Ariel
Ariel is a space telescope that will systematically probe the atmospheres of about a thousand exoplanets—ranging from gas giants to rocky planets, whether hot or temperate—orbiting stars of various types. ARIEL will measure the composition and structure of planetary atmospheres, constrain the nature of planetary cores, detect the presence of clouds, and study interactions with the host star.
The Role of the IAS
Starting in 2015, drawing on their accumulated expertise, teams from five French laboratories (IAP, DAp/AIM, IAS, LESIA, LAB) played a very significant role in the Ariel studies. Their contributions to the development of the scientific proposal, the mission scenario, and the feasibility studies for the infrared spectrometer—the satellite’s core component—were decisive. This led the French teams to take responsibility for the design and delivery of the infrared spectrometer. The spectrometer will be built, under the supervision of CNES, by CEA-Irfu with significant contributions from IAS and LESIA.
“Ariel is the logical next step in the exoplanet observation programs we will be conducting with the JWST. Ariel’s statistical approach is crucial; it is very encouraging that Europe can play a leading role in this new chapter in the history of exoplanet research,” concludes Pierre-Olivier Lagage.
"ARIEL is the key to unlocking the properties of other worlds' atmospheres!"
Status
In development
Partners (academic / industrial)
Funding Sources
Key Dates (tentative)
Key Steps
Launch: May 2028
Contacts
Advisors (scientific and technical)
- Marc Ollivier, Solar System and Planetary Systems Physics Teamat the IAS (CNRS / Université Paris-Saclay)
- Jean-Philippe Beaulieu, Paris Astrophysics Institute
- Pierre-Olivier Lagage, Department of Astrophysics at CEA-Irfu, UMR AIM Paris-Saclay
- Pierre Drossart, LESIA, Paris Observatory, CNRS, PSL, Sorbonne University, Paris-Diderot University
Selection of the Space Mission
The European Space Agency's Program Committee has selected the Ariel mission as the fourth intermediate-class mission (with a budget of 450 million euros) of the "Cosmic Vision" program.
Ariel will be launched from the Kourou spaceport in French Guiana in May 2028 and will be placed in orbit at the L2 Lagrange point, located 1.5 million kilometers from Earth. Ariel is a space telescope that will systematically probe the atmospheres of about a thousand exoplanets—ranging from gas giants to rocky planets, whether hot or temperate—orbiting various types of stars.
Ariel will measure the composition and structure of planetary atmospheres, determine the nature of planetary cores, detect the presence of clouds, and study interactions with the host star.
The selection process took place in several stages:
Call for mission proposals issued by the ESA in August 2014;
In June 2015, 3 of the 27 proposed projects were shortlisted for detailed concept studies;
Evaluation of the study findings by a committee of experts and recommendation of a field mission in November 2017;
Formal vote by the ESA Program Committee and public announcement on March 20, 2018.
Pierre Drossart notes:“The ARIEL mission study was conducted based on the EChO project, which was a candidate for ESA’s M3 mission in 2014. Advances in exoplanet research now clearly position spectroscopy as a major challenge for the coming decade in the study of exoplanet atmospheres.”
The Ariel mission was proposed by a consortium of more than 60 institutions in 15 European countries(*). The United Kingdom is responsible for scientific and technical coordination. A contribution from the United States is currently under consideration.
Ariel will consist of a telescope approximately one meter in diameter designed to collect visible and infrared light from stars around which an exoplanet orbits. A spectrometer will disperse this light into a “rainbow,” and when the exoplanet transits in front of its star, the resulting spectrum will show absorption lines caused by molecules in the exoplanet’s atmosphere absorbing the star’s light.
Marc Ollivier emphasizes:“Observation is particularly challenging because the information about the planet must be separated from the light of the star itself, which is 1,000 to 100,000 times brighter than the planet. The ultimate performance is achieved thanks to the instrument’s intrinsic photometric stability and a very thorough understanding of how it works.”
Ariel is based on research conducted over the past 10 years. In 2007, water vapor, followed by carbon dioxide and carbon monoxide, were detected in the atmosphere of the hot Jupiter HD189733b using the Spitzer and Hubble space telescopes. The initial results highlighted the difficulty of taking such measurements and the immense diversity of exoplanet atmospheres. To obtain such challenging measurements across a large number of planets, dedicated and optimized instruments are necessary. A group of scientists therefore began studies as early as 2008.
Artist's rendering of the Ariel satellite en route to its final destination: in orbit around the L2 Lagrange point.
ESA/STFC RAL Space/UCL/Europlanet-Science Office
Ariel will be placed in orbit around the L2 Lagrange point, 1.5 million kilometers from Earth. It will orbit the Sun in sync with Earth.
ESA/STFC RAL Space/UCL/Europlanet-Science Office