Physical conditions on early earth: Implications for the origin of life

1986 ◽  
Vol 16 (3-4) ◽  
pp. 179-180 ◽  
Author(s):  
Norman H. Sleep
2004 ◽  
Vol 213 ◽  
pp. 281-288
Author(s):  
P. Jenniskens

The unique rarefied flow and flash heating in meteors creates physical conditions that can change exogenous organic matter into unique prebiotic molecules. with the exception of rare giant comet impacts, most infalling matter at the time of the origin of life was deposited in the atmosphere during the meteor phase. Much new data has been obtained from observations in the Leonid Multi-Instrument Aircraft Campaign; a series of NASA and USAF sponsored Astrobiology missions that explored the 1998–2002 Leonid meteor storms. Here, we provide an overview of some of this recent insight, which provides a framework in which the prebiotic chemistry can be studied.


2019 ◽  
Author(s):  
Joana C. Xavier ◽  
Wim Hordijk ◽  
Stuart Kauffman ◽  
Mike Steel ◽  
William F. Martin

AbstractModern cells embody metabolic networks containing thousands of elements and form autocatalytic molecule sets that produce copies of themselves. How the first self-sustaining metabolic networks arose at life’ s origin is a major open question. Autocatalytic molecule sets smaller than metabolic networks were proposed as transitory intermediates at the origin of life, but evidence for their role in prebiotic evolution is lacking. Here we identify reflexively autocatalytic food-generated networks (RAFs)—self-sustaining networks that collectively catalyze all their reactions—embedded within microbial metabolism. RAFs in the metabolism of ancient anaerobic autotrophs that live from H2 and CO2 generate amino acids and bases, the monomeric components of protein and RNA, and acetyl-CoA, but amino acids and bases do not generate metabolic RAFs, indicating that small-molecule catalysis preceded polymers in biochemical evolution. RAFs uncover intermediate stages in the origin of metabolic networks, narrowing the gaps between early-Earth chemistry and life.


2020 ◽  
Author(s):  
Kazumu Kaneko ◽  
Yasuhito Sekine ◽  
Takazo Shibuya ◽  
Hisahiro Ueda ◽  
Natsumi Noda

Author(s):  
Martin Ferus ◽  
Vojtěch Adam ◽  
Giuseppe Cassone ◽  
Svatopluk Civiš ◽  
Václav Čuba ◽  
...  

2007 ◽  
Vol 6 (4) ◽  
pp. 321-323 ◽  
Author(s):  
W.M. Napier ◽  
J.T. Wickramasinghe ◽  
N.C. Wickramasinghe

AbstractMechanisms of interstellar panspermia have recently been identified whereby life, wherever it has originated, will disperse throughout the habitable zone of the Galaxy within a few billion years. This re-opens the question of where life originated. The interiors of comets, during their aqueous phase, seem to provide environments no less favourable for the origin of life than that of the early Earth. Their combined mass throughout the Galaxy overwhelms that of suitable terrestrial environments by about 20 powers of ten, while the lifetimes of friendly prebiotic environments within them exceeds that of localized terrestrial regions by another four or five powers of ten. We propose that the totality of comets around G-dwarf Sun-like stars offers an incomparably more probable setting for the origin of life than any that was available on the early Earth.


2011 ◽  
Vol 8 (6) ◽  
pp. 1465-1475 ◽  
Author(s):  
F. Orange ◽  
A. Chabin ◽  
A. Gorlas ◽  
S. Lucas-Staat ◽  
C. Geslin ◽  
...  

Abstract. The role of viruses at different stages of the origin of life has recently been reconsidered. It appears that viruses may have accompanied the earliest forms of life, allowing the transition from an RNA to a DNA world and possibly being involved in the shaping of tree of life in the three domains that we know presently. In addition, a large variety of viruses has been recently identified in extreme environments, hosted by extremophilic microorganisms, in ecosystems considered as analogues to those of the early Earth. Traces of life on the early Earth were preserved by the precipitation of silica on the organic structures. We present the results of the first experimental fossilisation by silica of viruses from extremophilic Archaea (SIRV2 – Sulfolobus islandicus rod-shaped virus 2, TPV1 – Thermococcus prieurii virus 1, and PAV1 – Pyrococcus abyssi virus 1). Our results confirm that viruses can be fossilised, with silica precipitating on the different viral structures (proteins, envelope) over several months in a manner similar to that of other experimentally and naturally fossilised microorganisms. This study thus suggests that viral remains or traces could be preserved in the rock record although their identification may be challenging due to the small size of the viral particles.


2018 ◽  
Vol 58 (7) ◽  
pp. 877-887
Author(s):  
M. V. Ragulskaya ◽  
E. G. Khramova ◽  
V. N. Obridko

2000 ◽  
pp. 527-544
Author(s):  
Everett L. Shock ◽  
Jan P. Amend ◽  
Mikhail Yu. Zolotov

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