The SETI Institute is pleased to announce that Dr. Andrew Siemion will be honored with the prestigious 2024 Drake Award for his exceptional and pioneering contributions to SETI and radio astronomy and his leadership in the field. Siemion's distinguished career includes his role as the Bernard M. Oliver Chair for SETI at the SETI Institute, Principal Investigator for the Breakthrough Listen Initiative at the University of Oxford, along with holding an Honorary Professorship at the University of Manchester, an Adjunct Appointment at the University of Malta, and directing the Berkeley SETI Research Center at the University of California, Berkeley. His dedication to SETI science and funding has been crucial in advocating for the scientific validity and importance of the field. Ahead of the awards reception, communications specialist Beth Johnson talks with Dr. Siemion about his career so far, receiving the Drake Award, and his vision for the future of SETI research. (Recorded 16 May 2024.)

T Coronae Borealis, or T CrB, is a well-studied nova system in the constellation Corona Borealis. In fact, T CrB produces a recurring nova — one of only five known in our galaxy — that erupts approximately every 80 years, making this a once-in-a-lifetime event. Astronomers predict that the star will explode again within the coming year, likely before this September. When it does erupt, the rather dim T CrB could become as bright as our North Star. Observers with the SETI/Unistellar Network have been watching this star system since last summer and now monitor it daily through the Cosmic Cataclysms citizen science program.

Join communications specialist Beth Johnson as she talks to Dr. Tom Esposito, SETI researcher and Lead of the Cosmic Cataclysms program, about this exciting nova and the efforts to catch it! (Recorded 9 May 2024.)

In a groundbreaking discovery, astronomers have identified an Earth-sized planet closer and younger than any previously known. Positioned remarkably close to both our planet (73 light-years away) and a Sun-like star, this newly found world offers a unique opportunity for scientists to study the evolution of planets. Catalogued as HD 63433 d, this hot exoplanet orbits its star in 4.2 days, making it one of the closest orbiting Earth-sized worlds. With its young age and proximity, HD 63433 d promises invaluable insights into planetary formation and evolution, unlocking mysteries about the processes shaping worlds beyond our own. A paper detailing the planet and its discovery was recently published in The Astronomical Journal.

Communications specialist Beth Johnson speaks with lead authors Melinda Soares-Furtado and Benjamin Capistrant about this amazing discovery and the implications for planetary formation studies. (Recorded 25 April 2024.)