Deinococcus,Radiodurans,-,This,Bacterium,Is,Known,For,Its,Extreme

Deinococcus radiodurans - this bacterium is known for its extreme resistance to ionizing radiation and oxidative stress (Credit: luchschenF on Shutterstock)

A New Experiment Strengthens The Case For Interplanetary Survival.

In A Nutshell

  • A Johns Hopkins team fired one of Earth’s toughest bacteria through lab-simulated Mars impact pressures and found it survived at rates near 95 percent.
  • The results strengthen the lithopanspermia hypothesis, the idea that life could travel between planets inside asteroid-launched rocks.
  • The bacterium, Deinococcus radiodurans, outperformed common lab microbes like E. coli by orders of magnitude under the same conditions.
  • The study does not prove life has ever traveled between planets, but it removes a major obstacle to the idea being physically possible.

Rocks from Mars have landed on Earth. Scientists have found them, meteorites with a chemical signature that could only have come from the Red Planet, scattered across Antarctica and other remote corners of the globe. The question that has never been answered is whether anything alive could have survived the trip.

A Johns Hopkins University team decided to test the most brutal part of that scenario: the moment an asteroid slams into Mars and hurls chunks of rock off the surface and into space. Could a living organism survive that initial violent launch? The team picked one of Earth’s toughest known bacteria, fired it through conditions designed to replicate a Martian impact ejection, and watched what happened. The results, published in PNAS Nexus, push survival limits well beyond what earlier impact experiments had shown.

At pressures comparable to those that send rocks off Mars at escape velocity, the bacterium Deinococcus radiodurans survived at rates near 95 percent. That puts this research at the center of a long-running debate called the lithopanspermia hypothesis, the idea that life can travel between planets aboard asteroid-launched rocks. Prior work had already shown this microbe can handle the radiation, cold, and drying of interplanetary space. Now it appears capable of surviving the launch phase under at least some realistic ejection pressures.

The Mars-Ready Microbe That Keeps Defying Expectations

Deinococcus radiodurans is not a typical lab microbe. Scientists first found it in the 1950s inside a can of ground beef that had been sterilized with radiation, only to discover something was still alive inside. Since then it has become the gold standard for biological toughness: radiation, drought, extreme cold, the vacuum of space. It passes every test researchers throw at it.

What had never been tested was its response to high-velocity impact pressure, the kind generated when an asteroid strikes a planet. That gap mattered enormously, since the launch phase of any interplanetary journey would expose microbial passengers to some of the most intense mechanical forces imaginable.

microbes space travel
After shooting the microbes, the team determined whether they survived and examined the survivors’ genetic material for clues to how they handled the pressure. The bacteria proved very hard to kill. They survived nearly every test at 1.4 Gigapascal of pressure and 60% at 2.4 Gigapascals of pressure. The cells showed no signs of damage after the lower pressure hits, but after the higher pressure experiments, the team observed some ruptured membranes and internal damage. (Credit: Johns Hopkins University)

Simulating a Mars Asteroid Impact in the Lab

To recreate a planetary impact, the team adapted a gas gun system originally built to study how materials behave under extreme stress. A metal projectile was fired into a target assembly holding a thin layer of bacteria sandwiched between two steel plates. Each collision lasted only microseconds, with pressures measured in real time by laser-based sensors.

About one billion D. radiodurans cells went into each test. Alongside every shot, the team ran control samples, identical bacteria that went through every step except the actual impact, to isolate precisely what the collision did to survival. Shots were fired at pressures between 1.4 and nearly 3 gigapascals. One gigapascal is roughly 10,000 times the air pressure at sea level on Earth. Computer models suggest rocks ejected from Mars at escape velocity experience pressures generally below 5 gigapascals, putting the team’s experiments squarely within real-world ejection territory.

Survival Rates That Change the Search for Life on Mars

At 1.4 gigapascals, D. radiodurans survived at around 95 percent across multiple trials. Survival dropped to about 86 percent at 1.9 gigapascals and roughly 60 percent at 2.4 gigapascals. Near 3 gigapascals, survival was still measurable but sharply reduced, with the 2.9 gigapascal test producing less than 10 percent survival, though the exact rate was difficult to pin down precisely due to experimental constraints. All tests used actively growing cells, not dormant spores, which tend to be hardier.

By comparison, common bacteria like Escherichia coli and Shewanella oneidensis survived at rates of just 0.01 to 1 percent under similar pressures in earlier studies.

“Our results suggested that microorganisms can survive much more extreme conditions than previously thought, potentially surviving conditions that result in the formation of ejecta that can move across planetary systems,” the authors wrote.

Electron microscope images confirmed the pattern. Bacteria hit at 1.4 gigapascals looked nearly normal afterward. Those hit at 2.4 gigapascals showed a mixed picture: some undamaged, others with ruptured membranes and internal damage that matched the lower survival count at that pressure.

After the hardest impacts, surviving cells switched into repair mode, turning on genes that fix damaged DNA and stabilize their outer membranes, while slowing down growth. a response pattern the researchers recognized from studies of D. radiodurans under intense radiation. The team noted this was the first time scientists had examined gene-level responses in microbes subjected to high-velocity impact pressures.

A structural advantage likely helps explain the organism’s edge. Its unusually thick, multi-layered cell envelope, including a crystalline protein coat called an S-layer, appears to provide reinforcement that ordinary bacteria lack. The researchers hypothesized that cells are most likely to rupture not during impact itself but during the rapid pressure release that follows, and that thicker-walled cells hold up better against that release.

The experiment simulated the pressure of an asteroid strike and ejection from Mars by sandwiching the microbe between metal plates and then firing a projectile at it from a gas gun. The projectile hit the plates at speeds up to 300 mph, generating 1 to 3 Gigapascals of pressure. (Credit: Johns Hopkins University)

A New Case for Life Traveling Between Planets

For decades, the explosive launch off a planet’s surface was considered one of the toughest obstacles to the idea of life traveling across the solar system. This research weakens that obstacle, at least for one exceptionally tough microbe under certain ejection pressures. It does not prove that life has ever made the trip, nor does it address what happens during the long journey through space or the violent entry into another planet’s atmosphere. But on the specific question of launch survival, the answer is more encouraging than scientists had reason to expect. As the authors noted, “it is possible for such life to be transported between planets in the Solar System as a result of major asteroid impacts.”

Martian rocks have already made it to Earth. The more unsettling question now isn’t only whether the trip is physically possible, but whether something was ever riding along.


Paper Notes

Study Limitations

This study focused exclusively on Deinococcus radiodurans, chosen for its known resilience. Whether other microbes, including organisms that may have once inhabited Mars, would behave similarly is unknown. The experimental setup is a carefully controlled laboratory approximation of impact conditions and cannot fully replicate a real planetary ejection event, where microbes inside porous rock would experience more varied stress states. The gene expression analysis lacked biological replicates due to the difficulty of conducting impact experiments, making those results semi-quantitative. The power-law model used to estimate survival at higher pressures is a mathematical approximation that may not hold at extreme values, and the authors note it may not be appropriate for very low survival rates.

Funding and Disclosures

This research was supported by the Planetary Protection Research program of the National Aeronautics and Space Administration (NASA) through grant number 80NSSC20K0667. The authors declared no competing interests.

Publication Details

Authors: Lily Zhao, Cesar A. Perez-Fernandez, Jocelyne DiRuggiero, and K. T. Ramesh, all affiliated with Johns Hopkins University, Baltimore, Maryland. Correspondence: K. T. Ramesh. | Journal: PNAS Nexus, Volume 5, March 2026. | Paper Title: “Extremophile survives the transient pressures associated with impact-induced ejection from Mars.” | DOI: https://doi.org/10.1093/pnasnexus/pgag018 | Advance Access Publication: March 3, 2026. This is an open-access article distributed under the Creative Commons Attribution-NonCommercial License.

About StudyFinds Analysis

Called "brilliant," "fantastic," and "spot on" by scientists and researchers, our acclaimed StudyFinds Analysis articles are created using an exclusive AI-based model with complete human oversight by the StudyFinds Editorial Team. For these articles, we use an unparalleled LLM process across multiple systems to analyze entire journal papers, extract data, and create accurate, accessible content. Our writing and editing team proofreads and polishes each and every article before publishing. With recent studies showing that artificial intelligence can interpret scientific research as well as (or even better) than field experts and specialists, StudyFinds was among the earliest to adopt and test this technology before approving its widespread use on our site. We stand by our practice and continuously update our processes to ensure the very highest level of accuracy. Read our AI Policy (link below) for more information.

Our Editorial Process

StudyFinds publishes digestible, agenda-free, transparent research summaries that are intended to inform the reader as well as stir civil, educated debate. We do not agree nor disagree with any of the studies we post, rather, we encourage our readers to debate the veracity of the findings themselves. All articles published on StudyFinds are vetted by our editors prior to publication and include links back to the source or corresponding journal article, if possible.

Our Editorial Team

Steve Fink

Editor-in-Chief

John Anderer

Associate Editor

Leave a Reply

1 Comment

  1. Kevin Ryder, PhD (but not a paleobiologist) says:

    I am curious as to hypotheses on why/how Deinococcus radiodurans evolved to be this resistant to forces that, for other bacteria, would be life ending? My initial thought (with the caveat that your first idea is ususally not your best), is that the species evolved in an environment where impacts were common, and that due to selective pressure over time, they evolved tougher outer membranes. The initial impacts selecting for this trait might not have been powerful enoufh to acheive ejection velocities, but over time could have evolved to such a state. A corrollary question is, going back a couple of billion years, which of Mars or Earth provided the most likely environment for such evolution; a variable in this would have been antmospheric density of each of Mars and Earth at the time, since greater density would affect both initial impact velocity/frequency as well escape velocity (though obviously gravities of each would also differ thereby affecting escape velocity).