Scientists have found the interstellar organic matter could produce an abundant supply of water by heating, suggesting that organic matter could be the source of terrestrial water.
Organic matter in nebula could be the source of terrestrial water. Photo: NASA, ESA, and theHubble Heritage Team (STScI/AURA)
There remains a number of mysteries on our planet including the elusive origin of water on the earth. Active studies suggested that terrestrial water had been delivered by icy comets or meteorites containing hydrous silicates that came from outside the “snow line” – the boundary beyond which ice can condense due the low temperatures. More recent studies, however, have provided observations opposing to cometary origin theory, yet still failing to suggest plausible substitutions for the source of terrestrial water. “Until now, much less attention has been paid to organic matter, comparing to ices and silicates, even though there is an abundance inside the snow line” says planetary scientist Akira Kouchi at Hokkaido University.
In the current study published in Scientific Reports , a group of scientists led by
Akira Kouchi demonstrates that heating of the interstellar organic matter at high temperature could yield abundant water and oil. This suggests that water could be produced inside the snow line, without any contribution of comets or meteorites delivered from outside the snow line
As a first step, the researchers made an analog of organic matter in interstellar molecular clouds using chemical reagents. To make the analog, they referred to analytical data of interstellar organics made by irradiating UV on a mixture containing H2O, CO, and NH3, which mimicked its natural synthetic process. Then, they gradually heated the organic matter analog from 24 to 400 ℃ under a pressured condition in a diamond anvil cell. The sample was uniform until 100 ℃, but was separated into two phases at 200 ℃. At approximately 350 ℃, the formation of water droplets became evident and the sizes of the droplets increased as the temperature rose. At 400 ℃, in addition to water droplets, black oil was produced.
The interstellar organic matter analog producing water droplets and oil as the heating temperature rose. At 102 ℃, analog of organic matter was uniform. At 350 ℃, water droplets were clearly seen. At 400 ℃, black oil was evidently produced. (Hideyuki Nakano et al., Scientific Reports, May 8, 2020)
The group conducted similar experiments with larger amounts of organic matter, which also yielded water and oil. Their analysis of absorption spectra revealed that the main component of the aqueous product was pure water. Additionally, chemical analysis of produced oil showed similar characteristics to the typical crude oil found beneath the earth.
After heating at 400 ℃, analog of interstellar organic matter clearly separated into two layers of oil (black) and water (yellowish transparent) (a: before heating, b: after heating at 400 ℃). (Hideyuki Nakano et al., Scientific Reports, May 8, 2020)
“Our results show that the interstellar organic matter inside the snow line is a potential source of water on the earth. Moreover, the abiotic oil formation we observed suggests more extensive sources of petroleum for the ancient Earth than previously thought,” says Akira Kouchi. “Future analyses of organic matter in samples from the asteroid Ryugu, which the Japan’s asteroid explorer Hayabusa2 will bring back later this year, should advance our understanding of the origin of terrestrial water.”
Nakano H. et al., Precometary Organic Matter: A Hidden Reservoir of Water Inside the Snow Line. Scientific Reports. May 8, 2020
This study was supported by the Ministry of Education, Culture, Sports, Science, and Technology Grants-in-Aid for Scientific Research (25108002), and by the Japan Society for the Promotion of Science (JSPS)’s KAKENHI grant (17H06087).