2022
DOI: 10.3847/1538-3881/ac63d0
|View full text |Cite
|
Sign up to set email alerts
|

Origins of Chiral Life in Interstellar Molecular Clouds

Abstract: The exploring of galactic chemical composition across the the Milky Way, and specifically across the solar neighborhood, provides insights into the chemical evolution of the universe. Since the formation of the first stars some hundred million years after the big bang (BB), heavier elements are synthesized in different stellar production processes at the expense of lighter elements. When the relative abundances of the life-forming elements evaluated for the Last Universal Common Ancestor (LUCA) are compared wi… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2023
2023
2024
2024

Publication Types

Select...
2
1

Relationship

0
3

Authors

Journals

citations
Cited by 3 publications
(1 citation statement)
references
References 50 publications
0
1
0
Order By: Relevance
“…There are two ways via which enantioenrichment may occur in the ISM. The first way could be through the asymmetry induced in elastic proton–proton scattering. Through this process, one enantiomer could be selectively destroyed. The other way of enantioenrichment is similar to what is done in terrestrial asymmetric synthesis, via the use of “chiral auxiliaries” .…”
Section: Discussionmentioning
confidence: 99%
“…There are two ways via which enantioenrichment may occur in the ISM. The first way could be through the asymmetry induced in elastic proton–proton scattering. Through this process, one enantiomer could be selectively destroyed. The other way of enantioenrichment is similar to what is done in terrestrial asymmetric synthesis, via the use of “chiral auxiliaries” .…”
Section: Discussionmentioning
confidence: 99%