Scheda ASTROCHEMISTRY@INAF- PROTOPLANETARY
FINAL
Informazioni generali
ASTROCHEMISTRY@INAF: from PROTOPLANETARY disks to primitive planetary system bodies
ASTROCHEMISTRY@INAF- PROTOPLANETARY
Programma
Programma
RSN2
RSN3
RSN5
Terza Missione
Attività: In Itinere; Data inizio: 2023; Data fine: 2030
claudio.codella claudio.codella@inaf.it
ASTROCHEMISTRY@INAF lavora sull'astrochimica di regioni di formazione di stelle di tipo Solare (su scale del Sistema Solare, SS). Il goal e' capire se il nostro SS ha ereditato la composizione chimica dalle prime fasi evolutive, creando un filo di Arianna con i dischi protoplanetari. La sinergia e' iniziata con i LP Herschel CHESS & WISH, e continuata con i LP IRAM sull'astrochimica: CALYPSO, ASAI, SOLIS. Siamo i co-PI dell'ALMA LP FAUST e PI di ALMA-DOT. Interpretiamo le osservazioni alla luce dei risultati dei laboratori INAF che simulano i grani interstellari e dai calcoli chimico-quantistici forniti dal link con le Università. Fondi: ASI, Astrofit, iALMA, 5 INAF/MIUR PRIN, H2020 EU ACO. Casi scientifici: SKA (Cradle of Life WG), SKA-MeerKAT+, Ariel (Planet formation WG).
ASTROCHEMISTRY@INAF is an INAF network on astrochemistry of Sun-like star forming regions, to study if our Solar System inherited its chemical composition from its earliest formation stages, creating an Ariadne thread with protoplanetary disks. The synergy started with the CHESS & WISH Herschel LPs and continued in all the IRAM LPs on astrochemistry: CALYPSO, ASAI, SOLIS. We are the co-PI of the ALMA LP FAUST, and PI of ALMA-DOT. Observations are interpreted in light of the results from the INAF laboratories that mimic the interstellar dust surface and of the quantum-chemical computations by our link with Universities. Fundings: ASI, iALMA, 5 INAF/MIUR PRINs, H2020 EU ACO. Science preparation for: SKA (Cradle of Life WG), SKA-MeerKAT+, and Ariel (Planet formation WG).
Mezzo interstellare, formazione di stelle e sistemi planetari
Origine ed evoluzione dei pianeti, satelliti e corpi minori
Bioastronomia, Astrobiologia e Astrofisica di laboratorio
Infrastrutture da Terra (utilizzo)
Comunicazione, Didattica, Divulgazione
Team Summary
15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 21
| Struttura | Nfte | N0 | TI 2024 | TI 2025 | TI 2026 | TD 2024 | TD 2025 | TD 2026 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| O.A. ARCETRI | 4 | 0 | 0.40 | 0.60 | 0.60 | 0.10 | 0.10 | 0.10 | 0 | 0.00 |
| IAPS ROMA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
| O.A. PALERMO | 1 | 0 | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0 | 0.00 |
| O.A. CATANIA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
| O.A. CAPODIMONTE | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 1 | 0.10 |
| O.A. PADOVA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
| Totali | 5 | 0 | 0.50 | 0.70 | 0.70 | 0.10 | 0.10 | 0.10 | 1 | 0.10 |
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 4
| # | Struttura | TI 2024 | TI 2025 | TI 2026 | TD 2024 | TD 2025 | TD 2026 | Extra |
|---|---|---|---|---|---|---|---|---|
| 1 | ORIGINS - Vera Rubin Research Fellow | 0 | 0 | 0 | 0.30 | 0.30 | 0.30 | 0.00 |
| 2 | ESO Research Fellow - Garching | 0 | 0 | 0 | 0.30 | 0.30 | 0.30 | 0.00 |
| 3 | IPAG - Grenoble | 0 | 0 | 0 | 0.30 | 0.30 | 0.30 | 0.00 |
| 4 | Dipartimento di Chimica, Università di Perugia | 0.20 | 0.20 | 0.20 | 0 | 0 | 0 | 0.00 |
| Totali | 0.20 | 0.20 | 0.20 | 0.90 | 0.90 | 0.90 | 0.00 |
Fondi a sostegno
21. Totale fondi a disposizione (dato aggregato, k€)
| Certi 2024 | Certi 2025 | Certi 2026 | Presunti 2024 | Presunti 2025 | Presunti 2026 |
|---|---|---|---|---|---|
| 271.0 | 132.0 | 0.0 | 0.0 | 0.0 | 0.0 |
Produzione scientifica e tecnologica
22. Produzione scientifica e tecnologica - Highlights
Informazioni Pubbliche
<p>Astrochemistry - Astrobiology - Planetary disks - Protostars - SKA_Science - Young Stellar Objects - Interstellar Medium - Interstellar Emission - Interstellar Molecules - Exoplanets - Interplanetary medium ** *** Campi di azione: Divulgazione scientifica. *** ASTROCHEMISTRY@INAF - PROTOPLANETARY has three related projects: ACO, FAUST, and ALMA-DOT ** ASTROCHEMISTRY@INAF - PROTOPLANETARY works in the SKA-SCIENCE context ** <span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">** ASTROCHEMISTRY@INAF - PROTOPLANETARY works in the SKA-MeerKAT+ context ** </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">ASTROCHEMISTRY@INAF - PROTOPLANETARY works in the Ariel context ** ASTROCHEMISTRY@INAF - PROTOPLANETARY is part of the JEDI program *** The total FTEs (760) are the sum of ASTROCHEMISTRY@INAF - PROTOPLANETARY + FAUST (daughter) project + ACO (daughter) project TILL 2030. </span></p>
The goal of the present program is to enlighten the INAF community working on astrochemistry in protostellar and protoplanetary disks and on the comparison with the chemical content of Solar System relics (comets, Solar System), using the outputs of the INAF laboratories to interpret the results. The projects inside ASTROCHEMISTRY@INAF - PROTOPLANETARY are also enriched by the collaboration with the chemists of the University of Perugia led by Prof. N. Balucani (INAF associated). Indeed, on 2020, INAF - OAA and the Chemistry Department of the Perugia University co-signed an agreement to officially exchange students, training them in the context of astrochemistry. In addition, through the ACO project (Scheda associated with ASTROCHEMISTRY@INAF - PROTOPLANETARY) INAF collaborate with chemists of University of Trento, Torino, and Bologna. These collaborations allow us to really study the chemistry at work in astronomical environments, i.e. working on *astrochemistry*.
ALMA; VLA; GBT; IRAM-30m; IRAM-NOEMA; SKA; SKA-MeerKAT+, SKA_SCIENCE; Ariel;
15. Team members, Informazioni generali
15. Personale INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2024/2025/2026) | FTE Presunte (2024/2025/2026) | Extra | ||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | claudio.codella | claudio.codella@inaf.it | O.A. ARCETRI | Y | DIRIGENTE DI RICERCA | co-PI di FAUST - responsabile INAF EU H2020 ITN ACO | X X X | X X X | X |
|
| 2 | davide.fedele | davide.fedele@inaf.it | O.A. ARCETRI | Y | PRIMO RICERCATORE | Dust continuum analysis | X X X | X X X | X |
|
| 3 | linda.podio | linda.podio@inaf.it | O.A. ARCETRI | Y | PRIMO RICERCATORE | PI ALMA-DOT project - Molecular Organics in protoplanetary disks | X X X | X X X | X |
|
| 4 | lorenzo.pino | lorenzo.pino@inaf.it | O.A. ARCETRI | Y | RICERCATORE | Exoplanets detection and atmosphere composition | X X X | X X X | X |
|
| 5 | gianrico.filacchione | gianrico.filacchione@inaf.it | IAPS ROMA | Y | PRIMO RICERCATORE | Solar System - Outer Solar System Objects | X X X | X X X | X |
|
| 6 | john.brucato | john.brucato@inaf.it | O.A. ARCETRI | Y | DIRIGENTE DI RICERCA | Laboratory experiments - Surface chemical reactions | X X X | X X X | X |
|
| 7 | mauro.ciarniello | mauro.ciarniello@inaf.it | IAPS ROMA | Y | PRIMO RICERCATORE | Solar System - Outer Solar System Objects | X X X | X X X | X |
|
| 8 | andrea.raponi | andrea.raponi@inaf.it | IAPS ROMA | Y | PRIMO RICERCATORE | Solar System - Outer Solar System Objects | X X X | X X X | X |
|
| 9 | angela.ciaravella | angela.ciaravella@inaf.it | O.A. PALERMO | Y | RICERCATORE ASTRONOMO | Complex organics induced in ice mixtures by X-ray and VUV radiation | X X X | X X X | X |
|
| 10 | antonio.jimenez | antonio.jimenez@inaf.it | O.A. PALERMO | Y | RICERCATORE | Complex organics induced in ice mixtures by X-ray and VUV radiation | X X X | X X X | X |
|
| 11 | maria.palumbo | maria.palumbo@inaf.it | O.A. CATANIA | Y | DIRIGENTE DI RICERCA | Laboratory experiments: experimental data analysis | X X X | X X X | X |
|
| 12 | giuseppe.baratta | giuseppe.baratta@inaf.it | O.A. CATANIA | Y | ASTRONOMO ASSOCIATO | Laboratory experiments: experimental data analysis | X X X | X X X | X |
|
| 13 | carlotta.scire | carlotta.scire@inaf.it | O.A. CATANIA | Y | TECNOLOGO | Laboratory experiments: experimental data analysis | X X X | X X X | X |
|
| 14 | vito.mennella | vito.mennella@inaf.it | O.A. CAPODIMONTE | Y | DIRIGENTE DI RICERCA | Laboratory experiments - Chemical reactions after exposure to UV photons by X-ray dispersive analysis method | X X X | X X X | X |
|
| 15 | ernesto.zona | ernesto.zona@inaf.it | O.A. CAPODIMONTE | Y | C.T.E.R. | Laboratory experiments - Chemical reactions after exposure to UV photons by X-ray dispersive analysis method | X X X | X X X | X |
|
| 16 | caterina.boccato | caterina.boccato@inaf.it | O.A. PADOVA | Y | PRIMO TECNOLOGO | Outreach and Dissemination | X X X | X X X | X |
|
| 17 | fabrizio.capaccioni | fabrizio.capaccioni@inaf.it | IAPS ROMA | N | ASSOCIATO QUIESCENTE | Solar System - Outer Solar System Objects | X X X | X X X | X |
|
| 18 | giovanni.sabatini | giovanni.sabatini@inaf.it | O.A. ARCETRI | N | RICERCATORE | Chemical evolution of protostellar regions - comparison with high-mass SFRs | X X X | X X X | X |
|
| 19 | riccardo.urso | riccardo.urso@inaf.it | O.A. CATANIA | Y | RICERCATORE | Laboratory experiments and data analysis | X X X | X X X | X |
|
| 20 | manuela.lippi | manuela.lippi@inaf.it | O.A. ARCETRI | N | RICERCATORE | Chemical composition of comets, comparison with protoplanetary disks | X X X | X X X | X |
|
| 21 | daniele.fulvio | daniele.fulvio@inaf.it | O.A. CATANIA | Y | PRIMO RICERCATORE | Laboratory experiments: experimental data analysis | X X X | X X X | X |
|
16. Personale Associato INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2024/2025/2026) | FTE Presunte (2024/2025/2026) | Extra | |
|---|---|---|---|---|---|---|---|---|---|
| 1 | eleonora.bianchi | eleonora.bianchi@origins-cluster.de | ORIGINS - Vera Rubin Research Fellow | N | Vera Rubin Fellow, INAF associated | Interstellar organics and large carbon chains from protoplanetary objects to comets - Observations and modelling | [0.3, 0.3, 0.3] | [-1.0, -1.0, -1.0] | -1.0 |
| 2 | marta.desimone | marta.desimone@eso.org | ESO Research Fellow - Garching | N | ESO Fellow, INAF associated | Molecular complexity of the earliest (protostellar) evolutionary stages of Sun-like analogs - Observations and Modelling | [0.3, 0.3, 0.3] | [-1.0, -1.0, -1.0] | -1.0 |
| 3 | lisa.giani | lisa.giani@univ-grenoble-alpes.fr | IPAG - Grenoble | N | PhD student, Associato INAF | Quantum-mechanical calculations - Gas-phase reactions - Prebiotic chemistry | [0.3, 0.3, 0.3] | [-1.0, -1.0, -1.0] | -1.0 |
| 4 | nadia.balucani | nadia.balucani@unipg.it | Dipartimento di Chimica, Università di Perugia | Y | FULL PROFESSOR | Quantum-chemical computations of complex organics in space | [0.2, 0.2, 0.2] | [-1.0, -1.0, -1.0] | -1.0 |
21. Fondi a Sostegno Iniziativa
The context of this program (Astrochemistry of Sun-like star forming regions) was awarded by several MIUR, INAF, ASI, EU fundings. More specifically, before 2020, we were supported by ASI-Science Herschel (195 kE), Premiale INAF iALMA (100 kE), INAF-Astrofit (210 kE), PRIN-MIUR 2016 STAR IN THE CAOS PRIN-MIUR project (Simulation Tools for Astrochemical Reactivity and Spectroscopy in the Cyberinfrastructure for Astrochemical Organic Species) PI. V. Barone (Total: 180 kE; Total INAF 20 kEuro), and GENESIS-SKA PRIN-INAF project (GEneral conNditions in Early Planetary Systems for the rISe of life with SKA), PI C. Codella (Total: 408 kEuro). After 2020: ASTRO-CHEMICAL ORIGINS (ACO) ITN H2020 EC MARIE SKŁODOWSKA-CURIE ACTIONS, PI C. Ceccarelli (Total: 4138 kEuro; Total INAF: 392 KEuro), the PRIN-MUR 2020 BEYOND-2p (Astrochemistry beyond the second period elements, PI: N. Balucani, Total: 478 kEuro, Total INAF: 91 kEuro), the PRIN MUR 2022 FOSSILS (Chemical origins: linking the fossil composition of the Solar System with the chemistry of protoplanetary disks, PI: L. Podio, Total: 250 kEuro; Total INAF: 137 kEuro), the project ASI-Astrobiologia 2023 MIGLIORA (Modeling Chemical Complexity, PI: R. Saladino, Total: 400 kEuro; Total INAF: 100 KEuro), and the INAF-GO 2023 fundings PROTO-SKA (Exploiting ALMA data to study planet forming disks: preparing the advent of SKA, PI: C. Codella, Total: 50 kEuro).
Tabella fondi:
| # | Provenienza | Certi 2024 (k€) | Certi 2025 (k€) | Certi 2026 (k€) | Presun. 2024 (k€) | Presun. 2025 (k€) | Presun. 2026 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
|---|---|---|---|---|---|---|---|---|---|
| 1 | ACO EU ITN H2020 | 41 | 0 | 0 | 0 | 0 | 0 | 41 | 0 |
| 2 | BEYOND-2p | 45 | 10 | 0 | 0 | 0 | 0 | 55 | 0 |
| 3 | PROTO-SKA | 25 | 25 | 0 | 0 | 0 | 0 | 50 | 0 |
| 4 | Chemical Origins | 100 | 37 | 0 | 0 | 0 | 0 | 137 | 0 |
| 5 | MIGLIORA | 50 | 50 | 0 | 0 | 0 | 0 | 100 | 0 |
| 6 | TRIESTE Minigrant Sabatini | 10 | 10 | 0 | 0 | 0 | 0 | 20 | 0 |
Tabella fondi Astrofisica Fondamentale e PNRR:
| # | Provenienza | Fondi 2024 (€) | Fondi 2025 (€) | Fondi 2026 (€) |
|---|