Aug. 25, 2026

Stellar Salvage: SpaceX's Starship Recovery and the Age of the Universe

Stellar Salvage: SpaceX's Starship Recovery and the Age of the Universe
SpaceTime Series 29 Episode 102 *SpaceX’s Starship arrives at Christmas Island After some 24 days at sea, a SpaceX recovery team has successfully towed its test flight 13 Starship into the remote Australian Indian Ocean territory of Christmas Island. The unplanned operation was hastily put together after the spacecraft unexpectedly held together following its splashdown off the Western Australian coast. *How old really is the universe? Astronomers have come up with a new way to work out the age of the universe finding it to be 13.6 billion years old – some 200 million years younger than previously thought. *Einstein’s general relativity theory still stands More than 100 years after Albert Einstein published his iconic general theory of relativity, it remains science’s best understanding of gravity and the universe on the cosmic scale. *The Science Report A new study shows that carrying a little extra weight could be beneficial as you get older. People lacking human connections more likely to turn to AI chatbots for companionship. The Southern Ocean and parts of the Pacific may be the best places to fertilise to remove CO2. How dogs have learnt to understand human facial expressions. Alex on Tech: The Galaxy passport sized Z Fold 8 tops the sales figures.

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The Astronomy, Space, Technology & Science News Podcast.

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This is Space Time, Series 29, Episode 102, for broadcast

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on the 26th of August, 2026. Coming up on Space Time.

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SpaceX's Starship arrives at Christmas Island. A new study looking

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at how old our universe really is. And despite more tests,

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Albert Einstein's general theory of relativity still stands the test

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of time. All that and more coming up on Space Time.

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Welcome to Space Time with Stuart Gary.

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After some 24 days at sea, a SpaceX recovery team

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has successfully towed Starship 40 into sheltered waters on the

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leeward side of the remote Australian Indian Ocean territory of

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Christmas Island. The unplanned operation had been hastily put together

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after the spacecraft unexpectedly held together following its splashdown off

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the western Australian coast. Starship 40 had been launched into

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orbit on Test Flight 13 from SpaceX's Boa Chica Starbase

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on the Texas Gulf Coast. The hour-long test flight saw

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the world's largest and most powerful rocket, a 122-meter-tall Starship

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Super Heavy, successfully blasted into space and achieve all its

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major test goals. The flight used the latest Block III

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incarnation of the rocket, together with a new ignition sequence

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for its 33 new more powerful Raptor III version engines.

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The successful stage separation saw the launch vehicle's first stage,

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known as the Super Heavy, carry out a textbook boost-back burn,

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returning to Earth and splashing down off the Texas coast. However,

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only 10 of the planned 13 Raptors lit up for

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the landing burn, with a further two failing shortly afterwards.

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Now that meant Super Heavy descended too quickly, and consequently

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hit the water much too hard. Meanwhile, the Starship Upper Stage,

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known simply as the ship, continued to climb to its

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planned suborbital altitude, where it successfully deployed 20 Starlink Version

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3 broadband test satellites and also successfully undertook a Raptor

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engine restart. It then re-entered the atmosphere, performing a perfect

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descent and water landing, gently splashing down and toppling over

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into the ocean. However, surprisingly, rather than sinking, it remained buoyant,

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bobbing up and down on the waves. Now, that's never

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happened before. but it gave SpaceX an opportunity to recover

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the vehicle for more detailed examination. See, usually SpaceX engineers

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only end up with data from onboard instruments and cameras,

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so having the actual spacecraft to look at was a

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huge bonus. SpaceX boss Elon Musk quickly organized a recovery

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operation with a SpaceX splashdown monitoring ship, Go Astralis, remaining

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stationed near ship 40. The splashdown occurred roughly 1,300 kilometres

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off the western Australian coast, and so required specialised ocean-going

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tugs for the operation. Two tugboats, Norman Ranger and Skimmer Tide,

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were contracted and quickly set out from the Australian port

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of Dampier to undertake recovery efforts. Norman Ranger is a

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big anchor-handling tug.

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It's used to.

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Dealing with huge quarter-million and half-million tonne iron ore bulk carriers,

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so an empty 200-tonne spacecraft shouldn't be a problem. The

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problem is Starship wasn't fitted with any anchor points to

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attach a tow rope to, and that's where Schematide came in.

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It delivered a string of large Yokohama rubber buffer fenders

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which would be placed around the spacecraft, encircling it like

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a lasso and cushioning it from damage so it could

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be towed. These buffer fenders used compressed air to absorb

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impact energy during ship-to-ship or ship-to-dock operations, protecting vessels and

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port structures from damage. However, the ocean currents and winds

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proved to be a major challenge for maneuvering the spacecraft,

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which was sitting high in the water. That meant slow

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progress and an awfully long journey back to Port Ampere.

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Making matters worse, the fenders were damaging the spacecraft's heat

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shield tiles, which was one of the key items engineers

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wanted to examine. So it was eventually decided to change plans.

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Remove the fenders and attach a tow line to one

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of the spacecraft's Raptor vacuum engines. and there was still

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that ongoing fight against the prevailing winds and swell. Eventually,

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SpaceX decided to change course. Instead of heading east to

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the Australian mainland, they'd head north to Christmas Island instead,

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arriving there a few days ago. The heavy lift ship

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Forte has now arrived at Christmas Island to load and

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transport Starship. Forte is a semi-submersible, meaning it will flood

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its ballast tanks to submerge just enough to allow Starship

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to be positioned above its deck. It'll then empty its

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ballast tanks again and refloat, lifting the spacecraft out of

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the water for transport back to the United States. Needless

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to say, NASA's monitoring these events closely, with a version

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of Starship called the HLS to be one of the

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vehicles used to transport Artemis crew from the Orion spacecraft

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down to the lunar surface and back again once manned

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operations to the lunar south pole get underway. A test

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of those capabilities is slated for next year in low-Earth

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orbit using the Artemis III mission, which will attempt docking

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a manned Orion capsule with the Starship. And if that

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goes well, then a manned lunar landing is likely to

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happen in 2028. This is Space Time. Still to come,

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a new debate on how old the universe is, and

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Einstein's general theory of relativity passes yet another test. All

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that and more still to come on Space Time. Astronomers

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think they've come up with a new way to work

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out the age of the universe, finding it to be 13.6

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billion years old. That's some 200 million years younger than

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previously thought. The findings reported in the journal Astronomy and

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Astrophysics are based on comparing estimates of the universe's age

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rather than its expansion rate as a new way to

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address the Hubble tension. This question of the Hubble tension,

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how quickly the universe is expanding and therefore how old

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it is, is one of the most debated topics in

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modern cosmology. Local measurements show a faster expansion rate than

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predictions calculated from the early universe. And that creates a

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statistical mismatch that standard physics simply can't explain. So what

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are these two methods? Well, the early universe cosmic microwave

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background radiation method uses telescopes to measure the cosmic microwave

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background radiation emitted when the first hydrogen atoms formed 280,000

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years after the Big Bang, which has now cooled down

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to just 2.7 degrees above absolute zero. Running this data

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through standard cosmological models predicts an expansion rate, or Hubble constant,

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of around 67 to 68 kilometers per second per megaparsec.

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On the other hand, the Late Universe Distance Ladder method

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uses stars known as Cepheid variables, which all pulsate at

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given rates based on their size and hence luminosity, and

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Type Ia supernovae, which are all roughly the same mass

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and hence explode with the same level of luminosity, thereby

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allowing astronomers to use the inverse square law to determine

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cosmic distances. It's a bit like looking at a row

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of streetlights down a road. They're all the same brightness,

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but they look progressively dimmer and dimmer the further away

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they are, or in cosmic terms, how fast things are

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moving away from you. This shows a faster Hubble constant

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of around 73 to 74 kilometers per second per megaparsec.

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And no matter how much scientists have tried, they haven't

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been able to reconcile the difference between these two measurements.

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That's the Hubble tension. Using precise stellar data, the study's

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authors determined ages for carefully selected very old Milky Way

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stars and concluded the most likely age for the universe

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as a whole would be 13.6 billion years. Now that's

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much younger than assumptions under standard cosmological models. The age

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is inconsistent with a younger universe, implied by Cepheid variable

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and supernova-based expansion measurements. But it is compatible with the

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older age inferred by observations of the cosmic microwave background radiation,

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the leftover heat from the Big Bang. Cosmological models link

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the current rate of expansion of the universe directly to

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its age, with a higher value of the Hubble constant

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implying a younger universe, while a lower value corresponds to

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an older one. Of course, the universe can't be any

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younger than the oldest stars it contains. and the authors

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of this new study use that as their guidestone. So

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if the ages of the older stars in our galaxy

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can therefore be measured with a high degree of precision,

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a robust lower limit for the age of the universe

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can be established. The project was initiated by an unusual

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collaboration between two research fields that have traditionally been very separate,

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a cosmology group from the University of Bologna and a

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stellar archaeology group from the Leibniz Institute of Astrophysics in Potsdam.

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The work was based on an existing catalogue of stellar

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ages from a previous study in which precise ages were

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measured by combining multiple pieces of information on the brightness,

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position and distance of more than 200,000 stars in the

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Milky Way. A crucial element for this study was the

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use of the third data release from the Gaia mission,

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which provides exceptionally accurate parallaxes and spectra and thus improved

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stellar parameters for a large number of nearby stars. From

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this combined dataset, a carefully selected group of the oldest

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stars with the most reliable age estimates was compiled. The

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focus was on quality over quantity, using only stars whose

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ages could be determined robustly and by removing potential contaminants.

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And with the NEXTGUIDE data release on the horizon, stellar

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ages could become a fundamental anchor of cosmology. Now, although

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these results are not yet conclusive due to remaining uncertainties

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in stellar age estimates, they are providing an important independent

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constraint on the debate over the Hubble tension, and consequently,

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the age of the universe. This is Space Time. Still

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to come, yet another experiment showing Einstein's general theory of

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relativity stands the test of time. Later in the science report,

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a new study shows how dogs have learnt to understand

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human facial expressions. All that and more still to come

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on Space-Time. More than a hundred years after Albert Einstein

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published his iconic general theory of relativity, it remains science's

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best understanding of gravity in the universe on the cosmic scale.

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And it's consistently withstood the very best tests scientists can devise.

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A report in the journal Science looked at one of

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the most comprehensive tests of general relativity near a supermassive

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black hole ever undertaken. The study's lead author, Andrea Gentz,

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from the University of California, Los Angeles, admits, based on

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her data, Einstein is still right. However, she points out

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that general relativity still can't fully explain gravity inside a

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black hole, and at some point, science will need to

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move beyond Einstein's theories to a more comprehensive understanding of

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gravity that explains exactly what a black hole is. Einstein's

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1915 general theory of relativity holds that what we perceive

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as the force of gravity arises from the curvature of

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space and time due to mass. Light from a star

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is bent by the mass of that star, as well

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as any other stars or objects as photons of light

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pass by. And it's not just light, even time changes

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due to mass and velocity. So Einstein's theory remains the

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best description science has of how gravity works. And these

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laws of physics, including gravity, should be valid everywhere in

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the universe. To test that, Jensen colleagues observed a star

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known as SO2 as it orbits Sagittarius A-star, the supermassive

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black hole at the center of our galaxy, the Milky Way.

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Located some 27,000 light-years away, Sagittarius A-star has some 4.3

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million times the mass of our Sun, and it's the

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pivot point around which our entire galaxy revolves. The star

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SO2 takes some 16 years to complete each orbit around

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Sagittarius A star, travelling at speeds of over 26 million

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kilometres an hour during its closest approach to the black hole.

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So Goetz and colleagues watched as this star undertook its

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orbital voyage, and they analysed the spectra coming from the

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star as it made its closest approach to the black hole.

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Spectra is the rainbow of light produced by the star,

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and it displays a series of so-called spectral lines, which

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provide a signature of the chemicals that make up that star.

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As well as its composition, spectra also tell you how

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luminous a star is. The thicker the spectral lines, the

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hotter the star. It can even tell you how fast

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the star is moving towards or away from you thanks

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to a Doppler shift in its spectral lines. Objects moving

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away have their spectral lines shifted towards the red end

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of the spectrum, redshifted. While objects moving towards you have

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those lines shifted towards the blue end of the spectrum,

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blue shifted. And how far those lines are shifted tells

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you how fast that object's moving towards or away from you.

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Goetz and colleagues took measurements of SO2 roughly every four

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nights during crucial periods of the star's orbit over a

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24-year period, using observations from the Keck Observatory at Topamanakeo

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as well as the Gemini and Subaru telescopes. Combined, this

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data allowed the authors to test general relativity to an

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unprecedented level. The authors were able to see a commingling

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of space and time near the supermassive black hole. Now,

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in Newton's version of gravity, space and time are separate.

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They do not commingle. But under Einstein, they get completely

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commingled near the black hole. Einstein had reported that in

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this region close to the black hole, photons have to

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do extra work. Their wavelength as they leave the star

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depends not only on how fast the star is moving,

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but also how much energy the photons expend to escape

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the black hole's powerful gravitational pull. Gett says while this

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tells us what happens on the universe side of the

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event horizon of a black hole, it doesn't explain what's

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going on between the event horizon and the singularity, the

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point of infinite density in zero volume.

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Black holes are deceptively simple and yet incredibly complex. A

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black hole is a region of space where the pull

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of gravity is so intense that nothing can escape, not

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even light. Music We don't have the physics to describe

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what a black hole is because it leads to a paradox,

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a breakdown in our understanding of how the universe works.

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We only have four fundamental forces to describe how the

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universe works. Gravity of those four is probably the one

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that we have the most intuition for. You throw something up,

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it comes back down. but it's actually the least explored.

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Einstein really recognized that gravitational fields are equivalent to talking

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about space and time not being separate entities.

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Einstein noticed that in certain situations, Newtonian laws of physics

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don't seem to hold. And that's why Einstein developed his

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theory of general relativity. We know that general relativity may

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not be a complete description of physics, and so in

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order to figure out where it's incomplete, you want to

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test it in regions that people haven't tested before. So

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people have tested general relativity on Earth, in the solar system,

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but never around a black hole that's four million times

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the mass of the Sun.

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The first question I was interested in was, is there

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a supermassive black hole at the center of our galaxy?

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If you had asked me would I still be doing

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this project, 20 odd years later when we first started,

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I would have just laughed at you. I grew up

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hearing the word no all the time. You're a girl,

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you can't do it. You're a girl, there's no way

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you can get into MIT. There's no way you can

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get into Caltech. I think I developed a passion for

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proving people wrong. We have been able to increase the

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evidence for supermassive black holes by a factor of 10 million.

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And we have done this by watching how stars move.

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My favorite star, its name is SO2, and it makes

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its journey every 16 years. We're at this point where

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it's closest to the black hole and is experiencing the

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strongest pull of gravity. So we have this first opportunity

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to get a direct measurement of how Einstein's theory of

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general relativity works near a supermassive black hole.

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What we've found this summer is that general relativity does

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actually describe the motion of the stars around the supermassive

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black hole.

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That's a transformational change in our understanding about not only

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the existence of supermassive black holes, but the physics and

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astrophysics associated with black holes.

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Andrea, to me, is a brilliant scientist. Her dedication and

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her persistence really has been at heart of this project

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in order to have the patience and the level of

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detail required to do this work.

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When I was young I wanted to be the first

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woman on the moon, but I think at the same

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00:17:48.380 --> 00:17:53.519
time I also wanted to be a ballerina. I just

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00:17:53.539 --> 00:17:59.029
became much more infatuated with the ideas rather than the

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physicality of moving myself. It's very poetic that we actually

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00:18:05.670 --> 00:18:09.769
see the stars in motion doing this dance around the

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black hole. So what we want to do is we

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want to improve our ability to see a star like

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our sun at the center of the galaxy. Because I

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think that's when we'll have the full view of how

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this dance really works.

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That's Andrea Goetz and Tuan Du from the University of California,

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Los Angeles. And this is Space Time. And time now

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to take another brief look at some of the other

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stories making use in science this week with a science report.

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A new study has shown that carrying a little extra

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weight could be beneficial as you get older, but not

298
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if it's a bigger tummy. A report in the Journal

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00:19:08.390 --> 00:19:11.369
of the American Geriatric Society claims the new findings are

300
00:19:11.470 --> 00:19:15.730
further pushing the disparity between body mass indexes and waist circumference.

301
00:19:16.390 --> 00:19:18.809
They say having a higher body mass index when you're

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00:19:18.849 --> 00:19:22.039
older has been linked to a significantly lower risk of dying,

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00:19:22.180 --> 00:19:24.859
whereas a bigger belly is linked to the opposite. The

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00:19:24.880 --> 00:19:28.579
researchers looked at data from 7,000 adults aged 65 or

305
00:19:28.700 --> 00:19:31.960
older finding overweight men and men with obesity, that's a

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00:19:32.000 --> 00:19:35.299
BMI of 30 to less than 40, had a 46

307
00:19:35.299 --> 00:19:38.519
to 51 percent lower risk of mortality compared to those

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00:19:38.589 --> 00:19:42.259
of normal weight. However, a higher waist circumference was linked

309
00:19:42.299 --> 00:19:45.680
to a 24% increased risk of mortality in men, with

310
00:19:45.759 --> 00:19:50.089
similar patterns seen in women. A new study claims that

311
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people who lack human connections tend to be more likely

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00:19:52.950 --> 00:19:57.269
to use an artificial intelligent chatbot for companionship. A report

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00:19:57.309 --> 00:20:00.730
in the journal Nature Human Behavior looked at 237 people's

314
00:20:00.829 --> 00:20:05.049
use of AI chatbots, specifically character AI, a widely used platform,

315
00:20:05.210 --> 00:20:07.890
and found people with fewer friends were more likely to

316
00:20:08.029 --> 00:20:10.990
end up using chatbots for companionship, which was in turn

317
00:20:11.150 --> 00:20:16.259
linked to worse self-reported well-being. The link between AI companionship

318
00:20:16.400 --> 00:20:19.180
and poor well-being was strongest among people who had more

319
00:20:19.259 --> 00:20:22.619
intense relationships with the AI and those who disclosed their

320
00:20:22.640 --> 00:20:27.420
most personal information during their chats. A new study has

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00:20:27.460 --> 00:20:29.640
found that the Great Southern Ocean, as well as parts

322
00:20:29.680 --> 00:20:31.920
of the Pacific Ocean near the equator, may be the

323
00:20:32.000 --> 00:20:34.920
best places on Earth to fertilize if humans want to

324
00:20:34.960 --> 00:20:37.400
remove most of the carbon dioxide in the atmosphere while

325
00:20:37.440 --> 00:20:41.869
minimizing the impact on the environment. Fertilizing the ocean involves

326
00:20:42.009 --> 00:20:45.289
adding iron to stimulate photoplankton to grow, which in turn

327
00:20:45.369 --> 00:20:49.140
removes carbon dioxide from the atmosphere. The authors compared the

328
00:20:49.180 --> 00:20:51.380
most likely amount of carbon that could be removed by

329
00:20:51.480 --> 00:20:54.390
fertilizing different parts of the oceans around the world, and

330
00:20:54.410 --> 00:20:57.430
they also looked at the environmental impact fertilization would have.

331
00:20:58.089 --> 00:21:00.769
The findings, reported in the journal Nature, claim that the

332
00:21:00.849 --> 00:21:04.430
Southern Ocean offers the best balance between ecological disturbance and

333
00:21:04.529 --> 00:21:10.839
carbon dioxide removal from the atmosphere, followed by the equatorial Pacific. Well,

334
00:21:10.880 --> 00:21:13.180
if you have a four-legged friend with a waggly tail

335
00:21:13.240 --> 00:21:15.859
and a wet nose, you probably already know dogs can

336
00:21:15.900 --> 00:21:20.279
distinguish quite well between different facial expressions, including anger, sadness

337
00:21:20.299 --> 00:21:23.900
and fear. And now new research has finally worked out

338
00:21:23.960 --> 00:21:27.640
what's going on. The findings reported in the journal iScience

339
00:21:27.849 --> 00:21:30.549
are based on brain scans of 12 dogs showing that

340
00:21:30.589 --> 00:21:33.309
specific regions of their brains were active when they saw

341
00:21:33.369 --> 00:21:37.039
happy faces compared to neutral negative ones. Now, one of

342
00:21:37.059 --> 00:21:40.099
these brain regions is also associated with reward, which the

343
00:21:40.180 --> 00:21:43.160
authors think suggests that happy human faces may be emotionally

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00:21:43.220 --> 00:21:46.880
significant to dogs. They also found differences in dogs' brain

345
00:21:46.920 --> 00:21:49.720
activity when they saw angry and fearful faces, small as

346
00:21:49.839 --> 00:21:53.099
sad versus fearful faces, but no difference between sad and

347
00:21:53.180 --> 00:21:56.980
angry expressions. The study shows that man's best friend has

348
00:21:57.019 --> 00:22:01.039
evolved the social skills necessary to understand and cooperate with people.

349
00:22:01.380 --> 00:22:05.710
The best way to know who's a good boy. Samsung's

350
00:22:05.750 --> 00:22:09.380
new passport-sized Galaxy Z Fold 8 has outsold its more

351
00:22:09.420 --> 00:22:12.920
conventionally proportioned Galaxy Z Fold 8 Ultra during its first

352
00:22:12.960 --> 00:22:16.970
weeks on the market with 51% of sales. With the details,

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00:22:16.990 --> 00:22:21.279
we're joined by technology editor Alex Saharov-Royd from TechAdvice.life.

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00:22:21.519 --> 00:22:24.519
It just went on sale and already in Australia, the

355
00:22:24.759 --> 00:22:27.099
passport size one with the widescreen version as opposed to

356
00:22:27.119 --> 00:22:30.259
the one that's square, that has narrowly outsold the square one.

357
00:22:30.420 --> 00:22:33.700
And that's because it's wider. Think of a wider iPhone

358
00:22:33.740 --> 00:22:36.450
mini style device that can then unfold into the 7.6

359
00:22:36.450 --> 00:22:41.789
inch widescreen tablet. I went out and purchased the Z Fold,

360
00:22:42.210 --> 00:22:45.609
and it is fantastic, the Z Fold 8, not the Ultra,

361
00:22:45.630 --> 00:22:47.619
which is the one that's square. So it's been really,

362
00:22:47.779 --> 00:22:50.359
really cool. I mean, everyone marvels at it. The crease

363
00:22:50.400 --> 00:22:53.400
is effectively no longer there. I mean, you can still

364
00:22:53.500 --> 00:22:54.740
see it if you hold it to the lightness. a

365
00:22:54.759 --> 00:22:57.309
certain way, you can just feel it. But compared to

366
00:22:57.329 --> 00:22:59.450
foldable phones from a couple of years ago where you

367
00:22:59.490 --> 00:23:01.930
could really feel this dip in the center of the

368
00:23:01.970 --> 00:23:04.779
screen when you moved your finger across, effectively the crease

369
00:23:04.819 --> 00:23:06.680
is gone. And this is what Apple has been waiting

370
00:23:06.700 --> 00:23:09.359
for for the last eight years for screens to get

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00:23:09.400 --> 00:23:12.880
into this state. Now, interestingly, Apple will launch its iPhone

372
00:23:12.920 --> 00:23:14.970
Fold or iPhone Ultra, whatever it's going to be called,

373
00:23:15.329 --> 00:23:17.910
in about three weeks' time. But the latest rumors say,

374
00:23:17.990 --> 00:23:20.650
because of the rampocalypse, because of the super high expensive

375
00:23:20.670 --> 00:23:24.710
prices for SSDs, that Apple will showcase it. They'll launch

376
00:23:24.750 --> 00:23:26.710
it in the U.S. first, but it won't come to

377
00:23:26.730 --> 00:23:29.390
the rest of the world until the first quarter or

378
00:23:29.410 --> 00:23:32.069
the second quarter of next year. And we've got Omdia,

379
00:23:32.369 --> 00:23:35.690
who's predicting that by 2028, shipments of these phones will

380
00:23:35.730 --> 00:23:38.920
double to 36 million units. So there's going to be

381
00:23:38.940 --> 00:23:41.480
a huge boom. I mean, already you see people with

382
00:23:41.500 --> 00:23:43.119
these folding phones, but there's going to be so many

383
00:23:43.160 --> 00:23:45.339
more of them. And gone are the days when the

384
00:23:45.359 --> 00:23:48.869
folding phones feel like two smartphones stuck together, this big,

385
00:23:48.950 --> 00:23:52.250
thick thing in your hand. The current smartphones, when they

386
00:23:52.430 --> 00:23:56.059
fold shut, the foldable phones, will feel like an ordinary smartphone.

387
00:23:56.470 --> 00:23:56.710
Phone.

388
00:23:56.750 --> 00:23:58.569
They feel like the thickness of a normal phone. And

389
00:23:58.589 --> 00:24:02.440
then they open up into this glorious landscape. And I'm

390
00:24:02.460 --> 00:24:04.740
just in love. I love this phone factor. It is

391
00:24:04.940 --> 00:24:06.359
stunningly good and cool.

392
00:24:06.420 --> 00:24:07.420
What about the trifold?

393
00:24:07.480 --> 00:24:11.759
Well, with the trifold phones, I was in Shenzhen in 2024,

394
00:24:11.759 --> 00:24:14.359
and I actually saw one of these phones in a

395
00:24:14.440 --> 00:24:15.180
Huawei store.

396
00:24:15.319 --> 00:24:17.799
That gives you the same aspect ratio as what you've

397
00:24:17.819 --> 00:24:19.789
got with the passport size phone, I take it?

398
00:24:19.809 --> 00:24:21.670
Well, yes and no, right? So you've got a phone

399
00:24:21.690 --> 00:24:25.309
that's 6.5 inches or thereabouts in size. And because there's

400
00:24:25.390 --> 00:24:28.369
three panels, when you unfold it, it sort of unfolds

401
00:24:28.390 --> 00:24:30.170
into a 10-inch tablet. And I guess it is, yes,

402
00:24:30.230 --> 00:24:32.880
it is more rectangular than it is square. But of course,

403
00:24:32.920 --> 00:24:35.619
it's a lot thicker. And Samsung actually had one of

404
00:24:35.660 --> 00:24:38.900
these at the EES earlier this year, 2026. And their phone,

405
00:24:39.059 --> 00:24:42.190
when it was unfolded, was quite thick. slim. Obviously, when

406
00:24:42.210 --> 00:24:45.210
you have three panels put together, it does feel thicker.

407
00:24:45.410 --> 00:24:48.390
And actually, Samsung stopped selling this phone because they launched

408
00:24:48.430 --> 00:24:50.950
it in South Korea first. And it's very expensive. You're

409
00:24:50.970 --> 00:24:54.369
talking $ 4, 000, $ 5, 000 Australian dollars to get one of these phones. Now,

410
00:24:54.410 --> 00:24:56.930
Samsung is apparently going to launch a second generation of

411
00:24:56.970 --> 00:25:00.859
this particular phone and hopefully will actually be much flatter.

412
00:25:00.880 --> 00:25:04.500
You'll still have the two creases, but they'll effectively be flat. And,

413
00:25:04.519 --> 00:25:07.519
you know, having that was extremely cool as well. You

414
00:25:07.539 --> 00:25:09.539
could go from a normal phone size into a tablet

415
00:25:09.559 --> 00:25:12.859
size in the single device. You could also, with the Huawei,

416
00:25:12.880 --> 00:25:15.720
you could actually have it as a two-panel display, so

417
00:25:16.009 --> 00:25:17.990
like a smaller tablet, and then unfold it into a

418
00:25:18.109 --> 00:25:18.950
three-panel display.

419
00:25:19.009 --> 00:25:21.470
How are phones being affected by the price of SSDs

420
00:25:21.529 --> 00:25:21.970
and memory?

421
00:25:22.009 --> 00:25:23.809
Well, the prices have had to go up. Apple had

422
00:25:23.829 --> 00:25:27.029
to raise the price of its MacBook Neo, its Mac range.

423
00:25:27.329 --> 00:25:29.509
It held the price of its current iPhone 17 range.

424
00:25:30.670 --> 00:25:32.420
But all the rumors say that Apple is going to

425
00:25:32.460 --> 00:25:35.779
be forced to increase the price of its smartphones later

426
00:25:35.819 --> 00:25:38.849
this year because even though Apple has fat margins, the

427
00:25:38.880 --> 00:25:41.509
price has gone up so much that this has caused

428
00:25:41.609 --> 00:25:43.049
the phones to come out with less memory. I mean,

429
00:25:43.109 --> 00:25:46.109
with the Google Pixel range, Pro and Pro XL, the

430
00:25:46.230 --> 00:25:49.539
entry-level model, which is 256 gigabytes, that only comes with

431
00:25:49.539 --> 00:25:51.920
512 gig of RAM. You need to buy the 512

432
00:25:51.920 --> 00:25:54.839
gig or the one terabyte model to go back to

433
00:25:54.839 --> 00:25:56.880
16 gigabytes of RAM, which is what they had last year.

434
00:25:56.900 --> 00:25:59.480
So we're seeing phones that have less memory than they

435
00:25:59.539 --> 00:26:02.740
had last year because the prices are so expensive. Demand

436
00:26:02.799 --> 00:26:04.849
is expected to last until 2028, 2029, 2030. What's going

437
00:26:04.869 --> 00:26:11.009
to change that is that the on-device AI the capabilities

438
00:26:11.069 --> 00:26:13.369
of the chips that are in our phones, tablets, and computers,

439
00:26:13.430 --> 00:26:16.250
and also the models that can run locally, not just

440
00:26:16.309 --> 00:26:18.289
on the GPU, but on the CPU, this is going

441
00:26:18.309 --> 00:26:21.769
to mean that you have advanced AI capabilities equal to

442
00:26:21.789 --> 00:26:24.710
the best of today in your laptop, phone, or tablet

443
00:26:24.809 --> 00:26:27.049
as standard by the end of the decade. At the moment,

444
00:26:27.130 --> 00:26:30.910
I'm already running models on my computer that they're slow.

445
00:26:30.950 --> 00:26:34.369
It's a little bit like seeing a 28.8K or 36K

446
00:26:34.450 --> 00:26:37.539
dial-up modem as opposed to the gigabit broadband speeds that

447
00:26:37.559 --> 00:26:38.710
we all take for granted today.

448
00:26:38.890 --> 00:26:43.700
That's Alex Haravroyd from techadvice.life. And this is Space Time.

449
00:26:59.269 --> 00:27:02.549
And that's the show for now. Space Time is available

450
00:27:02.630 --> 00:27:07.880
every Monday, Wednesday and Friday through bytes.com. SoundCloud, YouTube, your

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favorite podcast download provider, and from spacetimewithstuartgarry.com. Space Time's also

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broadcast through the National Science Foundation on Science Zone Radio

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and on both iHeart Radio and TuneIn Radio. And you

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can help to support our show by visiting the Space

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triple-episode commercial-free versions of the show, as well as lots

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of bonus audio content which doesn't go to air, access

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to our exclusive Facebook group, and other rewards. Just go

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to spacetimewithstuartgary.com for full details.

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You've been listening to Spacetime with Stuart Gary. This has

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