Calendar

May
2
Wed
Ricevimento studenti – Argiroffi
May 2 @ 10:00 – 13:00
May
3
Thu
riunione divulgazione
May 3 @ 8:00 – 13:15
May
8
Tue
Seminario S Hadjaje
May 8 @ 15:00 – 16:00
May
9
Wed
Ricevimento studenti – Argiroffi
May 9 @ 10:00 – 13:00
May
16
Wed
Ricevimento studenti – Argiroffi
May 16 @ 10:00 – 13:00
May
17
Thu
Seminario Hadjaje
May 17 @ 15:00 – 16:00
May
23
Wed
Ricevimento studenti – Argiroffi
May 23 @ 10:00 – 13:00
May
25
Fri
OAPA SF Meeting; TITOLO: Idee e progetti che coinvolgono il Gaia DR2 / Interventi liberi
May 25 @ 15:00 – 16:00

Questo meeting è organizzato allo scopo di mettere assieme idee e progetti di ricerca che comprendano l’utilizzo del secondo Data Release di Gaia.

L’idea è che chiunque abbia un progetto da presentare o discutere prepari una piccola presentazione, meglio utilizzando qualche immagine, e lo comunichi a Mario Guarcello (), che preparerà una scaletta dell’incontro.

May
28
Mon
Incontro Hadjaje
May 28 @ 15:00 – 16:00
May
30
Wed
“Extreme planet atmospheric escape: current standing and future observability”. Luca Fossati (Space Research Institute, Austrian Academy of Sciences, Austria)
May 30 @ 15:30 – 16:30

Planets in short-period orbits provide a unique opportunity to directly study atmospheric escape, which is a phenomenon having a profound impact on our understanding of the observed exoplanet demographics. Among all planets known to have an escaping atmosphere, those undergoing extreme mass loss are key: their escape may be representative of young planets, at a time when atmospheric escape matters most. I will review results obtained from the analysis of Hubble Space Telescope observations, particularly those of the extreme hot Jupiters WASP-12b, WASP-13b, and WASP-18b. I will then show how planet atmospheric escape may be at the origin of the correlation between the chromospheric activity of stars hosting hot Jupiters and the planets’ surface gravity. I will finally show how planets orbiting early-type stars might become of crucial importance in the near future and how their escaping atmospheres can be observationally studied.