Panspermia |
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What is Life |
Panspermia
Picture this. In the beginning a comet hurtles towards Earth. It collides with an almighty impact 3.8 billion years ago. Much of the cometry material is vapourised. But some survives including dormant microbes buried deep in the comets interior for tens of million of years. And 3.8 billion years after the impact, the phrase to describe this phenonema is coined, Panspermia.
So did life on Earth arrive on the back of a comet 3.8 billion years ago? Could life have been transported from other parts of the galaxy? The theory of Panspermia suggests that we are all descendents of aliens. We have seen how the universe appears to be teeming with the molecules which are essential for all life on Earth. But was early life indigenous to Earth or could it have arrived from space and seeded the Earth? Could our family ancestory be traced back to aliens? Many Scientists seem to think it's as viable a proposition as say, the 'primordial soup' or the 'hydrothermal vent' hypothesis. But how do these molecules get to rendezvous with a planet like Earth, and make their way down to the surface? Comets could be the answer! They may be capable of bringing both life and death to planets.
Evidence from Comets
In 2014, the ESA's Rosetta spacecraft, launched in 2004, will rendezvous with Comet 67P/Churyumov-Gerasimenko. It will release a lander onto the icy surface. The landers instruments as well as the Rosetta spacecraft itself may unlock many secrets for us. Hence the name! The chemical composition of comets is known to be similar to the chemical composition of the solar system at the time of its formation. So it's like a window to 4.5 billion years ago. But for now we must wait and see. Incidently, to accomplish this mission is no mean achievement. It is a ten year journey for Rosetta, chasing and manoeuvring into orbit around a 'cosmic bullet', playing catch-up by using gravational 'kicks' from the Earth (three times) and Mars (once).
But would organic material embedded in a comet survive an impact on a rocky planet like Earth? High impact experiments have taken place in laboratories, replicating cometry impacts. Using small grains of rock, containing microbes, scientists have shown that it is possible for some microbes to survive these extremely high impacts. The vast mayority of microbes are destroyed in the impact, but it only takes a small fraction to survive and start to replicate at rapid speeds as microbes do. These experiments further strengthen the case for panspermia and the possiblity that comets supplied the early Earth with the requisite chemical molecules, thus permitting the process of chemical evolution to take place leading to the origin of life on Earth.
An Abundance of Comets
The formation of Solar systems seems to end up with a cometery reservoir surrounding, and in the far reaches, of the solar system. Comets are concentrated in two main regions in our solar system, the Kuiper belt and the Oort cloud.
Comets orbit our sun just as the planets do. The orbits of comets will sometimes take them into the inner solar system. This can be due to collisions amongst themselves, the effects of gravity from nearby passing stars or the gravitational attraction of the planets.
As a comet advances towards the sun it heats up, and essentially disintegrates, and begin to eject material. A trail of material is left which sometimes the orbit of the Earth will intersect. This we see as a meteor shower. But not all the material in the trail burns up. Some settles down through the atmosphere and reaches the surface of the Earth intact. Today its estimated that cometery dust grains contribute about 300 tonnes of organic materials to the Earth each year, Meteorites also contribute organic material. This material is sealed inside the meteorite as it plunges throught the atmosphere and its estimated that meteorites contribute about 10 kilograms of organic material annually.
The Kuiper Belt is a disk of debris in the ecliptic plane of the solar system. This 'junkyard' of material, left over from the formation of the solar system, may contain up to 100 million small icy objects, which orbit the sun beyond Neptune. This frigid and mysterious outer realm of the solar system also contains many larger objects. In fact Pluto and its moon Charon (3.6 billion miles from the sun) may actually be considered Kuiper Belt objects, as can the recently discovered Eris (9 billion miles from the sun). Though they have also been recently reclassified as dwarf planets. Comets from the Kuiper Belt are considered short-period comets which frequently return to the inner solar system.
The Oort cloud is a spherical cloud of trillions of icy objects surrounding the solar system, at a vast distance of up to two light years from the sun. Because of this immense distance the gravitational attraction of the sun is weak, and they can easily have their orbits perturbed by nearby stars or molecular clouds. This can result in some comets beginning a journey towards the inner solar system. These comets are called long-period comets.
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