Using early data from the European Space Agency's Euclid space telescope, astronomers have analyzed over one million galaxies to test a long-standing idea in astrophysics: that galaxy mergers help trigger the growth of supermassive black holes. In this SETI Live, host Dr. Moiya McTier will explore two new Euclid studies that combine vast sky surveys, machine learning, and multi-wavelength observations to uncover when and why active galactic nuclei (AGN) ignite. The results show that galaxies in the midst of mergers are far more likely to host actively feeding black holes — and that the brightest AGN are almost always found in cosmic collisions. Dr. McTier will be joined by lead authors Dr. Berta Margalef-Bentabol, Dr. Lingyu Wang, and Dr. Antonio la Marca from the Space Research Organisation Netherlands (SRON). They will discuss how Euclid identifies merging galaxies at scale, how researchers measure the black hole's contribution to a galaxy's light, and what this tells us about the coevolution of galaxies and their central black holes. We'll also look ahead to what future Euclid data could reveal as the survey expands to billions of galaxies. (Recorded live 15 January 2026.)

2026 is a pivotal year for space science. From humans returning to the Moon to new telescopes opening more expansive windows on the universe, this year marks a turning point in how we explore space—and why it matters. SETI Institute communications specialist Beth Johnson and Senior Planetary Astronomer Franck Marchis will tour the biggest missions, milestones, and moments shaping space science in 2026. We'll look at crewed lunar exploration, robotic missions to asteroids and planets, next-generation observatories, and the celestial events unfolding above our own skies. Along the way, we'll talk about what these missions are designed to discover, the questions they're trying to answer, and how they fit into the bigger story of humanity's search to understand our place in the cosmos. Whether you follow every launch or love looking up at the night sky, this episode will connect the dots between ambitious engineering, fundamental science, and the sense of wonder that keeps us exploring. (Recorded live 8 January 2026.)

We're going live with Dr. Cynthia Phillips, Europa Clipper Project Staff Scientist and Science Communications Lead, from NASA's Jet Propulsion Laboratory, to explore a surprising and exciting new chapter in comet science. Recently, the Ultraviolet Spectrograph (UVS) aboard NASA's Europa Clipper spacecraft made unique observations of the interstellar comet 3I/ATLAS at a time when Earth- and Mars-based telescopes couldn't see it. In this livestream, communications specialist Beth Johnson and Dr. Phillips will unpack what these observations mean for our understanding of interstellar visitors and how instruments designed for one mission can yield discoveries well beyond their original goals. We'll lay out: • How Europa-UVS captured data on 3I/ATLAS's tails and coma while other assets were blocked by the Sun, bridging a critical observational gap. • What signatures of oxygen, hydrogen, and dust the instrument detected, and why that matters. • Why observations from unexpected vantage points — like those aboard Europa Clipper — can deepen our picture of interstellar objects. • What this tells us about the composition, activity, and evolution of a comet that formed around another star. Interstellar comets like 3I/ATLAS are cosmic time capsules from beyond our solar system, carrying clues about alien planetary systems. Capturing data from a spacecraft not originally tasked with comet science is a testament to scientific adaptability and ingenuity — and it gives researchers a rare look inside the workings of an object that has journeyed across the galaxy to visit us. Press release: https://science.nasa.gov/blogs/europa-clipper/2025/12/18/nasas-europa-clipper-observes-comet-3i-atlas/ (Recorded live 19 December 2025.)

Get ready for a fascinating deep dive into one of the biggest questions in astrobiology: How common are biological extraterrestrial intelligences in the Milky Way? Host Simon Steel, Deputy Director of the Carl Sagan Center for Research, is joined by Manuel Scherf and Helmut Lammer (Space Research Institute, Austrian Academy of Sciences) to explore new research that challenges long-held assumptions about "Earth-like" planets and what it really takes for a world to support complex life. Recent work from Scherf, Lammer, and colleagues revisits the idea of Eta-Earth — the number of truly Earth-like habitats in the Galaxy. Their models extend far beyond the basic "habitable zone" and incorporate a suite of filters, including stable atmospheres, oxygen-rich conditions, plate tectonics, subaerial land, and long-term planetary evolution. These filters significantly reduce the number of planets that could potentially host complex or technological life. The study finds that even under generous assumptions, the Milky Way may host at most 60,000 to 250,000 Earth-like habitats — and the number that actually evolve intelligent life could be far smaller. The result? A serious rethink of how rare (or precious) intelligent life might be. Join us as we explore what this means for SETI strategies, exoplanet surveys, and our own cosmic significance. It's a conversation that blends astrophysics, planetary science, and a bit of existential wonder — perfect for anyone curious about where life fits into the grand structure of the cosmos. Paper: https://www.liebertpub.com/doi/10.1089/ast.2023.0076 Conference Abstract: https://meetingorganizer.copernicus.org/EPSC-DPS2025/EPSC-DPS2025-1512.html (Recorded live 8 December 2025.)

In a special bonus SETI Live, communication specialist Beth Johnson welcomes astronomer and entrepreneur Franck Marchis to introduce SkyMapper, a new global network of smart telescopes and all-sky sensors designed to open the universe to everyone. SkyMapper brings together professional observatories, citizen astronomers, and classrooms into a single, decentralized platform. It enables real scientific discovery — from tracking satellites and meteors to monitoring comets and transient events in real time — while giving students and the public the chance to observe the sky, contribute data, and learn how modern astronomy works. We'll talk about the science, the outreach mission, the importance of the SETI Institute's partnership with SkyMapper, and why a worldwide, always-on view of the sky matters more than ever for research, education, and our shared curiosity. Join us live and discover how you can be part of this new way of exploring the universe. 📚 Learn more about SkyMapper: www.skymapper.io 👋 Join the SkyMapper community on Telegram: https://t.me/skymapper_community ✅ Follow SkyMapper on social media: BlueSky: @skymapper.bsky.social X (formerly Twitter): @Skymapperspace LinkedIn: https://www.linkedin.com/company/skymapper-inc/ Reddit: https://www.reddit.com/r/SkyMapper/ (Recorded live 5 December 2025.)

On this episode of SETI Live, host Moiya McTier welcomes two leading researchers—Gabriele Cugno (University of Zürich) & Sierra L. Grant (Carnegie Institution for Science)—to dive into an extraordinary discovery by the James Webb Space Telescope (JWST): a carbon-rich, moon-forming disk around the distant exoplanetary object CT Cha b, some 625 light-years away. What exactly is a "moon-forming disk"? Why is this discovery a game-changer for our understanding of how moons — and ultimately habitable environments around them — can form? Gabriele and Sierra walk us through spectroscopy, chemistry (including acetylene, benzene, and more), observational challenges, and the big philosophical questions: Could moons be even more common than planets? What does this tell us about our own Solar System's past — and the possibilities for life elsewhere? 📚 For more: NASA Press Release: https://science.nasa.gov/science-research/nasas-webb-telescope-studies-moon-forming-disk-around-massive-planet/ Research Paper: https://iopscience.iop.org/article/10.3847/2041-8213/ae0290 (Recorded live 4 December 2025.)

Join host Beth Johnson for a fascinating episode of SETI Live, featuring planetary scientists Dr Georgina Miles and Dr Carly Howett from the University of Oxford. We'll be unpacking their groundbreaking study showing that Enceladus — one of Saturn's icy moons — may harbor a stable subsurface ocean capable of supporting life. 📄 For more info: The study "Endogenic heat at Enceladus' north pole" has just been published in Science Advances: https://www.science.org/doi/10.1126/sciadv.adx4338 Official press release from the University of Oxford: https://www.ox.ac.uk/news/2025-11-10-saturn-s-icy-moon-may-host-stable-ocean-fit-life-new-study-finds (Recorded live 20 November 2025.)

What happens when a planet is full of water—but too hot for oceans? Meet the "steam worlds," exotic exoplanets wrapped in thick water vapor and boiling at thousands of degrees. These strange worlds may be far from habitable, but they're reshaping how scientists think about planets, water, and where life might exist. In this episode of SETI Live, host Beth Johnson talks with Artem Aguichine of the University of California, Santa Cruz, about his new research modeling the interiors and atmospheres of steam worlds—a class of water-rich sub-Neptunes that could dominate our galaxy. With data from the JWST revealing steam signatures on distant planets, these models are helping scientists decode what's really going on beneath the haze. Join us as we explore: • What defines a "steam world" and how it forms • How water behaves under crushing pressure and searing heat • Why JWST's new observations are changing the game • What these discoveries mean for the future search for life beyond Earth 🔗 Learn more: UCSC Press Release – https://news.ucsc.edu/2025/08/new-model-steam-worlds Research Paper – https://iopscience.iop.org/article/10.3847/1538-4357/add935 (Recorded live 13 November 2025.)