Saturday, July 4, 2026

In Anticipation of New Horizons Entering Interstellar Space, Researchers are Developing a Solar Wind Forecasting Method

Solar wind data and solar wind pressure forecasts provide important information for heliospheric models to help predict when the New Horizons spacecraft will encounter the heliospheric termination shock, on its way to joining the Voyager 1 and 2 spacecraft in interstellar space. Credit: Credit: NASA/IBEX/Adler Planetarium/SwRI

Southwest Research Institute (SwRI) scientists are using a solar wind forecasting method combined with analytic and numerical heliosphere models to find out where the first plasma boundary of the outer heliosphere lies as NASA’s New Horizons spacecraft hurtles toward this mysterious region of space.



Friday, July 3, 2026

A New Study into Dark Matter in the Bullet Cluster Could Disprove its Existence

A simulation of the formation of dark matter structures from the early universe until today. Credit: Ralf Kaehler/SLAC National Accelerator Laboratory/American Museum of Natural History

A study led by the University of Bonn presents new data that calls the existence of Dark Matter - a fundamental pillar of the current cosmological model - into question.



Bending Spacetime Reveals New Planet Hidden in Archived TESS Data

This artist’s concept visualizes Gaia23bra b, the first microlensing planet orbiting a distant star found by NASA’s TESS (Transiting Exoplanet Survey Satellite). This super-Jupiter orbits an orange dwarf star at a distance similar to Jupiter’s distance from the Sun.
NASA’s Goddard Space Flight Center

NASA’s Transiting Exoplanet Survey Satellite (TESS) has captured evidence of a Jupiter-like world orbiting another star, using a trick straight out of Einstein’s relativity: gravitational microlensing. The technique marks a first for TESS, and opens up the possibility of a whole new category of planets the spacecraft might uncover.



Astronomers Spot an Extremely Rare Galaxy Mega-Merger

JWST Image of Stephan's Quintet of galaxies, the left of which (NGC 7320) is much closer to Earth than the other four galaxies in the image. Credit - NASA, ESA, CSA, STScI

Scale in the universe is hard to understand from a purely human perspective. Many times the math just doesn’t sit well with our brains that evolved to capture and process data about the world around us rather than groking the complexities of stellar dynamics and galaxy mergers. But every once in a while astronomers find something that, if we can wrap our heads around the numbers, gives a sense of just how big the universe is. That is precisely what a new paper, available in preprint on arXiv from a group of astronomers led by Z.L. Wen of the Chinese Academy of Sciences, hopes to do when it describes a merger of not one, not two, but six supermassive galaxies and the active dynamics they’re subject to.



Thursday, July 2, 2026

This Giant Planet Survived the Death of its Star

This artist's illustration shows the giant exoplanet WD 1856 b orbiting its much smaller white dwarf star. Somehow, this planet survived the star's transition from main sequence star, to red giant, to white dwarf. How did that happen? What does it mean for potential habitability on planets like this? Image Credit: NASA, ESA, CSA, Ralf Crawford (STScI)

Some planets can survive when their main sequence stars "die" and evolve into red giants. Astronomers have found several of them. One of them in particular is orbiting extremely close to its star, providing an opportunity to study it with the JWST to determine how it got there.



An Extended Barrage of Asteroid Impacts Made Earth Too Hot to Form Continents

This artist's illustration shows Earth being bombarded by asteroids during the Late Heavy Bombardment (LHB). The LHB was caused by the migration of the Solar System's giant planets, which unlodged asteroids from their stable position and sent many careening into the inner planets. New research says the heat from the continual impacts slowed the formation of thick continental crust, explaining why we have almost no rock samples from the Hadean eon. Image Credit: NASA's Goddard Space Flight Center Conceptual Image Lab

New research shows that repeated impacts on Earth during the Hadean eon prevented thick and stable crustal material from forming. The heat from these impacts penetrated deep into the planet, and along with radiogenic heating, delayed the formation of a solid crust.



Wednesday, July 1, 2026

A Supermassive Black Hole Gets Blamed for Quenching Star Formation

The accretion disk of NGC 4151 is shown in blue, immediately surrounding the galaxy’s central black hole. Scientists, including University of Michigan astronomers, are showing how winds or outflows from the accretion disk reshape its host galaxy. The winds are shown as wispy light blue lines blowing across the more orange clouds surrounding the black hole. Image credit: JAXA (Used under a CC BY 4.0 INT license)

Some of the most massive galaxies in the Universe appear to be missing a lot of stars. That seems unusual, since birthing stars is one of a galaxy's main tasks as it grows. According to Xin "Cindy" Xiang of the University of Michigan, something is suppressing or quenching the births of stars in these and she thinks that black holes might be the culprit.