SETI Live

One of the coldest planetary-mass objects ever directly imaged has been hiding something unusual in its atmosphere: salt clouds.
Known as the "Pink Planet," GJ 504 b is a mysterious world orbiting a Sun-like star about 57 light-years from Earth. At roughly 25 times Jupiter's mass, it lies near the uncertain boundary between giant planets and brown dwarfs. It is also so cold and faint that previous attempts to study its atmosphere from the ground were unsuccessful.
Now, JWST has captured the first direct spectrum of GJ 504 b. The observations revealed an atmosphere containing water vapor, methane, carbon dioxide, ammonia, hydrogen sulfide, and other molecules. When researchers modeled the spectrum, they found that clouds—particularly salt clouds—were essential to explaining what JWST observed.
Join host Dr. Moiya McTier and lead author Dr. Aneesh Baburaj (Northwestern University) to learn how astronomers separated the faint light of GJ 504 b from the glare of its host star, what salt clouds can tell us about cold planetary atmospheres, and why scientists still are not sure whether the Pink Planet formed like a planet or a star.
Read the paper:
https://iopscience.iop.org/article/10.3847/1538-3881/ae6919 
Read the Northwestern University story:
https://news.northwestern.edu/stories/2026/06/famous-pink-planet-harbors-a-salty-surprise

NASA's next great observatory is here.
The Nancy Grace Roman Space Telescope is designed to revolutionize our understanding of the universe, from dark energy to thousands of newly discovered exoplanets. But one of its most exciting instruments is the Coronagraph—a cutting-edge technology that can block the overwhelming glare of distant stars, allowing astronomers to directly observe planets orbiting them.
Joining host Dr. Franck Marchis is Dr. Margaret Turnbull, senior scientist at the SETI Institute and Co-Principal Investigator on Roman's Coronagraph Instrument. She'll explain how this remarkable technology works, what we'll learn from the mission, and why Roman is paving the way toward future telescopes capable of imaging Earth-like worlds.
We'll discuss:
• Why Roman is NASA's newest flagship space observatory
• How a coronagraph "creates an artificial eclipse"
• The challenge of directly imaging exoplanets
• What Roman will reveal about giant planets and planetary systems
• How Roman prepares us to search for potentially habitable worlds
• What excites scientists most as launch approaches
Whether you're fascinated by exoplanets, space telescopes, or the search for life beyond Earth, this episode offers a behind-the-scenes look at one of NASA's most ambitious missions.

Fifty years ago, on July 20, 1976, Viking 1 became the first spacecraft to successfully land and operate on Mars, transforming our understanding of the Red Planet and launching a new era of planetary exploration. Today, sophisticated robotic explorers like Curiosity and Perseverance continue that legacy, searching for signs of ancient habitability and preparing the way for future human missions.
Join host Dr. Simon Steel and planetary scientist Dr. Pascal Lee as they explore the remarkable history of Mars rovers and landers—from Viking, Sojourner, Spirit, Opportunity, Curiosity, and Perseverance to the next generation of robotic explorers being developed for Mars, the Moon, and beyond. They'll discuss what we've learned from five decades of exploration, the technologies that made it possible, and where robotic exploration may take us next. Recent concepts even include adapting Mars rover technology for future lunar missions.
What have Mars rovers taught us about our neighboring world? What mysteries remain unsolved? And what might the next 50 years of planetary exploration look like?

Are we searching for extraterrestrial intelligence the wrong way?
For decades, SETI researchers have focused on finding narrowband radio signals that might stand out from the natural universe. But what if an advanced civilization that wanted to communicate chose a very different strategy?
Join host Dr. Lauren Sgro and UCLA astronomer Dr. Ben Zuckerman as they discuss his new paper, Broadband Searches for Extraterrestrial Technological Intelligence: A New Strategy to Find Nearby Alien Civilizations. The research proposes a new approach to SETI that focuses on broadband signals and existing astronomical surveys, potentially changing how we search for evidence of technological civilizations beyond Earth.
Could signs of extraterrestrial technology already be hidden in data we've collected for entirely different purposes? What can current observations tell us about the likelihood of nearby communicative civilizations? And what does the cosmos's apparent silence really mean?
Paper: https://iopscience.iop.org/article/10.3847/1538-4357/ae4c38

Could hazy exoplanet atmospheres be hiding important clues about alien worlds?
Many potentially habitable planets orbit small, active stars that frequently unleash powerful bursts of ultraviolet radiation. New research shows that this radiation can alter the chemistry and optical properties of atmospheric hazes, changing what astronomers see when they observe these distant worlds.
Join host Dr. Moiya McTier as she welcomes graduate researcher Lori Huseby (University of Arizona) and Dr. Sarah Moran (NASA Goddard Space Flight Center) to discuss how laboratory experiments are helping scientists understand how stellar radiation affects water-rich exoplanet atmospheres. Their findings could improve how we interpret James Webb Space Telescope observations and future missions searching for signs of habitability beyond our Solar System.
How do stellar flares reshape alien skies? What do atmospheric hazes tell us about a planet's environment? And could understanding these hazes help us identify worlds capable of supporting life?
Paper: https://iopscience.iop.org/article/10.3847/1538-4357/ae6cdb