Innovative and customized SAmple Container to transport, analyse and storage small extra-terrestrial samples between laboratory facilities
ISAC
Progetto
R & D
Laboratorio
RSN3
RSN5
Attività: Nuova; Data inizio: 2023; Data fine: 2025
fabrizio.dirri fabrizio.dirri@inaf.it
L’obiettivo del progetto è realizzare un portacampioni innovativo per l’analisi di materiale extraterrestre ritornato da Missioni Spaziali per analisi e trasporto nei laboratori e facilities INAF e Università partner. Missioni come Hayabusa1-2/JAXA, Osiris-REX/NASA, Tianwen2/CNSA, rappresentano un’ottima opportunità per analizzare i campioni riportati dai corpi planetari con tecniche: SEM, PIGE, PIXE XPS, spettroscopia infrarossa e irraggiamento da ioni per lo studio morfologico/composizionale e space weathering. Il Team proponente è coinvolto nelle missioni Hayabusa2 e Tianwen2 ed è stato selezionato dalla JAXA per analizzare due grani dell’asteroide Ryugu. In questo scenario, un portacampioni sviluppato ad-hoc è essenziale per il trasporto, analisi e stoccaggio presso i laboratori.
The project goal is to realize a new customized sample container for extraterrestrial returned samples from space missions to be used in different INAF and University laboratories facilities for transportation and analysis. The current missions as Hayabusa1-2/JAXA, Osiris-REX/NASA, Tianwen2/CNSA, are great opportunity to analyze the returned samples from planetary bodies by using different techniques: SEM, PIGE, XPS, infrared microscopy and ion-irradiation to study the morphological/compositional analysis and the space weathering. The team is involved in Hayabusa2 and Tianwen2 missions and recently was selected by JAXA to receive two returned grains of Ryugu asteroid. In this framework, a customized sample container would be essential for samples transportation, analysis and storage.
Tecnologie per la Planetologia
Infrastrutture da Terra (utilizzo)
Infrastrutture da Terra (sviluppo/operazioni)
Struttura | Nfte | N0 | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Nex | Extra |
---|---|---|---|---|---|---|---|---|---|---|
IAPS ROMA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
Totali | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
# | Struttura | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Extra |
---|---|---|---|---|---|---|---|---|
1 | Università di Firenze | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
Totali | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 |
Certi 2023 | Certi 2024 | Certi 2025 | Presunti 2023 | Presunti 2024 | Presunti 2025 |
---|---|---|---|---|---|
0 | 0 | 0 | 0 | 0 | 0 |
<p>Planetary astronomy (sample return from small bodies and planets)</p>
<p>INAF will be the Prime of the project and will lead the project coordination, i.e. Progress Meeting, laboratory activities at Space Materials-Lab, P-Lab and Ion-ENA Lab. INAF will design and develop the innovative sample container for extra-terrestrial samples with one prototype as HW output. <br></p>
<p>The following <b>INAF infrastructures, laboratories and facilities</b> are involved: </p><p><b style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">A. Space Materials Laboratory (SM-Lab) (IAPS-INAF)</b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"> for analysis of extraterrestrial samples and storage with the following facilities: </span><br></p><p><b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"> 1.</span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem; white-space: pre;"> </span></b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><b>Cleanroom ISO7 (20mq) </b>(planned in 2023): composed by 3 fun filter units and engines and pre-room area to avoid contamination;</span><br></p><p><b style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"> 2.</span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem; white-space: pre;"> </span></b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><b>Minilite II Q-switched Nd</b> (planned in 2023): YAG oscillator, Rate 1 – 15 Hz, Energy 50 mJ to 1064 nm; 25 mJ to 532 nm Pulse width 5 – 7 ns to 1064 nm; 3 – 5 ns to 532 nm, Beam diameter 33 mm;</span><br></p><p><b style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"> 3.</span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem; white-space: pre;"> </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">High Vacuum Thermal Processing Facility: </span></b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">45L, Pfeiffer Vacuum HiPace system 400 P, di CF-F Turbo Pump e KIT ACP15 Rotative pump, from 1013 mbar to 10-7 mbar; </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">controlled cold finger from -150°C to 100°C and provided of two power supply CPX400DP, </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">cryogenic valve and electronic controller PID CARELL i33 + Compact DaQ-9178 Chassis (National Instruments); </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">PC and customized Software for Vacuum Chamber managing. </span></p><p><b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"> 4.</span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem; white-space: pre;"> </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">Outgassing and Thermogravimetric Facility: </span></b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">15L, Pfeiffer Vacuum HiPace 80-Eco compact, da 1013 mbar a 10-7 mbar; </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">controlled cold finger from -80°C to 100°C and provided of two power supply CPX400DP; </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">cryogenic valve and electronic controller PID CARELL i33 + Compact DaQ-9174 Chassis (National Instruments); </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">PC and customized Software for Vacuum Chamber and QCM managing and testing.</span></p><p><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><br></span><b style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">B.</span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem; white-space: pre;"> </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">P-Lab M-IR (IAPS-INAF)</span></b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><b> </b>and</span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"> Bruker Hyperion 3000 (infrared microscopy technique) and equipped with LiN2 cooled MCT (Mercury-Cadmium-Telluride) IR detector (P-Lab). The facility is placed under a soft-wall cleanroom (Class ISO6) with low outgassing rate and provided by filter and engines to purify the air.</span></p><p><b style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">C. I</b><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;"><b>on-ENA Lab (IAPS-INAF) </b>with </span><span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">Ion and ENA Beam Facility with Ion-Irradiation source (IQP 10/63) of He+ with a fluence up to 1017 ions/cm2 and ion energy of 5 keV (Esolar wind He+ ~ 4 keV). </span><br></p><p><br></p><p><br></p>
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | ||
---|---|---|---|---|---|---|---|---|---|---|
1 | fabrizio.dirri | fabrizio.dirri@inaf.it | IAPS ROMA | N | TECNOLOGO | Principal Investigators | 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 | giovanna.rinaldi | giovanna.rinaldi@iaps.inaf.it | IAPS ROMA | Y | RICERCATORE | Co-I | X X X | X X X | X | |
4 | massimo.zambelli | massimo.zambelli@inaf.it | IAPS ROMA | Y | PRIMO TECNOLOGO | Co-I | X X X | X X X | X | |
5 | rosanna.rispoli | rosanna.rispoli@inaf.it | IAPS ROMA | Y | RICERCATORE | Co-I | X X X | X X X | X | |
6 | david.biondi | david.biondi@inaf.it | IAPS ROMA | Y | C.T.E.R. | Co-I | X X X | X X X | X |
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | |
---|---|---|---|---|---|---|---|---|---|
1 | giovanni.pratesi | giovanni.pratesi@unif.it | Università di Firenze | Y | Professore | Co-I | [0, 0, 0] | [0.0, 0.2, 0.2] | 0.0 |
La seguente scheda fa riferimento alla richiesta di finanziamento ISAC
# | Provenienza | Certi 2023 (k€) | Certi 2024 (k€) | Certi 2025 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Presun. 2025 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
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# | Provenienza | Fondi 2023 (€) | Fondi 2024 (€) | Fondi 2025 (€) |
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