The SWIFTT project invites forest professionals, researchers, and remote sensing experts to its upcoming webinar, “Leveraging AI Models for Insect Damage Detection in European Forests,” taking place online on 11 July 2025, from 14:00 to 15:00 CEST (Paris Time). 

New research led by Dr. James De Buizer at the SETI Institute and Dr. Wanggi Lim at IPAC at Caltech revealed surprising results about the rate at which high-mass stars form in the Galactic Center of the Milky Way. The researchers based their study primarily on observations from NASA's now-retired SOFIA airborne observatory, focusing on three star-forming regions—Sgr B1, Sgr B2, and Sgr C—located at the heart of the Galaxy. Although the central part of our Galaxy has a much higher density of star-forming material than the rest of the Milky Way, in the Galactic Center, the current rate of formation of massive stars (those larger than 8 times the mass of our Sun) appears to be lower compared to the rest of the Galaxy.

New research published by Michigan State University astrophysicists could help scientists answer a century-old question: where did galactic cosmic rays come from? 

SAN ANTONIO — June 9, 2025 — Star and planet formation has largely been considered separate, sequential processes. But in a new study, scientists at Southwest Research Institute (SwRI) have modeled a different scenario where planets start developing early — during the final stages of stellar formation — rather than after this phase ends, as previously assumed.

An international team of astronomers led by University of Galway, has discovered the likely site of a new planet in formation, most likely a gas giant planet up to a few times the mass of Jupiter.

Using the European Southern Observatory's Very Large Telescope (ESO’s VLT) in Chile, the researchers captured spectacular images around a distant young star for the first time in the form of scattered near-infrared light that revealed an exceptionally structured disk.