Earth and Mars May Have Shared Seeds of Life

Martian Rockbed
NASA's Curiosity rover identified weathered rock similar to those found in deltas where river sediment settled onto the lake floor. If the lakes lasted long enough, they could have housed microbial life in the early days of Mars. (Image credit: NASA/JPL-Caltech/MSSS)

Could Mars, of all places, be the place to look for early life on Earth?

It's an intriguing thought and one that astrobiologists take seriously as they consider the conditions during the early days of the solar system when both planets experienced frequent bombardments by asteroids and comets that resulted in debris exchange between one body and the other.

"We might be able to find evidence of our own origin in the most unlikely place, and this place is Mars," planetary scientist Nathalie Cabrolof the SETI institute said in a TED Talk in April 2015. [The Life on Mars Search: Photo Timeline]

Cabrol studies life in extreme conditions on Earth with the hope that her research might help improve the search for signs of life on the Red Planet.

"We can go to Mars and try to find traces of our own origin. Mars may hold that secret for us," she said. "This is why Mars is so special to us."

Throwing rocks

Mars orbits an average of 140 million miles (225 million kilometers) from Earth and has a similar size and composition. During the period of the Late Heavy Bombardment, about 3.8 billion to 4 billion years ago, the planets were pummeled with asteroids and comets, which may have also provided the water to much of the Earth's oceans. Earth and Mars were, in a sense, connected to each other by the violence of this era. 

"Earth and Mars kept throwing rocks at each other for a very long time," Cabrol said.

If life spawned on one planet, it could have clung to one or more of these samples and traveled to the other, a process scientists call panspermia. But if early Earth life did make it to Mars, it would have needed a hospitable arrival.

Today the planet is bleak and barren, resembling the Earth's most desolate deserts. With its thin atmosphere and almost completely waterless surface, any life that landed on Mars today would have a difficult time taking hold. But in the past, when the rocks were flying, Mars likely boasted a more habitable environment.

"At the time when life appeared on the Earth, Mars did have an ocean, it had volcanoes, it had lakes, and it had deltas," Cabrol said.

Yet unlike Earth, the Red Planet quickly lost its hold on habitability.

"When lifeexploded at the surface of the Earth, then everything went south for Mars," Cabrol said.

Because Mars lacks a protective magnetic field, the sun's solar wind stripped it of its atmosphere and exposed the surface to bombardment from cosmic rays and ultraviolet (UV) light. Most of the water left the surface, escaping into space. Only a few pockets remain on the surface today, at the poles, while some water may lurk beneath the ground.

"There is no life possible on the surface of Mars today, but it might still be hiding underground," Cabrol said.

Licancabur Lake lies at the top of the Andes Mountains, where the low oxygen, thin altitude and high ultraviolet radiation create conditions similar to those found on ancient Mars. (Image credit: The High Lakes Project: The SETI Institute Carl Sagan Center/NASA Ames/ NAI)


A time machine

To understand what life might have done as the planet's situation grew more bleak, Cabrol said scientists need the ability to peer back at the Mars of the past.

"You only need to go back 3.5 billion years ago in the past of a planet," she said. "We just need a time machine."

Today, Cabrol uses Earth as her time machine, traveling to regions that resemble the Red Planet in its past.

"I use planet Earth to go in very extreme environments where conditions were similar to those of Mars at the time when the climate changed," Cabrol said.

One of those regions lies at the top of the Andes Mountains in Chile. Volcanic lakes fill the cone of the volcano, making it a unique analogue to Mars. The region is situated at an elevation of 3.6 miles (5.872 km), where UV rays more easily pierce a thin atmosphere. Cabrol traveled there as part of the High Lakes project, funded by a grant from the NASA Astrobiology Institute (NAI) element of the Astrobiology Program at NASA.

"At this altitude, this lake is experiencing exactly the same conditions as those on Mars three and a half billion years ago," Cabrol said.

Cabrol and her team changed from mountain climbing equipment to diving gear to sample the interior of one such lake. They found that "life is everywhere, absolutely everywhere," she said.

Yet the amount of life in the lake can be deceiving. According to Cabrol, 36 percent of the samples her team took home were made up of only three species, typifying the deadly environment.

"There is a huge loss in biodiversity," she said. "Those three species are the ones that have survived so far."

If life exists on Mars, it is likely to be similarly lacking in biodiversity. Only the hardiest microbes may have survived the planet's decline.

In another nearby lake, similar conditions have driven the algae within to adapt, giving the water a reddish cast. On Earth, a score of 11 in the UV Index, which provides a forecast of the expected risk of overexposure to the sun's ultraviolet radiation, is considered to be extreme. During UV storms, the UV Index at Aguas Calientes lake can reach as high as 43, the highest UV radiation levels measured on Earth. The water is so clear that the algae have nowhere to hide from the deadly radiation, so they must find other ways to protect themselves.

The red color of Aguas Calientes comes from algae, which must create their protection from the harsh ultraviolet radiation coming from the sun. (Image credit: The High Lakes Project: The SETI Institute Carl Sagan Center/NASA Ames/ NAI)

"They are developing their own sunscreen," Cabrol said, "and this is the red color you see."

While the lakes give some insight into what could be happening on Mars in the past, they don't suggest what could have happened to organisms on the planet when there were no pools left to hide in.

"When all the water is gone from the surface, microbes have only one solution left — they go underground," Cabrol said.

In addition to studying pools at high altitude, her team also examined microbes that seek shelter from the sun's radiation. Cabrol showed images of semi-translucent rocks with microbes hiding beneath, while still taking some energy from the sun.

"They are using the protection of the translucence of the rocks to get the good part of the UV, and discard the part that could actually damage their DNA," Cabrol said.

Studying these organisms can help scientists searching for life on Mars with rovers such as Curiosity.

"If there was life on Mars three and a half billion years ago, it had to use the same strategy to actually protect itself," Cabrol said.

'Our legacy'

This illustration depicts a lake of water partially filling Mars' Gale Crater, collecting runoff from melting snow on the northern rim. If they lasted long enough, such lakes could have served as refuge for microbial life on Mars. (Image credit: NASA/JPL-Caltech/ESA/DLR/FU Berlin/MSSS)

Mars isn't the only place life might thrive in the solar system. Scientists think a subsurface ocean could exist on Jupiter's moons Europa and Ganymede, and on Saturn's moons Titan and Enceladus. Cabrol develops science exploration strategies for these icy moons, where microbes may have evolved.

Unlike Mars, other bodies in the solar system would have had a more difficult time exchanging material.

"Mars and Earth could have a common root to their tree of life, but when you go beyond Mars, it's not that easy," Cabrol said. "If we were to discover life on those planets [and moons], it would be different from us."

Extraterrestrial life in the form of microbes, should it be found, may not lead to an equal exchange of intelligence, but primitive life can still answer questions about the existence of life, Cabrol said.

"Organic material is going to tell you about environment, about complexity, and about diversity. DNA, or any information carrier, is going to tell you about adaptation, about evolution, about survival, about planetary change, and about the transfer of information," she said. "All together, they are telling us why what started as a microbial pathway sometimes ends up as a civilization or sometimes ends up as a dead end."

Within our solar system, these questions could be answered in the not-too-distant future, she said.

"This can be achieved by our generation," Cabrol said. "This can be our legacy—but only if we dare to explore."

This story was provided by Astrobiology Magazine, a web-based publication sponsored by the NASA astrobiology program. Follow on Twitter, Facebook and Google+.

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Nola Taylor Tillman
Contributing Writer

Nola Taylor Tillman is a contributing writer for She loves all things space and astronomy-related, and enjoys the opportunity to learn more. She has a Bachelor’s degree in English and Astrophysics from Agnes Scott college and served as an intern at Sky & Telescope magazine. In her free time, she homeschools her four children. Follow her on Twitter at @NolaTRedd