The extremotolerant bacterium Deinococcus radiodurans is used as a model to explore the limits of life on Earth and beyond. In experiments performed in an ultra-high vacuum chamber with a vacuum ultraviolet (VUV) synchrotron beamline, this microorganism was exposed to conditions present on an extraterrestrial environment unprotected by an atmosphere, such as outside a spacecraft or on an asteroid, relevant in the context of planetary protection and panspermia hypothesis. Different methods were used to obtain the biologically relevant information from this investigation. Counting of colony forming units, the traditional approach for viability assessment, is limited to measuring the survival of the cells. For a more in-depth study of damage mechanisms at subcellular levels, specific molecular probes (propidium iodide and dihydrorhodamine 123) were applied and whole populations could be analysed, cell by cell, by flow cytometry. VUV radiation caused a substantial loss of viability, though only a fraction of the cells presented membrane damages even at the largest tested fluences. Additionally, intracellular oxidative stress was also detected upon exposure. These results point to significant VUV inactivating effects extending beyond the cells' outermost structures, in contrast to a more superficial role that could be expected due to the highly interacting nature of this radiation range. Nevertheless, it was observed that microscopic-level shading sufficed to allow the persistence of a small surviving subpopulation for the longer expositions. This study contributes to unveiling the response of biological systems under space conditions, assessing not just cell viability but also the mechanisms that lead to inactivation.

Reliable spectroscopic data are needed for interpretation and modeling of observed astrophysical plasmas. For heavy element ions, which have complex spectra, experimental data are rather incomplete. To provide valuable fundamental quantities, such as precise wavelengths, level energies and semi-empirical transition probabilities, we are carrying out laboratory studies of high-resolution VUV emission spectra of moderately charged ions of transition metals and rare earth elements. Experimental and theoretical methods are summarized. Examples of studies are described.

We demonstrate that the methodology of frequency-resolved optical gating (FROG) is applicable to time-resolved reflection spectroscopy of a plasma mirror in the vacuum-ultraviolet (VUV) region. Our recent study [R. Itakura et al. Opt. Express 23, 10914 (2015)] has shown that a VUV waveform can be retrieved from a VUV reflection spectrogram of a plasma mirror formed on a fused silica (FS) surface by irradiation with an intense femtosecond laser pulse. Simultaneously, the increase in the reflectivity with respect to the Fresnel reflection of the unexcited FS surface can be obtained as a time-dependent reflectivity of the plasma mirror. In this study, we update the FROG analysis procedure using the least-square generalized projections algorithm. This procedure can reach convergence much faster than the previous one and has no aliasing problem. It is demonstrated that a significantly chirped VUV pulse as long as 1 ps can be precisely characterized.

We report results from a study of the integrated column density and expansion dynamics of ground-state-selected Ba+ ions in a laser–plasma plume using a new experimental system—VPIF (vacuum-ultraviolet photoabsorption imaging facility). The ions are tracked by recording the attenuation of a pulsed and collimated vacuum ultraviolet beam, tuned to the 5p–6d inner-shell resonance of singly ionized barium, as the expanding plasma plume moves across it. The attenuated beam is allowed to fall on a CCD array where the spatial distribution of the absorption is recorded. Time-resolved ion velocity and integrated column density maps are readily extracted from the photoionization images.