Monday, April 20, 2026

Behold, the Solar System in All its X-ray Glory

Reconstruction of how the diffuse X-ray sky should have appeared to eROSITA from May to October 2021. Credit: K. Dennerl, et al. (2026)/the eSASS team (MPE)/E. Churazov & M. Gilfanov (IKI)

Using the eROSITA space telescope, MPE researchers have successfully isolated the X-ray glow from our Solar System, revealing its impact on the soft X-ray sky. The findings, published in Science, underscore the importance of considering Solar System processes when analyzing X-ray data and highlight eROSITA’s role in advancing not only astrophysics but also heliophysics.



Exoplanets Without Lots of Water Can't Maintain Their Carbon Cycles

This image shows Venus on the left and three possible atmospheres on a recently discovered exoplanet, Gliese 12b. Arid planets like Gliese 12b, even ones in habitable zones, may not have enough liquid water for habitability. Water plays an important role in Earth's carbonate-silicate cycle, which is responsible for moderating the planet's temperature. But rainfall is a critical part of the cycle, and arid planets with low water abundances may not be able to resist a greenhouse climate state. This may have been what happened with Venus. Image Credit: NASA/JPL-Caltech/R. Hurt (Caltech-IPAC)

Water is critical to life because cells need liquid to function. That's why scientists focus on finding and studying exoplanets in habitable zones. But even if they're in habitable zones, exoplanets need lots of water to support their carbon cycles. So without water, exoplanets become inhospitable greenhouse planets, regardless if they're in habitable zones or not.



NASA’s SPHEREx Telescope Just Mapped the Cosmic Ices That Will Someday Build Planets

Cygnus X-1 binary star system, as captured by the MOSAIC camera. Credit - T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)

New missions mean new capabilities - and one particularly interesting new mission is finally up and running. Data is starting to come in from SPHEREx, the medium-class surveyor that is mapping the entire sky every six months. A paper based on some of that early data was recently published in The Astrophysical Journal, mapping ice and compounds called Polycyclic Aromatic Hydrocarbons (PAHs) throughout some interesting regions of our Milky Way.



Sunday, April 19, 2026

The Vera C. Rubin Observatory has Discovered 11,000 New Asteroids, and It's Barely Even Started!

A model of the inner Solar System showing the asteroids discovered by Rubin in light teal. Known asteroids are dark blue. Credit: NSF–DOE Vera C. Rubin Observatory/NSF NOIRLab/SLAC/AURA/R/NASA/Goddard/ESA/Gaia/DPAC

Rubin’s largest asteroid haul yet, gathered before the Legacy Survey of Space and Time even begins, is just the “tip of the iceberg”



Saturday, April 18, 2026

What Happens When Light Goes Boom? Part 4: What Brad Bradington Is Good For

The IceCube Neutrino Observatory at the South Pole, 2023. IceCube Collaboration / NSF. CC BY-SA 4.0.

Cherenkov radiation isn't just a beautiful phenomenon. It turns up in nuclear reactors, in the upper atmosphere, in gamma ray telescopes on three continents, in a cubic kilometer of Antarctic ice, and in hospital imaging suites. Here's what a light boom is actually good for.



"Immature" Lunar Soil Could Be Suitable for Roadways on the Moon

Artist's impression of NASA's Volatiles Investigating Polar Exploration Rover (VIPER) concept. Credit: NASA/Daniel Rutter

Using lunar regolith simulant, a team of researchers demonstrated that "immature" regolith similar to what is expected around the Moon's southern polar region is suitable for rovers to drive on.



Friday, April 17, 2026

What Happens When Light Goes Boom? Part 3: Brad Bradington Sprints

The Advanced Test Reactor at Idaho National Laboratory — the blue glow is Cherenkov radiation from electrons outracing light in water. Argonne National Laboratory. CC BY-SA 2.0, via Wikimedia Commons.

We have the crowd. We have the star. Now it's time to put them together. Here's exactly what happens — and why — when a charged particle outruns the local speed of light in a material. Also: why it's always blue.