Scheda PRESTIGE
FINAL
Informazioni generali
Pristine REturned Sample Testing InvestiGation and Examination
PRESTIGE
Progetto
Progetto
Missione spaziale Internazionale
Laboratorio
RSN3
Attività: Nuova; Data inizio: 2022; Data fine: 2026
ernesto.palomba ernesto.palomba@inaf.it
Il 6 dicembre 2020, la missione spaziale Hayabusa2 ha riportato a Terra circa 5 g di campioni raccolti sulla superficie dell'asteroide Ryugu.Precedenti studi suggeriscono che abbia subito space weathering(SW)(metamorfismo termico, impatti di micrometeoroidi e vento solare). Il principale obiettivo del progetto è studiare lo SW attraverso l'analisi dei campioni di Ryugu riportati a Terra e il confronto con i suoi analoghi (es. meteorite). Ci proponiamo di indagare questi campioni utilizzando tecniche analitiche come la spettroscopia micro-IR, XPS, PIGE, SEM,XRD,EBSD e simulare SW sugli analoghi con esperimenti controllati in laboratorio: camera termica (metamorfismo termico), irradiazione laser (bombardamento di micrometeoroidi), irraggiamento H+/He+ (vento solare).
On December 6th 2020, the Hayabusa2 space mission returned to Earth about 5 g of samples collected on the surface of the asteroid Ryugu.Previous studies of Ryugu’s surface suggest that it experienced space weathering (SW).The objective of this project is to understand how SW operates on Ryugu analysing the samples returned from its surface.These mechanisms can be better investigated combining observables(Ryugu grains)with controlled laboratory experiments on analogues.Laser irradiation will be used to simulate micrometeoroid bombardment,ion irradiation (H+/He+)to reproduce solar wind and a high temperature vacuum chamber to simulate thermal metamorphism. Samples will be
characterized by non-destructive analytical techniques such as XRD,XPS, PIGE, SEM,EBSD and micro-IR spectroscopy.
Origine ed evoluzione dei pianeti, satelliti e corpi minori
Bioastronomia, Astrobiologia e Astrofisica di laboratorio
Team Summary
15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 7
| Struttura | Nfte | N0 | TI 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| IAPS ROMA | 0 | 0 | 0.00 | 0.00 | 0.00 | 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 | 0 | 0.00 |
| Totali | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 5
| # | Struttura | TI 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | Extra |
|---|---|---|---|---|---|---|---|---|
| 1 | Università di Firenze | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 |
| Totali | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 |
Fondi a sostegno
21. Totale fondi a disposizione (dato aggregato, k€)
| Certi 2022 | Certi 2023 | Certi 2024 | Presunti 2022 | Presunti 2023 | Presunti 2024 |
|---|---|---|---|---|---|
| 0 | 0 | 0 | 0 | 0 | 0 |
Produzione scientifica e tecnologica
22. Produzione scientifica e tecnologica - Highlights
Informazioni Pubbliche
<p><span style="color: rgb(0, 0, 255);">Solar system astronomy, </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">Small Solar System bodies</span><br></p><p class="MsoNormal"><o:p></o:p></p>
<p>INAF has a significant role in study of Solar system bodies and in Space Weathering effects on planetary regoliths.The PI of this project is Ernesto Palomba(INAF-IAPS)who is an effective member of the Initial Analysis Team for the analysis of the samples returned from Ryugu.He is Co-Investigator of the Hayabusa2 ONC camera and NIRS3 spectrometer and has a very strong skills in the study of small bod of our Solar System. Relevant Bibliography by INAF(IAPS,OACT, OACN):<br><br>Palomba et al.,Icarus, 240, 58,2014<br>Palomba et al.,Icarus, 258, 120,2015<br>Palomba et al.,ApJL, 882 L22,2019<br>Palomba et al.,Icarus,318,188,2019<br>Longobardo et al.,Icarus,267,204,2016<br>Longobardo et al.,MNRAS, 469, 2,S346, 2017<br>Longobardo et al.,MNRAS,496, 1,125, 2020<br>Della Corte et al.,A&A,583,2015<br>Della Corte et al.,A&A,630,2019<br>Palumbo et al., JMoSt, 972,1-3, 64,2010<br>Palumbo et al., BSRSL, 84,33,2015<br>Baratta et al.,PSS,118, 211,2015<br>Scirè et al., AcSPa,219,288,2019<br>Fulvio et al.,MNRAS,483,381,2019<br>Fulvio et al.,Icarus,366,2021<br></p>
<p><b>INAF-IAPS</b></p><ul><li>Anneling setup in thermovacuum chamber for planetary analogue materials characterization at 10-6mbar and in the Trange: from 20 to 700°C</li><li>LEICA microscope</li><li>FTIR Spectrometer Bruker IFS 80</li><li>IR Hyperion microscope Bruker</li><li>Sieving system AS200 basic for planetary mixtures sieving at different grain size (from 20um to 5m)</li></ul><p class="MsoNormal" style="text-align:justify;line-height:11.75pt"><b>INAF-OACN</b></p><ul><li>ns-pulsed Nd: YAG laser (1064 nm, 10 Hz) faced to vacuum chamber for simulation of micrometeorite bombardment of planetary surfaces and for target vaporization and production of planetary analogues;<o:p><br></o:p></li><li>FTIR spectrometers: Bruker Vertex 70v, Bruker Equinox 55, and Bruker Vertex 80v for the spectroscopic characterization of samples in the NIR-MIR spectral range 1 - 20 micrometers;</li><li>UV-VIS-NIR spectrometer Perkin-Elmer Lambda 950, for the spectroscopic characterization of samples in the spectral range 0.2 - 3 micrometers;</li><li>Zeiss Axio M2m microscope, for the morphological characterization of samples;<o:p></o:p></li></ul><p class="MsoNormal" style="margin-bottom:0cm"><b>INAF-OACT</b><o:p></o:p></p><ul><li style="margin-bottom: 0cm; text-align: justify;">Ultra High vacuum chamber (UHV; pressure about 10^-9 mbar)</li><li style="margin-bottom: 0cm; text-align: justify;">Helium closed-cycle cryostat (CTI-350CP)</li><li style="margin-bottom: 0cm; text-align: justify;">Ion implanter (Danfysik-1080)</li><li style="margin-bottom: 0cm; text-align: justify;">FTIR spectrometer (Bruker Vertex 70)</li></ul><p style="margin-bottom: 0cm; text-align: justify;"><br></p><p><b>University of Firenze</b><br></p><ul><li style="margin-bottom: 0cm; line-height: normal;">Zeiss EVO MA15 – Scanning Electron Microscope<br></li><li style="margin-bottom: 0cm; line-height: normal;">Jeol JXA8230 Electron Micro-Probe </li><li style="margin-bottom: 0cm; line-height: normal;">Tandem accelerator – IBA </li><li style="margin-bottom: 0cm; line-height: normal;">Agilent 7800 ICP-MS <br></li><li style="margin-bottom: 0cm; line-height: normal;">ThermoFischer Triton-Plus TIMS instrument<br></li><li style="margin-bottom: 0cm; line-height: normal;">Horiba Jobin-Yvon LabRAM – MicroRaman and microFTIR <br></li><li style="margin-bottom: 0cm; line-height: normal;">Bruker SKYSCAN 1172 – X-ray Micro CT Scanner</li><li style="margin-bottom: 0cm; line-height: normal;">Single crystal diffractometer D8 Venture (Bruker) with double microsource</li><li style="margin-bottom: 0cm; line-height: normal;">Single crystal diffractometer XcaliburPX Ultra (Oxford Diffraction)</li><li style="margin-bottom: 0cm; line-height: normal;">Single crystal diffractometer Xcalibur3 (Oxford Diffraction)</li><li style="margin-bottom: 0cm; line-height: normal;">X-ray powder diffractometer D8 "Da Vinci" (Bruker)</li><li style="margin-bottom: 0cm; line-height: normal;">X-ray powder diffractometer D8 Advance (Bruker)</li><li style="margin-bottom: 0cm; line-height: normal;">X-ray Fluorescence Spectrometer Rigaku ZSX Primus II</li><li>X-ray Fluorescence Spectrometer Shimadzu EDX 7000</li></ul><p style="margin-bottom: 0cm; text-align: justify;"></p><p> <br></p><p><br></p>
15. Team members, Informazioni generali
15. Personale INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2022/2023/2024) | FTE Presunte (2022/2023/2024) | Extra | ||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | ernesto.palomba | ernesto.palomba@inaf.it | IAPS ROMA | Y | PRIMO RICERCATORE | PI | X X X | X X X | X |
|
| 2 | andrea.longobardo | andrea.longobardo@inaf.it | IAPS ROMA | Y | RICERCATORE | Co-I | X X X | X X X | X |
|
| 3 | vincenzo.dellacorte | vincenzo.dellacorte@inaf.it | IAPS ROMA | Y | PRIMO TECNOLOGO | Co-I | X X X | X X X | X |
|
| 4 | giuseppe.baratta | giuseppe.baratta@inaf.it | O.A. CATANIA | Y | ASTRONOMO ASSOCIATO | Co-I | X X X | X X X | X |
|
| 5 | maria.palumbo | maria.palumbo@inaf.it | O.A. CATANIA | Y | DIRIGENTE DI RICERCA | Co-I | X X X | X X X | X |
|
| 6 | carlotta.scire | carlotta.scire@inaf.it | O.A. CATANIA | Y | TECNOLOGO | Co-I | X X X | X X X | X |
|
| 7 | daniele.fulvio | daniele.fulvio@inaf.it | O.A. CAPODIMONTE | Y | RICERCATORE | Co-I | X X X | X X X | X |
|
16. Personale Associato INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2022/2023/2024) | FTE Presunte (2022/2023/2024) | Extra | |
|---|---|---|---|---|---|---|---|---|---|
| 1 | giovanni.pratesi | g.pratesi@unifi.it | Università di Firenze | Y | Professore Associato | Co-I | [0, 0, 0] | [0.2, 0.2, 0.2] | 0.0 |
| 2 | laura.chelazzi | laura.chelazzi@unifi.it | Università di Firenze | Y | Tecnologo | Co-I | [0, 0, 0] | [0.2, 0.2, 0.2] | 0.0 |
| 3 | franco.lucarelli | franco.lucarelli@unifi.it | Università di Firenze | Y | Professore Ordinario | Co-I | [0, 0, 0] | [0.2, 0.2, 0.2] | 0.0 |
| 4 | stefano.caporali | stefano.caporali@unifi.it | Università di Firenze | N | Ricercatore | Co-I | [0, 0, 0] | [0.2, 0.2, 0.2] | 0.0 |
| 5 | tiziano.catelani | tiziano.catelani@unifi.it | Università di Firenze | Y | Tecnologo | Co-I | [0, 0, 0] | [0.2, 0.2, 0.2] | 0.0 |
21. Fondi a Sostegno Iniziativa
Si chiede il finanziamento sul large program
Tabella fondi:
| # | Provenienza | Certi 2022 (k€) | Certi 2023 (k€) | Certi 2024 (k€) | Presun. 2022 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
|---|
Tabella fondi Astrofisica Fondamentale e PNRR:
| # | Provenienza | Fondi 2022 (€) | Fondi 2023 (€) | Fondi 2024 (€) |
|---|