Cosmic Queries – Starquakes with Conny Aerts
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In this episode of StarTalk Cosmic Queries, Neil deGrasse Tyson and co-host Matt Kirshen explore the fascinating science of astroseismology with guest Conny Aerts, a professor of astroseismology at Radboud University in the Netherlands and KU Leuven in Belgium. The conversation demystifies 'starquakes'—not violent events like earthquakes, but continuous, smooth oscillations in stars caused by internal sound waves. These oscillations, detectable through tiny brightness variations, allow scientists to probe the hidden interiors of stars, revealing their structure, rotation, and composition. Aerts explains how stellar 'music' can be sonified into audible frequencies, making astronomy accessible to blind audiences and transforming cosmic data into art. The episode also addresses listener questions about planetary quakes, the dimming of Betelgeuse, the role of the James Webb Space Telescope, and the potential dangers of stellar activity. Aerts emphasizes that starquakes are not destructive but essential tools for understanding stellar evolution, with future missions like PLATO poised to revolutionize the field through long-term, high-precision observations. Key takeaways include: starquakes are not abrupt but continuous oscillations that reveal internal stellar structure; sonification allows the 'music of the spheres' to be heard by all, including blind astronomers; rotation inside stars, previously unknown, is now measurable through frequency shifts; the dimming of Betelgeuse was due to ejected dust obscuring the star, not an imminent supernova; and long-duration space missions like Kepler and PLATO are essential for detecting low-frequency stellar oscillations. The episode concludes with a celebration of curiosity, inclusion, and the joy of discovery in astrophysics.
Starquakes are not violent events but continuous, smooth oscillations caused by internal sound waves in stars, allowing scientists to probe their hidden interiors.
By measuring tiny brightness changes over time, astroseismologists can determine a star's internal rotation, age, and composition—information impossible to obtain otherwise.
Sonification transforms stellar oscillation data into audible sound, enabling blind people to 'hear' the stars and making astrophysics more inclusive.
The dimming of Betelgeuse was caused by dust ejected from the star, not an imminent supernova, and is part of its normal late-life behavior.
Long-duration space missions like Kepler and the upcoming PLATO mission are essential for detecting low-frequency stellar oscillations and unlocking new insights.
…and 3 more takeaways available in PodZeus
Introducing Astroseismology: The Music of the Stars
“Stars are three dimensional musical halls, concert halls. Wow.”
Decoding Stellar Interiors Through Oscillations
“The stars are right. The theory is wrong if it doesn't match with each other, right?”
The Case of Betelgeuse and the Limits of Observation
“It's not bad. Because it will explode eventually, but that can take still some while.”
Starquakes, Binary Systems, and the Future of Astrophysics
The final segment tackles listener questions about the dangers of starquakes, the possibility of predicting them, and why the Sun is alone. Aerts clarifies that starquakes are not destructive but smooth, periodic motions that cannot tear apart a star. She explains that while binary systems are common, the Sun's solitary nature is statistically normal. The episode concludes with a celebration of curiosity, inclusion through sonification, and the promise of future missions like PLATO to unlock deeper secrets of the cosmos.
“The stars are right. The theory is wrong if it doesn't match with each other, right?”
“Stars are three dimensional musical halls, concert halls. Wow.”
“It's not bad. Because it will explode eventually, but that can take still some while.”
Hosts
Guest
Conny Aerts
person
Neil deGrasse Tyson
person
Matt Kirshen
person
Sun
other
Betelgeuse
other
Kepler mission
other
James Webb Space Telescope
other
Flatiron Institute
organization
PLATO
other
Coronal mass ejection
other
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