Slow-moving rocks better odds that life crashed to Earth from space

September 24, 2012 by Morgan Kelly, Princeton University

Researchers based at Princeton University, the University of Arizona and the Centro de Astrobiología in Spain used a low-velocity process called weak transfer to provide the strongest support yet for "lithopanspermia," the idea that the microorganisms that sprout life came to Earth -- or spread from Earth to other developing planets -- via collisions with meteorite-like planetary fragments. Under weak transfer, a slow-moving planetary fragment meanders into the outer edge of the gravitational pull, or weak stability boundary, of a planetary system. The system has only a loose grip on the fragment, meaning the fragment can escape and be propelled into space, drifting until it is pulled in by another planetary system. Credit: Amaya Moro-Martín
(—Microorganisms that crashed to Earth embedded in the fragments of distant planets might have been the sprouts of life on this one, according to new research from Princeton University, the University of Arizona and the Centro de Astrobiología (CAB) in Spain.

The researchers report in the journal that under certain conditions there is a high probability that life came to Earth—or spread from Earth to other planets—during the solar system's infancy when Earth and its planetary neighbors orbiting other stars would have been close enough to each other to exchange lots of solid material. The work will be presented at the 2012 European Congress on Sept. 25.

The findings provide the strongest support yet for "lithopanspermia," the idea that basic life forms are distributed throughout the universe via -like planetary fragments cast forth by such as and collisions with other matter. Eventually, another 's gravity traps these roaming rocks, which can result in a mingling that transfers any living cargo.

Previous research on this possible phenomenon suggests that the speed with which solid matter hurtles through the cosmos makes the chances of being snagged by another object highly unlikely. But the Princeton, Arizona and CAB researchers reconsidered lithopanspermia under a low-velocity process called weak transfer wherein meander out of the orbit of one large object and happen into the orbit of another. In this case, the researchers factored in velocities 50 times slower than previous estimates, or about 100 meters per second.

Using the star cluster in which our sun was born as a model, the team conducted simulations showing that at these lower speeds the transfer of solid material from one star's planetary system to another could have been far more likely than previously thought, explained first author Edward Belbruno, a and visiting research collaborator in Princeton's Department of Astrophysical Sciences who developed the principles of weak transfer.

The researchers suggest that of all the boulders cast off from our solar system and its closest neighbor, five to 12 out of 10,000 could have been captured by the other. Earlier simulations had suggested chances as slim as one in a million.

"Our work says the opposite of most previous work," Belbruno said. "It says that lithopanspermia 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."

Co-authors Amaya Moro-Martín, an astronomer at CAB and a Princeton visiting research collaborator in astrophysical sciences, and Renu Malhotra, a professor of planetary sciences at Arizona, 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. Dmitry Savransky, a Princeton mechanical and aerospace engineering doctoral student, conducted the simulations.

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 . 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 said, "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 researchers explored the likelihood that our solar system exchanged solid matter with its closest planetary-system neighbor during the first hundreds of millions of years it existed. At that time, our sun belonged to a tight-knit star cluster filled with other planetary systems. The above simulation shows that two planetary systems (green and blue dots) -- about 3.26 light years apart -- orbit a common center of mass. Over a period of roughly 8.7 million years, various objects (black dots) are pulled in and repelled by the systems' gravity. Displaying weak transfer, one object (red dot) first wanders into the green system's gravity boundary and partially orbits it before being cast off. The red object then drifts before being pulled in by the blue planetary system. Credit: Dmitry Savransky
All about velocities

The Princeton-Arizona-CAB paper cites two previous studies that present the odds of solid matter from one planetary system being captured by another as being more or less dismal.

The first, a 2003 paper published in Astrobiology by Jay Melosh, a Purdue University earth and atmospheric sciences professor, questioned the probability that meteorites have ever escaped a terrestrial planet in Earth's solar system and wound up on a terrestrial planet in another system. The report concluded that the chances—about one in 10,000, or 0.01 percent—are "overwhelmingly unlikely" considering the speed a meteorite would need to travel (about six kilometers per second) and the roominess of space.

Belbruno and his co-authors calculated that under this scenario of high velocities and dispersed planetary systems, the probability of solid material from any planetary system striking another falls to as little as five in 100,000, or 0.005 percent.

Star birth clusters, which are tightly confined groups of stars and planetary systems, were introduced as a possible setting for lithopanspermia in a 2005 Astrobiology paper by David Spergel, Princeton's Charles A. Young Professor of Astronomy on the Class of 1897 Foundation and chair of astrophysical sciences, and University of Michigan physics professor Fred Adams.

Factoring in velocities of two to five kilometers per second, Spergel and Adams found that the chances of an exchange of life-bearing rocks between star systems clustered in groups of 30 to 1,000 could be as unlikely as one in a million to as good as one in 1,000, or 0.0001 to 0.1 percent, respectively. Spergel and Adams, however, limited their study to binary stars—or planetary systems with two stars—which might elevate star-to-star solid matter exchanges, Moro-Martín said.

Nonetheless, in clusters similar to those considered by Spergel and Adams, weak transfer involves relative velocities of no more than one kilometer per second, which substantially increases the probability of capture by other stars in the cluster. In other words, star clusters provide an ideal setting for weak transfer, Belbruno said.

The researchers suggest that ideal conditions for lithopanspermia in the sun's birth cluster, in the solar system and on Earth overlapped for several hundred million years (blue shaded area). Rock evidence suggests that the Earth (bottom line) contained surface water during a period when the relative velocities between the sun and its closest cluster neighbors (top line) were small enough to allow weak transfer to other planetary systems, and when the solar system (middle line) experienced high meteorite activity within the sun's weak gravitational boundary. If life arose on Earth shortly after surface water was available, life could have journeyed from Earth to another habitable world during this time, or vice versa if life had an early start in another planetary system. Credit: Amaya Moro-Martín

Chaotic in nature, weak transfer happens when a slow moving object such as a meteorite wanders into the outer edge of the gravitational pull of a larger object with a low relative velocity, such as a star or massive Jupiter-like planet. The smaller object partially orbits the large object, but the larger object has only a loose grip on it. This means the smaller object can escape and be propelled into space, drifting until it is pulled in by another large object.

Belbruno first demonstrated weak transfer with the Japanese lunar probe Hiten in 1991. A mechanical malfunction left the probe with insufficient fuel to enter the moon's orbit the traditional way, which is to approach at a high speed then fire retrorockets to slow down. Instead, Belbruno designed a weak-transfer trajectory that got the probe into orbit around the moon using a minimal amount of fuel.

Adams, co-author of the 2005 paper with Spergel, said that the work by Belbruno and his co-authors succeeds at pulling together the various factors of earlier lithopanspermia models and adding a substantial new element—chaos. Adams is familiar with the study but had no role in it.

"This paper takes the type of calculations that have been done before and makes an important generalization of previous work," Adams said. "Their work on chaos in this context also carries the subject forward. They make a careful assessment of a process that is dynamically quite complicated and chaotic in nature.

"They are breaking new ground from the viewpoint of dynamical astrophysics," Adams said. "Regarding the problem of lithopanspermia, this type of weak capture and weak escape is interesting because it allows for the ejection speeds to be small, and these slow speeds allow for higher probabilities of rock capture. To say it another way, chaos, in part, enhances the prospects for lithopanspermia."

To the simulator!

Star birth clusters satisfy two requirements for weak transfer, Moro-Martín said. First, the sending and receiving planetary systems must contain a massive planet that captures the passing solid matter in the weak-gravity boundary between itself and its parent star. Earth's solar system qualifies, and several other stars in the sun's birth cluster would too.

Second, both planetary systems must have low relative velocities. In the sun's stellar cluster, between 1,000 and 10,000 stars were gravitationally bound to one another for hundreds of millions of years, each with a velocity of no more than a sluggish one kilometer per second, Moro-Martín said.

The team simulated 5 million trajectories between single-star planetary systems—in a cluster with 4,300 stars—under three conditions: the solid matter's "source" and "target" stars were both the same mass as the sun; the target star was only half the sun's mass; or the source star was half the sun's mass.

The odds of a star capturing solid matter from another planetary system under these three scenarios are 15 (0.15 percent), five (0.05 percent) and 12 (0.12 percent) in 10,000, respectively, the researchers report—probabilities that exceed those under the conditions proposed by Melosh by a factor of 1 billion.

To estimate the actual amount of solid matter that could have been exchanged between the sun and its nearest star neighbor, the researchers used data and models pertaining to the movement and formation of asteroids, the Kuiper Belt—the solar system's massive outer ring of asteroids—and the Oort Cloud, a hypothesized collection of comets, ice and other matter about one light year from Earth's sun widely believed to be a primary source of comets and meteorites.

The researchers used this data to conclude that during a period of 10 million to 90 million years, anywhere between 100 trillion to 30 quadrillion solid matter objects weighing more than 10 kilograms transferred between the sun and its nearest cluster neighbor. Of these, some 200 billion rocks from early Earth could have been whisked away via weak transfer.

For lithopanspermia to happen, however, microorganisms first have to survive the long, radiation-soaked journey through space.

Moro-Martín and Malhotra consulted a 2009 paper an international team published in the Astrophysical Journal that determined how long microorganisms could survive in space based on the size of the solid matter hosting them. That group's computer simulations showed that survival times ranged from 12 million years for a boulder up to 3 centimeters (roughly one inch) in diameter, to 500 million years for a solid objects 2.67 meters (nearly nine feet) across.

The researchers estimated that under weak transfer, solid matter that had escaped one planet would need tens of millions of years to finally collide with another one. This falls within the lifespan of the sun's birth cluster, but means that lithopanspermia by weak transfer would have been limited to planetary fragments at least one meter, or about three feet, in size.

Matching the theory with life

As for the actual transfer of life, the researchers suggest that roughly 300 million lithopanspermia events could have occurred between our solar system and the closest planetary system.

But even if survived the trip to Earth, the planet had to be ready to receive them. The researchers reference rock-dating evidence suggesting that the Earth contained water when the solar system was only 288 million years old and that very early life might have emerged before the solar system was 718 million years old.

The sun's birth cluster—assumed to be roughly the same age as the Earth's solar system—slowly broke apart when the solar system was approximately 135 million to 535 million years old, Moro-Martín said. In addition, the sun could have been ripe for weak transfer up to 700 million years after the solar system formed.

So, if life arose on Earth shortly after surface water was available, there were possibly about 400 million years when life could have journeyed from the Earth to another habitable world, and vice versa, the researchers report. If life had an early start in other planetary systems and developed before the sun's birth cluster dispersed, life on Earth may have originated beyond our .

The paper stops short of calculating the likelihood of extrasolar life taking root on a terrestrial planet such as Earth, but the higher probability the researchers determined for solid-matter transfer makes that a more worthwhile pursuit, Moro-Martín said.

"Our study stops when the solid matter is trapped by the second planetary system, but for lithopanspermia to be completed it actually needs to land on a terrestrial planet where life could flourish," Moro-Martín said. "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.

"Our study does not prove lithopanspermia actually took place," Moro-Martín said, "but it indicates that it is an open possibility."

Explore further: Super-Earth unlikely able to transfer life to other planets

More information: The paper, "Chaotic Exchange of Solid Material between Planetary Systems: Implications for Lithopanspermia," was published Sept. 12 by Astrobiology. … 0.1089/ast.2012.0825

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1.7 / 5 (11) Sep 24, 2012
Second, both planetary systems must have low relative velocities. In the sun's stellar cluster, between 1,000 and 10,000 stars were gravitationally bound to one another for hundreds of millions of years, each with a velocity of no more than a sluggish one kilometer per second, Moro-Martín said.

Whatever gave you the idea that the Sun was inside a star cluster?

Last I check, the Sun wasn't known to be orbiting anything other than the CoG of the Milkyway.

For life to allegedly cross the galaxy at that velocity would take 36 billion years, or 18 billion years if it started near the center and expanded out radially, under ideal expansions.

In any case, this is 45% to nearly 200% longer than the alleged age of the universe
3.8 / 5 (10) Sep 24, 2012
Sigh! Stars are born in clusters where interstellar gas and dust become thick enough for gravity to dominate radiation pressure. After the stars are created, the biggest stars will turn into supernovas that will remove the remaining gas and dust from the cluster.

At this point star creation stops, and the new stars drift apart, since the gas and dust blown away by the supernovas leaves the stars not gravitationally bound to one another.

(Actually some pairs, triplets, quadruplets, etc. will remain gravitationally bound to become double, triple, and quadruple star systems.)
1.7 / 5 (11) Sep 24, 2012
So goes the hypothesis.
1.8 / 5 (5) Sep 25, 2012
Totally hypothetical and probably never provable.
not rated yet Sep 25, 2012
The problem with transpermia is that the likeliest environment for a rapid transit between chemical and biological evolution was here on Earth. In modern hydrothermal vent pathways life originates within ~ 0.1 million years, the longest lifetime of vents.

Even the more likely transpermia from Mars can't compete with such a rapid evolution of life if you run current numbers for hypervelocity impact and travel time survival.
5 / 5 (3) Sep 25, 2012
@ Lurker2358:

Read again, the research is not on transpermia to "cross the galaxy" but within the cluster stars that originate with the molecular clouds that makes stars.

It has been long known that the solar system originated within such a cluster as other stars by its observation in a number of tests, originally on inclusions that originate as the system's earliest bodies. [ http://www.aanda....d=129%22 ] The earliest calcium-aluminum inclusions (CAI) radioactive 60Fe and 26Al record showing a seeding supernova event, predicts formation of "the Sun in a relatively small cluster ... in agreement with dynamical requirements, i.e. stability of planetary orbits, existence of the Kuiper belt object Sedna, and formation of the Oort cloud (Adams 2010; Brasser et al. 2012)."

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