July 8, 2026

How a Passing Star Redirected Comets and Redefined Our Milky Way Map

How a Passing Star Redirected Comets and Redefined Our Milky Way Map

Sponsor Link: This episode of SpaceTime is brought to you by Inconi. Take back your privacy and data online with Incogni. Check out our special offer: https://www.incogni.com/stuartgary SpaceTime Series 29 Episode 81How a passing star redirected...

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This episode of SpaceTime is brought to you by Inconi. Take back your privacy and data online with Incogni. Check out our special offer: www.incogni.com/stuartgary

SpaceTime Series 29 Episode 81How a passing star redirected comets to the inner solar systemA fascinating new study reveals how a passing star, HD 7977, may have altered the trajectory of comets from the Oort Cloud, sending them cascading into the inner solar system. This event, which occurred approximately 2.47 billion years ago, could still be influencing comet activity today. Researchers used data from the European Space Agency's Gaia mission to refine the distances involved and suggest that the gravitational perturbations from HD 7977 temporarily dominated the generation of new comets.Changing our map of the Milky Way GalaxyAstronomers have redrawn the map of our Milky Way galaxy, moving its outer arms up to 10% further away than previously estimated. This revised picture is based on observations of gamma-ray bursts and the subsequent echoes of X-rays that helped to measure distances within the galaxy. New techniques have allowed for a clearer understanding of the Milky Way's structure, confirming the existence of its four spiral arms.Evidence of vast hidden magma systems inside MarsNew findings suggest that Mars once hosted extensive magmatic systems beneath its surface, despite the absence of plate tectonics. Data from NASA's InSight mission has revealed a previously unidentified boundary layer deep within the Martian crust, indicating complex geological processes that may have allowed the Red Planet to develop a habitable environment. This challenges long-held assumptions about the geological capabilities of rocky planets without tectonic activity.The Science RobertA new study indicates that the mental health of high school peers can significantly affect individual mental health outcomes. Additionally, research finds no link between paracetamol use during pregnancy and the risk of autism or ADHD. A detailed analysis of a fossilised pterosaur wing reveals insights into its diet, while scientists discover new methods to control quantum light sources, bringing us closer to practical quantum technologies.1. How a passing star redirected comets to the inner solar system 2. Changing our map of the Milky Way Galaxy 3. Evidence of vast hidden magma systems inside Mars 4. The Science RobertIf you’d like to support the podcast and gain access to bonus content by becoming a SpaceTime crew member, you can do just that through The Big Bang editions on Patreon, Spotify, and Apple Podcasts. Details on the Support page on our website https://www.bitesz.com/show/spacetime/support/

The Astronomy, Space, Technology & Science News Podcast.

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Stuart Gary: This is space Time Series 29, episode

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81, for broadcast on the 8th of July,

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2026. Coming up on Space,

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how a passing star redirected comets to the

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inner solar system, a, uh, change in our map

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of the Milky Way galaxy, and evidence of

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vast hidden magma systems inside Mars.

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All that and more coming up on, uh, uh, Space

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Time. Welcome to Space

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Time with Stuart G.

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A new study has shown how a passing star

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redirected a stream of comets from the

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distant Oort Cloud to the inner solar system.

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Consequently, closer to Earth. And the

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cascade may not be over yet. The

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Oort Cloud is a collection of comets, frozen

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worlds and icy debris orbiting in the dark

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outer reaches of our solar system and

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extending more than a light year deep into

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interstellar space. The clouds, thought to

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include leftover objects from the formation

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of Our solar system 4.6 billion years ago, as

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well as interstellar objects that are tagging

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along after being captured by the Sun's

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gravitational field. About

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2.47 billion years ago, a spectral

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type G yellow dwarf star similar to and about

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1.07 times the mass of our sun, which is

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catalogued as HD7977,

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passed close to our solar system. But

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exactly how close is still a bit of a

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mystery. Today, HD

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7977 is located in the constellation

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Cassiopeia, about 246.9

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light years away. But during its close

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encounter with our solar system, calculations

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based on observations by the Gaia spacecraft

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suggest that it may have passed within the

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Oort Cloud, coming to within

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0.064 and

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0.4 light years from the Sun.

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Now, by comparison, the nearest star to us

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today is Proxima Centauri, which is 4.25

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light years away, which makes it eight or

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more times further than this closest

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approach. Now, uh, this new study by Nathan

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Cabe from the Planetary Science Institute and

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Sean Raymond from the University of Bordeaux,

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have further refined those distances,

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suggesting that HD7977's close

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encounter with our solar system could have

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been as near as 0.095 to

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0.185 light years from the Sun.

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Ah, at its nearest, that means it was just

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6,000 times further away from the sun than

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what the Earth is. Their research, which has

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been presented at the American Astronomical

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Society Division of Dynamical Astronomy,

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suggests that the gravitational perturbations

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triggered by such an encounter would have

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altered the orbits of some of the Oort Cloud

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objects, sending them cascading into the

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inner solar system. In other words, where the

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Earth is and they believe that we may still

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be feeling the effects of that passage today.

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The European Space Agency's Gaia mission was

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a, UH, telescope that precisely measured the

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changing positions and brightnesses of

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thousands of stars and other objects in our

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galaxy relative to background quasars and

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galaxies. Its combination of a

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spectrograph to measure motions towards and

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away from us and its high resolution cameras

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to measure proper motion across the sky has

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allowed three dimensional motions to be

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calculated for roughly 1% of the objects in

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ah, our galaxy, including the star HD

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7977. It allowed

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astronomers to understand the history of our

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solar system in new ways.

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Normally, the gravity of the galaxy's outer

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disc is the primary force causing icy objects

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in our solar system to change their orbits.

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This pull spreads out what was once a

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disc of material into what researchers

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calculate is currently a spherical shell of

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objects. This shell, the Oort Cloud, is

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named after its discoverer Jan Oort. And this

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same galactic tug should also dominate the

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orbits of new comets entering our solar

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system for the first time. And once it enters

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the solar system, the effects of the planets

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and its passage near the sun can radically

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change a comet's orbit. And these forces

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should leave a distinct signature in the

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direction that a comet orbits relative to our

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Milky Way's midplane. Now, uh, if

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HD7977 passed as near as Kabe

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and Rayman propose, its gravitational

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influence would temporarily dwarf that of the

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galaxy and the galactic signature should be

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absent from current comet orbits. And

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that's exactly what Cape and Raymond found

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when they analysed the orbits of several new

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comets. Cabe says the distribution of comet

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orbits suggests that we're living through an

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unusual time where HD7977

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has dominated the generation of new comets

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and not the larger gravitational field of the

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Milky Way as it usually would. This would

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also mean that we're living through the late

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stages of a pretty rare, powerful cometary

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shower. To test this

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idea, Cabe and Raymond ran a series of

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computer simulations to understand what

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comets would look like as a result of

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HD7977 passing at different distances.

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The computer models were then compared to the

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passage of 112 long period comets that have

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been observed since 1989, when professional

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surveys first made it possible to detect new

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comets in both hemispheres. By the way, long

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period comets are identified because they

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have highly elliptical orbits that typically

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take thousands to millions of years to

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complete. Brand new comets on their first

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passage to the inner solar system have

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orbital periods measured in millions of

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years, while older comets on Subsequent

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visits have much shorter periods due to their

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prior interactions with the planets and the

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Sun. The authors found the observed

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orbits of comets on their first passage into

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our solar systems. Inner regions matched

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HD7977, triggering a wave of long

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period comets to enter our solar system. All

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the comets on repeated passages are

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consistent with the galactic disc, pulling

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and clustering, creating their orbits. The

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authors say their predictions will be tested

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in the next six to 12 months. That's when the

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next data drop from Gaia is released.

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This is space time still to come.

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Changing our map of the Milky Way Galaxy and

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evidence of vast hidden magma systems deep

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below the surface of the Red Planet Mars.

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All that and more still to come on

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spacetime.

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Astronomers have redrawn our map of the Milky

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Way galaxy, moving its outer arms up to 10%

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further away than previous estimates. The

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revised picture is based on new data, uh,

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from both NASA's Chandra and the European

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Space Agency's XMM Newton X ray space

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telescopes. They were observing the aftermath

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of three bright explosions thrown out by

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three separate gamma ray bursts echoing

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through the outer spiral of the Milky Way

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galaxy. By measuring the distance to these

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echoes, astronomers were able to refine the

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distance to the outer arms. The thing

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is, we really don't know much about the

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structure of our galaxy's outer regions.

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That's because it's like looking at the

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forest through the trees. It's difficult to

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observe our galaxy from the inside. The

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solar system is well embedded inside its

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disc, preventing a bird's eye view. And as

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well as that, many regions are obscured by

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thick clouds of cosmic dust. But by

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using data from ESA's Gaia space telescope,

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it's allowed astronomers to gain a better

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perspective for mapping the Milky Way and

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doing so in more detail than ever before by

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measuring more precise distances to its

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stars. Before Gaia, astronomers weren't even

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sure if our galaxy had two or four spiral

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arms. We now know there are four.

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Beatriz Vallia from Italy's National

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Institute of Astrophysics says now another of

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ESA's missions has found a new way to map the

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extremities of our galaxy. Faias, uh, says

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astronomers usually model the Milky Way's

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outer arms indirectly based on what we know

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about how our galaxy rotates. But doing

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this leaves room for error. So instead,

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she looked at the aftermath of three cosmic

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explosions that took place far away in more

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distant galaxies. These explosions

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flung out X rays that echoed through several

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of the Milky Way's outer arms. And she

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measured the distances to these echoes

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directly. The X rays bounced around and

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were scattered by dust grains within the

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Milky Way spiral arms, forming bright rings

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that were then picked up by the xmm, Newton

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and Chandra space telescopes. By studying

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how these ring shaped echoes slowly expanded

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over time, Vaire and colleagues were able to

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pinpoint the distance to the scattering dust

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grains. As these grains lie within

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clouds within the arms of the galaxy, the

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authors were able to directly measure the

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distance to those arms. Besides

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confirming the known distance of the Perseus

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Arm, the authors also found that two of the

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Milky Way Galaxy's arms, the Artus Scutum

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Centaurus Arm and the Outer arm, are located

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up to 10% further away than

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previously thought. This is

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space time. Still to come. Evidence

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of vast hidden magma systems inside the Red

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planet Mars. And later in the Science

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report, a new study finds that your

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mental health might m well be impacted by the

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mental health of the people you went to

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school with. All that and more still to come

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on, uh, space time.

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A new study has uncovered that the Red planet

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Mars once hosted enormous Earth like

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magmatic systems deep beneath its surface.

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That's despite the planet lacking any plate

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tectonics, which was long thought necessary

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for this kind of geological complexity. The

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findings, reported in the journal Nature

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Astronomy, reveal fascinating new

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possibilities for how rocky planets could

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become habitable. Mars is often

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described as a stagnant lid planet.

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Unlike the Earth, its surface is not broken

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up into moving tectonic plates. Because

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plate tectonics drives volcanism, recycling

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and continent building on Earth, many

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scientists assumed Mars m lacked the

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conditions needed to produce similarly

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complex crust. However, this new study

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challenges that view, suggesting that Mars

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could have produced highly evolved crust

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through intense internal recycling. The

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findings are based on Data recorded by NASA's

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2018 InSight Lander Mission to the surface of

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the Red Planet. Insight investigated

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seismic waves from meteorite impacts and

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massquakes, the Martian equivalent of

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earthquakes. The authors used that data to

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investigate a mysterious boundary layer about

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24 kilometres beneath the Martian surface.

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Uh, now previous studies had identified this

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boundary, but no one knew what it really

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represented. To test the idea that

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this boundary may have marked a transition

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between two different rock types, the authors

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compared hundreds of possible rock

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compositions with the seismic data. Using

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thermodynamic modelling and statistical

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techniques, they found that while rocks above

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the 24 kilometre boundary appear to be MAFIC,

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that is they contained high proportions of

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silica. Rocks below the boundary seemed to be

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ultramafic, which means they're rich in iron

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and magma, but low in silica. The authors

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suggest this buried layer would have formed

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where molten rock pulled deep underground.

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And gradually separated into two distinct

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materials. This would leave behind a thick

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residue of dense crystals at the base of the

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crust, while lighter, uh, more evolved melts

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rose upwards. On Earth, similar

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processes occur beneath volcanic arcs and are

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linked to the formation of the continents.

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The study's lead author, Tobermori Mackie

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Champion from Oxford University says

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scientists have traditionally assumed that

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volcanism on Mars was relatively simple

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compared to that on the Earth. But this new

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discovery suggests Mars could sustain large

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long lived systems where molten rock evolved

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and reprocessed itself throughout the entire

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crust. The studies suggest that this layer,

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uh, may extend sideways for hundreds, even

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thousands of kilometres around the northern

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Martian hemisphere, indicating that the Red

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Planet once hosted enormous interconnected

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magmatic systems rather than simple isolated

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volcanoes. This phenomenon, known as

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transcrustal magmatism, was previously

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thought to be unique to Earth. These

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geological processes are closely linked to

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how planets develop atmospheres, oceans and

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potentially habitable environments. For

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instance, here on Earth, geological recycling

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helps regulate climate and supports long term

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cycling of water and other volatile elements.

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Scientists have often assumed um, plate

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tectonics were essential for creating these

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conditions. But the new findings suggest

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planets may not need Earth, uh, style

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tectonics to build complex crusts or sustain

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the conditions that support life.

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One of the big questions in science has

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always been whether planet Earth is unique.

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If Mars could develop this kind of complex

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crust without plate tectonics, then maybe the

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conditions needed for habitability could have

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emerged on more planets than just Earth, uh,

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including those previously dismissed based on

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their size or their apparent lack of tectonic

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activity. It's all just another part of the

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amazing treasure trove of Data coming from

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NASA's InSight mission on the Elysium

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Planitia region of the Red Planet.

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This report on INSIGHT from NASA tv

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Touchdown confirmed. INSIGHT is on. The

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surface of

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Bruce Bannert: INSIGHT has been fantastically successful.

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We've gotten more science than we had ever

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dreamed that we would get. During the course

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of the this mission. InSight's primary goal

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was to better understand how the

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terrestrial planets, the rocky planets, uh,

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formed and evolved.

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Mark Panning: First we landed an incredibly sensitive

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seismometer on the surface of Mars. And with

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that we were able to record over 1300

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marsquakes.

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Bruce Bannert: And these range all the way from tiny little

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templars that just barely go over the noise

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background to a handful of quakes that

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were larger than magnitude

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Kathy Ezamora Garcia: and feeling those vibrations. The scientists

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can actually take that information and use

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that to reconstruct all the material

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that those Mars quakes travelled through and

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thereby see the interior of the planet.

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Mark Panning: We looked at its core which is Big and

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not very dense. We looked at its mantle,

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which is not so hot, and we looked at its

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crust, which is not too

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thick and not too dense compared to some of

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our preferences.

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Bruce Bannert: By measuring the detailed

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structure of the inside of Mars, it gives us

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a snapshot of what the planet looked like

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four and a half billion years ago. The other

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thing that we've been able to do is make a

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very detailed record of the weather at

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Mars. We have a really good weather

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station which has allowed meteorologists to

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study the weather at the Insight landing site

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and relate that to the climate changes on

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Mars.

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Mark Panning: What we didn't do, unfortunately, was make

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the heat flow measurement we wanted to make.

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Our heat flow probe was supposed to get three

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to five metres down and we were

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unable to reach that depth.

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Kathy Ezamora Garcia: But we were able to get some of those

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measurements, such as the heat transfer

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amongst the soil.

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Mark Panning: Uh, it's left a permanent mark on me. I

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literally tattooed Insight onto my arm. I'll

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never let it go.

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Bruce Bannert: We've really rewritten sort of the

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chapter of the encyclopaedia on the interior

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of Mars. That was our last big

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hole in our understanding of the planet.

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Mark Panning: There's a lot of data that people are going

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to be looking at for decades to come.

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Kathy Ezamora Garcia: We accomplished so many of our science goals

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and we're going to have something to look

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back on and be proud.

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Stuart Gary: And, uh, in that report from NASA tv, we

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heard from INSIGHT Principal Investigator

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Bruce Bannert, Insight Project Scientist Mark

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Panning and INSIGHT Deputy Project Manager

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Kathy Ezamora Garcia.

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Uh, this is space, time.

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And time out of tech. Another brief look at

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some of the other storeys making news in

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Science this week with the Science Report. A

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new study in Finland has shown that the

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mental health of your high school mates may

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impact your own mental health. Uh, the

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findings reported in the Journal of the

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American Medical association indicate that

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people who had high school peers with a

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genetic predisposition for mental health

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disorders or a diagnosis of a mental health

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disorder were also at an increased risk of

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being diagnosed with a mental health disorder

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themselves. The authors say having peers with

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diagnosed depression or anxiety may make

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teens more aware of symptoms, reduce stigma

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and encourage them to seek treatment.

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A large new study of over 120,000

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kids has found no link between

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paracetamol use during pregnancy and the risk

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of autism or adhd. The, uh, study

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published in the Journal of the American

399
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Medical association, compared pairs of

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siblings to try and remove genetics and

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family environment from the equation. Because

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both HDAD and autism have a strong

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inherited component, the authors found no

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link between paracetamol use in pregnancy and

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increased risk of either autism or ADHD

406
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related Regardless of the timing pattern or

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dose of paracetamol use,

408
00:17:25.750 --> 00:17:28.550
a detailed study of a fossilised 113

409
00:17:28.550 --> 00:17:30.670
million year old pterosaur wing has found it

410
00:17:30.670 --> 00:17:32.870
was so well preserved in three dimensions

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that it even retained chemical traces hinting

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at its diet. The findings reported in the

413
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journal Eye Science, suggest the ancient

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flying reptile, which lived during the age of

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dinosaurs, had a diet rich in fish and squid.

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The authors were able to make that

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determination thanks to traces of steroids

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preserved in the remains, an unusual mix of

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special bacteria and a unique ancient marine

420
00:17:54.840 --> 00:17:56.800
environment, preserving not just the

421
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structure but even the subtle chemical traces

422
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of the animal's biology. The discovery

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highlights the growing potential for

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molecular palaeontology to unlock secrets

425
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from deep time.

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Scientists have found a new way to control

427
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quantum light sources, which is one of the

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key elements needed before quantum

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technologies can be used reliably in the real

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world world. The research reported in the

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journal Science Advances brings scientists a

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step closer to being used in practical

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quantum computing, secure communications and

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ultra high resolution sensing. The authors

435
00:18:30.020 --> 00:18:32.300
from the University of Technology Sydney say

436
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they were able to significantly shift the

437
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colour and wavelength of the light emitted.

438
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Unlike, um, many experiments where a device

439
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is made at one twist angle and left alone,

440
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the authors were able to pick up twist and

441
00:18:42.580 --> 00:18:45.340
restack hexagonal boron nitrate repeatedly

442
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and use that twist to modify the emitters,

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which you can't do with traditional materials

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like diamond or silicon carbide. These

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materials could eventually be used for

446
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applications such as healthcare cyber

447
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security and improved GPS and give more

448
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control over the building blocks needed to

449
00:19:01.030 --> 00:19:01.550
get there.

450
00:19:02.990 --> 00:19:04.950
Beta testers are uh, continuing to play

451
00:19:04.950 --> 00:19:07.430
around with Apple's new Siri AI ahead of this

452
00:19:07.430 --> 00:19:10.030
month's public beta launch. Among those

453
00:19:10.030 --> 00:19:11.990
testing the new Google Gemini based

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artificial intelligence is technology editor

455
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Alex Zaharov Vroith From Tech Advice Start

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00:19:16.790 --> 00:19:17.150
Life

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Jonathan Nally: at the worldwide Developer conference, Apple

458
00:19:19.770 --> 00:19:22.610
announced its long awaited upgrade to Siri.

459
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So it's now called Siri AI and although it's

460
00:19:25.050 --> 00:19:27.970
using the Gemini brains from Google,

461
00:19:27.970 --> 00:19:30.490
it's not just a uh, plugin. Apple's been

462
00:19:30.490 --> 00:19:32.810
training its own models with Google's models

463
00:19:32.810 --> 00:19:35.130
and they have a lot of where they can on

464
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device work and the private cloud compute

465
00:19:37.930 --> 00:19:39.970
work to make sure that your queries and as

466
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much of your activity remains as private as

467
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possible. And this has given Apple

468
00:19:45.370 --> 00:19:47.410
the AI the ability to have natural

469
00:19:47.410 --> 00:19:49.090
conversations, the same sort of things we see

470
00:19:49.090 --> 00:19:51.510
with Gemini and ChatGPT. You can now edit

471
00:19:51.510 --> 00:19:54.150
photos in a much more performant way, it can

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00:19:54.310 --> 00:19:56.950
rewrite things more effectively, it has real

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world knowledge. And look, at the moment it's

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only available to beta testers and we just

475
00:20:01.310 --> 00:20:03.710
have the first and second developer betas.

476
00:20:03.710 --> 00:20:05.870
There will be a, uh, public beta sometime in

477
00:20:05.870 --> 00:20:07.710
July and the whole thing will be ready for

478
00:20:07.710 --> 00:20:10.310
the public in September when the new iPhones

479
00:20:10.310 --> 00:20:12.870
also launch. So unless you are a real tech

480
00:20:12.870 --> 00:20:14.910
head and you've got spare iPhones, I wouldn't

481
00:20:14.910 --> 00:20:17.830
be updating your primary device to these beta

482
00:20:17.830 --> 00:20:19.310
versions. Even when the public beta comes

483
00:20:19.310 --> 00:20:21.610
out, it's always a bit of a gamble as to

484
00:20:21.610 --> 00:20:24.570
whether you should because the um, beta

485
00:20:24.570 --> 00:20:26.610
version can have bugs. Now people have said

486
00:20:26.610 --> 00:20:28.370
these latest betas are very smooth, but you

487
00:20:28.370 --> 00:20:31.170
go to Reddit and you read the iOS beta forum

488
00:20:31.250 --> 00:20:34.250
and you know the litany of beta problems

489
00:20:34.250 --> 00:20:36.450
that people have every year when this happens

490
00:20:36.450 --> 00:20:38.650
are there for all to see. So not recommended

491
00:20:38.650 --> 00:20:40.830
for the general public. But, uh, all the, uh,

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00:20:40.830 --> 00:20:42.770
app developers and you know, people with

493
00:20:42.770 --> 00:20:44.690
spare iPhones that love tinkering, they're

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well into it.

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00:20:45.370 --> 00:20:47.450
Stuart Gary: That's Alex Zaharov Vroit from TechAdvice

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Start Life. And this is Space Time.

497
00:21:05.490 --> 00:21:08.330
And that's the show for now. Space Time

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00:21:08.330 --> 00:21:10.450
is available every Monday, Wednesday and

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00:21:10.450 --> 00:21:13.250
Friday through bytes.com, soundcloud,

500
00:21:13.330 --> 00:21:15.730
YouTube, your favourite podcast download

501
00:21:15.730 --> 00:21:16.930
provider, and from

502
00:21:16.930 --> 00:21:19.010
spacetimewithstuartgarry.com

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00:21:19.750 --> 00:21:21.590
Space Time's also broadcast through the

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00:21:21.590 --> 00:21:23.830
National Science foundation on Science Zone

505
00:21:23.830 --> 00:21:26.830
Radio and on both iHeartradio and TuneIn

506
00:21:26.830 --> 00:21:29.470
radio. And you can help to support our show

507
00:21:29.470 --> 00:21:32.110
by visiting the Space Store for a range of

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promotional merchandising goodies, or by

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00:21:39.110 --> 00:21:41.150
versions of the show, as well as lots of

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bonus audio content which doesn't go to air,

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access to our exclusive Facebook group and

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other rewards. Just go to

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spacetimewithstuartgarry.com for full

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details. You've been listening to Space Time

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with Stuart Gary. This has been another

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quality podcast production from bytes.com.