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Astronomers have captured the clearest picture yet of how massive stars are born. A team led by Dr. Qizhou Zhang from the Center for Astrophysics | Harvard & Smithsonian used the Atacama Large Millimeter/submillimeter Array (ALMA) to conduct the largest and most detailed survey to date of magnetic fields in 17 regions where clusters of massive stars are forming.

For twenty years, two European spacecraft have been watching the red planet. Now, by combing through their vast archives, scientists have done something remarkable: they've created the first global map of Martian "dust devils," the tornado-like whirlwinds that sculpt the planet's surface. The findings, published in Science Advances, track over a thousand of these twisters, revealing a dynamic weather system with winds far faster than we ever expected.

Astronomers from Australia and Serbia have performed multi-band photometric observations of a binary star known as V717 Andromedae, finding it to be an active, low-mass-ratio contact binary system. The research, published on the arXiv preprint server, provides the first detailed look at this fascinating system, where two stars are locked in an extreme gravitational dance.

First discovered by NASA's Parker Solar Probe near the sun, magnetic "switchbacks" are S-shaped kinks in magnetic field lines. Now, researchers analyzing data from the Magnetospheric Multiscale mission have observed a switchback-shaped structure in Earth's own magnetic field.

Not all stars are created equally. The first stars after the Big Bang were made almost purely of hydrogen and helium. Each successive generation was forged from the ashes of the last, becoming progressively richer in heavier elements. Now, astronomers led by Alexander Ji believe they have found the most "pristine" star on record—SDSS J0715-7334—a red giant that offers an unprecedented window into the universe's infancy.

In the hunt for extraterrestrial life, astronomers are looking beyond sun-like stars to a surprising candidate: white dwarfs, the hot, dense remnants of dead stars. While these stellar embers have habitable zones, it was thought that gravitational nudges from nearby planets would trigger lethal tidal heating. However, new simulations show that Einstein's theory of general relativity can stabilize these worlds, preserving their oceans and their potential for life.

Sagittarius B2 (Sgr B2) is a titan of star formation, a dense cloud near our galactic center churning out new stars at a furious pace. Using the unprecedented power of the James Webb Space Telescope's infrared eyes, astronomers have pierced through the obscuring dust to get their clearest view yet of this stellar nursery, revealing hidden structures and challenging previous assumptions about how stars form in extreme environments.

Textbook illustrations often depict rocky planets with neat, uniform layers: a crust, mantle, and core. But for Mars, the reality is far messier. Seismic data from NASA's InSight lander has uncovered a chunky interior, where fragments from colossal, planet-forming impacts are still preserved like geological fossils, giving us a unique glimpse into the chaotic first 100 million years of the solar system.

In the search for life, astrobiologists follow the water. It turns out the most common type of exoplanet, the "sub-Neptune," is likely water-rich. But there's a catch. Orbiting far closer to their stars than Earth, these worlds are too hot for liquid oceans. Instead, they are "steam worlds," with thick, steamy atmospheres over bizarre, high-pressure phases of water. Now, researchers at UC Santa Cruz have developed a new model to finally understand the anatomy of these exotic

In the local universe, the most massive galaxies are "slow-rotators"—giant, evolved systems supported by the random, chaotic motion of their stars rather than orderly rotation. They are the "retired" galaxies of the cosmos, having stopped forming stars long ago. Finding such a galaxy in the *early* universe (at high redshift) is rare.

Quasars, or quasi-stellar objects (QSOs), are the most luminous objects in the universe. They are the blazing centers of active galaxies, powered by supermassive black holes (SMBHs) devouring matter at an immense rate. A team of astronomers, led by Yunyi Choi of Seoul National University, has just announced the discovery of 62 new, previously undetected bright quasars, adding to a growing catalog that helps us understand black hole growth and galaxy evolution.

Ultraluminous X-ray Sources (ULXs) are point-like sources that are bafflingly bright—emitting more X-ray radiation than one million suns combined. Their true nature is elusive, as they are too bright to be normal stellar-mass black holes, but not at the center of galaxies like supermassive black holes. The leading theories suggest they are powered by either stellar-mass black holes feeding at an extreme rate, or by highly magnetized neutron stars (pulsars).