The science of EChO (Exoplanet Characterisation Observatory)
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
The science of extra-solar planets is one of the most rapidly changing areas of astrophysics and since 1995 the number of planets known has increased by almost two orders of magnitude. A combination of ground-based surveys and ded-icated space missions has resulted in 700-plus planets being detected, and over 1200 that await confirmation. NASA's Kepler mission has opened up the possibility of discovering Earth-like planets in the habitable zone around some of the 100,000 stars it is surveying during its 3 to 4-year lifetime. The new Gaia mission is expected to discover thousands of new planets around stars within 200 parsecs of the Sun. Yet among the exoplanets detected or proposed, so far there is actually little resemblance to the morphology of the Solar System.
The key challenge now is moving on from discovery, important though that remains, to characterisation: what are these planets actually like, and why are they as they are?
In the past ten years, we have learned how to obtain the first spectra of exoplanets using transit transmission and emis-sion spectroscopy. With the high stability of Spitzer, Hubble, and large ground-based telescopes the spectra of bright close-in massive planets can be obtained and species like water vapour, methane, carbon monoxide and dioxide have been detected. With transit science came the first tangible remote sensing of these planetary bodies and so one can start to extrapolate from what has been learnt from Solar System probes to what one might plan to learn about their faraway siblings. As we learn more about the atmospheres, surfaces and near-surfaces of these remote bodies, we will begin to build up a clearer picture of their construction, history and suitability for life.
The Exoplanet Characterisation Observatory, EChO, will be the first dedicated mission to investigate the physics and chemistry of Exoplanetary Atmospheres. By characterising spectroscopically more bodies in different envi-ronments we will take detailed planetology out of the Solar System and into the Galaxy as a whole.
EChO has now been selected by the European Space Agency to be assessed as one of four M3 mission candidates. Dr Giovanna Tinetti (UCL) has been selected as the ESA science team lead scientist for the assessment study phase, and Professor Bruce Swinyard (RAL/UCL) has been named as a member of the ESA science team. Our UK-led consortium has received full support from UKSA to complete the technical studies of the EChO payload. It is now paramount to secure the UK scientific return, and we estimate that a twenty-four months PDRA would provide Tinetti and Swinyard the needed support.
The key challenge now is moving on from discovery, important though that remains, to characterisation: what are these planets actually like, and why are they as they are?
In the past ten years, we have learned how to obtain the first spectra of exoplanets using transit transmission and emis-sion spectroscopy. With the high stability of Spitzer, Hubble, and large ground-based telescopes the spectra of bright close-in massive planets can be obtained and species like water vapour, methane, carbon monoxide and dioxide have been detected. With transit science came the first tangible remote sensing of these planetary bodies and so one can start to extrapolate from what has been learnt from Solar System probes to what one might plan to learn about their faraway siblings. As we learn more about the atmospheres, surfaces and near-surfaces of these remote bodies, we will begin to build up a clearer picture of their construction, history and suitability for life.
The Exoplanet Characterisation Observatory, EChO, will be the first dedicated mission to investigate the physics and chemistry of Exoplanetary Atmospheres. By characterising spectroscopically more bodies in different envi-ronments we will take detailed planetology out of the Solar System and into the Galaxy as a whole.
EChO has now been selected by the European Space Agency to be assessed as one of four M3 mission candidates. Dr Giovanna Tinetti (UCL) has been selected as the ESA science team lead scientist for the assessment study phase, and Professor Bruce Swinyard (RAL/UCL) has been named as a member of the ESA science team. Our UK-led consortium has received full support from UKSA to complete the technical studies of the EChO payload. It is now paramount to secure the UK scientific return, and we estimate that a twenty-four months PDRA would provide Tinetti and Swinyard the needed support.
Planned Impact
Maximising the return for the UK industry - our goal is to get UK industry as prime contractor for EChO or, at the very least, to be providing a significant part of the spacecraft system. The EChO mission requires some technological development, in particular of detectors, and we see major potential benefits to UK industry in developing solutions for EChO. We are working alongside UK industry to specify and assist in the development of those solutions to maximise the economic and technological return to the UK.
Outreach - The discovery of over 700 extrasolar planets in the last 15 years is probably the most exciting development of modern astronomy. It resonates enormously with a public that has already been shown to have high interest levels in the exploration of the diverse worlds of our own Solar System, and an insatiable hunger for news about space exploration. It directly addresses deep philosophical issues that concern our fellow citizens: what are other worlds like? how do they form and evolve? Are we alone in the universe? So that means that public outreach that aims to engage our fellow citizens with the excitement of EChO and its science objectives will be at the forefront of our planning.
We will also have a pro-active programme of briefing and informing policy makers at a national and European level, through one-on-one meetings, seminars for politicians, exhibitions at venues such as the European Parliament, and public events that will involve political figures as keynote speakers.
Attracting the Next Generation of Scientists and Engineers - the UK future economy and competitiveness depends on strong science and engineering sectors. The promotion of observational and space sciences is crucial to inspire development of the next generation of scientists and engineers. Extrasolar planets are today one of the most trendy subject, inspiring young people to take up the (physical) sciences in later studies and in their careers.
Outreach - The discovery of over 700 extrasolar planets in the last 15 years is probably the most exciting development of modern astronomy. It resonates enormously with a public that has already been shown to have high interest levels in the exploration of the diverse worlds of our own Solar System, and an insatiable hunger for news about space exploration. It directly addresses deep philosophical issues that concern our fellow citizens: what are other worlds like? how do they form and evolve? Are we alone in the universe? So that means that public outreach that aims to engage our fellow citizens with the excitement of EChO and its science objectives will be at the forefront of our planning.
We will also have a pro-active programme of briefing and informing policy makers at a national and European level, through one-on-one meetings, seminars for politicians, exhibitions at venues such as the European Parliament, and public events that will involve political figures as keynote speakers.
Attracting the Next Generation of Scientists and Engineers - the UK future economy and competitiveness depends on strong science and engineering sectors. The promotion of observational and space sciences is crucial to inspire development of the next generation of scientists and engineers. Extrasolar planets are today one of the most trendy subject, inspiring young people to take up the (physical) sciences in later studies and in their careers.
Publications
Al-Refaie A
(2022)
A Comparison of Chemical Models of Exoplanet Atmospheres Enabled by TauREx 3.1
in The Astrophysical Journal
Al-Refaie A. F.
(2022)
TauREx3: Tau Retrieval for Exoplanets
in Astrophysics Source Code Library
Allard N
(2013)
Collisional line profiles of sodium perturbed by H 2 from the optical to the infrared spectral range
in EAS Publications Series
Allard N
(2012)
Theoretical and laboratory spectra of sodium perturbed by molecular hydrogen
in Astronomy & Astrophysics
Anisman L
(2022)
Cross-sections for heavy atmospheres: H 2 O continuum
in Journal of Quantitative Spectroscopy and Radiative Transfer
Anisman L
(2022)
Cross-sections for heavy atmospheres: H 2 O self-broadening
in Journal of Quantitative Spectroscopy and Radiative Transfer
Anisman Lara O.
(2022)
Cross-sections for heavy atmospheres: H$_2$O self-broadening
in arXiv e-prints
Barstow J
(2022)
A retrieval challenge exercise for the Ariel mission
in Experimental Astronomy
Bocchieri A
(2022)
Detecting molecules in Ariel Tier 1 transmission spectra
Bocchieri A
(2023)
Detecting molecules in Ariel low resolution transmission spectra
in Experimental Astronomy
Description | We have assessed the feasibility of a dedicated space mission to observe exoplanet atmospheres in the infrared. The outcome of this study allowed the selection of the ARIEL space mission by ESA in 2018 |
Exploitation Route | All the scientific and technical results were published in open access journals and software developed made publicly available on gitHub. |
Sectors | Aerospace, Defence and Marine,Education |
Description | 1) During the grant, we developed a new instrument simulator to evaluate the performances of a dedicated transit spectroscopy mission (EChOSIM) (Waldmann and Pascale, 2014; Pascale te al., 2014; Varley et al., 2014) 2) We found new statistical methods to detrend the planet signal from the stellar activity and instrument systematics (ICA, Gaussian processes etc.) (Waldmann, 2012; Danielski et al., 2014; Waldmann et al., 2013; Waldmann, 2014; Morello et al., 2014) 3) We developed a new spectral retrieval model to extract the maximum information out of an exoplanet spectrum (TauRex) (Waldmann et al., 2014) |
First Year Of Impact | 2013 |
Sector | Aerospace, Defence and Marine,Creative Economy,Education |
Impact Types | Cultural,Economic |
Description | Chair of Hubble and Spitzer space telescope panels |
Geographic Reach | North America |
Policy Influence Type | Participation in a guidance/advisory committee |
Description | European Research Council Consolidator grant |
Amount | £2,000,000 (GBP) |
Organisation | European Research Council (ERC) |
Sector | Public |
Country | Belgium |
Start | 05/2014 |
End | 04/2019 |
Description | Royal Society URF renewal |
Amount | £311,507 (GBP) |
Organisation | The Royal Society |
Sector | Charity/Non Profit |
Country | United Kingdom |
Start | 10/2013 |
End | 09/2016 |
Description | EChO consortium |
Organisation | ECHO |
Country | United Kingdom |
Sector | Private |
PI Contribution | Prof. Giovanna Tinetti (UCL) was the PI of the EChO mission candidate during the assessment study phase. Members of the UK-led instrument study consortium were France, Italy, Spain, MPS-Germany, Ireland, Denmark, Poland, Belgium, Austria, NL, US. The UK has demonstrated world-leading expertise in the modelling of planetary and exoplanetary atmospheres and is well-placed to lead the spectroscopic characterisation of exoplanets. By taking the PI role we could direct the specification and design of the mission to ensure that UK scientific interests remain at the forefront of the mission goals. Concerning the payload, the UK were in charge of the management, AIV, coolers, IR detectors characterisation, and goal channel 11-16 micron. |
Collaborator Contribution | France: 5-11 micron channel, detectors characterisation, scheduling, spectroscopy Italy: 0.5-2.5 micron channel, stellar activity, targets Spain: 0.25-5 micron channel, stellar activity and targets Germany & NL: read out electronics Poland, Belgium, Austria: FGS |
Impact | Multidisciplinary: exoplanets, spectroscopy, atmospheric science, planet formation, space instruments, stellar physics |
Start Year | 2010 |
Company Name | Blue Skies Space Ltd |
Description | The aim of our company is to "enable cost effective, quickly-delivered scientific instruments for users worldwide through a service based model." |
Year Established | 2014 |
Impact | BSSL was setup in 2014 to allow our team to develop the "Twinkle" satellite. |
Website | http://www.blueskiesspace.co.uk |
Description | Academic seminars and conference talks (G. Tinetti) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | Yes |
Geographic Reach | International |
Primary Audience | Professional Practitioners |
Results and Impact | http://giotin.org/pages/conferences.html http://www.ucl.ac.uk/~ucapgti/seminar/ |
Year(s) Of Engagement Activity | 2012,2013,2014,2015,2016,2017,2018,2019,2020 |
URL | http://giotin.org/pages/conferences.html |
Description | Public talks and outreach activities (I. Waldmann) |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | Yes |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | All information is available here: http://www.ingowaldmann.com/static/waldmann_cv_jan2020.pdf All information is available here: http://zuserver2.star.ucl.ac.uk/~ingo/Talks.html |
Year(s) Of Engagement Activity | 2012,2013,2014,2015,2016,2017,2018,2019,2020 |
URL | http://www.ingowaldmann.com/static/waldmann_cv_jan2020.pdf |