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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.

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

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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