The Bubble Nebula
The building blocks for DNA could have been generated or combined within these interstellar clouds of the amazing Bubble Nebula!

Over 13 billion years ago at least one of the domains of life may have begun in nebular clouds, such as the Bubble Nebula. If restricted to the Milky Way, which is 13.6 billion years old, the first chemical combinations would have had billions of years to become a self-replicating organism with a DNA genome long before the existence of Earth.
The Bubble Nebula, NGC 7635 shown above, was discovered in 1787 by William Herschel and is shown here in a Hubble Space Telescope WFC3 image. The outer edge of the bubble – 7 light years across – comprises cold interstellar gas displaced by winds from a 45-solar-mass young O star (BD +60°2522), seen off-center at 10 o’clock. Dense pillars of cool hydrogen gas appear above and behind the bubble. Blue colors indicate oxygen, green is hydrogen, and red is nitrogen.

Above and left of the Bubble’s center is the hot, O-type star, several 100,000 times more luminous and approximately 45 times more massive than our Sun. Fierce stellar winds and intense radiation from that star has blasted out the structure of glowing gas against denser material in a surrounding molecular cloud.

The Bubble Nebula
The Bubble Nebula, also known as NGC 7635, is an emission nebula located 8 000 light-years away. This stunning new image was observed by the NASA/ESA Hubble Space Telescope to celebrate its 26th year in space.

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Nebular clouds are thought to be most likely environment for synthesizing and promoting the evolution of molecules needed for the origin of life. The building blocks for DNA could have been generated or combined within interstellar clouds and DNA would become part of the molecular-protein-amino acid complex. Hydrogen, oxygen, carbon, calcium, sulfur, nitrogen and phosphorus for example are continually irradiated by ions, which can generate small organic molecules which evolve into larger complex organic molecules that result in the formation of amino acids and other compounds.

Phosphorus, for example, is rare in our solar system and may have been non-existent on the early Earth; phosphorus is essential for the manufacture of DNA.

Polarized radiation in the nebula cloud leads to the formation of proteins, nucleobases and then DNA. The combination of hydrogen, carbon, oxygen, nitrogen, cyanide and several other elements, could create adenine, which is a DNA base, whereas oxygen and phosphorus could ladder DNA base pairs. Glycine has also been identified in the interstellar clouds.

Fast forward 4.6 billion years, on Earth the steps leading from the random mixing of chemicals to the first nano-particle would likely require hundreds of millions and even billions of years before the first self-replicating molecular compound was fashioned. Even after billions of years, the first replicon may not have possessed DNA.

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