REVEALing Signatures of Habitable Worlds Hidden by Stellar Activity
REVEAL unites experts to tackle stellar variability, enhancing exoplanet detection and atmospheric analysis, ultimately aiming to identify Earth-like planets and potential signs of life.
Projectdetails
Introduction
For millennia, people have wondered, “Do other Earths exist?” “Are they common?” “Would they show signs of life?” We now have the technical capability to answer these questions. New radial-velocity spectrometers are capable of detecting the reflex motions of stars hosting Earth-mass planets in their habitable zones; the James Webb Space Telescope has the power to probe the atmospheres of rocky exoplanets.
The Variability Problem
Yet the unprecedented precision of these instruments’ measurement capabilities is up against a fundamental astrophysically-imposed barrier to achieving these goals: contamination of exoplanetary signals by stellar activity and variability. Further progress is contingent on solving this “variability problem”.
Project Overview
REVEAL gathers world-leading experts in exoplanetary and stellar physics to tackle this problem in synergy:
- We will build on recent advances in magnetohydrodynamic simulations of stellar atmospheres, and data-driven efforts to separate the exoplanet signal from the stellar variability.
- We will simulate the “ground truth” of the turbulent physics of entire stellar photospheres resolved at the level of individual convective cells for a broad class of stars.
- We will model the emergent spectra of these “virtual” stars and “observe” them using the same data-processing pipelines as stellar radial-velocity and transit-spectroscopy observations.
Observational Strategy
We will continue to observe the Sun and stars hosting small planets found with TESS and PLATO. The stars’ own spectra will REVEAL the clues needed to disentangle stellar variability from our measurements of their planets’ masses and the fingerprints of molecules in their atmospheres.
Conclusion
Our unified efforts will enable the new cutting-edge space observatories and ground-based facilities to realize the full potential of their designs, bringing us closer to the most profound discoveries we could hope to achieve in our lifetimes - the identification of another Earth or even possible signs of life on another planet.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 6.831.455 |
Totale projectbegroting | € 6.831.455 |
Tijdlijn
Startdatum | 1-4-2024 |
Einddatum | 31-3-2030 |
Subsidiejaar | 2024 |
Partners & Locaties
Projectpartners
- UNIVERSITAET GRAZpenvoerder
- MASSACHUSETTS INSTITUTE OF TECHNOLOGY
- MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
- Association of Universities for Research in Astronomy, Inc.
- THE UNIVERSITY COURT OF THE UNIVERSITY OF ST ANDREWS
Land(en)
Vergelijkbare projecten binnen European Research Council
Project | Regeling | Bedrag | Jaar | Actie |
---|---|---|---|---|
Early Earth, Mars and Venus as Exoplanets (EASE)This project aims to model the atmospheric evolution of Earth, Venus, and Mars to enhance understanding of exoplanet habitability using JWST data and advanced numerical simulations. | ERC Consolid... | € 1.985.871 | 2024 | Details |
Physical modelling of stellar activity effects to discover and measure exoearthsThe SPOTLESS project aims to model and correct stellar activity effects in exoplanet research using advanced simulations and machine learning, enhancing the detection and characterization of exoearths. | ERC Advanced... | € 2.477.355 | 2024 | Details |
FInding ExoeaRths: tackling the ChallengEs of stellar activityFIERCE aims to enhance exoplanet detection by developing methods to model and correct stellar noise, using the Paranal solar Espresso Telescope to improve precision in identifying Earth-like planets. | ERC Advanced... | € 2.458.705 | 2022 | Details |
Exometeorology: Probing Extrasolar AtmospheresThe Exo-PEA program aims to investigate clouds, winds, and aurorae in exoplanet atmospheres using advanced telescopes to enhance our understanding of potential Earth-like worlds. | ERC Starting... | € 1.499.964 | 2025 | Details |
Radio stars and exoplanets: Discovering the space weather of other worldsThis project aims to enhance our understanding of exoplanet habitability by using low-frequency radio techniques to analyze space weather conditions around stars and their interactions with orbiting planets. | ERC Starting... | € 1.485.971 | 2025 | Details |
Early Earth, Mars and Venus as Exoplanets (EASE)
This project aims to model the atmospheric evolution of Earth, Venus, and Mars to enhance understanding of exoplanet habitability using JWST data and advanced numerical simulations.
Physical modelling of stellar activity effects to discover and measure exoearths
The SPOTLESS project aims to model and correct stellar activity effects in exoplanet research using advanced simulations and machine learning, enhancing the detection and characterization of exoearths.
FInding ExoeaRths: tackling the ChallengEs of stellar activity
FIERCE aims to enhance exoplanet detection by developing methods to model and correct stellar noise, using the Paranal solar Espresso Telescope to improve precision in identifying Earth-like planets.
Exometeorology: Probing Extrasolar Atmospheres
The Exo-PEA program aims to investigate clouds, winds, and aurorae in exoplanet atmospheres using advanced telescopes to enhance our understanding of potential Earth-like worlds.
Radio stars and exoplanets: Discovering the space weather of other worlds
This project aims to enhance our understanding of exoplanet habitability by using low-frequency radio techniques to analyze space weather conditions around stars and their interactions with orbiting planets.