
Thanks to John Harrigan of Foolish People for pointing this interesting article out.

Thanks to John Harrigan of Foolish People for pointing this interesting article out.
“Eventually, the day will come when life on Earth ends. Whether that’s tomorrow or five billion years from now, whether by nuclear war, climate change, or the Sun burning up its fuel, the last living cell on Earth will one day wither and die. But that doesn’t mean that all is lost. What if we had the chance to sow the seeds of terrestrial life throughout the universe, to settle young planets within developing solar systems many light-years away, and thus give our long evolutionary line the chance to continue indefinitely?
According to Michael Mautner, Research Professor of Chemistry at Virginia Commonwealth University, seeding the universe with life is not just an option, it’s our moral obligation.
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Mautner says that “directed panspermia” missions can be accomplished with present technology.
“We have a moral obligation to plan for the propagation of life, and even the transfer of human life to other solar systems which can be transformed via microbial activity, thereby preparing these worlds to develop and sustain complex life,” Mautner explained “Securing that future for life can give our human existence a cosmic purpose.”
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the strategy is to deposit an array of primitive organisms on potentially fertile planets and protoplanets throughout the universe. Like the earliest life on Earth, organisms such as cyanobacteria could seed other planets, digest toxic gases (such as ammonia and carbon dioxide on early Earth) and release products such as oxygen which promote the evolution of more complex species. To increase their chances of success, the microbial payloads should contain a variety of organisms with various environmental tolerances, and hardy multicellular organisms such as rotifer eggs to jumpstart higher evolution. These organisms may be captured into asteroids and comets in the newly forming solar systems and transported from there by impacts to planets as their host environments develop.”
Read more at PhysOrg