orbit in over 50 years, testing the Orion crew capsule on a 10-day mission around the moon.
- Purdue University to Launch Suborbital Research Mission: In an exciting development, Purdue University will send a team to suborbital space aboard a Virgin Galactic flight in 2027. This mission, called Purdue One, will allow researchers and students to conduct hands-on experiments in microgravity, showcasing the growing accessibility of space research.
- Hubble Telescope Captures Cosmic Oddity: The Hubble Space Telescope has imaged NGC 2775, a galaxy that appears to blend characteristics of elliptical and spiral galaxies. This unique structure challenges existing models of galaxy formation, highlighting the complexity of our universe.
- New Insights from Asteroid Ryugu Samples: Research from the Hayabusa 2 mission reveals that water flowed through the parent body of asteroid Ryugu for over a billion years, suggesting that asteroids could have delivered essential ingredients for life to early Earth over an extended period.
- Dynamic History of Mars Revealed: Findings from NASA's Perseverance rover indicate that ancient rivers on Mars were more powerful than previously thought, reshaping our understanding of the planet's geological history.
- Hubble Observes White Dwarf Consuming Icy Object: The Hubble Space Telescope has observed a white dwarf star consuming a Pluto-like object, revealing a chemical signature rich in water ice. This discovery suggests that icy bodies similar to those in our solar system are common in other star systems.
- For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTubeMusic Music, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
- Thank you for tuning in. This is Anna and Avery signing off. Until next time, keep looking up and exploring the wonders of our universe.
IMAP Launch Details
[NASA](https://www.nasa.gov/)
BION-M M2 Mission Update
[Russian Space Agency](https://www.roscosmos.ru/)
Artemis Program Update
[NASA](https://www.nasa.gov/)
Purdue University Mission Announcement
[Purdue University](https://www.purdue.edu/)
Hubble Telescope Findings
[NASA](https://www.nasa.gov/)
Asteroid Ryugu Research
[JAXA](https://www.jaxa.jp/)
Mars Perseverance Rover Discoveries
[NASA](https://www.nasa.gov/)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)
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
WEBVTT
0
00:00:00.000 --> 00:00:02.960
Anna: Hello, and welcome to Astronomy Daily,
1
00:00:03.200 --> 00:00:05.840
the podcast that brings you the latest news
2
00:00:05.840 --> 00:00:08.560
from across the cosmos. I'm your host,
3
00:00:08.560 --> 00:00:09.200
Anna.
4
00:00:09.520 --> 00:00:11.640
Avery: And I'm, um, Avery. It's great to be with
5
00:00:11.640 --> 00:00:14.440
you. We have a packed show today covering
6
00:00:14.440 --> 00:00:16.880
everything from an important upcoming launch
7
00:00:17.280 --> 00:00:19.600
and the Biological Space Lab's return
8
00:00:20.160 --> 00:00:22.240
to groundbreaking new plans for lunar
9
00:00:22.240 --> 00:00:24.840
missions and astonishing discoveries from the
10
00:00:24.840 --> 00:00:25.840
Hubble Telescope.
11
00:00:26.620 --> 00:00:28.420
Anna: Let's start with the action at Cape
12
00:00:28.420 --> 00:00:31.180
canaveral. NASA and SpaceX are
13
00:00:31.180 --> 00:00:34.020
counting down to a major launch from Florida
14
00:00:34.020 --> 00:00:36.780
this Wednesday morning. The primary payload
15
00:00:36.780 --> 00:00:39.580
is the agency's Interstellar Mapping and
16
00:00:39.580 --> 00:00:42.059
Acceleration Probe, better known as
17
00:00:42.059 --> 00:00:42.860
imap.
18
00:00:43.180 --> 00:00:45.940
Avery: It's a really ambitious mission. IMAP is
19
00:00:45.940 --> 00:00:47.900
designed to journey about a million miles
20
00:00:47.900 --> 00:00:50.860
from Earth To Lagrange point 1, a
21
00:00:50.860 --> 00:00:53.380
gravitationally stable spot between us and
22
00:00:53.380 --> 00:00:56.190
the Sun. From there, it will study the
23
00:00:56.190 --> 00:00:58.390
boundary of the heliosphere, which is the
24
00:00:58.390 --> 00:01:01.190
giant magnetic bubble our sun creates around
25
00:01:01.190 --> 00:01:03.630
the solar system. It's essentially our
26
00:01:03.630 --> 00:01:06.110
protective shield against harsh galactic
27
00:01:06.110 --> 00:01:07.310
cosmic radiation.
28
00:01:07.710 --> 00:01:10.670
Anna: Understanding that boundary is crucial not
29
00:01:10.670 --> 00:01:13.390
just for pure science, but for protecting
30
00:01:13.390 --> 00:01:16.150
future astronauts on long duration missions
31
00:01:16.150 --> 00:01:18.990
to the Moon or Mars. But as you mentioned
32
00:01:18.990 --> 00:01:21.830
earlier, IMAP isn't flying solo on
33
00:01:21.830 --> 00:01:23.230
its Falcon 9 rocket launchers.
34
00:01:23.700 --> 00:01:26.100
Avery: Exactly. This is a ride share
35
00:01:26.180 --> 00:01:28.180
mission. Joining IMAP is
36
00:01:28.180 --> 00:01:30.980
NOAA's Space Weather Follow on
37
00:01:31.300 --> 00:01:34.300
SFWO L1 satellite. This
38
00:01:34.300 --> 00:01:36.700
will be a critical tool for monitoring solar,
39
00:01:36.700 --> 00:01:39.419
wind and coronal mass ejections, which can
40
00:01:39.419 --> 00:01:41.460
disrupt our power grids and communications
41
00:01:41.460 --> 00:01:43.820
satellites here on Earth. There's also a
42
00:01:43.820 --> 00:01:46.620
third payload, the Carruthers Geo Corona
43
00:01:46.620 --> 00:01:49.260
Observatory, which will study Earth extended
44
00:01:49.260 --> 00:01:51.500
Atmosphere. Liftoff is scheduled for
45
00:01:51.500 --> 00:01:54.060
Wednesday at 7:30am Eastern Time.
46
00:01:54.220 --> 00:01:57.060
That's 11:30 UTC. So it's an early
47
00:01:57.060 --> 00:01:58.860
start for a triple header of important
48
00:01:58.940 --> 00:02:00.580
science from a.
49
00:02:00.580 --> 00:02:03.380
Anna: Mission just beginning to one that has just
50
00:02:03.380 --> 00:02:06.219
concluded. A Russian biological research
51
00:02:06.300 --> 00:02:08.780
satellite, BION m M number two,
52
00:02:09.100 --> 00:02:11.540
successfully touched down on September
53
00:02:11.540 --> 00:02:14.540
19th in the steppes of the Orenburg region.
54
00:02:14.940 --> 00:02:17.180
After spending a full month in Earth.
55
00:02:17.180 --> 00:02:19.590
Avery: Orbit, this mission has been nicknamed a
56
00:02:19.590 --> 00:02:22.230
Noah's Ark in space. And when you look at the
57
00:02:22.230 --> 00:02:25.070
passenger list, you can see why. The descent
58
00:02:25.070 --> 00:02:27.630
module carried an incredible variety of life.
59
00:02:28.110 --> 00:02:30.910
75 mice, over 1500
60
00:02:30.910 --> 00:02:33.310
fruit flies, as well as various cell
61
00:02:33.310 --> 00:02:36.110
cultures, microorganisms, and, um, even
62
00:02:36.110 --> 00:02:36.990
plant seeds.
63
00:02:37.230 --> 00:02:39.870
Anna: It's a continuation of a long series
64
00:02:39.950 --> 00:02:42.590
of studies into how living organisms
65
00:02:42.670 --> 00:02:45.400
respond to the space environment. The
66
00:02:45.400 --> 00:02:47.680
primary challenges, of course, are
67
00:02:47.680 --> 00:02:50.160
microgravity and increased radiation
68
00:02:50.160 --> 00:02:53.080
exposure. Scientists will be looking closely
69
00:02:53.080 --> 00:02:55.360
at the specimens to see the effects on
70
00:02:55.440 --> 00:02:58.280
everything from bone density and muscle mass
71
00:02:58.280 --> 00:03:01.079
in the mice to genetic changes in the flies
72
00:03:01.079 --> 00:03:03.960
and microorganisms. The data gathered
73
00:03:03.960 --> 00:03:06.280
is vital. It helps us understand the
74
00:03:06.280 --> 00:03:08.920
fundamental risks of long term space travel
75
00:03:08.920 --> 00:03:11.360
for humans and develop countermeasures.
76
00:03:11.830 --> 00:03:13.990
It's a floating laboratory that provides
77
00:03:13.990 --> 00:03:16.630
insights we simply can't get on the ground.
78
00:03:17.350 --> 00:03:20.110
Speaking of human spaceflight, NASA is
79
00:03:20.110 --> 00:03:22.310
forging ahead with its Artemis program.
80
00:03:22.790 --> 00:03:25.710
Agency officials provided an exciting update
81
00:03:25.710 --> 00:03:28.630
this week saying that the Artemis 2 mission
82
00:03:28.870 --> 00:03:31.550
could take flight as early as February of
83
00:03:31.550 --> 00:03:34.230
2026. This marks the very
84
00:03:34.230 --> 00:03:36.750
first time humans will venture beyond low
85
00:03:36.750 --> 00:03:39.190
Earth orbit in more than 50 years.
86
00:03:39.900 --> 00:03:42.580
Avery: It's a hugely significant step. This will be
87
00:03:42.580 --> 00:03:44.740
the very first crewed flight for both the
88
00:03:44.740 --> 00:03:47.540
powerful Space Launch System rocket and the
89
00:03:47.540 --> 00:03:50.220
Orion crew capsule. The four person
90
00:03:50.220 --> 00:03:52.940
crew, NASA astronauts Reid Wiseman,
91
00:03:52.940 --> 00:03:55.820
Victor Glover and Christina Koch, along
92
00:03:55.820 --> 00:03:58.340
with Canadian Space Agency astronaut Jeremy
93
00:03:58.340 --> 00:04:00.980
Hansen, won't be landing on the moon just
94
00:04:00.980 --> 00:04:03.940
yet. Instead, they will fly a challenging
95
00:04:03.940 --> 00:04:06.300
10 day mission on a free return
96
00:04:06.380 --> 00:04:08.860
trajectory that will loop them around the far
97
00:04:08.860 --> 00:04:09.900
side of the moon.
98
00:04:10.550 --> 00:04:13.390
Anna: The goal is to test all of Orion's life
99
00:04:13.390 --> 00:04:15.830
support systems, navigation and
100
00:04:15.910 --> 00:04:18.470
communication capabilities in deep space.
101
00:04:19.190 --> 00:04:21.870
It's essentially the final dress rehearsal
102
00:04:21.870 --> 00:04:24.630
for the Artemis 3 mission that aims to
103
00:04:24.630 --> 00:04:27.110
land astronauts including the first woman
104
00:04:27.430 --> 00:04:30.270
on the lunar surface. It's truly the
105
00:04:30.270 --> 00:04:33.070
spiritual successor to the Apollo 8 mission
106
00:04:33.070 --> 00:04:35.310
that first orbited the moon in
107
00:04:35.310 --> 00:04:38.180
1968. Pushing the launch to
108
00:04:38.180 --> 00:04:41.140
early 2026 gives teams the
109
00:04:41.140 --> 00:04:43.020
time they need to address technical
110
00:04:43.020 --> 00:04:45.860
challenges like those with the capsule's heat
111
00:04:45.860 --> 00:04:48.620
shield. Ensuring the crew's safety is the
112
00:04:48.620 --> 00:04:49.540
top priority.
113
00:04:50.260 --> 00:04:53.179
Avery: Absolutely. It's a methodical, step by
114
00:04:53.179 --> 00:04:55.580
step approach to a very complex
115
00:04:55.580 --> 00:04:58.020
endeavor. But the excitement is
116
00:04:58.020 --> 00:05:00.740
palpable. Seeing that crew launch on a
117
00:05:00.740 --> 00:05:03.180
path around the moon will be a historic
118
00:05:03.180 --> 00:05:05.860
moment for a new generation. And it's not
119
00:05:05.860 --> 00:05:07.940
just government agencies planning ambitious
120
00:05:07.940 --> 00:05:10.340
flights. We're seeing more and more
121
00:05:10.340 --> 00:05:12.700
academic institutions getting directly
122
00:05:12.700 --> 00:05:15.500
involved. Purdue University just announced
123
00:05:15.500 --> 00:05:18.380
it will send a team of researchers, students
124
00:05:18.380 --> 00:05:21.020
and alumni to suborbital
125
00:05:21.020 --> 00:05:23.660
space aboard a Virgin galactic flight in
126
00:05:23.660 --> 00:05:24.540
2027.
127
00:05:25.340 --> 00:05:28.220
Anna: This is fantastic news. The mission,
128
00:05:28.220 --> 00:05:31.100
called Purdue One, really highlights the
129
00:05:31.100 --> 00:05:33.890
democratization of space access. The
130
00:05:33.890 --> 00:05:35.970
flight will carry five passengers from the
131
00:05:35.970 --> 00:05:38.850
university community. Two have already been
132
00:05:38.850 --> 00:05:41.730
named. Steven Collicot, a professor of
133
00:05:41.730 --> 00:05:44.730
aerospace engineering, and Abigail Mizzy,
134
00:05:44.810 --> 00:05:46.010
a UH graduate student.
135
00:05:46.570 --> 00:05:49.450
Avery: It's an incredible opportunity. For a
136
00:05:49.450 --> 00:05:51.050
few minutes, they'll experience a
137
00:05:51.050 --> 00:05:53.810
microgravity environment, allowing them to
138
00:05:53.810 --> 00:05:56.650
conduct hands on research that was once the
139
00:05:56.650 --> 00:05:59.530
exclusive domain of NASA astronauts.
140
00:06:00.070 --> 00:06:02.470
The experiments could cover a range of fields
141
00:06:02.550 --> 00:06:05.110
like fluid dynamics in zero G,
142
00:06:05.510 --> 00:06:08.310
material science, or even biomedical
143
00:06:08.310 --> 00:06:08.710
studies.
144
00:06:09.270 --> 00:06:11.750
Anna: And beyond the specific research, the
145
00:06:11.750 --> 00:06:14.070
inspirational value is immense.
146
00:06:14.550 --> 00:06:17.030
Having students and professors become
147
00:06:17.030 --> 00:06:19.910
astronauts sends a powerful message.
148
00:06:20.310 --> 00:06:22.830
It Makes a career in space feel more
149
00:06:22.830 --> 00:06:25.750
attainable and will surely ignite the passion
150
00:06:25.750 --> 00:06:28.390
of countless future engineers and scientists.
151
00:06:29.280 --> 00:06:32.040
Let's zoom out now. Way beyond our solar
152
00:06:32.040 --> 00:06:34.840
system, the Hubble Space Telescope has
153
00:06:34.840 --> 00:06:37.360
once again captured an image of something
154
00:06:37.360 --> 00:06:39.760
both beautiful and baffling.
155
00:06:40.240 --> 00:06:42.530
Its latest picture of the week features a,
156
00:06:42.530 --> 00:06:44.560
uh, galaxy named NGC
157
00:06:45.200 --> 00:06:47.920
2775, located
158
00:06:47.920 --> 00:06:50.560
about 67 million light years away
159
00:06:50.720 --> 00:06:53.640
in the constellation Cancer that simply
160
00:06:53.640 --> 00:06:55.440
refuses to be put in a box.
161
00:06:56.150 --> 00:06:59.030
Avery: It's a genuine cosmic oddity. When
162
00:06:59.030 --> 00:07:01.190
you look at its center, you see a large,
163
00:07:01.510 --> 00:07:04.230
smooth central bulge with almost
164
00:07:04.230 --> 00:07:06.470
no gas or ongoing star formation.
165
00:07:07.030 --> 00:07:09.630
In that respect, it looks very much like an
166
00:07:09.630 --> 00:07:12.630
old, settled elliptical galaxy. But
167
00:07:12.630 --> 00:07:15.150
then your eyes move outward and you see this
168
00:07:15.150 --> 00:07:17.830
magnificent, intricate ring of gas and
169
00:07:17.830 --> 00:07:18.230
dust.
170
00:07:18.790 --> 00:07:21.670
Anna: And that ring is filled with chaotic,
171
00:07:21.750 --> 00:07:24.710
unevenly distributed clusters of bright,
172
00:07:24.790 --> 00:07:27.620
young blue stars. This structure
173
00:07:27.620 --> 00:07:29.540
is more typical of what's called a, uh,
174
00:07:29.540 --> 00:07:32.380
flocculant spiral galaxy, One where
175
00:07:32.380 --> 00:07:35.020
the spiral arms are patchy and not well
176
00:07:35.020 --> 00:07:37.660
defined. It's like two different types of
177
00:07:37.660 --> 00:07:39.340
galaxies were stitched together.
178
00:07:40.060 --> 00:07:42.060
Avery: Astronomers are still trying to understand
179
00:07:42.140 --> 00:07:44.660
the evolutionary path that leads to such a
180
00:07:44.660 --> 00:07:47.620
hybrid structure. It challenges our models of
181
00:07:47.620 --> 00:07:50.420
galaxy formation and shows that nature
182
00:07:50.420 --> 00:07:52.700
is always more creative than we imagine.
183
00:07:53.260 --> 00:07:55.420
It's a stunning reminder of the vast,
184
00:07:55.660 --> 00:07:58.660
complex, and often strange universe we live
185
00:07:58.660 --> 00:08:01.500
in. Now let's bring our focus
186
00:08:01.660 --> 00:08:03.900
back to our own cosmic backyard.
187
00:08:04.460 --> 00:08:07.380
Incredible new research on samples returned
188
00:08:07.380 --> 00:08:09.580
from the asteroid Ryugu Is
189
00:08:09.580 --> 00:08:11.980
overturning some long held beliefs.
190
00:08:12.380 --> 00:08:15.380
The analysis from Chaksa's Hayabusa 2
191
00:08:15.380 --> 00:08:18.180
mission reveals that water flowed through
192
00:08:18.180 --> 00:08:20.980
the asteroid's parent body for much
193
00:08:20.980 --> 00:08:22.780
longer than ever thought possible.
194
00:08:23.770 --> 00:08:26.690
Anna: This is a really big deal. For a long time,
195
00:08:26.690 --> 00:08:29.650
the consensus was that water activity on
196
00:08:29.650 --> 00:08:32.410
asteroids, the interaction of water with
197
00:08:32.410 --> 00:08:35.090
rock, was something that only happened in the
198
00:08:35.090 --> 00:08:37.690
very earliest moments of the solar system's
199
00:08:37.690 --> 00:08:40.570
formation, maybe within the first few million
200
00:08:40.570 --> 00:08:42.170
years M. But.
201
00:08:42.170 --> 00:08:44.490
Avery: This new data shows evidence of water
202
00:08:44.490 --> 00:08:46.970
circulation more than 1 billion
203
00:08:47.130 --> 00:08:49.850
years after the asteroid itself formed.
204
00:08:50.510 --> 00:08:52.430
This suggests that the interior of these
205
00:08:52.430 --> 00:08:55.190
ancient bodies could have remained warm
206
00:08:55.190 --> 00:08:57.950
and wet for an extended geological
207
00:08:57.950 --> 00:08:58.670
timescale.
208
00:08:58.750 --> 00:09:01.670
Anna: The implications for our own planet are
209
00:09:01.670 --> 00:09:03.830
profound. Ryugu is a
210
00:09:03.830 --> 00:09:06.390
carbonaceous asteroid, A, uh, type
211
00:09:06.390 --> 00:09:09.150
believed to be rich in water and organic
212
00:09:09.150 --> 00:09:11.870
compounds. If these asteroids were
213
00:09:11.870 --> 00:09:14.670
capable of holding liquid water for so
214
00:09:14.670 --> 00:09:17.110
long, it means they could have delivered
215
00:09:17.110 --> 00:09:19.750
these essential ingredients for life to the
216
00:09:19.750 --> 00:09:22.650
early Earth over a much longer period,
217
00:09:23.050 --> 00:09:26.050
and perhaps in greater quantities than our
218
00:09:26.050 --> 00:09:27.850
previous models suggested.
219
00:09:28.170 --> 00:09:30.410
Avery: And while we're exploring our own solar
220
00:09:30.410 --> 00:09:32.650
system, let's turn to the Red Planet for a
221
00:09:32.650 --> 00:09:35.450
moment. New findings from NASA's Perseverance
222
00:09:35.450 --> 00:09:38.049
rover are uh, painting a much more dynamic
223
00:09:38.049 --> 00:09:40.850
picture of Mars ancient past. It
224
00:09:40.850 --> 00:09:42.970
appears a river that once flowed into the
225
00:09:42.970 --> 00:09:45.930
Jezero crater was far more powerful and
226
00:09:45.930 --> 00:09:47.890
fast moving than scientists previously
227
00:09:47.890 --> 00:09:50.830
imagined. A torrent of water carving through
228
00:09:50.830 --> 00:09:53.550
the landscape. The discoveries just keep on
229
00:09:53.550 --> 00:09:53.910
coming.
230
00:09:54.390 --> 00:09:57.270
Anna: For our final story today, we have another
231
00:09:57.350 --> 00:09:59.990
remarkable finding from the Hubble Space
232
00:10:00.070 --> 00:10:02.630
Telescope. It has observed a
233
00:10:02.630 --> 00:10:05.510
burned out star, what's known as a
234
00:10:05.510 --> 00:10:08.390
white dwarf, in the act of consuming
235
00:10:08.390 --> 00:10:10.790
the fragments of a Pluto like object.
236
00:10:11.270 --> 00:10:13.670
This cosmic drama is unfolding
237
00:10:13.670 --> 00:10:15.910
relatively close to us, just
238
00:10:15.910 --> 00:10:17.830
260 light years away.
239
00:10:18.370 --> 00:10:21.170
Avery: A white dwarf is the incredibly dense remnant
240
00:10:21.170 --> 00:10:23.810
core of a star like our sun, after it has
241
00:10:23.810 --> 00:10:26.810
exhausted its nuclear fuel. The gravity of
242
00:10:26.810 --> 00:10:29.250
this one is so intense that it's tearing
243
00:10:29.250 --> 00:10:31.930
apart this small icy body that strayed too
244
00:10:31.930 --> 00:10:34.290
close. And we're effectively seeing the
245
00:10:34.290 --> 00:10:36.730
star's atmosphere become polluted with the
246
00:10:36.730 --> 00:10:39.370
remains of this object, allowing us to study
247
00:10:39.370 --> 00:10:42.130
its composition. As a material falls into the
248
00:10:42.130 --> 00:10:45.050
star, its chemical signature is revealed in
249
00:10:45.050 --> 00:10:45.970
the star's light.
250
00:10:46.340 --> 00:10:49.180
Anna: And the composition is what makes this so
251
00:10:49.180 --> 00:10:51.980
exciting. The fragments are loaded with
252
00:10:51.980 --> 00:10:54.820
volatiles, elements that vaporize at low
253
00:10:54.820 --> 00:10:57.380
temperatures like nitrogen, carbon,
254
00:10:57.540 --> 00:11:00.300
sulfur and oxygen. This chemical
255
00:11:00.300 --> 00:11:02.820
signature strongly indicates the presence.
256
00:11:02.820 --> 00:11:05.780
Avery: Of a lot of ice, an incredible amount
257
00:11:05.780 --> 00:11:08.180
in fact. The Hubble data suggests this
258
00:11:08.180 --> 00:11:10.660
exopluto object is composed of
259
00:11:10.660 --> 00:11:12.980
64% water ice.
260
00:11:13.570 --> 00:11:15.770
It's a powerful confirmation that the kind of
261
00:11:15.770 --> 00:11:18.450
water rich icy worlds we see in the outer
262
00:11:18.450 --> 00:11:20.810
reaches of our own solar system, like Pluto
263
00:11:20.810 --> 00:11:23.570
and other Kuiper Belt objects, are likely
264
00:11:23.650 --> 00:11:26.490
common in other star systems too. It tells us
265
00:11:26.490 --> 00:11:28.570
that the fundamental building blocks for life
266
00:11:28.570 --> 00:11:30.970
as we know it are widespread throughout the
267
00:11:30.970 --> 00:11:31.490
galaxy.
268
00:11:32.050 --> 00:11:33.610
Anna: That's all the time we have for.
269
00:11:33.610 --> 00:11:36.210
Avery: This episode and join us next time for more
270
00:11:36.210 --> 00:11:37.650
news from across the universe.
271
00:11:37.970 --> 00:11:40.730
Anna: I'm Anna, and on behalf of Avery and
272
00:11:40.730 --> 00:11:43.450
myself, thank you for listening and we'll see
273
00:11:43.450 --> 00:11:45.910
you tomorrow with more space and astronomy
274
00:11:45.910 --> 00:11:48.430
news. In the meantime, keep looking up.
0
00:00:00.000 --> 00:00:02.960
Anna: Hello, and welcome to Astronomy Daily,
1
00:00:03.200 --> 00:00:05.840
the podcast that brings you the latest news
2
00:00:05.840 --> 00:00:08.560
from across the cosmos. I'm your host,
3
00:00:08.560 --> 00:00:09.200
Anna.
4
00:00:09.520 --> 00:00:11.640
Avery: And I'm, um, Avery. It's great to be with
5
00:00:11.640 --> 00:00:14.440
you. We have a packed show today covering
6
00:00:14.440 --> 00:00:16.880
everything from an important upcoming launch
7
00:00:17.280 --> 00:00:19.600
and the Biological Space Lab's return
8
00:00:20.160 --> 00:00:22.240
to groundbreaking new plans for lunar
9
00:00:22.240 --> 00:00:24.840
missions and astonishing discoveries from the
10
00:00:24.840 --> 00:00:25.840
Hubble Telescope.
11
00:00:26.620 --> 00:00:28.420
Anna: Let's start with the action at Cape
12
00:00:28.420 --> 00:00:31.180
canaveral. NASA and SpaceX are
13
00:00:31.180 --> 00:00:34.020
counting down to a major launch from Florida
14
00:00:34.020 --> 00:00:36.780
this Wednesday morning. The primary payload
15
00:00:36.780 --> 00:00:39.580
is the agency's Interstellar Mapping and
16
00:00:39.580 --> 00:00:42.059
Acceleration Probe, better known as
17
00:00:42.059 --> 00:00:42.860
imap.
18
00:00:43.180 --> 00:00:45.940
Avery: It's a really ambitious mission. IMAP is
19
00:00:45.940 --> 00:00:47.900
designed to journey about a million miles
20
00:00:47.900 --> 00:00:50.860
from Earth To Lagrange point 1, a
21
00:00:50.860 --> 00:00:53.380
gravitationally stable spot between us and
22
00:00:53.380 --> 00:00:56.190
the Sun. From there, it will study the
23
00:00:56.190 --> 00:00:58.390
boundary of the heliosphere, which is the
24
00:00:58.390 --> 00:01:01.190
giant magnetic bubble our sun creates around
25
00:01:01.190 --> 00:01:03.630
the solar system. It's essentially our
26
00:01:03.630 --> 00:01:06.110
protective shield against harsh galactic
27
00:01:06.110 --> 00:01:07.310
cosmic radiation.
28
00:01:07.710 --> 00:01:10.670
Anna: Understanding that boundary is crucial not
29
00:01:10.670 --> 00:01:13.390
just for pure science, but for protecting
30
00:01:13.390 --> 00:01:16.150
future astronauts on long duration missions
31
00:01:16.150 --> 00:01:18.990
to the Moon or Mars. But as you mentioned
32
00:01:18.990 --> 00:01:21.830
earlier, IMAP isn't flying solo on
33
00:01:21.830 --> 00:01:23.230
its Falcon 9 rocket launchers.
34
00:01:23.700 --> 00:01:26.100
Avery: Exactly. This is a ride share
35
00:01:26.180 --> 00:01:28.180
mission. Joining IMAP is
36
00:01:28.180 --> 00:01:30.980
NOAA's Space Weather Follow on
37
00:01:31.300 --> 00:01:34.300
SFWO L1 satellite. This
38
00:01:34.300 --> 00:01:36.700
will be a critical tool for monitoring solar,
39
00:01:36.700 --> 00:01:39.419
wind and coronal mass ejections, which can
40
00:01:39.419 --> 00:01:41.460
disrupt our power grids and communications
41
00:01:41.460 --> 00:01:43.820
satellites here on Earth. There's also a
42
00:01:43.820 --> 00:01:46.620
third payload, the Carruthers Geo Corona
43
00:01:46.620 --> 00:01:49.260
Observatory, which will study Earth extended
44
00:01:49.260 --> 00:01:51.500
Atmosphere. Liftoff is scheduled for
45
00:01:51.500 --> 00:01:54.060
Wednesday at 7:30am Eastern Time.
46
00:01:54.220 --> 00:01:57.060
That's 11:30 UTC. So it's an early
47
00:01:57.060 --> 00:01:58.860
start for a triple header of important
48
00:01:58.940 --> 00:02:00.580
science from a.
49
00:02:00.580 --> 00:02:03.380
Anna: Mission just beginning to one that has just
50
00:02:03.380 --> 00:02:06.219
concluded. A Russian biological research
51
00:02:06.300 --> 00:02:08.780
satellite, BION m M number two,
52
00:02:09.100 --> 00:02:11.540
successfully touched down on September
53
00:02:11.540 --> 00:02:14.540
19th in the steppes of the Orenburg region.
54
00:02:14.940 --> 00:02:17.180
After spending a full month in Earth.
55
00:02:17.180 --> 00:02:19.590
Avery: Orbit, this mission has been nicknamed a
56
00:02:19.590 --> 00:02:22.230
Noah's Ark in space. And when you look at the
57
00:02:22.230 --> 00:02:25.070
passenger list, you can see why. The descent
58
00:02:25.070 --> 00:02:27.630
module carried an incredible variety of life.
59
00:02:28.110 --> 00:02:30.910
75 mice, over 1500
60
00:02:30.910 --> 00:02:33.310
fruit flies, as well as various cell
61
00:02:33.310 --> 00:02:36.110
cultures, microorganisms, and, um, even
62
00:02:36.110 --> 00:02:36.990
plant seeds.
63
00:02:37.230 --> 00:02:39.870
Anna: It's a continuation of a long series
64
00:02:39.950 --> 00:02:42.590
of studies into how living organisms
65
00:02:42.670 --> 00:02:45.400
respond to the space environment. The
66
00:02:45.400 --> 00:02:47.680
primary challenges, of course, are
67
00:02:47.680 --> 00:02:50.160
microgravity and increased radiation
68
00:02:50.160 --> 00:02:53.080
exposure. Scientists will be looking closely
69
00:02:53.080 --> 00:02:55.360
at the specimens to see the effects on
70
00:02:55.440 --> 00:02:58.280
everything from bone density and muscle mass
71
00:02:58.280 --> 00:03:01.079
in the mice to genetic changes in the flies
72
00:03:01.079 --> 00:03:03.960
and microorganisms. The data gathered
73
00:03:03.960 --> 00:03:06.280
is vital. It helps us understand the
74
00:03:06.280 --> 00:03:08.920
fundamental risks of long term space travel
75
00:03:08.920 --> 00:03:11.360
for humans and develop countermeasures.
76
00:03:11.830 --> 00:03:13.990
It's a floating laboratory that provides
77
00:03:13.990 --> 00:03:16.630
insights we simply can't get on the ground.
78
00:03:17.350 --> 00:03:20.110
Speaking of human spaceflight, NASA is
79
00:03:20.110 --> 00:03:22.310
forging ahead with its Artemis program.
80
00:03:22.790 --> 00:03:25.710
Agency officials provided an exciting update
81
00:03:25.710 --> 00:03:28.630
this week saying that the Artemis 2 mission
82
00:03:28.870 --> 00:03:31.550
could take flight as early as February of
83
00:03:31.550 --> 00:03:34.230
2026. This marks the very
84
00:03:34.230 --> 00:03:36.750
first time humans will venture beyond low
85
00:03:36.750 --> 00:03:39.190
Earth orbit in more than 50 years.
86
00:03:39.900 --> 00:03:42.580
Avery: It's a hugely significant step. This will be
87
00:03:42.580 --> 00:03:44.740
the very first crewed flight for both the
88
00:03:44.740 --> 00:03:47.540
powerful Space Launch System rocket and the
89
00:03:47.540 --> 00:03:50.220
Orion crew capsule. The four person
90
00:03:50.220 --> 00:03:52.940
crew, NASA astronauts Reid Wiseman,
91
00:03:52.940 --> 00:03:55.820
Victor Glover and Christina Koch, along
92
00:03:55.820 --> 00:03:58.340
with Canadian Space Agency astronaut Jeremy
93
00:03:58.340 --> 00:04:00.980
Hansen, won't be landing on the moon just
94
00:04:00.980 --> 00:04:03.940
yet. Instead, they will fly a challenging
95
00:04:03.940 --> 00:04:06.300
10 day mission on a free return
96
00:04:06.380 --> 00:04:08.860
trajectory that will loop them around the far
97
00:04:08.860 --> 00:04:09.900
side of the moon.
98
00:04:10.550 --> 00:04:13.390
Anna: The goal is to test all of Orion's life
99
00:04:13.390 --> 00:04:15.830
support systems, navigation and
100
00:04:15.910 --> 00:04:18.470
communication capabilities in deep space.
101
00:04:19.190 --> 00:04:21.870
It's essentially the final dress rehearsal
102
00:04:21.870 --> 00:04:24.630
for the Artemis 3 mission that aims to
103
00:04:24.630 --> 00:04:27.110
land astronauts including the first woman
104
00:04:27.430 --> 00:04:30.270
on the lunar surface. It's truly the
105
00:04:30.270 --> 00:04:33.070
spiritual successor to the Apollo 8 mission
106
00:04:33.070 --> 00:04:35.310
that first orbited the moon in
107
00:04:35.310 --> 00:04:38.180
1968. Pushing the launch to
108
00:04:38.180 --> 00:04:41.140
early 2026 gives teams the
109
00:04:41.140 --> 00:04:43.020
time they need to address technical
110
00:04:43.020 --> 00:04:45.860
challenges like those with the capsule's heat
111
00:04:45.860 --> 00:04:48.620
shield. Ensuring the crew's safety is the
112
00:04:48.620 --> 00:04:49.540
top priority.
113
00:04:50.260 --> 00:04:53.179
Avery: Absolutely. It's a methodical, step by
114
00:04:53.179 --> 00:04:55.580
step approach to a very complex
115
00:04:55.580 --> 00:04:58.020
endeavor. But the excitement is
116
00:04:58.020 --> 00:05:00.740
palpable. Seeing that crew launch on a
117
00:05:00.740 --> 00:05:03.180
path around the moon will be a historic
118
00:05:03.180 --> 00:05:05.860
moment for a new generation. And it's not
119
00:05:05.860 --> 00:05:07.940
just government agencies planning ambitious
120
00:05:07.940 --> 00:05:10.340
flights. We're seeing more and more
121
00:05:10.340 --> 00:05:12.700
academic institutions getting directly
122
00:05:12.700 --> 00:05:15.500
involved. Purdue University just announced
123
00:05:15.500 --> 00:05:18.380
it will send a team of researchers, students
124
00:05:18.380 --> 00:05:21.020
and alumni to suborbital
125
00:05:21.020 --> 00:05:23.660
space aboard a Virgin galactic flight in
126
00:05:23.660 --> 00:05:24.540
2027.
127
00:05:25.340 --> 00:05:28.220
Anna: This is fantastic news. The mission,
128
00:05:28.220 --> 00:05:31.100
called Purdue One, really highlights the
129
00:05:31.100 --> 00:05:33.890
democratization of space access. The
130
00:05:33.890 --> 00:05:35.970
flight will carry five passengers from the
131
00:05:35.970 --> 00:05:38.850
university community. Two have already been
132
00:05:38.850 --> 00:05:41.730
named. Steven Collicot, a professor of
133
00:05:41.730 --> 00:05:44.730
aerospace engineering, and Abigail Mizzy,
134
00:05:44.810 --> 00:05:46.010
a UH graduate student.
135
00:05:46.570 --> 00:05:49.450
Avery: It's an incredible opportunity. For a
136
00:05:49.450 --> 00:05:51.050
few minutes, they'll experience a
137
00:05:51.050 --> 00:05:53.810
microgravity environment, allowing them to
138
00:05:53.810 --> 00:05:56.650
conduct hands on research that was once the
139
00:05:56.650 --> 00:05:59.530
exclusive domain of NASA astronauts.
140
00:06:00.070 --> 00:06:02.470
The experiments could cover a range of fields
141
00:06:02.550 --> 00:06:05.110
like fluid dynamics in zero G,
142
00:06:05.510 --> 00:06:08.310
material science, or even biomedical
143
00:06:08.310 --> 00:06:08.710
studies.
144
00:06:09.270 --> 00:06:11.750
Anna: And beyond the specific research, the
145
00:06:11.750 --> 00:06:14.070
inspirational value is immense.
146
00:06:14.550 --> 00:06:17.030
Having students and professors become
147
00:06:17.030 --> 00:06:19.910
astronauts sends a powerful message.
148
00:06:20.310 --> 00:06:22.830
It Makes a career in space feel more
149
00:06:22.830 --> 00:06:25.750
attainable and will surely ignite the passion
150
00:06:25.750 --> 00:06:28.390
of countless future engineers and scientists.
151
00:06:29.280 --> 00:06:32.040
Let's zoom out now. Way beyond our solar
152
00:06:32.040 --> 00:06:34.840
system, the Hubble Space Telescope has
153
00:06:34.840 --> 00:06:37.360
once again captured an image of something
154
00:06:37.360 --> 00:06:39.760
both beautiful and baffling.
155
00:06:40.240 --> 00:06:42.530
Its latest picture of the week features a,
156
00:06:42.530 --> 00:06:44.560
uh, galaxy named NGC
157
00:06:45.200 --> 00:06:47.920
2775, located
158
00:06:47.920 --> 00:06:50.560
about 67 million light years away
159
00:06:50.720 --> 00:06:53.640
in the constellation Cancer that simply
160
00:06:53.640 --> 00:06:55.440
refuses to be put in a box.
161
00:06:56.150 --> 00:06:59.030
Avery: It's a genuine cosmic oddity. When
162
00:06:59.030 --> 00:07:01.190
you look at its center, you see a large,
163
00:07:01.510 --> 00:07:04.230
smooth central bulge with almost
164
00:07:04.230 --> 00:07:06.470
no gas or ongoing star formation.
165
00:07:07.030 --> 00:07:09.630
In that respect, it looks very much like an
166
00:07:09.630 --> 00:07:12.630
old, settled elliptical galaxy. But
167
00:07:12.630 --> 00:07:15.150
then your eyes move outward and you see this
168
00:07:15.150 --> 00:07:17.830
magnificent, intricate ring of gas and
169
00:07:17.830 --> 00:07:18.230
dust.
170
00:07:18.790 --> 00:07:21.670
Anna: And that ring is filled with chaotic,
171
00:07:21.750 --> 00:07:24.710
unevenly distributed clusters of bright,
172
00:07:24.790 --> 00:07:27.620
young blue stars. This structure
173
00:07:27.620 --> 00:07:29.540
is more typical of what's called a, uh,
174
00:07:29.540 --> 00:07:32.380
flocculant spiral galaxy, One where
175
00:07:32.380 --> 00:07:35.020
the spiral arms are patchy and not well
176
00:07:35.020 --> 00:07:37.660
defined. It's like two different types of
177
00:07:37.660 --> 00:07:39.340
galaxies were stitched together.
178
00:07:40.060 --> 00:07:42.060
Avery: Astronomers are still trying to understand
179
00:07:42.140 --> 00:07:44.660
the evolutionary path that leads to such a
180
00:07:44.660 --> 00:07:47.620
hybrid structure. It challenges our models of
181
00:07:47.620 --> 00:07:50.420
galaxy formation and shows that nature
182
00:07:50.420 --> 00:07:52.700
is always more creative than we imagine.
183
00:07:53.260 --> 00:07:55.420
It's a stunning reminder of the vast,
184
00:07:55.660 --> 00:07:58.660
complex, and often strange universe we live
185
00:07:58.660 --> 00:08:01.500
in. Now let's bring our focus
186
00:08:01.660 --> 00:08:03.900
back to our own cosmic backyard.
187
00:08:04.460 --> 00:08:07.380
Incredible new research on samples returned
188
00:08:07.380 --> 00:08:09.580
from the asteroid Ryugu Is
189
00:08:09.580 --> 00:08:11.980
overturning some long held beliefs.
190
00:08:12.380 --> 00:08:15.380
The analysis from Chaksa's Hayabusa 2
191
00:08:15.380 --> 00:08:18.180
mission reveals that water flowed through
192
00:08:18.180 --> 00:08:20.980
the asteroid's parent body for much
193
00:08:20.980 --> 00:08:22.780
longer than ever thought possible.
194
00:08:23.770 --> 00:08:26.690
Anna: This is a really big deal. For a long time,
195
00:08:26.690 --> 00:08:29.650
the consensus was that water activity on
196
00:08:29.650 --> 00:08:32.410
asteroids, the interaction of water with
197
00:08:32.410 --> 00:08:35.090
rock, was something that only happened in the
198
00:08:35.090 --> 00:08:37.690
very earliest moments of the solar system's
199
00:08:37.690 --> 00:08:40.570
formation, maybe within the first few million
200
00:08:40.570 --> 00:08:42.170
years M. But.
201
00:08:42.170 --> 00:08:44.490
Avery: This new data shows evidence of water
202
00:08:44.490 --> 00:08:46.970
circulation more than 1 billion
203
00:08:47.130 --> 00:08:49.850
years after the asteroid itself formed.
204
00:08:50.510 --> 00:08:52.430
This suggests that the interior of these
205
00:08:52.430 --> 00:08:55.190
ancient bodies could have remained warm
206
00:08:55.190 --> 00:08:57.950
and wet for an extended geological
207
00:08:57.950 --> 00:08:58.670
timescale.
208
00:08:58.750 --> 00:09:01.670
Anna: The implications for our own planet are
209
00:09:01.670 --> 00:09:03.830
profound. Ryugu is a
210
00:09:03.830 --> 00:09:06.390
carbonaceous asteroid, A, uh, type
211
00:09:06.390 --> 00:09:09.150
believed to be rich in water and organic
212
00:09:09.150 --> 00:09:11.870
compounds. If these asteroids were
213
00:09:11.870 --> 00:09:14.670
capable of holding liquid water for so
214
00:09:14.670 --> 00:09:17.110
long, it means they could have delivered
215
00:09:17.110 --> 00:09:19.750
these essential ingredients for life to the
216
00:09:19.750 --> 00:09:22.650
early Earth over a much longer period,
217
00:09:23.050 --> 00:09:26.050
and perhaps in greater quantities than our
218
00:09:26.050 --> 00:09:27.850
previous models suggested.
219
00:09:28.170 --> 00:09:30.410
Avery: And while we're exploring our own solar
220
00:09:30.410 --> 00:09:32.650
system, let's turn to the Red Planet for a
221
00:09:32.650 --> 00:09:35.450
moment. New findings from NASA's Perseverance
222
00:09:35.450 --> 00:09:38.049
rover are uh, painting a much more dynamic
223
00:09:38.049 --> 00:09:40.850
picture of Mars ancient past. It
224
00:09:40.850 --> 00:09:42.970
appears a river that once flowed into the
225
00:09:42.970 --> 00:09:45.930
Jezero crater was far more powerful and
226
00:09:45.930 --> 00:09:47.890
fast moving than scientists previously
227
00:09:47.890 --> 00:09:50.830
imagined. A torrent of water carving through
228
00:09:50.830 --> 00:09:53.550
the landscape. The discoveries just keep on
229
00:09:53.550 --> 00:09:53.910
coming.
230
00:09:54.390 --> 00:09:57.270
Anna: For our final story today, we have another
231
00:09:57.350 --> 00:09:59.990
remarkable finding from the Hubble Space
232
00:10:00.070 --> 00:10:02.630
Telescope. It has observed a
233
00:10:02.630 --> 00:10:05.510
burned out star, what's known as a
234
00:10:05.510 --> 00:10:08.390
white dwarf, in the act of consuming
235
00:10:08.390 --> 00:10:10.790
the fragments of a Pluto like object.
236
00:10:11.270 --> 00:10:13.670
This cosmic drama is unfolding
237
00:10:13.670 --> 00:10:15.910
relatively close to us, just
238
00:10:15.910 --> 00:10:17.830
260 light years away.
239
00:10:18.370 --> 00:10:21.170
Avery: A white dwarf is the incredibly dense remnant
240
00:10:21.170 --> 00:10:23.810
core of a star like our sun, after it has
241
00:10:23.810 --> 00:10:26.810
exhausted its nuclear fuel. The gravity of
242
00:10:26.810 --> 00:10:29.250
this one is so intense that it's tearing
243
00:10:29.250 --> 00:10:31.930
apart this small icy body that strayed too
244
00:10:31.930 --> 00:10:34.290
close. And we're effectively seeing the
245
00:10:34.290 --> 00:10:36.730
star's atmosphere become polluted with the
246
00:10:36.730 --> 00:10:39.370
remains of this object, allowing us to study
247
00:10:39.370 --> 00:10:42.130
its composition. As a material falls into the
248
00:10:42.130 --> 00:10:45.050
star, its chemical signature is revealed in
249
00:10:45.050 --> 00:10:45.970
the star's light.
250
00:10:46.340 --> 00:10:49.180
Anna: And the composition is what makes this so
251
00:10:49.180 --> 00:10:51.980
exciting. The fragments are loaded with
252
00:10:51.980 --> 00:10:54.820
volatiles, elements that vaporize at low
253
00:10:54.820 --> 00:10:57.380
temperatures like nitrogen, carbon,
254
00:10:57.540 --> 00:11:00.300
sulfur and oxygen. This chemical
255
00:11:00.300 --> 00:11:02.820
signature strongly indicates the presence.
256
00:11:02.820 --> 00:11:05.780
Avery: Of a lot of ice, an incredible amount
257
00:11:05.780 --> 00:11:08.180
in fact. The Hubble data suggests this
258
00:11:08.180 --> 00:11:10.660
exopluto object is composed of
259
00:11:10.660 --> 00:11:12.980
64% water ice.
260
00:11:13.570 --> 00:11:15.770
It's a powerful confirmation that the kind of
261
00:11:15.770 --> 00:11:18.450
water rich icy worlds we see in the outer
262
00:11:18.450 --> 00:11:20.810
reaches of our own solar system, like Pluto
263
00:11:20.810 --> 00:11:23.570
and other Kuiper Belt objects, are likely
264
00:11:23.650 --> 00:11:26.490
common in other star systems too. It tells us
265
00:11:26.490 --> 00:11:28.570
that the fundamental building blocks for life
266
00:11:28.570 --> 00:11:30.970
as we know it are widespread throughout the
267
00:11:30.970 --> 00:11:31.490
galaxy.
268
00:11:32.050 --> 00:11:33.610
Anna: That's all the time we have for.
269
00:11:33.610 --> 00:11:36.210
Avery: This episode and join us next time for more
270
00:11:36.210 --> 00:11:37.650
news from across the universe.
271
00:11:37.970 --> 00:11:40.730
Anna: I'm Anna, and on behalf of Avery and
272
00:11:40.730 --> 00:11:43.450
myself, thank you for listening and we'll see
273
00:11:43.450 --> 00:11:45.910
you tomorrow with more space and astronomy
274
00:11:45.910 --> 00:11:48.430
news. In the meantime, keep looking up.