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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.

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

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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