SETI Live

Exoplanets are planets that orbit stars outside our solar system. We've been finding potential exoplanets more often since the Kepler and TESS spacecraft were launched. But confirming these planets takes time, and telescope time is limited. To speed up the process, amateur astronomers are using their own telescopes. One program, called UNITE (Unistellar Network Investigating TESS Exoplanets), brings together a global group of volunteer and professional astronomers. They use Unistellar telescopes to gather data when exoplanets pass in front of their stars, blocking some of the light. Scientists from the SETI Institute and Unistellar analyze this data. Recently, they confirmed two exoplanets—a hot Jupiter and a warm sub-Saturn. Dr. Lauren Sgro, UNITE’s Exoplanets Lead, talks with communications specialist Beth Johnson about exoplanets, community science, and how science is evolving. (Recorded live 19 September 2024.)

In the quest to find life beyond Earth, icy worlds within our solar system are full of potential. Europa, one of Jupiter's four largest (Galilean) moons, is one possible target because of the vast ocean beneath its icy shell. That ocean, heated by the push and pull of Jupiter, could contain life. The Europa Clipper mission will send a spacecraft to the distant moon, and the spacecraft's instruments will determine if the conditions truly are suitable. This week, NASA announced that Europa Clipper passed another milestone toward the October 10 launch window. Communications specialist Beth Johnson is joined by Project Staff Scientist and Science Communications Lead Cynthia Phillips to discuss the mission and how it could answer the question, "Are we alone?" (Recorded live 12 September 2024.)

There are supermassive black holes. There are stellar mass black holes. And based on the idea that galaxies evolve as they merge, there should be black holes in between -- intermediate mass black holes. However, finding these middle-of-the-road beasts has been difficult. Now, a new paper in Nature identifies the first ever mid-size sedan in a universe of compact cars and SUVs. This black hole resides in the center of the Omega Centauri star cluster, which is thought to be the core of a galaxy that merged with the Milky Way billions of years ago. Deputy Director of the Carl Sagan Center Simon Steel chats with lead author Maximilian Häberle (Max Planck Institute for Astronomy) about just what this discovery means for astrophysics and galaxy evolution. (Recorded live 5 September 2024.)

When a star at its life's end explodes, a debris cloud expands away from the now-dead star. The debris forms intricate and amazing structures in the expanding cloud and can cause the formation of a variety of molecules. Using the James Webb Space Telescope, scientists have collected information regarding Cassiopeia A (Cas A), the youngest known supernova remnant in the Milky Way. The observations shed light on how molecules and dust form and are destroyed in the aftermath of an explosion. These results suggest that supernovae, like Cas A, are key sources of the dust observed in ancient galaxies. A recent paper highlights the findings of this work, including the temperatures measured and molecules formed. Deputy Director of the Carl Sagan Center Simon Steel chats with lead author Jeonghee Rho and co-authors Danny Milisavljevic and Ilse De Looze about the data collected and what it means for dust formation in the universe. (Recorded live 29 August 2024.)

Scientists now can work out what the atmospheres of worlds outside our solar system are made of. Using the James Webb Space Telescope, we have seen water, carbon dioxide, methane, and other gases. Could we, from this distance, know how those gases formed? Possibly. Looking for planets with signs of being intentionally changed - terraforming - would give us proof of an advanced civilization, and a new paper explores just how the investigation process would work. Senior astronomer Franck Marchis talks with authors Edward W. Schwieterman and Daniel Angerhausen about what these gases would be and why they would work as evidence of life. (Recorded 28 August 2024.)

A super-Earth in a distant star system may explain what Mars, Venus, and Earth were like billions of years ago -- incredibly hot and covered in magma oceans. Those oceans may have supplied the planets with early atmospheres full of gases needed for life. While Venus's atmosphere became thick and heavy and Mars couldn't hold on to its atmosphere, Earth became a truly habitable world where life thrives. What can 55 Cancri e, over 40 light years away, teach us about our early solar system? Planetary scientist Beth Johnson asks Renyu Hu (NASA JPL) about his recent paper that uses JWST to examine the distant world's atmosphere. (Recorded 22 August 2024.)

"The Secret Life of the Universe" by Dr. Nathalie Cabrol, the SETI Institute's chief scientist and Director of the Carl Sagan Center at the SETI Institute, is coming out this week, both in the US (August 13, 2024) and in the UK (August 15, 2024). Scriber/Simon & Schuster publishes both editions. Cabrol articulates an overview of where we stand today in our search for life in the universe, what's coming, and how looking out for life beyond Earth teaches us about our place on our planet. Nathalie joins communications specialist Beth Johnson during this week's SETI Live to celebrate this occasion and discuss her latest work. (Recorded live 15 August 2024.)

Join SETI Institute CEO Bill Diamond as he explores NASA's AI-driven mission planning, data analysis, and anomaly detection. Since 2015, the SETI Institute’s Frontier Development Lab (FDL) has partnered with NASA, using machine learning (ML) to classify data, predict outcomes, and uncover trends. With FDL's support, ML tools automate tasks, streamline decision-making, save resources, and maximize NASA's science data potential. Guests will be Megan Ansdell, Program Officer in the Planetary Science Division (PSD) and the Astrophysics Division (APD) at NASA Headquarters; Victoria Da Poian, Data Scientist, NASA Goddard Space Flight Center; Eric Lyness, Principal Systems Engineer, NASA Goddard Space Flight Center and Janice Bishop, Senior Research Scientist, SETI Institute. (Recorded live 1 August 2024.)

In late 2019, an unremarkable galaxy with the catalog number SDSS1335+0728 suddenly started shining brighter than ever. Curious as to why, astronomers used data from space and ground-based observatories to track changes in the galaxy’s brightness and concluded that we are witnessing the sudden awakening of the massive black hole at the galaxy's core. The results were published in Astronomy & Astrophysics in June 2024 with lead author Paula Sánchez Sáez, an astronomer at the European Southern Observatory in Germany. Join Deputy Director of the Carl Sagan Center, Simon Steel, in a chat with Dr. Sánchez Sáez about these results and what they mean for our understanding of galaxies and their black holes. (Recorded 1 August 2024.) Press release: https://www.eso.org/public/news/eso2409/

Imagine standing on the shore of a vast lake, watching the waves crash against the beach after a storm. Now put that beach on Saturn's largest moon, Titan, where the lakes contain liquid methane and ethane. Perhaps do not imagine yourself there after all, but enjoy the thought that even with the unfamiliar and hazardous contents, lakes on Titan are shaped by the same processes as lakes on Earth - crashing waves cause coastal erosion. Such is the discovery in new work published in Science Advances and led by USGS scientist Dr. Rose Palermo. Join Beth Johnson and Dr. Palermo for an interesting conversation about the similarities between the two vastly different worlds and their lakes. (Recorded live 11 July 2014.)