I Science in the News


Science in the News
http://edu-observatory.org/olli/SciNews/index.html


Mike Meetz and Sam Wormley team up to provide a lively
discussion with OLLI members about science in the news. A 
deep understanding of science is not required to share and
discuss recent Science in the News.  Past Classes.


⓵ Early humans in America endured climate chaos-new research
   https://phys.org/news/2026-10-early-humans-america-climate-chaos.html

   

   Some 23,000 years ago, during the coldest part of the last
   ice age, people walked across the muddy margins of an
   ancient lake in what is now White Sands National Park, New
   Mexico. The footprints they left behind have transformed our
   understanding of when people first reached the Americas When
   we reported dates for the White Sands footprints in 2021,
   our findings were met with controversy. They placed people
   in North America thousands of years earlier than other
   widely accepted sites.

   Subsequent work using several independent dating techniques
   strengthened that chronology. Our latest research takes the
   story a step further. Rather than simply asking when people
   were at White Sands, we can begin to ask: What sort of world
   did they experience? Our work is published in Science
   Advances and Fossil Studies.

   The answer is a surprisingly dynamic one that was marked by
   periods of rapid climate change. Our expanded excavations at
   White Sands have identified 20 different horizons or
   packages of sediment containing human footprints. Together
   they span almost two millennia, from about 23,500 to 21,700
   years ago, firmly within the last glacial maximum (the
   height of the last ice age).




⓶ Same Calories, Same Nutrients - but One Meal Triggered a 
   Surprising Reaction in the Body
   https://scitechdaily.com/same-calories-same-nutrients-but-one-meal-triggered-a-surprising-reaction-in-the-body/
   https://www.nature.com/articles/s42255-026-01619-4/figures/1

   Ultraprocessed foods supply more than half of the average
   American’s daily calories, and their place in diets
   worldwide is growing. Formulated to be convenient,
   accessible, affordable, and highly palatable, they can be
   easy to overeat. Understanding their effects on health,
   however, requires untangling the influence of processing
   from that of the nutrients they contain.

   Meals with the same basic nutritional profile are generally
   expected to affect blood sugar in similar ways. Yet in a
   Virginia Tech study, healthy adults expended more energy and
   burned less carbohydrate after eating an ultraprocessed meal
   than after a minimally processed one. Both meals contained
   300 calories and were closely matched for carbohydrates,
   fat, protein, water, salt, and weight. The findings appeared
   in Nature Metabolism.

   Related
   Healthy Food vs. Highly Processed Food: What to Know
   https://www.healthline.com/nutrition/junk-food-vs-healthy-food
   Mediterranean Diet (Science and Recipes)
   http://edu-observatory.org/olli/Mediterranean/index.html




⓷ Import AI 477: In which I tell the IMF the Singularity has begun
   https://importai.substack.com/p/import-ai-477-in-which-i-tell-the

   The singularity is here. The implications reach across every
   aspect of life. But the most important implication is a
   simple one: we should expect that in the coming years, the
   whole pace of progress of not just AI, but science as a
   whole, will speed up. This will feel confusing and
   disorienting, and it will bring with it great wealth and
   potentially great peril.

   Today, I'm going to concentrate on the first point: the
   potential benefits of rapid AI progress, and what we need to
   do to share in these benefits together.

   So many of the ways that humanity will benefit from Al come
   from science. I believe that Al-driven scientific invention
   will change the course of the global economy, alter the ways
   countries plan and build their own infrastructure, make us
   all healthier and able to spend more time with our loved
   ones, and - at the same time — cause us all to ask deep
   philosophical questions about choices we should make about
   its continued development.

   I'll develop my claim: For the last half century, most
   countries have dealt with falling research productivity
   while researcher headcount grows rapidly - ideas and
   inventions appear to be getting harder to find.

   But something important has changed: we've now built AI
   systems which have been able to augment, extend, and
   automate aspects of human labor. This has most obviously
   happened in software development, where Al systems are now
   more capable and efficient than the vast majority of the
   world's software engineers. As a consequence, the field of
   software development is changing - A single person is now
   able to write software for anything they can imagine,
   creating things that previously would have taken entire
   teams of humans.

        ————————————————————

   In artificial intelligence, the “singularity” (often called
   the technological singularity) refers to a hypothetical
   future point at which AI surpasses human intelligence and
   begins improving itself at an accelerating rate, triggering
   changes so rapid and profound that the world afterward
   becomes difficult or impossible for humans to predict or
   comprehend.

   The idea rests largely on the concept of an “intelligence
   explosion,” first described by mathematician I.J. Good in
   1965: a machine smart enough to design better machines could
   create successively more capable versions of itself, each
   iteration arriving faster than the last. The term was
   popularized by science fiction author and mathematician
   Vernor Vinge in the 1990s and later by futurist Ray
   Kurzweil, who predicted it would arrive around 2045.

   The word itself borrows from mathematics and physics, where
   a singularity is a point at which normal rules break down,
   like the center of a black hole. Views on it vary widely:
   some see it as an inevitable and potentially utopian turning
   point, others warn of serious risks if superintelligent
   systems don’t share human values, and skeptics argue that
   intelligence may not scale so neatly or that physical,
   economic, and practical limits would slow any such runaway
   growth.




⓸ Oxygen collisions show evidence of jet quenching, a signature 
   of early-universe matter
   https://phys.org/news/2026-10-oxygen-collisions-evidence-jet-quenching.html

   New results from the STAR experiment at the Relativistic
   Heavy lon Collider (RHIC) provide strong evidence that
   smashing oxygen nuclei together at nearly the speed of light
   generates a quark-gluon plasma (QGP), a type of matter that
   existed just after the birth of the universe. The data, just
   published in Physical Review Letters, show that energetic
   jets of particles lose energy as they traverse the hot,
   dense matter left in the collision's wake. This energy loss
   phenomenon, known as jet quenching, has been one of the
   "smoking gun" signatures of QGP formation in collisions of
   larger atomic nuclei at RHIC, a U.S. Department of Energy
   (DOE) Office of Science user facility that operated at DOE's
   Brookhaven National Laboratory from 2000 until earlier this
   year.

   This signature has also been observed in oxygen-oxygen
   collisions at the Large Hadron Collider (LHC), located at
   CERN, the European Particle Physics Laboratory. The analysis
   from RHIC at significantly lower collision energy sets a new
   lower boundary for the conditions capable of producing the
   primordial QGP in this small collision system. "The QGP is
   believed to be the form of matter that filled the early
   universe-before the protons and neutrons that make up
   today's atoms formed.

        ————————————————————

   Quark-gluon plasma is the state of matter that filled the
   universe for roughly the first few millionths of a second
   after the Big Bang, before quarks and gluons cooled enough
   to bind into protons and neutrons. Recreating it in
   heavy-ion colliders like RHIC and the LHC lets physicists
   look directly at that early epoch and test quantum
   chromodynamics, the theory of the strong force, in a regime
   where it is otherwise very hard to calculate. It also shows
   how confinement works, meaning why quarks are never seen
   alone and how most of the mass of ordinary matter arises
   from strong-force interactions rather than from the quarks
   themselves.

   The plasma has also surprised researchers by behaving like a
   nearly perfect liquid with extremely low viscosity rather
   than a dilute gas. That finding has links to other strongly
   interacting systems such as ultracold atomic gases, to the
   interiors of neutron stars, and, through holographic
   dualities, to string theory and black hole physics.
   



⓹ The sun may have stripped away meters of interstellar comet 3I/ATLAS
   https://phys.org/news/2026-10-sun-meters-interstellar-comet-3iatlas.html

   The interstellar comet 3I/ATLAS brought material from
   another planetary system within reach of our telescopes, but
   reading its chemistry poses a problem. Energetic particles
   encountered during its journey through space may have
   changed its outer layers, so how much of what astronomers
   detect still reflects the comet's birthplace? The sun may
   have helped reveal a clearer record. Using published
   measurements of escaping gas only, researchers estimate that
   solar heating removed the equivalent of a surface layer
   about 1.7-5.2 meters (5.6-17 feet) thick. Including
   plausible amounts of lost dust pushes some estimates beyond
   10 meters (33 feet).

   

   Here are the highlights:

   1. Discovery and identity: It was found on July 1, 2025, by
   the ATLAS survey telescope in Chile, making it the third
   confirmed interstellar object after ‘Oumuamua in 2017 and
   2I/Borisov in 2019. Unlike ‘Oumuamua, it was clearly an
   active comet from the start.

   2. Speed and age: It’s the fastest interstellar object ever
   recorded (roughly 58 km/s relative to the Sun). Its
   trajectory suggests it may come from the Milky Way’s older
   “thick disk,” possibly making it billions of years older
   than our solar system.

   3. Early appearance: VLT spectra taken two days after
   discovery showed a red, dust-dominated coma with no
   detectable gas, redder than most Solar System comets but
   similar to some trans-Neptunian objects and Centaurs.

   4. Unusual chemistry: JWST and others found an unusual
   prevalence of carbon dioxide over water, and a
   nickel-to-iron ratio differing from Solar System comets.
   Nickel vapor was detected with little or no iron, which was
   surprising.

   5. Perihelion behavior: It passed closest to the Sun in late
   October 2025, when it was hidden behind the Sun from Earth.
   Spacecraft such as Mars orbiters, PUNCH and Juice observed
   it. Its activity rose sharply after perihelion, with ices
   sublimating and releasing water, carbon dioxide and
   hydrocarbons. It also showed non-gravitational acceleration
   from outgassing and an unusual sunward “anti-tail.”

   6. Nucleus size: Hubble put an upper limit of a few
   kilometers on the nucleus. The bright coma made a precise
   measurement hard.

   7. Natural origin: Its quirks prompted some speculation
   about artificial origins, but NASA confirmed it is an
   interstellar comet and shared data from multiple missions
   supporting that conclusion.

   Overall, it gave scientists their best look so far at a
   comet from another star system. The data will also help
   prepare for future missions like ESA’s Comet Interceptor.
      	



⓺ NASA'S Roman Space Telescope Is Sharper Than Anyone Expected
   https://scitechdaily.com/nasas-roman-space-telescope-is-sharper-than-anyone-expected/

   NASA's Roman Space Telescope has achieved nearly 30% better
   optical performance than required, promising stunningly
   sharp views of the universe and its greatest mysteries.

   NASA's Nancy Grace Roman Space Telescope is performing even
   better than scientists anticipated after engineers completed
   an extensive series of tests and precision adjustments. The
   work has sharpened the observatory's focus and brought its
   primary instrument closer to regular scientific operations.
   Remarkably, the telescope's Wide Field Instrument is now
   delivering optical performance nearly 30% better than
   predicted. "All of Roman's sweeping surveys will rely on the
   Wide Field Instrument," said Dave Hickey, a Wide Field
   Instrument systems engineer at NASA's Goddard Space Flight
   Center in Greenbelt, Maryland. "Many of the mission's
   primary goals, like studying dark matter and dark energy,
   wouldn't be possible without it, so it's both exciting and a
   huge relief to see that it's working well"

        ————————————————————

   Extra Spy satellite turn into a state-of-the art
   astronomical telescope. NASA's Roman Space Telescope
   launched on August 30, 2026 and is now being commissioned,
   with first public images targeted for early 2027. Its main
   new capabilities:

   1. Huge field of view: At least 100 times larger than
   Hubble’s, potentially measuring light from a billion
   galaxies in its lifetime. It keeps Hubble-level sharpness
   while covering far more sky.

   2. Fast, wide infrared surveys: It can map in weeks or
   months what would take Hubble centuries. It is expected to
   send about 1 TB of data daily.

   3. Dark energy and dark matter: It is designed to explore
   dark energy and dark matter by charting how galaxies and
   cosmic structure grew over time, using weak lensing, galaxy
   clustering, and supernovae.

   4. Exoplanet hunting through microlensing: A survey of the
   Milky Way’s central bulge is expected to find thousands of
   planets. These include cold, distant worlds and “rogue”
   planets with no host star, which other methods largely miss.

   5. Coronagraph technology demo: It will test advanced
   starlight-blocking technology to directly image giant
   planets and dusty disks around nearby stars. This prepares
   the way for future missions searching for Earth-like
   planets.

   6. Mapping the galaxy: It will chart vast numbers of stars
   across the Milky Way and nearby galaxies.

   7. Open data for everyone: Beyond its own objectives, it
   will provide data to astronomers pursuing other goals.

   8. Location and lifespan: It will operate at the Sun–Earth
   L2 point near JWST. Its primary mission is five years, with
   a design that supports a five-year extension. The launch
   was so precise, saving propellant, that the mission could 
   remain fruitful for 22 years or so.





Related Material from some recent OLLI courses
  http://edu-observatory.org/olli/classes.html

Alan Lightman On Richard Feynman's Amazing Mind, Or How 
"Hawking Radiation" Could Well Be "Feynman Radiation" (6min)
  https://player.vimeo.com/video/104516539

   
   
   


  
    sam.wormley@icloud.com