Space News & Blog Articles

The Sun is far more than a steadily glowing sphere as our ancestors once thought. Across its surface and atmosphere, countless tiny features flicker in and out of existence, magnetic loops hundreds of times larger than Earth, and plasma flows in ways that still puzzle scientists. Understanding this complexity requires more than just looking harder, it requires looking from multiple angles at once.

Omega Centauri dominates the southern sky as the Milky Way's largest and brightest globular cluster, a dense sphere containing roughly ten million stars. Earlier this year, astronomers found evidence that an intermediate mass black hole hides within the cluster's core, revealed by seven stars moving far too quickly to remain bound unless something massive holds them gravitationally. Now researchers have searched for the black hole itself using radio telescopes, and their discovery is what they didn't find.

The giant planets weren't always where we find them today. Jupiter, Saturn, Uranus and Neptune formed in a more compact configuration and later underwent a violent reshuffling that scattered them to their current positions. Exactly what triggered this chaos remains uncertain, but researchers at the Laboratoire d'Astrophysique de Bordeaux and the Planetary Science Institute now propose a close encounter with a wandering substellar object during the Sun's youth.

The universe is getting bigger, and there's a problem. Two different ways of measuring its expansion rate give two different answers, and nobody knows why. Now researchers at the University of Tokyo have demonstrated a completely independent method that adds compelling evidence this discrepancy represents something real, not just measurement error.

Since it commenced science operations in mid-2022, the James Webb Space Telescope has made significant strides in detecting atmospheres around exoplanets. These included providing the first clear evidence of carbon dioxide in an exoplanet atmosphere (WASP-39b), atmospheric water vapor (WASP-96 b), and even heavier elements like oxygen and carbon (HD149026b). According to the latest release, researchers announced that they have detected the strongest evidence to date for an atmosphere around a rocky planet.

Carl Sagan famously said that “We’re all made of star-stuff”. But he didn’t elaborate on how that actually happened. Yes, many of the molecules in our bodies could only have been creative in massive supernovae explosions - hence the saying, and scientists have long thought they had the mechanism for how settled - the isotopes created in the supernovae flew here on tiny dust grains (stardust) that eventually accreted into Earth, and later into biological systems. However, a new paper from Martin Bizzarro and his co-authors at the University of Copenhagen upends that theory by showing that much of the material created in supernovae is captured in ice as it travels the interstellar medium. It also suggests that the Earth itself formed through the Pebble Accretion model rather than massive protoplanets slamming together.

(This is Part 3 of a series exploring the mythic side of the Big Bang. Check out Part 1 and Part 2!)

For decades, scientists have recognized that large galaxies in our Universe have supermassive black holes (SMBHs) at their centers. These behemoths, which are millions to billions of times the mass of our Sun, play a vital role in star formation and the long-term evolution of galaxies. According to a recent study based on observations performed using NASA's Chandra X-ray Observatory, it appears that most dwarf galaxies may buck this trend. This stands in stark contrast to their theory that nearly every galaxy has a massive black hole within its core.