Does the organic material of comets pre-date our solar system?

The Rosetta space probe discovered a large amount of organic material in the nucleus of comet 67P Churyumov-Gerasimenko. Researchers now advance the theory that this matter has its origin in interstellar space and before the solar system formed. According to a new paper by Jean-Loup Bertaux and Rosine Lallement – from the Laboratoire Atmosphères, Milieux, Observations Spatiales (CNRS / UPMC / Université de Versailles Saint-Quentin-en-Yvelines) and the Galaxies, Étoiles, Physique et Instrumentation department of the Paris Observatory (Observatoire de Paris / CNRS / Université Paris Diderot), respectively – these organic molecules were produced in interstellar space, well before the formation of the Solar System. Bertaux and Lallement further assert that astronomers are already familiar with much of this matter. They refer to the diffuse interstellar bands, discovered nearly 100 years ago. For some time now there has been strong evidence that these absorption bands, observed in the spectra of stars seen through and dimmed by dense interstellar clouds, originate from large molecular carriers. Science Daily continues the story:

For [more than] seventy years, scientists have known that analysis of stellar spectra indicates unknown absorptions, throughout interstellar space, at specific wavelengths called the diffuse interstellar bands (DIBs). DIBs are attributed to complex organic molecules that US astrophysicist Theodore Snow believes may constitute the largest known reservoir of organic matter in the Universe. This interstellar organic material is usually found in the same proportions. However, very dense clouds of matter [such as nebulae which are or may go on to forming stars] are exceptions. In the middle of these nebulae, where matter is very dense, DIB absorptions plateau or even drop. This is because the organic molecules responsible for DIBs clump together there. The clumped matter absorbs less radiation than when it floated freely in space. Such primitive nebulae end up contracting to form a solar system like our own, with planets, and comets. The Rosetta mission taught us that comet nuclei form by gentle accretion of grains progressively greater in size. First, small particles stick together into larger grains. These in turn combine into larger chunks, and so on, until they form a comet nucleus a few kilometers wide. Thus, the organic molecules that formerly populated the primitive nebulae — and that are responsible for DIBs — were probably not destroyed, but instead incorporated into the grains making up cometary nuclei. And they may have remained there for longer than the 4.6 billion year age of the solar system. A sample-return mission would allow laboratory analysis of cometary organic material [to identify and date this material] and finally reveal the identity of the mysterious interstellar matter underlying observed absorption lines in stellar spectra. If cometary organic molecules were indeed produced in interstellar space — and if they played a role in the emergence of life on our planet, as scientists believe today — might they not also have seeded life on many other planets of our galaxy?

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