May 24, 2023

Saturn's 62 new moons // Wild Martian river // Finding black holes

Saturn's 62 new moons // Wild Martian river // Finding black holes

In this episode of SpaceTime with Stuart Gary, you'll learn about the amazing discovery of 62 new moons around Saturn, the evidence of a wild river on ancient Mars, and the new technique to find black holes in the sky. You'll also get the latest...

In this episode of SpaceTime with Stuart Gary, you'll learn about the amazing discovery of 62 new moons around Saturn, the evidence of a wild river on ancient Mars, and the new technique to find black holes in the sky. You'll also get the latest science news, including the link between bone fractures and mortality, the genetic modification of bananas to prevent extinction, and the impressive achievement of Chat GPT-4 AI in radiology. Tune in to SpaceTime for an informative and entertaining podcast about astronomy and space science.
#astronomy #space #sceience #news #spacetime #podcast

The Astronomy, Space, Technology & Science News Podcast.

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This is Spacetime Series twenty six,
episode sixty two, for broadcast on the

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twenty fourth of May twenty twenty three. Coming up on Spacetime, Saturn get

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sixty two new moons, discovery of
a wild Martian river on the Red planet,

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and astronomers develop a better way of
finding black holes or that are more.

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Coming up on Spacetime Welcome to Spacetime
with Stewart Garry, Astronomers have discovered

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another sixty two moons orbiting the ringed
ward of Saturn. The work catapots the

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Attorney System back into first place as
the planet with the most number of known

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moons now totaling one hundred and forty
five. That compares to Jupiter, which

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is ninety five known moons. Over
the past two decades, Satin surroundings have

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been repeatedly examined for tiny moons with
increasing sensitivity. The latest study used a

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technique known as shift in stack in
order to find fainter and the small at

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Saturnian moons. The same method has
been used before to search for moons around

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Neptune and Uranus, but never before
for Satin. It works by shifting a

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set of sequential images at the rate
at which the Moon's moving across the sky.

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The results enhanced the Moon's signal when
all the datas combined and stacked together,

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allowing moons that were simply too faint
to be seen in individual images to

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become visible in the stacked image.
The images were taken using the Canada France

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Hawaii Telescope, a type of mona
k in Hawaii, between twenty nineteen and

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twenty twenty one. By shifting and
stacking many sequential images taken during three hour

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spans a stripe, them as were
able to detect moons around Satin down to

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just two and a half kilometers in
diameter, not bad when they're quite literally

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billions of kilometers away. The original
discoveries were made in twenty nineteen, uncovering

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the moons in a meticulous search of
the deep imaging acquired that year. But

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just finally, an object close to
Satin the sky doesn't necessarily mean it's the

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Moon. It could simply be a
passing asteroid. To be absolutely sure,

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the objects need to be tracked for
several years in order to be certain that

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they are really orbiting the planet.
After painstakingly matching objects detected on different nights

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over two years, the authors managed
to track down sixty three objects, thus

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confirming them as new moons. Now. One of these new moons, designated

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S twenty nineteen S one, was
announced back in twenty twenty one, with

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the rest being announced over the last
couple of weeks. Now, all of

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these new moons belong to a class
known as irregular moons. These are thoughts

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will initially been being captured by Saturn
from their original host planet long ago.

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Compared to regular moons, irregular moons
are characterized by their large, elliptical and

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inclined orbits. The number of known
Saturnian irregular moons has now doubled to one

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hundred and twenty one, with fifty
eight previously known before the search began.

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Now, irregular moons tend to clump
together in orbital groups based on the tilt

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of their orbits. In the Saturnian
system, there are three such groups,

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whose names are drawn from different mythologies. There's the Inuit group, the Gaelic

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group, and the much more populated
Norse group, and all the new moons

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fall into one of these three known
categories, with the Norse group again being

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the most populated among the new moons. These three groups are thought to be

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the result of collisions where the current
moons in the group are remnants of one

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or more earlier collisions involving the originally
captured moons. The authors have suggested that

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the large number of smaller moons in
retrograde orbit is the result of a relatively

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recent list in astronomical terms, but
really sometime over the last one hundred million

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years or so, fairly recent disruption
of a moderately sized irregular moon that's now

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been broken down into many fragments that
are all cataloged in the Norse group this

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space time still to come, discovery
of a wild Martian river on the Red

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planet, and astronomers just got a
better way of finding black holes. All

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that are more still to come on
spacetime. New evidence discovered in rocks is

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leading scientists to rethink what water environments
look like on ancient Mars. The new

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images taken by nassa's Mars Perseverance Rover
show sig answer what was once a wild

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river raging across the Martian landscape,
a river that was deeper and faster moving

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than scientists had ever seen evidence for
on the Red planet in the past.

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This river was part of a network
of waterways that flowed into jesuro Crater,

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the area the six wild car sized
rob has been exploring since landing on the

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Red planet more than two years ago. Understanding these water environments could help scientists

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in the rivers to seek outsides of
ancient microbi or life that may have been

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preserved in the Martian rock. Perseverance
is exploring the top layer of a fan

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shaped pile of sedimentary rock that stands
about two hundred and fifty meters tall and

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features curving layers suggestive of flowing water. It's a geologically fossilized ancient river delta.

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One question sitist need an answer to
is whether the water in this river

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flowed in relatively shallow streams closer to
White NASA's Curiosity rover has found evidence for

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gell Crater or whether this was a
more powerful river system. Stitched together from

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hundreds of images captured by Perseverance's mass
Caamze instrument, the tunumusics created by NASA

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tend to suggest the latter, revealing
coarse river sediment grains and cobbles libby ives

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from NASA's Jeopropulsion Laboratory. In passing
into California, says these indicate a high

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energy river that's moving swiftly and transporting
lots of sediment and debris downstream. The

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more powerful the flow of the water, the more easily it can move large

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pieces of material. Ives, who
has a background in stating Earth rivers,

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has spent the last six months analyzing
images of Martian rivers on the red planet's

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surface. Years ago. Site has
noticed a series of curving bands of layered

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rock within just Row Crater, which
they dubbed the curvy linear Unit. They

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could clearly see these layers from space, but they're only now able to see

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them up close thanks to persevere One
location within the curvy linear unit, nicknamed

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Shrinkle Haven, is likely to have
been formed by powerfully flowing water, but

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Maskemseas detailed images have left scientists debating
exactly what kind of flow we're talking about.

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Are we talking about a big river
like the Mississippi, which winds and

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snakes its way across the landscape,
or are we talking about braided rivers like

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Nebraska's Plate, which forms small islands
of sedimentary sandbars. When viewed from the

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ground, the curved layers appear arranged
in rows that ripple out across the landscape.

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They therefore could be the remnants of
river banks that shifted over time,

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or the remnants of sandbars that formed
in the river. These layers will very

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much taller in the past. Sinus
suspect that after these piles of sediment turned

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to rock, there were sandblasted by
wind over the eons and eventually carved down

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to their present size, the wind
acting like a scalpel cutting the tops of

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these deposits. Now, scientists do
see deposits like this on Earth, but

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they've never been as well exposed as
what they are on Mars because here are

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on Earth, they're of course covered
with vegetation and that hides the layers.

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Second mersey captured by Perseverance shows a
second location that's also part of the Curvey

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Illinear unit, and he's located about
four hundred and fifty meters from Shrinkle Haven.

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Called Pine Stand. It's an isolated
hill bearing sedimentary layers that curves skyward,

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some as high as twenty meters.
Sidists think these tall layers may also

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being formed by powerful river flows,
although they're exploring other explanations as well.

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I have says these layers are enormously
tall for rivers on Earth, but at

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the same time, the most common
way to create these land forms would be

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a river. The STATIS authors are
continuing to examine mass camas these images for

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additional clues. They're also peering below
the surface using the ground penetrating radar instrument

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on Persevere called rim FACTS, which
is short for Radar Imager for Mars subsurface

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experiments. What they learned from both
instruments will contribute to an ever expanding body

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of knowledge about Mars's ancient watery past. What's exciting here is that we've entered

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a new phase of Gesro's history,
and it's the first time we're seeing environments

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like this on Mars. Of course, a key objective of Perseverance's mission on

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Mars is astrobiology, including the search
for science of ancient microbial life. Scientists

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believe that if evidence of past life
is likely to be found on Mars,

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places like this ancient river delta is
where scientists should be looking. As it

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traverses the fan, Perseverance will characterize
the geology and past climate of Mars,

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having the way for human exploration on
the Red planet. And of course it's

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also the first mission to collect install
Mars samples for eventual return to Worth.

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Subsequent NASA missions, in cooperation with
the European Space Agency, will send SPACECRAFTOMAS

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to collect these sealed samples and then
return them to Earth for in depth analysis

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this space time still to come.
Astronomers just got a better way of finding

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black holes. All that are more
still to come on space time. One

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of the big problems about black holes
is not knowing where they are. After

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all, they're black, and so
is the rest of space around them.

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That makes them really hard to see. It's a bit like sitting next to

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an invisible bomb, which only appears
when it's too late to stop it or

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move away. But that's the thing
about black holes. Their gravity is so

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strong nothing not even like can escape, and so they only make their presents

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clear when they start feeding. Then
material begins falling into the black hole,

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and this material releases vast amounts of
energy as it's ripped apart of the subatomic

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level, before disappearing beyond the monsters
of that horizon, a sort of point

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of no return beyond which escape is
impossible. The quite invisible black holes will

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remain a problem, but astronomers have
now developed a new way of detecting the

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active ones those that are feeding,
and the new method they've come up with

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not only points them out, but
can also measure how much food they're sacking

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in Most, if not all,
galaxies are thought to contain supermassive black holes

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at their centers, but not all
supermassive black holes are feeding. Sagittarius a

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star is the supermassive black hole at
the center of our own galaxy, the

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Milky Way. It's around four point
three million times the mass of our Sun,

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and it's located at twenty seven thousand
light years away, and importantly,

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it appears to be quiet, at
least at the moment. Still, massive

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cone shaped gamma ray clouds known as
fermi bubbles stretch out tens of thousands of

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light years above and below the center
of the galaxies, disc clear evidence of

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past meals consumed by Sagittaries A star. The new technique which the astronomers have

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come up with can determine if super
massive black holes are feeding in distant galaxies,

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and it can be applied to literally
into galaxies across the sky. Until

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now, identifying feeding black holes has
been challenging, with astronomers having to specifically

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look for them individually, using complex
methods unique to individual types of telescopes radio

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optical, X ray and gamma ray. Instead, this new technique works on

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typical telescope observations that already exist for
millions of galaxies. One of the studies

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authors, Sabine Blasted from the University
of Western Australian Nerd of the International Center

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of Radio strongly your research, says
the new tea eglows scientists to search large

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numbers of galaxies at once and learn
about their central black holes. I am

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doctor Sabina Belstead. I am a
research associate here at AKRA. Black holes

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are just one aspect of a galaxy, and they're embedded in the middle.

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And when you look at a galaxy, it's bright, but you don't necessarily

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obviously see the black hole because it
is black. We've been looking at pictures

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of galaxies in many different wavelengths of
light and using that then to have some

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really fancy code that we can model
this light and pick where a black hole

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is. So the type of black
hole that we're interested in in our work

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is a supermassive black hole in the
middle of a galaxy. It's a very

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enormous kind of black hole, and
in particular, one of the reasons why

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we're interested in understanding more about them
is because they really change the way a

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galaxy looks to us. We're interested
in galaxy is because we want to understand

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how they have evolved and changed with
time. If we don't know enough about

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the supermassive black hole inside them,
then everything we about galaxies isn't quite right,

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and so we need to learn that
more carefully to learn about how galaxies

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have changed. The most exciting element
about this research is the fact that we

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can now look at huge samples of
galaxies, hundreds of thousands, and even

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in the future, millions of galaxies, and without having to do anything separately

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to the analysis we've done before.
We can now look at all of these

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galaxies and with one fell swoop we
can understand which of them have mass supermassive

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black holes in them that are shining
brightly, and which of them don't.

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Devils is a survey that has been
conducted on the Anglo Australian Telescope in New

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Wales. In Australia, we've been
using the telescope to collect what is known

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as a redshift, so a measure
of the distance to a galaxy for about

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sixty thousand galaxies and a tiny patch
of the sky. These galaxies are some

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of them nearby, others they are
billions and billions of years in the past,

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so they're very very far away.
These are the galaxies that we've been

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analyzing in this research to analyze how
it is that they've changed and how it

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is that their supermassive black holes have
changed over time. There's currently a telescope

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in Chili that is undergoing a renovation. That renovation wants complete will enable new

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surveys to begin, bigger and better
than we've done before. One of those

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will be the Wave Survey, which
is looking at galaxies about one point six

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million of them. Once we have
those data, we will be able to

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analyze those millions of galaxies in the
same way that we're doing with this study,

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and we'll learn more about them on
a scale thus far unknown. The

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study's co author Jessica Thorne, also
from the University of Western Australia's node of

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the International Center for Radio Astronomy Research. This is the new technique combines multi

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bands of electromagnetic wavelengths from a range
of telescopes in order to identify which galaxies

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contained feeding supermassive black holes and which
are quiet. My name is Jess Thorne.

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I'm a PhD student at KWA.
Black Holes are some of the darkest

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and most elusive objects in the universe. We don't know all that much about

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what happens within inside them, but
in the centers of most massive galaxies in

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the universe, they can be some
of the most luminous objects, so they

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can suck in stuff from around them, and as they do this, the

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stuff gets heated up and becomes super
super bright, and in some cases this

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can outshine the host galaxy of the
black hole. Usually we find these active

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galactic nuclei these central black holes by
using specialist telescopes like the X ray or

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the radio, and using specialist techniques
to reduce the data and find these black

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holes. We've taken a new technique
where we can use existing imaging from multiple

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telescopes, combine it altogether, using
images of the galaxy in multiple wavelengths,

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and use it to identify which galaxies
host these active galactic nuclei. This research

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is really exciting because generally in the
past, to find these active galactic nuclei,

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we have to point an X ray
telescope by the same patch of sky

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for millions of seconds. Whereas this
new research will allow us to combine imaging

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that already exists and takes much less
time to collect. We can piece it

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all together to find these active galactic
nuclei a lot quicker than previous methods.

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This research excites me a lot because
these active galactic nuclei can have a huge

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impact on their host galaxies. They're
sucking in large amount of matter, emitting

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a large amount of light, and
we expect that this will have a huge

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impact on the host galaxy itself.
We think that this might lead to a

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shutdown of staff formation in the galaxy
and can potentially kill all staffmation in their

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galaxy. And we can use these
to understand what the future of the universe

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will be like. That's Jessica Thorn
from the University of Western Australia and this

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space Time and Time met to take
another brief look at some of the other

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stories making us in science this week
with a science report. A new stay

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is measured the extent to which a
burn fracture could lead to early death,

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and they've created a publicly available tool
which doctors and patients can use to calculate

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the risk. The findings, reported
in the journal E Life, examined data

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from over one point six million adults. The authors found that a burn factor

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was associated with a loss of one
to seven years of life, depending on

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gender, age, and burn side. The symetric has now been incorporated into

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an online calculator that measures burn fragility
in order to help doctors and patients better

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understand the true gravity of burn fractures. Scientists have developed a genetically modified variety

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of Cavendish bananas designed to help save
the world's Cavendish banana production. The new

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variety, called QCAV four, has
now been submitted for regulatory approval to the

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federal government. The QCAV four banana
is in fact the first to strange genetically

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modified through or should that be herb, to be submitted for assessment. If

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approved, it would offer potential safety
net against the devastating Panama disease Tropical Race

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four, which threatens the world's twenty
billion dollar banana industry. QCV four bananas

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have been grown in fill trials in
the Northern Territory for over six years out

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of proven to be highly resistant to
Panama disease. Panama disease has already crippled

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Cavendish banana production in Asia and has
now started to take a foothold in South

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America. It already occurs in Australia
in both the Northern Territory and Northern Queensland.

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QCV four is a Cavendish grand name
banana which has been bioengineered with a

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single gene r GA two from the
world Southeast Asian banana. Mind you,

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normal Cavendish bananas already contained the same
gene, but it lies dormant, and

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the aim of this exercise has been
to develop a variety that gets the gene

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to do its thing, and that's
important. It was Cavendish bananas account for

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ninety seven percent of all global banana
production. Well, it seems artificial intelligence

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has taken another step towards its eventual
Skynet like takeover of human civilization, with

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researchers finding that humans tend to be
more empathetic towards AIS if they seem to

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disclose personal information. A report in
the journal Class One showed how researchers instructive

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participants to have a text based chat
with an online AI at to play at

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a scenario between two co workers.
In each conversation, the AI appeared to

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self disclose either highly work relevant personal
information, less relevant information about a hobby,

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or no personal information at all.
So I had to say that compared

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with the less relevant sharing or no
sharing at all, bots that chatted about

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themselves and work end up getting far
or empathy from human participants. Meanwhile,

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after earlier passing its medical licensing exam
with sixty percent accuracy and scoring two hundred

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ninety seven on its Legal Buyer exam, which would have been enough to be

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admitted to practice law in most American
states, the chat GPT four AI has

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now successfully passed its Radiological Board exam. A report in the journal Radiology says

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chat GPT four managed to exceed the
passing threshold with a score of eighty one

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percent, showcasing significant improvements, especially
in a higher order thinking questions. Apple

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has rolled at its emergency SOS satellite
link feature the iPhone fourteen users in Australia,

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New Zealand. The new feature has
only been available up to now for

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devices in North America and Europe.
With the details were joined by technology editor

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Alek Sahara of rout from Tech Advice
Start Life. Yeah, it's the Emergency

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SOS VIA satellite. A lift has
now arrived in Australia and New Zealand the

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en It is exclusive to the four
iPhone fourteen models, the Phone fourteen,

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the Plus, the Pro and the
Pro Max. And it's been about only

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about eight months. I mean I
was actually in Hawaii at the Qualcom conference

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on the day that Apple made the
capability available in the US, and I

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was testing it out there, and
when they made it available in Australia,

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I was able to immediately go outside, hold my phone to the sky,

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go into the settings though to the
Emergency SOS section. Scroll down to the

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bottom and try the Emergency SOS VIS
Satellite demo, which takes you through a

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simulated experience. However, it does
actually connect you to a real satellite and

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you have to hold the phone to
the sky. It's asked me to turn

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left or turn rise, and the
satellites are moving obviously very quickly overhead.

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It can take some minutes for the
connection, but it within a couple of

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minutes I was connected. And then
it is using a series of pre determined

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questions and it compresses the text by
three times to make sure that the message

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can be set as quickly as possible, and already at a stated lives of

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the twelve countries that it is apparently
available, so no doubt we will be

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here very soon. That it has
also saved lives in Australia and New Zealand

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because as soon as you're in an
area where there's no mobile reception, some

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00:23:07.039 --> 00:23:11.839
people I didn't note we're commenting,
oh, I've seen my phone saying no

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00:23:11.960 --> 00:23:14.559
service, but I was still able
to get a call through to Triple O.

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00:23:14.839 --> 00:23:18.839
And that's because Telstra, the biggest
carrier in Australia, has one point

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two million square kilometers of additional coverage
compared to its competitors. So even if

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you're on one of the other phone
providers, or you're on a mobile virtual

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never operator that operates on Telstra's wholesale
network, you may still be a range

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00:23:30.960 --> 00:23:33.480
of Telstra's entire network, in which
case the Tripolo call will go through.

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00:23:33.519 --> 00:23:37.480
But when you're not in any coverage
area at all, you're staff and as

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00:23:37.480 --> 00:23:41.759
somebody drives by. So it's really
a wonderful thing that undertook them eight months

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00:23:41.759 --> 00:23:45.119
to bring it to the Southern Hemisphere, which is very impressive. And we

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00:23:45.160 --> 00:23:49.160
did have Qualcom announced at CES in
January that they would have a pole to

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00:23:49.279 --> 00:23:53.359
pole service that would know Qualcom satellite
that would be available next year. I'm

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00:23:53.359 --> 00:23:56.359
all later this year, but I'm
sure that by the time that Qualcom service

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00:23:56.400 --> 00:24:00.480
will launch, Apples will also most
likely cover pole to pole and it will

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00:24:00.519 --> 00:24:04.240
signal the new era of being able
to connect de vice headlight's just using your

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00:24:04.240 --> 00:24:10.319
phone and eventually your phone will deliver
phone calls and browsing and all the restlans.

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00:24:10.319 --> 00:24:12.720
For the time being, it's just
text, yeah, but it's also

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00:24:12.839 --> 00:24:17.799
the ability for your friends and family
to track you with your permission using the

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00:24:17.839 --> 00:24:19.480
find my service. So you're if
you're in the Blue Mountains in Australia,

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00:24:19.519 --> 00:24:23.000
for example, you're in the outback
somewhere and you aren't able to be connected

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00:24:23.039 --> 00:24:26.480
to a Wi Fi or three G, four G or five G network,

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00:24:26.559 --> 00:24:30.720
then you can still be tracked by
satellite, which is quite incredible. System

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00:24:30.960 --> 00:24:34.279
replace the EPERB or not really.
They do not replace the EPERBS, which

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00:24:34.319 --> 00:24:40.359
goes for Emergency position indicating radio beacons, and they also don't replace a traditional

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00:24:40.519 --> 00:24:42.839
satellite phones which cost about a thousand
dollars to buy. You also have these

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00:24:42.880 --> 00:24:48.279
personal locator beacons as well. I
did have a company either be saying hey

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00:24:48.400 --> 00:24:52.559
we sell at Australia, a brand
of personal located beacons is recording that they

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00:24:52.680 --> 00:24:56.759
have a seven year battery. Live
though for the true adventurer, just relying

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00:24:56.799 --> 00:24:59.759
on your iPhone is probably not going
to be enough. You're going to want

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00:24:59.799 --> 00:25:04.480
to have You're gonna want to have
a satellite Vegan. That's Alexahara Royd from

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00:25:04.559 --> 00:25:26.240
Tech Advice, Start Live and that's
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00:25:26.279 --> 00:25:30.279
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