Study Findings: Electrical Conductivities of (Mg,Fe)O at Extreme Pressures and Implications for Planetary Magma Oceans

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Image (Credit): Artist’s rendering of deep layers of molten rock inside a super-earth generating powerful magnetic fields. (University of Rochester Laboratory for Laser Energetics illustration / Michael Franchot)

Nature Astronomy abstract of study findings:

During planet formation, planets undergo many impacts that can generate magma oceans. When these crystallize, part of the magma densifies via iron enrichment and migrates to the core–mantle boundary, forming an iron-rich basal magma ocean (BMO). The BMO could generate a dynamo in early Earth and super-Earths if the electrical conductivity of the BMO, which is thought to be sensitive to its Fe content, is sufficiently high. To test this hypothesis, here we conduct laser-driven shock experiments on ferropericlase (Mgx,Fe1−x)O (0.95 ≤ x ≤ 1) as an Fe-rich BMO analogue, perform density functional theory molecular dynamics simulations on MgO and calculate the long-term evolution of super-Earths. We find that the d.c. conductivities of MgO and (Mg,Fe)O are indistinguishable between 467 GPa and 1,400 GPa, despite previous predictions. We predict that super-Earths larger than 3–6 Earth masses can produce BMO-driven dynamos that are almost one order of magnitude stronger than core-driven dynamos for several billion years.

Citation: Nakajima, M., Harter, S.K., Jasko, A.V. et al. Electrical conductivities of (Mg,Fe)O at extreme pressures and implications for planetary magma oceans. Nat Astron (2026).

https://doi.org/10.1038/s41550-025-02729-x

Study-related stories:

University of Rochester – “Hidden Magma Oceans Could Shield Rocky Exoplanets from Harmful Radiation”

Earth Sky – “Powerful Magnetic Fields on Super-Earths Could Boost Chances of Life”

Universe Today – “Deep Magma Oceans Could Help Make Super-Earths Habitable”

Video: Brian Cox Talks About Alien Life – A 2026 Special

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Image (Credit): Professor Brian Cox discussing the evolution of intelligence. (Science Time channel)

If you have followed the career of English physicist Brian Cox, then you know he is a dynamic speaker who has hosted several series on astronomy, including Wonders of the Solar System and Wonders of the Universe.

In this short video from Science Time channel, “Brian Cox Talks About Alien Life – A 2026 Special,” Professor Cox walks the viewer through the chances of finding intelligent life among the 60 billion exoplanets in our galaxy that lie within the habitable zone. To be clear, he is not very optimistic.

The series does not cover much new ground except for some hopeful comments about the James Webb Space Telescope investigating the atmospheres of exoplanet (with Professor Cox wondering whether we will find life on an exoplanet before we find it on Mars). Even so, it is still enjoyable to spend a little bit of time playing around with the Fermi Paradox again.

One of the more intriguing ideas being discussed here and elsewhere is the idea that we may not want to limit our ideas to biological life. The longevity of a civilization may be dependent on its ability to evolve from carbon-based to silicon-based lifeforms. While not explicitly discussed in the video, that could broaden our search beyond a star’s habitable zone yet also frustrate our attempts to find biological signatures in an exoplanet’s atmosphere.

Again, it is worth your time to listen in. I would just ignore the goofy animations that accompany the discussion.

Pandora and Friends Start New Missions

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Image (Credit): An artist’s rendering of NASA’s Pandora mission. (NASA)

Earlier today, NASA’s Pandora mission got its start aboard a SpaceX rocket launched from California’s Vandenberg Space Force Base.

The Pandora satellite, once fully operational, will view exoplanet atmospheres and their host stars to learn more about these exotic worlds. In its first year, the satellite will focus on approximately 20 known exoplanets. This NASA video describes the process.

The 716-pound Pandora satellite is much smaller than the 14,300-pound James Webb Space Telescope (JWST). Of course, the JWST has a much larger mission that expands over a much longer time period.

If you are looking for something small, you might be interested in the two CubeSats launched with Pandora. One is called the Star-Planet Activity Research CubeSat (SPARCS), which will study coronal mass ejections on small stars, while the second is named the Black Hole Coded Aperture Telescope (BlackCAT) with the mission of observing X-ray flares from active galaxies with supermassive black holes as well as gamma-ray bursts.

It was a successful Sunday for NASA and space enthusiasts everywhere.

Study Findings: A Carbon-rich Atmosphere on a Windy Pulsar Planet

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Image (Credit): Artist’s rendering of of an exoplanet orbiting a rapidly spinning neutron star called a pulsar. (NASA, ESA, CSA, Ralf Crawford (STScI))

Abstract of pre-publication study findings:

A handful of enigmatic Jupiter-mass objects have been discovered orbiting pulsars. One such object, PSR\,J2322-2650b, uniquely resembles a hot Jupiter exoplanet due to its minimum density of 1.8 g/cm^3 and its ~1900 K equilibrium temperature. We use JWST to observe PSR J2322-2650b’s emission spectrum across an entire orbit. In stark contrast to every known exoplanet orbiting a main-sequence star, we find an atmosphere rich in molecular carbon (C3, C2) with strong westward winds. Our observations open up new exoplanetary chemical (ultra-high C/O and C/N ratios of >100 and >10,000, respectively) and dynamical regimes (ultra-fast rotation with external irradiation) to observational study. The extreme carbon enrichment poses a severe challenge to the current understanding of “black widow” companions, which were expected to consist of a wider range of elements due to their origins as stripped stellar cores.

Citation: Michael Zhang et al. A carbon-rich atmosphere on a windy pulsar planet. ApJL (2025).

https://doi.org/10.48550/arXiv.2509.04558

Study-related stories:

University of Chicago – “NASA’s Webb Telescope Finds Bizarre Atmosphere on a Lemon-shaped Exoplanet”

Scientific American – “This Planet Is the Shape of a Lemon. That May Be the Least Weird Thing about It”

Space Daily – “Webb Maps Carbon Rich Atmosphere on Distorted Pulsar Planet”

Space Quote: British Satellite to Study Impact of Stars on Exoplanets

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Credit: Blue Skies Space

“Mauve will open a new window on stellar activity that has previously been largely hidden from view…By observing stars in ultraviolet light, wavelengths that can’t be studied from Earth, we’ll gain a much deeper understanding of how stars behave and how their flares may impact the environment of orbiting exoplanets. Traditional ground-based telescopes just can’t capture this information, so a satellite like Mauve is crucial for furthering our knowledge.”

–Statement by Professor Giovanna Tinetti, Chief Scientist and Co-founder of Blue Skies Space, regarding today’s launch of the Mauve cubesat satellite. This satellite contains a 13 cm telescope that will be used to observe hundreds of stars in the ultraviolet and visible wavelengths over a three-year period. Data from this mission will be sold via subscriptions, and used to study the stars and how their activity influences the habitability of distant exoplanets. You can find more information on the mission here.