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Renowned researchers David Chalmers and Anil Seth join Brian Greene to explore how far science and philosophy have gone toward explaining the greatest of all mysteries, consciousness–and whether artificially intelligent systems may one day possess it.

This program is part of the Big Ideas series, supported by the John Templeton Foundation.

Participants:
David Chalmers.
Anil Seth.

Moderator:
Brian Greene.

00:00 — Introduction.
02:35 — Participant Introductions.
03:50 — Will an Artificial System Ever Become Conscious?
05:32 — The Hard Problem of Consciousness.
08:32 — Thought Experiment: Mary and the Nature of Conscious Experience.
13:28 — The Hard Problem and The Real Problem of Consciousness.
21:53 — The Brain as a Prediction Machine.
25:41 — Possible Solutions to the Hard Problem.
33:15 — Will AI Systems Become Conscious and How Will We Know?
40:11 — Is Human Consciousness the Only One Example of Conscious-like Experience?
42:19 — The Future of Creating Consciousness and the Ethical Questions.
44:39 — Credits.

Based on our experiments, the ‘safe’ sampling depth for amino acids on Europa is almost 8 inches (around 20 centimeters) at high latitudes of the trailing hemisphere (hemisphere opposite to the direction of Europa’s motion around Jupiter) in the area where the surface hasn’t been disturbed much by…


How deep will future landers to Jupiter’s moon, Europa, and Saturn’s moon, Enceladus have to dig to find organic molecules aka the building blocks of life? This is what a recent study published in Astrobiology hopes to address as an international team of researchers investigated whether near-surface organic molecules on Europa and Enceladus could survive the intense solar and cosmic radiation since neither moon has a magnetic field like the Earth to shield it. This study holds the potential to help scientists better understand the conditions for finding life beyond Earth and the methods for finding that life, as well.

Image of Jupiter’s moon, Europa, obtained by NASA’s Juno spacecraft in September 2022. (Credit: NASA/JPL-Caltech/SwRI/MSSS Image processing: Kevin M. Gill CC BY 3.0)

Image of plumes emanating from the south pole of Enceladus obtained by NASA’s Cassini spacecraft. (Credit: NASA/JPL/Space Science Institute)

For the study, the researchers exposed several amino acids in ices and dead organisms using liquid nitrogen to varying levels of radiation to ascertain how fast they degrade under these harsh conditions. The goal was to determine if organic molecules could survive the harsh environments on Europa and Enceladus since neither moon possesses a magnetic field like the Earth to shield their surfaces from harmful cosmic radiation. The team discovered that while certain amino acids experienced initial declines at low doses, no further declines were observed for increased doses, which they note could bode well for sampling from the surfaces of Europa or Enceladus.