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Salt may have helped turn Earth into a frozen world 700 million years ago

Earth may have been pushed deeper into a global deep freeze by something surprisingly ordinary: salt. Around 700 million years ago, Earth entered periods of extreme glaciation known as Snowball Earth, when ice is thought to have spread across much or potentially all of the planet’s surface. Scientists have long known that expanding ice could have helped drive this transition: As bright ice replaces darker ocean water, more sunlight is reflected back into space, causing the planet to cool further and allowing even more ice to form.

Now, Aksel Samuelsberg, from University of Tromsø—The Arctic University of Norway, and colleagues have identified another possible feedback that could have amplified this cooling: salt crystals accumulating on the surface of sea ice. Their modeling suggests that these crystals could have made the frozen surface even more reflective, helping temperatures fall rapidly during the early stages of a Snowball Earth event.

How the sun’s galactic journey and superflare-filled youth shaped Earth’s climate

At the center of our solar system, the sun influences every planet that orbits it. In two recent studies, scientists uncovered how ancient events in the sun’s history may have helped create Earth’s unique climate and driven previously unexplained climatic shifts.

In new research, scientists at NASA’s SHIELD (Solar Wind with Hydrogen Ion charge Exchange and Large-Scale Dynamics) center—one of NASA’s DRIVE (Diversify, Realize, Integrate, Venture, Educate) Science Centers—trace the trajectory of the heliosphere, the massive bubble created by our sun that envelops our solar system, as it moved through our galaxy and influenced Earth’s climate along the way. In another paper, a NASA scientist and co-authors investigate how the younger, dimmer sun managed to heat Earth by seeding the production of potent greenhouse gases.

Scientists Finally Solve a 20-Year Mystery About Diamond Melting

Direct measurements of diamond melting under extreme pressure resolved a long-standing theory-experiment mismatch and could improve both fusion research and planetary models.

Diamond is not only a gemstone. This exceptionally hard form of carbon is also used in the tiny capsules that surround fuel in inertial confinement fusion experiments, and researchers think carbon may form diamonds that fall through the interiors of ice giants such as Neptune and Uranus.

Both environments expose diamond to immense pressure, yet experiments and computer simulations have long produced conflicting descriptions of what happens to the material under such extreme conditions.

How Mercury formed its graphite crust and core

As the BepiColombo mission prepares to enter the final phase of its journey to Mercury, a series of studies conducted by researchers at the University of Liège and KU Leuven sheds new light on the early stages of the evolution of the planet closest to the sun. Using experimental petrology, the researchers are reconstructing in the laboratory the formation of Mercury’s core, the crystallization of its magma ocean and the formation of its mantle. The studies are published in Earth and Planetary Science Letters, Nature Communications and Advances in Geochemistry and Cosmochemistry.

The terrestrial planets (Mercury, Venus, Earth and Mars) are the result of more than four billion years of evolution, which began with accretion from the disk surrounding the young sun. During the early stages of evolution, the heat released caused these planets to melt, creating what is known as a magma ocean.

This key stage determines the distribution of elements between the metallic core and the mantle. As it crystallizes, this ocean structures the solid mantle, the partial melting of which will subsequently generate the magmas that form the crust. It is also at this stage that an initial atmosphere may form.

Japan Is Launching a Probe to Collect the FirstEver Samples From a Martian Moon

Once on the surface, a robotic arm will drill cylindrical tubes into the surface to collect samples. The probe is also equipped with a device first developed by NASA that uses a stream of nitrogen gas to collect fine particles from the very top layer of dust. Whether or not Phobos originated from an impact with the planet, experts believe Martian sand can be obtained from the lunar surface. Over time, meteorite impacts have blasted materials off Mars, coating its moons. Scientists expect about 0.1 percent of the samples collected will be debris from Mars itself.

Costing about $345 million US, this mission marks Japan’s first Mars probe launch in 28 years. Beyond the scientific insights it’s expected to provide, from an engineering perspective, the mission aims to test new technologies that could aid future sampling and round-trip travel to Mars.

MMX is scheduled to launch from the Tanegashima Space Center on October 20, 2026.

Mars Curiosity rover discovers massive field of polygons

The surface of Mars is home to some of the most breathtaking and awe-inspiring landscapes in the solar system. This is primarily because the Red Planet lacks several resurfacing processes that Earth possesses, including plate tectonics, volcanism and flowing water.

While Mars does have dust storms, these have done little to reshape the planet’s surface, which has remained largely undisturbed for billions of years. However, this near-pristine landscape has enabled scientists to look back in time while slowly piecing together what Mars was like long ago.

Now, NASA’s Mars Curiosity rover recently beamed back images of a landscape featuring polygon-like features. This unique landscape has been observed in other regions of Mars but was a first-time observation for the car-sized rover.

AI suggests new physics experiments that could outperform human-designed setups

Research means asking questions of the universe. For centuries, clever minds have advanced science by devising ingenious experiments designed so their results reveal something about the laws of nature as clearly and unambiguously as possible.

An international research team has now asked: Can this process be automated? Can artificial intelligence develop new ideas for experiments? The answer is a clear yes. In various areas of physics, AI can propose experiments that enable more precise results than experiments designed by humans.

In the journal Nature, the team presented the current state of this new approach to research.

Physicists test the weak equivalence principle in an orbiting space station

The weak equivalence principle (WEP) is central to Einstein’s general relativity. It posits that gravity must accelerate everything equally, regardless of what it is made from. For the first time, a team led by Ming-Sheng Zhan at the Wuhan Institute of Physics and Mathematics has tested the principle using clouds of continuously free-falling atoms aboard an orbiting space station.

Their research has been published in Science Advances.

PACMAN AI framework for controlling fusion systems safely makes key decisions in milliseconds

Inside some fusion energy systems, particles hotter than the core of the sun can become unruly in a few thousandths of a second, far faster than any human operator can react. A new software framework developed by researchers at the U.S. Department of Energy’s (DOE) Princeton Plasma Physics Laboratory (PPPL) and Princeton University hands those split-second decisions to artificial intelligence (AI), while keeping the machine safe and humans firmly in charge of the goals.

Known as PACMAN (a novel abbreviation for Prediction And Control using MAchiNe learning), the AI framework was successfully tested on a real fusion system in five experiments. The framework’s design and first results are detailed in a new paper in the journal Nuclear Fusion.

Fusion could one day serve as a virtually unlimited source of electricity. Scientists are working on several ways to perfect the process here on Earth, including devices called tokamaks, which use powerful magnetic fields to hold a plasma: an electrically charged gas often called the fourth state of matter. Keeping the plasma hot, dense and stable requires constant adjustments to the tokamak, including its heating systems, magnets and gas injectors. The fusion reaction can be thwarted by small disturbances in the plasma, known as instabilities, that grow in milliseconds.

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