Decelerating Cosmos and Solar Secrets: Unravelling Dark Energy and the Sun's Magnetic Dance

(00:00:00) Decelerating Cosmos and Solar Secrets: Unravelling Dark Energy and the Sun's Magnetic Dance
(00:00:45) More confirmation that the Universe's expansion is slowing
(00:08:53) First glimpse of the Sun’s polar magnetic field in motion
(00:14:09) Space Weather events ramping up
(00:18:24) The Science Report
(00:20:29) Alex on Tech NEO the humanoid housekeeper

In this episode of SpaceTime, we explore significant revelations about the universe's expansion, the Sun's magnetic field, and the current surge in solar weather activity.
The Universe's Expansion Rate is Slowing
A new study has confirmed that the universe's rate of expansion, which began after the Big Bang 13.8 billion years ago, is slowing down. This finding contradicts previous theories suggesting that the expansion was accelerating due to dark energy. We delve into the implications of this research, which indicates that dark energy may be evolving more rapidly than previously understood, potentially marking a paradigm shift in cosmology. The episode discusses various scenarios for the universe's future, including the Big Crunch, Steady State theory, Big Freeze, and Big Rip, and how these new observations could reshape our understanding of cosmic fate.
First Glimpse of the Sun's Polar Magnetic Field
Astronomers have captured their first detailed view of the Sun's polar magnetic field in motion, revealing unexpected rapid movements. The Solar Orbiter spacecraft has provided insights into the Sun's magnetic activity, which follows an 11-year cycle. This segment highlights the significance of the findings, which enhance our understanding of solar dynamics and the implications for space weather.
Current Surge in Space Weather Events
As the Sun reaches solar maximum, astronomers are observing increased solar storm activity, including multiple X-class and M-class solar flares. This segment discusses the effects of coronal mass ejections on Earth, including spectacular auroras and potential disruptions to technology and power grids. We explore the science behind solar flares and their impact on our planet, providing a comprehensive overview of current space weather conditions.
www.spacetimewithstuartgary.com
✍️ Episode References
Monthly Notices of the Royal Astronomical Society
Astrophysical Journal Letters
Nature Geoscience
Journal of the American Medical Association
Become a supporter of this podcast: https://www.spreaker.com/podcast/spacetime-your-guide-to-space-astronomy--2458531/support.

Episode Transcript

Speaker 1 (00:00):
This is Spacetime Series twenty eight, Episode one hundred and
thirty three, for broadcast on the taunt of November twenty
twenty five. Coming up on space Time, more confirmation that
the universe's rate of expansion is slowing, our first glimpse
of the Sun's polymagnetic field in motion. And while we're
on the subject of our local star space weather events

(00:21):
ramping up this week. All that and more coming up
on Spacetime.

Speaker 2 (00:27):
Welcome to space Time with Stuart Gary.

Speaker 1 (00:46):
A new study has confirmed earlier observations that the universe's
rate of expansion out from the Big Bang thirteen point
eight billion years ago is slowing down. The findings, reported
in the Monthly Notices the Royal Astronomical Society are at
odds with earlier studies which showed that the cosmos wasn't
just expanding, but that its rate of expansion was accelerating

(01:07):
due to a mysterious force known as dark energy. Instead,
these new observations are supporting other more recent studies, which
is showing no evidence of an accelerating universe. After the
Big Bang and the rapid expansion of the universe some
thirteen point eight billion years ago, gravity slowed it down,
But in nineteen ninety eight it was established that nine

(01:28):
billion years after the universe began, expansion started to speed
up again, driven by a mysterious force Astronomers dubbed this
dark energy, But despite making up more than seventy percent
of the universe's total mass energy budget, it's still considered
to be one of the greatest mysteries in science. Understanding
the universe's rate of expansion is important for understanding our

(01:50):
ultimate fate right now. There are four likely scenarios. The
Big Crunch sees the universe's rate of expansion slow down
and eventually stop before gravity takes over and the universe
starts to contract again, eventually collapsing down into a great crunch.
Then there's the steady state theory, in which the universe's
rate of expansion eventually slows down to a crawl for

(02:12):
finally stopping altogether, leaving us with pretty much the sort
of universe we have today. Until of these new studies,
the most popular hypothesis was called the Big Freeze, in
which the universe's rate of expansion would continue until eventually
all the galaxies would move so far away from each
other only those in our local group would be visible,
leaving the universe a very dark, empty place. An expansion

(02:36):
of that hypothesis was called the Big Rip, in which
not only would dark energy cause the universe to continue
to expand forever, but its rate of expansion would continue
to accelerate. Eventually, not only would all the galaxies be
beyond the cosmic horizon, but star systems themselves would move
away from each other. Even more disturbing, dark energy could

(02:56):
become so strong that planets could move away from their star.
A matter itself would start to expand away, ripping atoms
away from each other, and even ultimately warks being ripped apart.
That's the Big Rip. But these new observations and similar
recent ones are showing no evidence of an accelerating universe. Now.

(03:16):
If the results are confirmed, it could open up an
entirely new chapter in science's quest to uncover the true
nature of dark energy, resolve the Hubble tension, and provide
a better understanding of both the past and future of
our universe. The studies lead author, Yong Wook Lee from
Yonce University in South Korea, says the new research shows

(03:37):
the universe has already ended a phase of deccelerated expansion
in the present epoch, and that dark energy is evolving
with time much more rapidly than previously thought. If these
results are confirmed, it would mark a major paradigm shift
in cosmology. Since the discovery of dark energy twenty seven
years ago. For the past three decades, astronomers have widely

(03:59):
believe that the U universe is expanding at an ever
increasing rate, driven by this unseen phenomenon known as dark energy,
which acts as a kind of anti gravity. That conclusion
was based on distance measurements to far away galaxies using
a type of stellar explosion called a type one A supernova.
These thermonuclear explosions marking the death of sunlike stars involves

(04:22):
stars of similar size exploding with similar levels of luminosity.
It allows astronomers to use them as standard candles, applying
the inverse square low to determine their true distance based
on their apparent brightness. It's like looking at a set
of street lights down a road and judging how far
away each light is by how bright it appears to be. However,

(04:44):
the new evidence suggests that type one A supernervae are
actually strongly affected by the age of their progenitor stars,
even after luminosity standardization, supernervae from young stellar populations appears
systematically fainter, all those from older populations appear brighter now.
Based on a much larger host galaxy sample of three

(05:06):
hundred galaxies, the new study confirmed this effect at an
extremely high significance of ninety nine point nine nine nine
percent confidence that suggests that the dinning of distant supernovae
arises not only from cosmological effects but also from stellar
astrophysical effects. And when the systematic bias was corrected, the

(05:26):
supernova data no longer matched the standard lambda cold dark
matter cosmological model. Instead, it aligns far better with a
new model, one favored by the Dark Energy Spectroscopic Instrument
or DESI project, that's derived from baryonic acoustic oscillations, which
are pressure waves generated by the Big Bang, and from
cosmic microwave background radiation data. The left over heat from

(05:49):
the Big Bang created three hundred and eighty thousand years
after the Big Bang, when the quak gluon plasma of
the early cosmos koled enough for the first atoms to form.
Now at just two point seven degrees above absolute zero,
this cosmic microwave background radiation can be easily detected as
the white noise or static between stations on old analog

(06:10):
radios and TVs. The corrected supernova data and the baryonic
acoustic ostellations and cosmic microwave background radiation data both indicate
that dark energy weakens and evolves significantly with time. More importantly,
when the corrected supernova data is combined with the baryonic
acoustic ostellations and cosmic microwave background radiation results, the standard

(06:33):
lambda cold dark matter cosmological model is ruled out with
the overwhelming significance. Most surprising of all, however, this combined
analysis indicates that the universe is not accelerating today it's
previously thought, but has already transitioned. These says. The key
results from the DESI project were obtained by combining uncorrected

(06:54):
supernova data with baryonic acoustic oscillation measurements, leading to the
conclusion that while the universe will accelerate in the future,
it was still accelerating at present. But by contrast, this
new analysis, which applies the age bias correction, shows that
the universe has already entered a decelerating phase today. Remarkably,

(07:15):
this agrees with what's already independently predicted from baryonic acoustic
ostellations alone or baryonic acoustic ostellations plus cosmic microwave background
radiation analysis. The further confirm the results. The authors are
now carrying out an evolution free test. They'll use only
supernervate from young host galaxies across the full redshift range,

(07:37):
and their first results from this study are already supporting
their previous main conclusion. Li says within the next five years,
with the Veriic Ruben Observatory discovering more than twenty thousand
new supernova host galaxies, precise age measurements will allow for
a far more robust and definitive test of supernova cosmology.
The Veric Ruben Observatory in the Chin and is home

(08:01):
to what is the world's largest and most powerful digital camera.
It began scientific operations this year and could answer vital
questions not just about our solar system, but about the
wider universe as a whole. The hope is that with
these new tools in their arsenal, astronomers will now be
better equipped than ever to find clues about exactly what
dark enage is and exactly how it influences the universe.

(08:25):
This is space time still to come first glimpse of
the Sun's polar magnetic field in motion and hang on
space weather events are ramping up. All that and more
still to come on space time. Astronomers have had their

(08:55):
first ever glimpse of the Sun's south pole magnetic field
in motion, and analysis of the data from the European
Space agency Solar Orbitior spacecraft has revealed a major surprise.
It seems the magnetic field is carried towards the pole
much faster than the astronomers it expected. Our Sun is
governed by a strict rhythm. The magnetic activity of the

(09:17):
Sun displays a cyclic variation, reaching a maximum approximately every
eleven years, to enormous plasma circulations when in each of
the Sun's hemispheres set the pace for this rhythm, thus
defining the Sun's eleven year solar cycle. Near the surface,
these plasma flows carry the magnetic field lines of the
Sun from the equator to the poles, and in the

(09:40):
solar interior, the plasma flows back to the equator in
a huge cycle spanning the entire hemisphere. But important details
of this solar magnetic field conveyor built system are still
poorly understood, and the exact process is taking place at
the Sun's poles are likely to be crucial. From Earth,
astronomers only have a great zing view of this region,

(10:01):
making it impossible to determine the properties of the magnetic field.
And the problem is most space probes have a similar
limited perspective and that's where Solar ORBITA comes in. It
can now provide the missing piece of this puzzle. Since
February twenty twenty, Solar Orbiter has been traveling in elongated
ellipses around the Sun, and in March to his sheer,

(10:23):
it began the process of tilting its orbit away from
the ecliptic, the plane around the Sun upon which the
planets orbit. From its trajectory tilted by seventeen degrees, Solar
ORBITA now for the first time has a better view
of the Sun's poles. The new findings, reported in the
Astrophysical Journal Letters, provides information about the direction of plasma

(10:43):
flows and the magnetic field on the solar surface. The
data reveals a refined picture of the supergranulation and magnetic
network of the Sun at the south pole for the
first time. Super Granules are cells of hot plasma each
about two to three times the size of the Earth,
which densely cover the surface of the Sun. Their horizontal

(11:03):
surface flows wash magnetic field lines to their edges, creating
the Sun's magnetic network a web of strong magnetic fields.
But to the surprise of the authors, the magnetic fields
were seen to drift towards the poles that approximately ten
to twenty metues per second on average. It's almost as
fast as their counterparts at lower latitudes. Previous studies based

(11:24):
on the ecliptic plane observations have seen slower drift a
magnetic field in the high polar latitudes. The emotion offers
important new clues about the Sun's global plasma and magnetic
field circulation. It's still unclear whether the Sun's global magnetic
conveyor built really doesn't slow down near the poles, but
the new data is providing a brief snapshot of the

(11:46):
entire solar cycle. This report from ACTV.

Speaker 2 (11:55):
What if we could look at the Sun from a
whole new angle I've never seen before. For the first time,
Solar ORBITA has captured close up images of the Sun's
mysterious poles, regions long hidden from view until now. Every
image of the Sun you've ever seen was taken around

(12:18):
its equator. That's because Earth, the other planets, and most
spacecraft travel in a flat orbit around the Sun, but
Solar Orbiter is different. In twenty twenty five, it tilted
its path out of this plane, giving us a first
ever look at the Sun's south pole. Remarkably, it found

(12:41):
both the north and south magnetic fields tangled together. This
is a sign that the Sun is at the peak
of its eleven year activity cycle when its magnetic poles flip.
With its powerful instruments, Solar Orbitter captures what's happening in
the Sun's outer layers, from its surface, through the layers

(13:02):
in between, all the way to the outer atmosphere. This
is keid understanding solar wind and solar storms, which can.

Speaker 3 (13:11):
Disrupt satellites, power grids, and radio signals here on Earth.
As Solar Orbiter climbs to even higher orbits over the
next years, its view will become even clearer, bringing us
more views we've never seen before.

Speaker 1 (13:32):
This is space time still to space weather events ramping up,
with Earth being hit by a series of modible X
and M class solar flares, and later in the Science
Report and You study warns that kids who spend a
lot of time on screens are less likely to do
well in primary or elementary school tests. All that and
more still to come on space time. Astronomers are recording

(14:10):
increased levels of solar storm activity right now, with multiple
X class and strong M class solar flares erupting from
the Sun. At least three coronal mass ejections have either
grazed or directly hit the Earth in recent days, sparking
strong geomagnetic storms resulting in spectacular auroral lights, and more
are expected. The Sun is now at what we call

(14:33):
solar maximum, that's the climax of its eleven year solar cycle.
It's a time of heightened solar activity, with increased solar
flare and coronal mass ejection activity as the number of
sunspots increases. Sun spots are cooler regions of the Sun's
surface where magnetic field lines from deep below the photosphee
burst out into space. The Sun is a huge ball

(14:55):
of plasma and different latitudes revolve at different rates, and
this causes magnetic field lines to twist and snap, and
these ruptures can trigger soil of flares, flinging vast amounts
of energy deep into space. And they can also trigger
more powerful chronal mass ejections, which say not just energy,
but also huge plumes of charged particles the magnetic field

(15:18):
into space. Now, if these explosions are pointed towards the Earth,
they generate geomagnetic storms, triggering spectacular auroral events like the
Aurora Australis, the Southern lights, and the Aurora Borealis the
Northern lights, which we're experiencing now. The problem is they
also damage or destroy spacecraft, increase radiation exposure for people

(15:39):
in space and in high altitude aircraft, disrupt communications and
navigation systems, and even black out terrestrial power grids. Syracuse
University physicist Sam sampri Is these events can leave major legacies.

Speaker 4 (15:53):
Within the last let's just say year, we've been getting
alerts on the news. Hey go outside tonight and look
up and a few of clear skies you might see
the aurora. And the reason that's happening now is because
right now we're in a period of the solar cycle
solar max where we get solar flares happening kind of frequently.

(16:16):
So when we have a solar flare, that's when a
region on the surface of the Sun explodes one way
this thing can explode is just by emitting a lot
of electromagnetic radiation in the form of X rays and
gamma rays and very extreme ultraviolet light. You know, for
the most part, that doesn't really bother us. But something

(16:38):
that can accompany a solar flare is a coronal mass ejection,
and that's when a stream of particles is also going
to explode out the surface of the Sun. So it's
a big plasma ball with a complex magnetic field. Smallest
ones we don't even notice them, but the most powerful
ones can knock out radio canmmunications on Earth. They can

(17:02):
mess with our satellites in orbit, they can destroy the
photovoltaic cells on satellites in orbit. And what protects us
from most of these solar flares is the Earth's magnetic
field and the atmosphere, and they kind of get caught
up in the magnetic field, so they never really do
reach the Earth. But those particles spiraling around, that's what

(17:23):
causes the aurora. And when it's a strong storm, there
are more of those particles and the aurora can spread
to more southern latitudes and we can see those pretty
colors in the sky. Most interesting thing to me I
think is just the vast magnitude of our Sun. We

(17:45):
think of this massive solar eruption and it spews out
so many thousands, ten billions, millions of kilograms of material,
and that's like a drop in the bucket compared to
the size of the Sun's That's just fascinating to me.

Speaker 1 (18:03):
That Syracuse University physicist Sam sam Prey and this space
time and time that to take another brief look at

(18:26):
some of the other stories making news and science this
week with a science report, A new study has shown
that Hectoria glacier on the Antarctic Peninsula retreated by at
least eight kilome it is in just two months between
November and December twenty twenty two. The findings, reported in
the journal Nature Geoscience, show the glacier's rate of retreat
was nearly ten times faster than previously measured for a

(18:49):
grounded glacier. The authors studied both satellite and neighborne images
taken off the glacier between February twenty twenty two and
August twenty twenty three, during which time it retreated using
twenty five kilometers. The scientists say a glacier destabilization process
may have caused this rapid retreat, and understanding the process
is important to evaluate the potential for similar events and

(19:12):
their impact on sea level rise. A new study has
found that kids who spend a lot of time on
screens are less likely to do well in tests at
primary or elementary school level. The findings, reported in the
Journal of the American Medical Association, are based on a
Canadian study of more than five thousand children. The authors
found that with each extra hour of screen time per

(19:34):
day as reported by parents, the children had about a
ten percent lower chance of high marks in standardized tests
for maths and reading. A new study has found that
large language models such as CHAT, GPT and deep seek
can still struggle to pick up when someone's expressing a
factually untrue belief. A report in the General Nature Machine

(19:56):
Intelligence as the twenty four of the most advanced large
language models on thirteen thousand questions to evaluate how well
they could distinguish beliefs from knowledge and fact from fiction
when responding to a false first person belief phrased as
I believe that. The authors found that all models systematically
failed to correct for the false belief. The authors say

(20:17):
this weakness of large language models needs to be considered
when using them, especially in high stakes areas such as
law or medicine, or in mental health care, where picking
up and challenging a patient's false beliefs can be crucial.

Speaker 4 (20:30):
Well.

Speaker 1 (20:30):
A better history has been made this week with the
world's first consumer ready humanoid robot designed to do domestic
chores being released for sale. The one ex Home Robotics
new neo can at your command, become a personal housekeeper
that will complete household tasks. The humanoids powered by a
large language model, artificial intelligence that learns and remembers what

(20:51):
the user's preferences are when it comes to cleaning the
house or washing clothes, and it can make informed suggestions
such as what to cook for dinner. However, if it
can complete it, sure the company can take control tetch
it what to do. Of course, that raises all sorts
of potential security and safety questions. I mean, could you
teach the human to kill someone you don't like? With

(21:14):
the details, we're joined by technology editor alexhov Royt from
tech Advice Start Life.

Speaker 5 (21:19):
It's a home robot that can do chores like answer
the door, do vacuuming by actually holding a vacuum clean
not like Rosie the Robot, where the vacum cleaner popped
out from a number. Rosie and the Jetson George Jetson
was born in twenty twenty two, on July thirty first,
so in the show, which was in twenty sixty two,
he's forty years old. And the show was premiered in

(21:42):
nineteen sixty two, so it was definitely set one hundred
years in the future. And of course we had flying cars,
and we had zoom calls, and we had robots and
a few things that haven't quite come true yet. But
Neo now that twenty thousand dollars US to buy. You
can put a two hundred dollars US down payment, and
if you don't want to spend twenty K, you can
lease it for four hundred and ninety Union dollars a
month on a subscription. And it is designed to be autonomous,

(22:04):
so it will load your dishwasher, it will put the
clothes in the washing machine and put them into the dryer.
It can water your plants outside, it can answer the door,
help you carry your groceries inside. I mean, it's a
home robot of the sort that Science Section has been
promising us for decades. The robot looks futuristic. I mean
at the same time it looks a little bit creepy.
One thing that people have been concerned about is that

(22:27):
if the robot doesn't know how to do a task,
one of the things you can do is you can
look at your phone and see what the robot is
seeing through its side, so you can spa on the
robot as it works. But that also means that somebody
else can be at your invitation, unless I guess someone
hacks into the robot. They can log into the robot
with a VA headset and that can control its arms
and legs and help it to do things. And the
purpose of helping it to do things is to teach it,

(22:49):
because if it gets stuck on something it doesn't know
how to do something in particular, then you might need
help from the company, and the company can log in
and control the robot for you. It is the first
robot that's actually on sale that isn't a vacuum cleaner,
that can act like a human and do human level things.
So the future that we've been promised has finally arrived,
and no doubt the Chinese and others will be copying

(23:11):
this and by twenty thirty you should be able to
go into a Walmart, Best Buy, a Harvey Norman, a JB.
High Fight, you know, your your traditional electronics stores, and
it won't just be robot vacuum cleaners you'll be buying,
but actual humanoid robots.

Speaker 1 (23:23):
Julian and Grant has forgotten about the social media angle
on computer games.

Speaker 4 (23:28):
It seems it's.

Speaker 5 (23:29):
Always been known that yes, you can contact other people
and talk to them through games. It seems that the
Eseftic Commissioner is sort of turning more into a regulator.
This was always going to be a moving target because
the Internet has evolved. The eath Aftic Commissioner's digital idea
and other laws are yet to come into play. That's
going to be in mid December twenty twenty five. No

(23:49):
doubt there will be a huge spike in VPN usage
as we've seen in the UK when similar laws were
put into place there, and people will find a way
around it. But then also you know companies will be
wanting to block anybody using a VPN. You try using
a VPN with certain services already like Netflix or Amazon
or others, and that they were just right to know
you saying we know you're connected to a VPN because

(24:10):
we recognize the ports that you're coming from, and you
know that a lot of people come from those books.
We know their VPN ports, and so we'll just block you.
So what's going to happen to people's ideas that they
can log into services using VPN if that's going to
be the case. So it's the all cat and mouse game.
It's just one of those things where the dead hand
of government, as at were now, often they do something
and it has the opposite effect. Hold on to your horses,

(24:30):
pulling your seat belt. It's going to be a rough right,
It's probably not going to be a smooth journey through cyberspace.

Speaker 1 (24:35):
That's alexeharov Royd from Take Advice, Start Life, and that's
the show for now. Space Time is available every Monday,

(24:58):
Wednesday and Friday through dot com, SoundCloud, YouTube, your favorite
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(25:21):
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Speaker 2 (25:40):
You've been listening to space Time with Stuart Gary.

Speaker 4 (25:43):
This has been another quality podcast production from bytes dot com.