Experimental and Numerical Modeling of Liposome Congregation in Meteorite Craters of Early Earth

editorAstrobiology5 hours ago7 Views

Experimental and Numerical Modeling of Liposome Congregation in Meteorite Craters of Early Earth

Summary of particle dynamics. The top and bottom rows compare results for steel and aluminum rods, respectively, while the left and right columns show the initial and final stages. (b) Dropping steel bars led to nearly complete particle collection at the center after N = 40 drops. (d) Dropping aluminum bars resulted in a profile that, although somewhat peaked, remained noticeably wide even after 80 drops. — Life

This paper provides experimental and numerical evidence supporting the occurrence of liposome congregation at the floors of meteor craters on Early Earth.

This work builds on our earlier research, which demonstrated that liposomes submerged in a shallow Archean pond are protected from harmful UV radiation.

This protection enables them to survive sufficiently long for autocatalytic amphiphile replication and for the mutation and selection of assemblies that enhance membrane stability.

For liposomes to fuse, grow, exchange contents and membrane components, and divide, they must establish a population, i.e., form a dense conglomerate that enables close physical contact.

The study demonstrates that such a congregation is feasible in bowl-shaped meteor craters on Early Earth, especially under periodic seismic disturbances.

Experimental and Numerical Modeling of Liposome Congregation in Meteorite Craters of Early Earth, Life (open access)

Astrobiology

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