Contents

Beyond the birthplace

Why another home

Survival matters, but the affirmative case begins with the good of building and discovery

Earth is irreplaceable, the only world known to hold oceans, children, and the accumulated life of a civilization. Expanding beyond it should deepen our care for this home rather than weaken it. A second, genuinely self-sustaining population could also reduce the risk that one catastrophe ends every human story. That is a reason for expansion, though not a command and not the whole case.

Earthrise, photographed from lunar orbit on December 24, 1968

One home in the dark Earthrise, photographed from lunar orbit by the Apollo 8 crew on December 24, 1968. Seeing Earth’s vulnerability should intensify care for it, whether or not another home is ever built. via Wikimedia Commons

The ultimate astronomical limit is unimaginably far away. In roughly five billion years, the Sun is expected to swell into a red giant. That horizon should not guide next year’s budget; it simply reveals what becomes true on a long enough clock. A civilization that survives long enough may eventually need another home.

Nearer risks make the insurance argument less remote, but also less tidy. Different threats have different probabilities, warning times, and remedies. A second self-sustaining population might protect against some catastrophes; it would do little against dangers carried deliberately or inadvertently between worlds, and building it would create risks of its own. A base that depends on constant cargo from Earth provides no independent refuge. It is still another room of the same house, connected by a very long hallway.

The distance is real

The Moon is days away. Mars is months away when the planets are favorably placed. The nearest star, Proxima Centauri, is about 4.25 light-years from Earth, a distance no existing propulsion system makes into a human journey. Voyager 1 is moving away from the Sun at about 3.5 astronomical units per year; at that speed, crossing the distance to Proxima would take tens of thousands of years.

“The stars” therefore names a direction and a scale of ambition. The practical work begins nearby with projects such as NASA’s current Moon to Mars architecture, which aims at sustained lunar operations and eventual human exploration of Mars. Those are exploration plans. An independent city is a much harder thing.

The difference appears when the first generation is no longer temporary. Explorers can tolerate extraordinary danger because they expect to go home; settlers eventually have to produce more of what they need locally, recover from a missed ship without assuming another will arrive in time, raise children, care for the injured and old, and bury people who never return to Earth.

Once residents expect to remain, settlement stops being mainly a transportation problem. It becomes a question of whether a place can support dependence as well as performance, recover when plans fail, and give later residents lives not wholly assigned by the founders.

More than insurance

Survival is the sternest reason to expand, but it is too thin to sustain the whole undertaking. Another world could offer discoveries that remote instruments may never make, the intrinsic good of difficult exploration, and room for communities whose institutions develop differently from those on Earth—provided settlers remain citizens rather than property of the government or company that financed their passage.

The stronger case is more ordinary. Life is good, and human possibility is not exhausted. We do not know what music would be written under another sky, what customs would grow out of another landscape, or what a child raised on Mars would notice about Earth that we have missed. Those are not returns that fit neatly into a project plan. They are part of what the project is for.

Nothing about population growth guarantees this future. A civilization that no longer replaces itself simply reaches for it with less margin and fewer successors.