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Astronomy

How Microbes Survive Interplanetary Ejection: Life, Rocks, and Panspermia

Quick fact

Some meteorites found on Earth are confirmed as Martian in origin, blasted off Mars by impacts. Experiments show that certain Earth microbes can survive the extreme acceleration and shock pressures of such an ejection, and even survive in space for years—hinting that life could indeed travel between planets.

Why this is interesting

Imagine a rock blasted off Mars, carrying a tiny community of microbes, crashing into Earth millions of years later. Could those ancient hitchhikers survive the journey and spark life here?

Read the full explanation

Understanding How Microbes Survive Interplanetary Ejection: Life, Rocks, and Panspermia

Think of a rock like a tiny spaceship. When an asteroid hits a planet, the impact can accelerate rocks to great speeds, overcoming gravity and sending them into space. Inside these rocks, microbes might be protected from the vacuum and radiation. The journey is long, but if the rock is big enough, its interior stays shielded from deadly cosmic rays. On arrival, the rock must survive a fiery dive through the new planet's atmosphere. Most burn up, but some break into smaller pieces that cool quickly and land safely. If the planet has liquid water, surviving microbes could potentially establish a new colony.

A deeper explanation

The survival of microbes during ejection and transit depends on beating several hurdles. First, the impact itself creates extreme shock pressures and temperatures. Some microbes, like the bacterium Deinococcus radiodurans, can withstand pressures up to tens of gigapascals and temperatures of hundreds of degrees Celsius for short periods—conditions found in impact ejecta. During the ejection process, the surface of the rock is heated and compressed, but the interior can remain cool. Next, the rock must survive millions of years in space, facing cosmic radiation and vacuum. Microbes in dormant spores can repair radiation damage upon rehydration. Finally, atmospheric entry heats the rock, but large rocks only heat on the surface, leaving the interior largely unaffected. Upon landing, the rock must not be completely sterilized, and the new world must be habitable. Laboratory experiments (e.g., on the International Space Station) and computer models confirm that these stages are physically plausible, which is why panspermia remains a serious scientific hypothesis rather than science fiction.

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