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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.

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

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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