|
Space Topics: Search for Extraterrestrial IntelligenceCan SETI Succeed?
|
|||||
![]()
Carl Sagan
Credit: The Planetary Society |
SETI proponents argue that our own galaxy has hundreds of billions of stars, and we live in a universe with billions of galaxies, so life should be common in this cosmic realm. There should be many habitable planets, each sheltering its brood of living creatures. Some of these worlds should develop intelligence and the technological ability and interest in communicating with other intelligent creatures.
Using electromagnetic waves, it should be possible to establish contact across interstellar distances and exchange information and wisdom around the galaxy. Some fraction of the extraterrestrial civilization should be providing an electromagnetic signature that we should be able to recognize.
![]() Ernst Mayr |
But because we have been unable to find a single piece of concrete evidence of alien intelligence yet, a philosophical battle has risen between those who might be called contact optimists — who generally embrace the orthodox view of SETI — and the proponents of the uniqueness hypothesis, which suggests that Earth is probably the only technological civilization in our galaxy.
Here we present both sides of the philosophical and scientific debate. First, one of the most prominent evolutionary specialists of this century, the late Ernst Mayr of Harvard University's Museum of Comparative Zoology, delivers the main arguments of the uniqueness hypothesis. Mayr notes that, since they are based on facts, the various degrees of uniqueness are a problem for SETI, not a hypothesis. The late Carl Sagan of The Planetary Society and Cornell University's Laboratory of Planetary Studies responds to Mayr's statements and expresses the optimist's view.
Which view is more palatable? Read on and decide for yourself.
Read Can SETI Succeed? Not Likely, by Ernst Mayr
Read The Abundance of Life-Bearing Planets, by Carl
Sagan
Read Ernst Mayr's final comments
Read Carl Sagan's final comments
The SETI debate originally appeared in the Planetary Society's Bioastronomy News, beginning with vol. 7, no. 3, 1995.)