Life could have arrived on Earth in rocks from other solar systems, scientists revealed today.
Fragments of distant planets might have 'seeded' Earth with alien life billions of years ago in the early history of the solar system.
The finding hints that life might be more common in the universe than scientists had thought.
Researchers from Princeton University have calculated that there is a 'high probability' under certain conditions that life arrived in 'chunks' of other worlds.
Up to 100 trillion rocks are thought to have blasted between worlds when the Earth was still part of a cluster of nearby stars.
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The researchers say that the discovery has implications for life in the universe as a whole.
“Our work says the opposite of most previous work,” says Belbruno. “It says that this transfer might have been very likely, and it may be the first paper to demonstrate that.
"If this mechanism is true, it has implications for life in the universe as a whole. This could have happened anywhere.”
The findings provide the strongest support yet for lithopanspermia, the hypothesis that basic life forms are distributed throughout the universe via meteorite-like planetary fragments cast forth by disruptions such as volcanic eruptions and collisions with objects such as asteroids.
Eventually, another planetary system’s gravity traps these roaming rocks, which can result in a mingling that transfers any living cargo.
Previous research on this possible phenomenon suggested that the speed at which objects hurtle through space made the chance of them being captured by another planet very small.
However, this new research, based on computer simulations of the star cluster our Sun was born in, suggests that a process called weak transfer, in which solid objects can gradually meander out of the orbit of one object and into another, greatly increase the odds that this process could have happened.
The research is based on principles of weak transfer developed by mathematician Edward Belbruno (Princeton University), and is presented at EPSC by his collaborator Amaya Moro-Martín (Centro de Astrobiología and Princeton University).
Belbruno first demonstrated weak transfer in 1991 when guiding the Hiten probe to the Moon using minimal amounts of fuel.
The team noted that low velocities offer very high probabilities for the exchange of solid material via weak transfer, and also found that the timing of such an exchange could be compatible with the actual development of the solar system, as well as with the earliest known emergence of life on Earth.
The researchers report that the solar system and its nearest planetary-system neighbor could have swapped rocks at least 100 trillion times well before the Sun struck out from its native star cluster.
Furthermore, existing rock evidence shows that basic life forms could indeed date from the Sun’s birth cluster days -- and have been hardy enough to survive an interstellar journey and eventual impact.
“The conclusion from our work,” Moro-Martín says, “is that the weak transfer mechanism makes lithopanspermia a viable hypothesis because it would have allowed large quantities of solid material to be exchanged between planetary systems, and involves timescales that could potentially allow the survival of microorganisms embedded in large boulders.”
The study shows that exchange of material between different planetary systems is likely, but it stops short when the solid matter is captured by the second planetary system. For lithopanspermia to actually take place, the material needs to land on an Earth-like planet where life could flourish.
“The study of the probability of landing on a terrestrial planet is work that we now know is worth doing because large quantities of solid material originating from the first planetary system may be trapped by the second planetary system, waiting to land on a terrestrial planet,” says Moro-Martín. “Our study does not prove lithopanspermia actually took place, but it indicates that it is an open possibility.”