14 Settembre, 2022, ore 11:00 Link:https://meet.google.com/tid-ifhn-fcc Speaker: David Rothery da The Open University di Milton Keynes, UK Abstract: Mercury’s volcanic activity has decreased over time, but probably continued into the geologically recent …
Near-Earth Asteroids: risks and opportunities
13 Luglio, 2022, ore 11:00 Speaker: Davide Perna da Osservatorio Astronomico di Roma Abstract: The proximity of near-Earth asteroids (NEAs) allows us to investigate the physical properties of small bodies down to …
Hydrogen Abundance Estimations on asteroid (101955) Bennu and (162713) Ryugu, targets of the OSIRIS-REX
Link:https://meet.google.com/tid-ifhn-fcc Title: Hydrogen Abundance Estimations on asteroid (101955) Bennu and (162713) Ryugu, targets of the OSIRIS-REX and Hayabusa2 missions Speaker: Alice Praet da Observatoire de Paris Abstract: Two asteroid sample return missions are …
Title: On the interpretation of the BepiColombo’s observation at Mercury with numerical simulations
30 Giugno, 2022, ore 10:30 Speaker: Esa Kallio da School of Electrical Engineering, Department of Electronics and Nanoengineering, Aalto University, Helsinki, Finland Abstract: One major science goal of the BebiColombo Mercury mission …
The spectral signature of BHs versus NS sources
22 Giugno, 2022, ore 14:30 Link: meet.google.com/tid-ifhn-fcc Abstract: In 2017 the work on the Comptonization (Sunyaev-Titarchuk) seen in the X-ray spectra of astrophysical sources was a candidate for the Nobel Prize in Physics. …
Deciphering ALMA observations of protoplanetary disks
15 Giugno, 2022, ore 14:30 Link: meet.google.com/tid-ifhn-fcc Speaker: Cornelis P. “Kees” Dullemond da University of Heidelberg – Zentrum für Astronomie Abstract: ALMA has given us a whole new view on planet-forming circumstellar disks. We …
Polar volatiles on Mercury and the Moon: Investigations of their delivery, evolution, and current state
Speaker: Ariel Deutsch da NASA-AMES Link: meet.google.com/tid-ifhn-fc The poles of Mercury and the Moon both show evidence for water ice, but the deposits on Mercury have a greater areal distribution and a more pure concentration. For example, ice …
The ultimate fate of turbulence in weakly-collisional plasmas: phase-space
Abstract: Understanding the dynamics of turbulent, weakly-collisional plasmas at kinetic scales is crucial to address long-standing issues, such as the dissipation of turbulent energy and the consequent plasma heating. Owing to …
Episodic accretion in high-mass young stellar objects (HMYSOs)
30 Marzo, 2022, ore 11:00 Link: meet.google.com/tid-ifhn-fcc Speaker: Dr.Alessio Caratti o Garatti da INAF-OACN Abstract: In the past few years, accretion bursts in young stellar objects (YSOs) have gained increasing relevance in star …
Electromagnetic counterparts of high-frequency gravitational wave sources
23 Marzo, 2022, ore 11:00 Speaker: Dr.Giulia Stratta da INAF-IAPS Abstract: The achieved advances in gravitational wave (GW) detectors and the strong coordinations among different observatories are paving the way for a …