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Pint of Science 2024: Dalla Polvere ai Buchi Neri

Joyce Irish pub Via Montesano 46, Catania, Italia

Tu potresti morire ma il deserto nasconderebbe il segreto della tua morte che rimarrebbe dopo di te per coprire la tua memoria con il vento… scrive John Fante in Ask the dust, Chiedi quindi alla polvere ma di una stella se vuoi sapere cosa ci attende se cadessimo in un Buco Nero, dove lo spazio diventa tempo e il tempo diventa spazio, dove forse si cela il passaggio verso un nuovo Universo gemello del nostro. Siete pronti a questo viaggio cosmico?

ESP2024 – PLATO PLANETARY SYSTEMS: Formation to Observed architectures

Department of Physics and Astronomy "Ettore Majorana" (DFA) of the Catania University Via Santa Sofia 64, Catania, Italia

PLATO is the 3rd mission of class M in the ESA Cosmic Vision program. Its main goal is detecting terrestrial planets in the habitable zone of solar type stars. With its huge FOV, most of the PLATO targets are bright stars that will be monitored with high cadence (25 s) for at least 2-3 years during the long duration observing program, while contemporary a number of very bright stars in the sample will be observed with 2.5 s cadence. The collected data, photometry from space and high resolution spectroscopy from the ground, will provide accurate planetary structures as well as architectures and evolutionary stage - via asteroseismic analysis - of a large number of planetary systems. PLATO is planned for a launch in Dec 2026.

Pint of Science 2024: La conquista dello spazio

Joyce Irish pub Via Montesano 46, Catania, Italia

Partendo dallo storico viaggio di Gagarin, si parlerà di come il genere umano ha conquistato lo spazio che ci circonda, delle prospettive future a breve e lungo termine e, per i pochi a quel punto ancora ragionevolmente sobri, delle ricadute sulla vita di tutti i giorni delle tecnologie spaziali.

Etna Comics 2024

Le Ciminiere viale Africa 222, Catania

L'Istituto Nazonale di Astrofisica sarà presente all'edizione 2024 di Etna Comics, rassegna di fumetti e giochi che si svolge a Catania dal 6 al 9 giugno.

Resilience of Eukaryotic Life in Mars-Like Simulated Conditions

Sede A. Riccò Via Santa Sofia 78, Catania

Constraining the survivability of different organisms to space-like conditions is of great interest
for Astrobiology. Extreme conditions can lead to alteration in the metabolic pathways of biological
systems. To identify organisms of interest for future astrobiological studies, it is necessary to
investigate their physiological parameters to understand the mechanisms involved in metabolic
rearrangement.

Neural Networs: new models for recovering the Cosmic Microwave Background

Sede A. Riccò Via Santa Sofia 78, Catania

The Cosmic Microwave Background, the relic emission from the primordial Universe, is one of the most important observables in Cosmology. Its recovery is generally carried out by parametric and (semi) blind methods after removing several Galactic and extragalactic emissions. However, in order to take into account their non-linear behaviors, Machine Learning approaches such Neural Networks seem to be promising for that task. In this talk, I will describe how they begin to be an alternative and reliable methods for recovering the Cosmic Microwave Background.

Galactic Archaeology: decoding the fossil record of Galaxy formation and evolution

Sede A. Riccò Via Santa Sofia 78, Catania

One of most important issue in Astrophysics is the achievement of a robust understanding of the sequence of processes that contributed to the building up of the Milky Way. This is obviously important not only "on a local scale" in order to recover the history of formation and evolution of the Galaxy, but also, more in general, for understanding the formation process of spiral galaxies. In the last decade, the advent of high precision photometric and spectroscopic surveys as well as the possibility to estimate, thanks to the ESA Gaia mission, accurate distance for a huge number of field stars, combined with the development of an accurate theoretical framework, is actually opening a new era for this kind of investigations.
We will present some recent results - obtained by using this updated observational and theoretical framework - about the formation and early evolution of the Milky Way.

The Hot Neptune Desert

Sede A. Riccò Via Santa Sofia 78, Catania

The vast majority of close-in planets are either massive hot Jupiters capable of holding their atmosphere against the stellar photoevaporation or small rocky planets completely drained by the stellar radiation. We observe an unexpected dearth of highly irradiated Neptune- and Saturn-like planets orbiting their host star in less than 4-10 days, called "Hot Neptune Desert". In this talk, I will present our recent findings from uniformly vetting 250 hot Neptune TESS candidates using a two-step vetting technique, as well as discuss a cutting-edge approach to examine the problem under a new perspective. I will also discuss how the PLATO mission may enhance our understanding of the Hot Neptunes.
We will present some recent results - obtained by using this updated observational and theoretical framework - about the formation and early evolution of the Milky Way.

Notte Europea dei Ricercatori 2024

In occasione della Notte Europea dei Ricercatori 2024, l’INAF-Osservatorio Astrofisico di Catania ha organizzato varie attività per il pubblico che si svolgeranno tra il 27 e il 28 settembre.

Unraveling Space Weathering on Planetary and Astrophysical Surfaces

Sede A. Riccò Via Santa Sofia 78, Catania

It is well known that the interaction of energetic ions, electrons and photons with surfaces and interfaces leads to non-thermal desorption via a process typically referred to as desorption induced by electronic transitions (DIET).  When DIET involves either electrons or photons, these processes are generally referred to as electron-stimulated desorption and photon-stimulated desorption (PSD), respectively.  Recent attention has focused on understanding the role of non-thermal “space weathering” in the processing of interstellar grains and ices.
Specifically, there is deep interest in understanding the radiation processing of carbon grains in the solar nebula and unraveling the H2O formation mechanisms in solar nebula and planetary systems, including the Moon. Using graphite grains, the VUV photon-simulated oxidation of carbon grains via reactive scattering of water fragments produced by dissociative electron attachment at the buried interface was examined. The results suggested that VUV PSD at the buried water:carbon grain interface may help control the carbon inventory during planet formation. The inverse process, (i.e, the formation of water) may happen on metal-oxide samples such as mineral grains and lunar regolith samples, that contain or are terminated by hydroxyl groups. Solar wind space weathering experiments of several Apollo lunar samples demonstrated that thermally activated recombinative desorption (RD) can be H2O sources and that electron-stimulated reactive scattering to produce water may also be occurring, especially when the Moon is in the magnetopause.  RD can occur on a diurnal basis on the Moon and is prevalent during meteoroid impacts. The latter is simulated by laser irradiation studies followed by state and velocity resolved detection of the produced water.  Finally, evidence of space weathering and surface alteration has also been revealed using spatially resolved, high-resolution nanoscale Fourier transform infrared imaging/spectroscopy correlated with photoluminescence (PL) on Apollo samples with different origins and history.