The PLATO mission

PLATO (PLAnetary Transits and Oscillations of stars) is ESA’s M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large number of stars. PLATO will detect small planets (down to <2R ) around bright stars (<11 mag), including terrestrial planets in the habitable zone of solar-like stars. With the complement of radial velocity observations from the ground, planets will be characterised for their radius, mass, and age with high accuracy (5%, 10%, 10% for an Earth-Sun combination respectively). PLATO will provide us with a large-scale catalogue of well-characterised small planets up to intermediate orbital periods, relevant for a meaningful comparison to planet formation theories and to better understand planet evolution. It will make possible comparative exoplanetology to place our Solar System planets in a broader context. In parallel, PLATO will study (host) stars using asteroseismology, allowing us to determine the stellar properties with high accuracy, substantially enhancing our knowledge of stellar structure and evolution. The payload instrument consists of 26 cameras with 12cm aperture each. For at least four years, the mission will perform high-precision photometric measurements. Here we review the science objectives, present PLATO‘s target samples and fields, provide an overview of expected core science performance as well as a description of the instrument and the mission profile towards the end of the serial production of the flight cameras. PLATO is scheduled for a launch date end 2026. This overview therefore provides a summary of the mission to the community in preparation of the upcoming operational phases

The PLATO mission

PLATO (PLAnetary Transits and Oscillations of stars) is ESA’s M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large number of stars. PLATO will detect small planets (down to <2REarth) around bright stars (<11 mag), including terrestrial planets in the habitable zone of solar-like stars. With the complement of radial velocity observations from the ground, planets will be characterised for their radius, mass, and age with high accuracy (5%, 10%, 10% for an Earth-Sun combination respectively). PLATO will provide us with a large-scale catalogue of well-characterised small planets up to intermediate orbital periods, relevant for a meaningful comparison to planet formation theories and to better understand planet evolution. It will make possible comparative exoplanetology to place our Solar System planets in a broader context. In parallel, PLATO will study (host) stars using asteroseismology, allowing us to determine the stellar properties with high accuracy, substantially enhancing our knowledge of stellar structure and evolution. The payload instrument consists of 26 cameras with 12cm aperture each. For at least four years, the mission will perform high-precision photometric measurements. Here we review the science objectives, present PLATO‘s target samples and fields, provide an overview of expected core science performance as well as a description of the instrument and the mission profile towards the end of the serial production of the flight cameras. PLATO is scheduled for a launch date end 2026. This overview therefore provides a summary of the mission to the community in preparation of the upcoming operational phases

Interaction of the Rattlesnake Toxin Crotamine with Model Membranes

Crotamine is one of the main constituents of the venom of the South American rattlesnake Crotalus durissus terrificus. A common gene ancestry and structural similarity with the antimicrobial beta-defensins (identical disulfide bond pattern and highly positive net charge) suggested potential antimicrobial activities for this snake toxin. Although crotamine demonstrated low activity against both Gram-positive and Gram-negative bacteria, a pronounced antifungal activity was observed against Candida spp., Trichosporon spp., and Cryptococcus neoformans. Crotamine's selective antimicrobial properties, with no observable hemolytic activity, stimulated us to evaluate the potential applications of this polypeptide as an antiyeast or candicidal agent for medical and industrial application. Aiming to understand the mechanism(s) of action underlying crotamine antimicrobial activity and its selectivity for fungi, we present herein studies using membrane model systems (i.e., large unilamellar vesicles, LUVs, and giant unilamellar vesicles, GUVs), with different phospholipid compositions. We show here that crotamine presents a higher lytic activity on negatively charged membranes compared with neutral membranes, with or without cholesterol or ergosterol content. the vesicle burst was not preceded by membrane permeabilization as is generally observed for pore forming peptides. Although such a property of disrupting lipid membranes is very important to combat multiresistant fungi, no inhibitory activity was observed for crotamine against biofilms formed by several Candida spp. strains, except for a limited effect against C. krusei biofilm.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Biotox Network (CYTED)Universidade Federal de São Paulo UNIFESP, Dept Farmacol, BR-04044020 São Paulo, BrazilInst Butantan, Lab Especial Ecol & Evolucao, BR-05503900 São Paulo, BrazilUniv São Paulo, Inst Fis, Dept Fis Aplicada, BR-05508090 São Paulo, BrazilUniversidade Federal de São Paulo UNIFESP, Dept Med, BR-04021001 São Paulo, BrazilUniv São Paulo, Dept Bioquim & Imunol, BR-14096000 São Paulo, BrazilUniversidade Federal de São Paulo UNIFESP, Dept Biofis, BR-04021001 São Paulo, BrazilUniversidade Federal de São Paulo UNIFESP, Dept Farmacol, BR-04044020 São Paulo, BrazilUniversidade Federal de São Paulo UNIFESP, Dept Med, BR-04021001 São Paulo, BrazilUniversidade Federal de São Paulo UNIFESP, Dept Biofis, BR-04021001 São Paulo, BrazilWeb of Scienc

Interaction of the Rattlesnake Toxin Crotamine with Model Membranes

Crotamine is one of the main constituents of the venom of the South American rattlesnake <i>Crotalus durissus terrificus</i>. A common gene ancestry and structural similarity with the antimicrobial β-defensins (identical disulfide bond pattern and highly positive net charge) suggested potential antimicrobial activities for this snake toxin. Although crotamine demonstrated low activity against both Gram-positive and Gram-negative bacteria, a pronounced antifungal activity was observed against <i>Candida</i> spp., <i>Trichosporon</i> spp., and <i>Cryptococcus neoformans</i>. Crotamine’s selective antimicrobial properties, with no observable hemolytic activity, stimulated us to evaluate the potential applications of this polypeptide as an antiyeast or candicidal agent for medical and industrial application. Aiming to understand the mechanism(s) of action underlying crotamine antimicrobial activity and its selectivity for fungi, we present herein studies using membrane model systems (i.e., large unilamellar vesicles, LUVs, and giant unilamellar vesicles, GUVs), with different phospholipid compositions. We show here that crotamine presents a higher lytic activity on negatively charged membranes compared with neutral membranes, with or without cholesterol or ergosterol content. The vesicle burst was not preceded by membrane permeabilization as is generally observed for pore forming peptides. Although such a property of disrupting lipid membranes is very important to combat multiresistant fungi, no inhibitory activity was observed for crotamine against biofilms formed by several <i>Candida</i> spp. strains, except for a limited effect against <i>C. krusei</i> biofilm