We are not alone: Our Sun escaped together with stellar “twins” from galaxy center
Peer-Reviewed Publication
This May brings a rare celestial treat, two full moons in one month! We’re exploring the science of space and how astronomy connects us through curiosity, discovery, and a shared wonder for what lies beyond.
Updates every hour. Last Updated: 6-Jun-2026 13:16 ET (6-Jun-2026 17:16 GMT/UTC)
Tokyo, Japan – Researchers have uncovered evidence for our Sun joining a mass migration of similar “twins” leaving the core regions of our galaxy, 4 to 6 billion years ago. The team created and studied an unprecedentedly accurate catalogue of stars and their properties using data from the European Space Agency’s Gaia satellite. Their discovery sheds light on the evolution of our galaxy, particularly the development of the rotating bar-like structure at its center.
Could there be simple life floating within the freezing lakes of methane on Titan? A new study presents one of the first experimental tests of the azotosome hypothesis, which proposes that molecules on Titan could form stable closed membranes similar to cells. The findings contradict the hypothesis, showing that the ingredients of Titan’s lakes are more likely to form crystal-like structures instead of membrane-like compartments. Titan is Saturn’s largest moon and has long piqued the interest of astronomers due to its many similarities with Earth. The moon boasts a dense atmosphere and is one of the few places in the Solar System that possesses large bodies of surface liquid. Unlike on Earth, Titan’s seas and lakes are made of liquid methane and ethane, which are extremely cold. Nevertheless, Titan is a prime candidate in the search for extraterrestrial life, with some scientists theorizing that exotic life could form within the moon’s standing methane lakes. One hypothesis posits that compounds named acrylonitriles could assemble into self-enclosed structures called azotosomes capable of housing biochemical reactions. However, models have yielded conflicting results about whether and how azotosomes could form. Here, Tuan Vu and Robert Hodyss performed some of the first experimental tests of the azotosome hypothesis. Using microscopy and calorimetry, they interrogated the chemical behavior and thermodynamic properties of acrylonitrile-methane and acrylonitrile-ethane in liquid methane and ethane, under conditions that simulated Titan’s lakes. These studies revealed that acrylonitriles tended to crystallize within liquid methane and ethane, and didn’t form any structures resembling an azotosome. “This finding further reduces the prospect for vesicles on Titan from a thermodynamic standpoint, but it does not rule out the possibility that they might exist temporarily or be transiently stable,” Vu and Hodyss write. “Titan’s surface habitability thus remains an intriguing notion, whether by way of vesicles or other means.”
Sixteen years ago, theoretical astrophysicists at UC Berkeley and elsewhere proposed that highly magnetized, spinning neutron stars — magnetars — were the power source behind some superluminous supernovae. A 2024 supernova provided the smoking gun. Based on data obtained by Las Cumbres Observatory, a UC Santa Barbara graduate student proposed that a general relativistic precession in an accretion disk around the magnetar can explain the rising frequency of oscillations in the light curve, producing something like a bird chirp.