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Hot-TEA SIGNED

Hot Terrestrial Exo-planet Atmospheres: preparing new generation instrument observations with a global climate model

Total Cost €

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EC-Contrib. €

0

Partnership

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 Hot-TEA project word cloud

Explore the words cloud of the Hot-TEA project. It provides you a very rough idea of what is the project "Hot-TEA" about.

host    extreme    predict    characterisation    prospects    strongest    astrophysics    explore    hot    signature    efforts    mass    near    devoted    atmosphere    terrestrial    typifying    solar    tackle    decade    unconstrained    more    circulation    theoretical    life    sensitivity    atmospheric    worlds    climates    last    observations    nowadays    innovative    detect    habitable    tea    jupiter    observables    frontier    detection    hope    resolution    orbit    detecting    predicted    signatures    closest    planets    effect    missions    outcome    interpret    radius    perspective    realistic    vast    model    planetary    close    scenarios    diversity    3d    quantify    planet    observational    combine    discovery    esp    modifies    tools    expertise    techniques    extra    proposes    completely    decades    envisaged    global    zone    atmospheres    plus    size    modeling    venus    instruments    variety    climate    generation    earth    rapid    telescopes    spectrographs    ideally   

Project "Hot-TEA" data sheet

The following table provides information about the project.

Coordinator
FCIENCIAS.ID - ASSOCIACAO PARA A INVESTIGACAO E DESENVOLVIMENTO DE CIENCIAS 

Organization address
address: CAMPO GRANDE, EDIFICIO C1, PISO 3
city: LISBON
postcode: 1749 016
website: http://www.fciencias-id.pt

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Portugal [PT]
 Total cost 148˙635 €
 EC max contribution 148˙635 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2017
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2018
 Duration (year-month-day) from 2018-09-01   to  2020-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    FCIENCIAS.ID - ASSOCIACAO PARA A INVESTIGACAO E DESENVOLVIMENTO DE CIENCIAS PT (LISBON) coordinator 148˙635.00

Map

 Project objective

The rapid growth of extra-solar planet (ESP) discovery and characterisation over the last two decades increases our hope to detect life signatures in other worlds in the near future. Given the variety of planetary atmospheres in our Solar System and the number of ESP observed so far, a vast diversity among ESP climate is expected. The study of ESP atmospheres is nowadays seen as the new frontier in Astrophysics, crucial for typifying planets in the habitable zone. Innovative and promising techniques, used so far to identify hot-Jupiter atmospheres, are envisaged to detect Earth-size planet atmospheres by exploiting high resolution spectrographs and large telescopes. To tackle this challenge, major efforts are devoted to 1) find closest ESP targets with the strongest atmospheric signature 2) develop 3D theoretical tools to predict realistic climates. In the perspective of detecting more and more close-in-orbit hot terrestrial planets, Hot-TEA proposes to address observational prospects to Venus-like planets, with the goal of studying how the planet’s atmosphere modifies the observables. With mass and radius similar to the Earth, but a completely different climate, Venus is the best analogue of those future targets. This proposal will ideally combine: my expertise on modeling Venus atmosphere, with the large know-how of the host institute in detection and characterisation of ESP systems, plus the vast expertise in modelling ESP atmospheres of the second host. To reach our objectives, a generic global circulation model adapted to Venus conditions will be used to: explore model sensitivity to unconstrained parameters, quantify the effect of those parameters on the observables, test extreme cases and propose a number of climate scenarios for the targets. The main outcome of Hot-TEA, key predicted observables, will open the way to interpret future observations during the next decade using a whole new generation of European instruments and missions.

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The information about "HOT-TEA" are provided by the European Opendata Portal: CORDIS opendata.

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