Inside the cores of ice giant planets, the pressure and temperature are so extreme that the water residing there transitions into a phase completely unfamiliar under the normal conditions of Earth. Known as “superionic water”, this form of water is a type of ice. However, unlike regular ice it’s actually hot, and also black. For decades, scientists thought that the superionic water in the core of Neptune and Uranus is responsible for the wild, unaligned magnetic fields that the Voyager 2 spacecraft saw when passing them. A series of experiments described in a paper published in Nature Communications by Leon Andriambariarijaona and his co-authors at the SLAC National Accelerator Laboratory and the Sorbonne provides experimental evidence of why exactly the ice causes these weird magnetic fields - because it is far messier than anyone expected.
As 2026 dawns, look for HHS Secretary Robert F. Kennedy Jr. to ramp up his assault on vaccines using policy-based evidence making and altering Vaccine Court standards.
The post RFK Jr. is definitely coming for your vaccines (part 6): Liability, ethics, and policy-based evidence making first appeared on Science-Based Medicine.Here we have an 83-minute interview of Matthew Crick by Michael Shermer; the topic is Francis Crick as described in Matthew’s new book Crick: A Mind in Motion. Talking to a friend last night, I realized that the two best biographies of scientists I’ve read are Matthew’s book and Janet Browne’s magisterial two-volume biography of Darwin (the two-book set is a must-read, and I recommend both, though Princeton will issue in June a one-volume condensation).
At any rate, if you want to get an 83-minute summary of Matthew’s book, or see if you want to read the book, as you should, have a listen to Matthew’s exposition at the link below. I have recommended his and Browne’s books because they’re not only comprehensive, but eminently readable, and you can get a sense of Matthew’s eloquence by his off-the-cuff discussion with Shermer.
Click below to listen.
I’ve put the cover below because Shermer mentions it at the outset of the discussion:
I now have two sets of photos after this one, but I’m still nervous. If you have good wildlife photos, please sent them in. Thanks!
It’s been a cold week in Chicago (right now it’s 9°F or -13°C), and it’s going to be cold this coming week as well. I hope the turtles at the bottom of Botany Pond are okay. But given the weather it’s appropriate that today we have photographs of Antarctica from reader Paul Turpin. Paul’s captions are indented, and you can enlarge the photos by clicking on them.
My brother Mark recently returned from a cruise to the Antarctic on the Scenic Eclipse. I told him you loved penguins and he gave me permission to send you these photos. I believe these are all gentoo penguins [Pygoscelis papua] except for one which included a chinstrap friend [Pygoscelis antarcticus]. The open water photo is when they were at the Antarctic Circle.
A new census of more than 8,000 galaxies finds active black holes rising in frequency with galaxy mass, jumping sharply in galaxies similar in mass to the Milky Way.
Our nearest neighbor, the Moon, is still something of a mystery to us. For decades, scientists have wondered why it appears so lopsided, with dark volcanic plains on the near side (the side we see) and rugged, cratered mountains and a thicker crust on the far side. Now we might be closer to knowing why.
Physicists at the University of Oxford have contributed to a new study which has found that iron-rich asteroids can tolerate far more energy than previously thought without breaking apart - a breakthrough with direct implications for planetary defence strategies.
This collection of new images taken by NASA’s Hubble Space Telescope showcases protoplanetary disks, the swirling masses of gas and dust that surround forming stars, in both visible and infrared wavelengths. Through observations of young stellar objects like these, Hubble helps scientists better understand how stars form. These visible-light images depict dark, planet-forming dust disks […]
Chemistry on other worlds varies widely from that on Earth. Much of Earth’s chemistry is driven by well-understood processes, which typically involve water and heat in some form. Mars lacks both of those features, which makes how some of its chemicals formed a point of ongoing debate in the scientific community. A new paper led by Alian Wang and Neil Sturchio of Washington University of St. Louis and the University of Delaware, respectively, and published recently in Earth and Planetary Science Letters offers a new framework for understanding chemical reaction processes on Mars. Despite the differences, Earthlings will still be familiar with the driving force behind Martian chemistry - electricity.