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Lecture 42: The Fermi Paradox
So, Where is Everybody? Interstellar colonization, in principle, is an
exponential growth process that would fill the galaxy in a few million
years even with a very modest star flight capability. This is a small
fraction of the lifetime of the Milky Way Galaxy, so the Galaxy should
be teaming with life. But, we so far have no compelling evidence of
extraterrestrial visitations, alien artifacts, or any other evidences
that the Galaxy is populated. Physicist and Nobel Laureate Enrico
Fermi's apparent paradox and some of the proposed resolutions are the
topic of this lecture. I will review the Fermi Paradox and describe the
most common possible resolutions. The Fermi Paradox is useful in
helping to frame the question of extraterrestrial life, even if we so
far have no answers. At the end I only touch on the Rare Earth
Hypothesis, but this is a very nuanced question which requires a whole
other lecture to explore that I have not had time to fully prepare for
during this busy quarter. Recorded live on 2009 Nov 30 in Room 1005
Smith Laboratory on the Columbus campus of The Ohio State University.
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By Richard Pogge
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184184 ratings
So, Where is Everybody? Interstellar colonization, in principle, is an
exponential growth process that would fill the galaxy in a few million
years even with a very modest star flight capability. This is a small
fraction of the lifetime of the Milky Way Galaxy, so the Galaxy should
be teaming with life. But, we so far have no compelling evidence of
extraterrestrial visitations, alien artifacts, or any other evidences
that the Galaxy is populated. Physicist and Nobel Laureate Enrico
Fermi's apparent paradox and some of the proposed resolutions are the
topic of this lecture. I will review the Fermi Paradox and describe the
most common possible resolutions. The Fermi Paradox is useful in
helping to frame the question of extraterrestrial life, even if we so
far have no answers. At the end I only touch on the Rare Earth
Hypothesis, but this is a very nuanced question which requires a whole
other lecture to explore that I have not had time to fully prepare for
during this busy quarter. Recorded live on 2009 Nov 30 in Room 1005
Smith Laboratory on the Columbus campus of The Ohio State University.
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