More evidence that the building blocks of life on Earth came from meteorites

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There is more evidence that the building blocks of life on Earth came from meteorites, according to international researchers, who analysed three carbon-rich meteorites and found evidence of multiple compounds needed for DNA or RNA. The researchers used state-of-the-art analytical techniques on the meteorites, finding guanine, adenine, uracil, cytosine, and thymine molecules which they say may have served as building blocks of life on Earth. 

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From: Springer Nature

Planetary science: Building blocks of DNA detected in meteorites

Pyrimidine nucleobases that are necessary for building DNA or RNA may have been delivered to Earth by carbon-rich meteorites, suggests a paper published in Nature Communications.

Two types of chemical building blocks, or nucleobases, are needed to form DNA and RNA. These are the pyrimidines, which include cytosine, uracil and thymine, and the purines, for example guanine and adenine. Thus far, only purine nucleobases and uracil have been identified in meteorites. However, the detection of pyrimidines in laboratory experiments simulating conditions in the interstellar media — the space between stars — has led to speculation that meteoritic delivery may have occurred.

Using state-of-the-art analytical techniques optimised for the small-scale quantification of nucleobases, Yasuhiro Oba and colleagues analysed 3 carbon-rich meteorites; the Murchison, Murray and Tagish Lake meteorites. In addition to compounds that have previously been detected in meteorites — such as guanine, adenine and uracil — the authors identify various pyrimidine nucleobases, such as cytosine and thymine, for the first time at concentration levels up to parts per billion. These compounds are present at concentrations similar to those predicted by experiments replicating conditions which existed prior to the formation of the solar system.

The authors conclude that these findings suggest that such compounds may have been partly generated by photochemical reactions in the interstellar media, which later led to their incorporation into asteroids as the solar system formed. Their eventual delivery to Earth by meteorites may have subsequently played a role in the emergence of genetic functions for early life.

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conference:
Nature Communications
Research:Paper
Organisation/s: Hokkaido University, Japan
Funder: This work was partly supported by JSPS KAKENHI Grant Numbers JP21H04501 and JP21H05414 (to Y.O.), JP20H02019 and 21KK0062 (to Y.T.), 21J00504 (to T.K), JP20H00202 and JP20H05846 (to H.N.), NASA Astrobiology Institute through award 13-13NAI7-0032 to the Goddard Center for Astrobiology (GCA), NASA’s Planetary Science Division Internal Scientist Funding Program through the Fundamental Laboratory Research (FLaRe) work package at NASA Goddard Space Flight Center, and a grant from the Simons Foundation (SCOL award 302497 to J.P.D.). This study was conducted in accordance with the Joint Research Promotion Project at the Institute of Low-Temperature Science, Hokkaido University (21G008 to Y.O., Y.T., and H.N.).
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