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Humanity Will Change | Pantropy

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Imagine a civilization reaches something like a Type II level, advanced enough to move through interstellar space and keep large populations alive for generations. At that stage, the challenge is developing ships that can cross the void, and also making sure the people inside them can survive radiation, isolation, and extreme travel times. That could mean heavy genetic engineering before the journey begins, changing bone density, metabolism, resistance to disease, tolerance for low gravity, or even sensory systems and respiration. But when they finally arrive, they may still find that the planet is wrong for them, maybe the air is toxic, the gravity is crushing, the temperatures are extreme, or the native chemistry is incompatible with human biology.

At that point, they face two paths. One is terraforming, which means trying to remake an entire planet into something closer to Earth. That could involve thickening or thinning an atmosphere, warming a frozen world, cooling a hot one, importing water, altering soil chemistry, introducing engineered microbes, building orbital mirrors or shades, and managing the planet for centuries or even millennia. The scale of that project is absurdly expensive, not just in money but in energy, infrastructure, labor, time, and raw materials. You are not changing a city or even a continent, you are trying to rewrite a whole world.

The other option is pantropy. Instead of forcing the planet to become Earth-like, the colonists change themselves to fit the planet. They might alter their lungs to breathe a different atmospheric mix, redesign their skin to handle harsher radiation, reduce their size for lower resource use, strengthen their bodies for higher gravity, or even become something so biologically different that they no longer look fully human. That is the core idea of pantropy, adapting the colonists to the world rather than adapting the world to the colonists.

The term was coined by James Blish, and he used it in connection with the stories collected in The Seedling Stars, especially “Surface Tension.” which was first published in 1952 in Galaxy Science Fiction.

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Von Neumann Probes: The Self-Replicating Robots That Could Consume the Galaxy

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What happens when machines can build more of themselves—and never stop? In this episode of Entropy Rising, Jacob and Lucas unravel the strange, fascinating world of von Neumann probes: self-replicating systems that could mine asteroids, build Dyson swarms, and maybe even terraform entire planets. But the same tech could go off the rails—accidentally wiping out alien life, turning planets into grey goo, or mutating into something far worse. Are these machines the key to a post-scarcity future, or the seeds of cosmic disaster? We explore the science, the speculation, and the existential questions behind one of the most provocative ideas in futurism.

Stick around for a bonus post-show discussion—available free on our Patreon.

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Terraforming Mars: Modeling engineered aerosols to warm the planet

Whenever humans arrive on Mars, they’re going to find it a difficult place to exist. Mars is cold, with an average surface temperature of −55°C; temperatures can plunge to −125°C with dust storms lasting months; its atmosphere is very thin and almost all carbon dioxide; and all the water is frozen and mixed with ice made of CO2. Oh, and solar radiation will be hazardous on Mars’ surface since the planet has no ozone layer to block ultraviolet radiation, especially so during solar flares. Disneyland it is not.

New Martians will need to live underground until, someday, maybe, Mars can be terraformed to, if not quite looking like Earth, at least a planet more hospitable to fragile human creatures.

There are arguments for and against terraforming Mars. If humans do terraform, one of the first suggestions is to increase Mars’ greenhouse effect by melting the CO2-ice caps.

From stellar engines to Dyson bubbles, alien megastructures could hold themselves together under the right conditions

New theoretical models have strengthened the case that immense, energy-harvesting structures orbiting their host stars could exist in principle in distant stellar systems. With the right engineering precautions, calculations published in Monthly Notices of the Royal Astronomical Society, carried out by Colin McInnes at the University of Glasgow, show that both stellar engines and Dyson bubbles can become gravitationally stable, allowing them to tap into the vast amounts of energy emitted by their host stars.

For decades, astronomers have pondered the possibility of alien civilizations far more technologically advanced than our own. While these studies remain entirely speculative, many have converged on similar ideas for harvesting stellar energy: envisioning vast structures deployed around host stars.

If such structures could exist, they would provide civilizations with vastly more energy than any planet could offer—enough for ventures ranging from the terraforming of new worlds, to interstellar journeys spanning many generations.

Greening the Solar System

A lovely, thoughtful, and evidence-based essay on the technical prerequisites for terraforming Mars and other nearby planets and asteroids. While this will take a long time, I believe it ought to be one of the main priorities towards opening up a bright and beautiful future for humanity.


A future where life flourishes beyond Earth is closer than you think. How, precisely, will we get there?

The idea of bringing life to other worlds has captured the imagination of many scientists and thinkers, from the founding father of astronautics, Konstantin Tsiolkovsky, in the 1890s to Carl Sagan, Freeman Dyson and other visionaries in the 20th century. Today, we know much more about spaceflight, biology, and the nature of habitable environments. We are entering an era of rapid and cheap access to space, and with it, we find ourselves on the brink of being able to extend Earth’s biosphere across the solar system, billions of times beyond its current bounds.

The possibilities for how we might do this range widely, from terraforming Mars (and possibly other planets or moons) to generating habitable bubbles on free-floating asteroids. While technological challenges remain, many of these techniques appear surprisingly feasible — making a detailed assessment of their merits all the more important.

GENETIC ENGINEERING, a Journey into the Future

This is a sci-fi documentary looking at the future of genetic engineering and how it applies to space exploration, astronauts, terraforming planets and even Earth.

What is DNA, and how can it be engineered. What is CRISPR, and the future technology used in genetic engineering and biotechnology.

Personal inspiration in creating this video came from: Jurassic Park (the book), and The Expanse TV show (the protomolecule).

Other topics in the video include: how genetic engineering can change food allergies, cryosleep astronauts using hibernation biology borrowed from bears, squirrels and hedgehogs, engineering plants for terraforming other planets, and entries from The Encyclopedia of the Future.

PATREON
The third volume of ‘The Encyclopedia of the Future’ is now available on my Patreon.

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Scientists Reveal the Hidden Chemistry of Air Pollution

The interactions between light and nitroaromatic hydrocarbon molecules have important implications for chemical processes in our atmosphere that can lead to smog and pollution. However, changes in molecular geometry due to interactions with light can be very difficult to measure because they occur at sub-Angstrom length scales (less than a tenth of a billionth of a meter) and femtosecond time scales (one millionth of a billionth of a second).

The relativistic ultrafast electron diffraction (UED) instrument at the Linac Coherent Light Source (LCLS) at SLAC National Accelerator Laboratory provides the necessary spatial and time resolution to observe these ultrasmall and ultrafast motions. The LCLS is a Department of Energy (DOE) Office of Science light source user facility.

In this research, scientists used UED to observe the relaxation of photoexcited o–nitrophenol. Then, they used a genetic structure fitting algorithm to extract new information about small changes in the molecular shape from the UED data that were imperceptible in previous studies. Specifically, the experiment resolved the key processes in the relaxation of o-nitrophenol: proton transfer and deplanarization (i.e., a rotation of part of the molecule out of the molecular plane). Ab-initio multiple spawning simulations confirmed the experimental findings. The results provide new insights into proton transfer-mediated relaxation and pave the way for studies of proton transfer in more complex systems.

The Last Fuel We’ll Ever Need?

I stormed a castle in Burbank that is home to the Terraformer — a machine that uses air, water, and sunlight to produce all the fuel we’d ever need. It’s cheap and can be run in almost any condition, anywhere in the world. The only problem? It’s wildly inefficient – but for the first time in history, solar power is so cheap that it no longer matters.

Plus, we get to see the misuse of a cake mixer to further the cause of science! Leave a comment to let us know if this is your favorite misuse of a cake mixer.

Timestamps:
0:00 — Welcome to Hard Reset.
1:16 — Meet Casey Handmer.
3:06 — A cheaper kind of fuel.
6:13 — Casey’s plan.
7:08 — The terraformer.
8:27 — The carbon capture system.
10:50 — The power of methane.
12:16 — An inefficient process.
13:50 — Terraform Industries’ next step.

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