Microscopic morphology of Haloarcula sp. NS06 in light (A), scanning electron (B) and thin section electron microscopy (C,D). (A) In a 2-days-old artificial sea water (ASW) suspension culture, single cells
Microscopic morphology of Haloarcula sp. NS06 in light (A), scanning electron (B) and thin section electron microscopy (C,D). (A) In a 2-days-old artificial sea water (ASW) suspension culture, single cells
Elements of the deep water cycle on rocky planets that are discussed in this chapter. Reservoirs are labelled in sans serif font. The dominant form of ‘water’ in certain reservoirs
How will Science Fiction inspire the way in which we mount Astrobiology missions to other worlds? Grok via Astrobiology.com Students in our introductory courses are often familiar with astronomy concepts
Schematic picture of the system assumed in this study. (a) A supernova explosion occurs at a distance 𝑑 from the protosolar disk, and (b) the expanding supernova shockwave contacts the
Prior to ca. 2.32 Ga, during deposition of the upper Rooihoogte and lower Timeball Hill formations, atmospheric pO2 10−6 PAL facilitated sulfur isotope mass-independent fractionation (S-MIF) signatures and a global ocean dominated
Representative SEM images of jarosite synthesized at 25 °C (Fe2+ oxidation) and under hydrothermal conditions (Fe3+ hydrolysis). For each halogen-bearing group, the sample with the highest halogen content is shown.
Very Large Array — NRAO The history of astronomical discovery shows that many of the most detectable phenomena, especially detection firsts, are not typical members of their broader class, but
Diversity in sub-Neptune transmission spectra. a. The JWST transmission spectra of TOI-270 d12, K2-18 b9 , and LP 791-18 c are shown with their 1σ error bars and respective best-fit
Processes occurring in the protocell at each time step. Continuous arrows show polymers being produced, segmented arrows show peptide catalysis of CO2 fixation and templated polymerisation, and dotted arrows indicate
Tracking The Evolution Of Planetary Systems And Planets The spring school “Tracking the evolution of planetary systems and planets” which is co-organised by the COST Action “The birth of solar






