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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.

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

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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