AEROSPACEPHYS

Multiphysics models and simulations for reacting and plasma flows applied to the space exploration program

 Coordinatore INSTITUT VON KARMAN DE DYNAMIQUE DES FLUIDES 

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 Nazionalità Coordinatore Belgium [BE]
 Totale costo 1˙494˙892 €
 EC contributo 1˙494˙892 €
 Programma FP7-IDEAS-ERC
Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call ERC-2010-StG_20091028
 Funding Scheme ERC-SG
 Anno di inizio 2010
 Periodo (anno-mese-giorno) 2010-09-01   -   2015-08-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    INSTITUT VON KARMAN DE DYNAMIQUE DES FLUIDES

 Organization address address: CHAUSSEE DE WATERLOO 72
city: RHODE SAINT GENESE
postcode: 1640

contact info
Titolo: Mr.
Nome: Dominick
Cognome: Hemeryck
Email: send email
Telefono: +32 2 359 96 11
Fax: +32 2 359 96 00

BE (RHODE SAINT GENESE) hostInstitution 1˙494˙892.20
2    INSTITUT VON KARMAN DE DYNAMIQUE DES FLUIDES

 Organization address address: CHAUSSEE DE WATERLOO 72
city: RHODE SAINT GENESE
postcode: 1640

contact info
Titolo: Prof.
Nome: Thierry Edouard Bertrand
Cognome: Magin
Email: send email
Telefono: +32 2 359 96 38
Fax: +32 2 359 96 00

BE (RHODE SAINT GENESE) hostInstitution 1˙494˙892.20

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

basic    shield    transition    manned    physico    heat    chemical    space    flux    planetary    surface    experimental    computational    robotic    radiation    prediction    models    safety    payload    mission    exploration    data   

 Obiettivo del progetto (Objective)

'Space exploration is one of boldest and most exciting endeavors that humanity has undertaken, and it holds enormous promise for the future. Our next challenges for the spatial conquest include bringing back samples to Earth by means of robotic missions and continuing the manned exploration program, which aims at sending human beings to Mars and bring them home safely. Inaccurate prediction of the heat-flux to the surface of the spacecraft heat shield can be fatal for the crew or the success of a robotic mission. This quantity is estimated during the design phase. An accurate prediction is a particularly complex task, regarding modelling of the following phenomena that are potential “mission killers:” 1) Radiation of the plasma in the shock layer, 2) Complex surface chemistry on the thermal protection material, 3) Flow transition from laminar to turbulent. Our poor understanding of the coupled mechanisms of radiation, ablation, and transition leads to the difficulties in flux prediction. To avoid failure and ensure safety of the astronauts and payload, engineers resort to “safety factors” to determine the thickness of the heat shield, at the expense of the mass of embarked payload. Thinking out of the box and basic research are thus necessary for advancements of the models that will better define the environment and requirements for the design and safe operation of tomorrow’s space vehicles and planetary probes for the manned space exploration. The three basic ingredients for predictive science are: 1) Physico-chemical models, 2) Computational methods, 3) Experimental data. We propose to follow a complementary approach for prediction. The proposed research aims at: “Integrating new advanced physico-chemical models and computational methods, based on a multidisciplinary approach developed together with physicists, chemists, and applied mathematicians, to create a top-notch multiphysics and multiscale numerical platform for simulations of planetary atmosphere entries, crucial to the new challenges of the manned space exploration program. Experimental data will also be used for validation, following state-of-the-art uncertainty quantification methods.”'

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