Names | Atmospheric Remote-sensing Infrared Exoplanet Large-survey |
---|---|
Mission type | Space telescope |
Operator | ESA |
Website | arielmission sci |
Mission duration | 4 years (planned) [1] |
Spacecraft properties | |
Launch mass | 1,300 kg (2,900 lb) [2] |
Dry mass | 1,000 kg (2,200 lb) |
Payload mass | 300 kg (660 lb) |
Start of mission | |
Launch date | 2029 (planned) [3] |
Rocket | Ariane 62 |
Launch site | Centre Spatial Guyanais, Kourou, ELA-4 |
Contractor | Arianespace |
Orbital parameters | |
Reference system | Sun–Earth L2 orbit [4] |
Main Cassegrain reflector | |
Diameter | 1.1 m × 0.7 m (3 ft 7 in × 2 ft 4 in) |
Focal length | f/13.4 |
Collecting area | 0.64 m2 |
Wavelengths | visible and near-infrared |
Instruments | |
Telescope assembly (TA) Ariel infrared spectrometer (AIRS) Fine Guidance System (FGS) | |
ARIEL mission insignia |
The Atmospheric Remote-sensing Infrared Exoplanet Large-survey (ARIEL) is a planned space telescope and the fourth medium-class mission of the European Space Agency's Cosmic Vision programme. The mission is aimed at observing at least 1000 known exoplanets using the transit method, studying and characterising the planets' chemical composition and thermal structures. Compared to the James Webb Space Telescope, ARIEL will be a much smaller telescope with more observing time available for planet characterisation. ARIEL is expected to be launched in 2029 aboard an Arianespace Ariane 6 together with the Comet Interceptor.
ARIEL will observe 1000 planets orbiting distant stars and make the first large-scale survey of the chemistry of exoplanet atmospheres. [5] The objective is to answer fundamental questions about how planetary systems form and evolve. [6] A spectrometer will spread the light into a spectrum ("rainbow") and determine the chemical fingerprints of gases in the planets' atmospheres. [6] This will enable scientists to understand how the chemistry of a planet links to the environment in which it forms, and how its formation and evolution are affected by its parent star. [6] ARIEL will study a diverse population of exoplanets in a wide variety of environments, but it will focus on warm and hot planets in orbits close to their star. [6]
The ARIEL mission is being developed by a consortium of various institutions from eleven member states of the European Space Agency (ESA), [a] and international contributors from four countries. [b] The project is led by principal investigator Giovanna Tinetti of the University College London, [8] [9] who had previously led the unsuccessful Exoplanet Characterisation Observatory (EcHO) proposal for the M3 Cosmic Vision launch slot. [10] [11] Operations of the mission and the spacecraft will be handled jointly by ESA and the consortium behind the mission's development, through a coordinated Instrument Operations and Science Data Centre (IOSDC). [7] A Mission Operations Centre (MOC) will be set up at the European Space Operations Centre (ESOC) in Darmstadt, Germany, while a concurrent ARIEL Science Operations Centre (SOC) will be set up at the European Space Astronomy Centre (ESAC) near Madrid, Spain. [7] The MOC will be responsible for the spacecraft itself, while the SOC will be responsible for archiving mission data and scientific data downlinked from the spacecraft. The IOSDC will help develop results from the mission based on data received by the SOC. [7]
In August 2017, NASA conditionally selected Contribution to ARIEL Spectroscopy of Exoplanets (CASE) as a Partner Mission of Opportunity, pending the result of ESA's Cosmic Vision selection. [12] Under the proposal NASA provides two fine guidance sensors for the ARIEL spacecraft in return for the participation of U.S. scientists in the mission. [13] CASE was officially selected in November 2019, with JPL astrophysicist Mark Swain as principal investigator. [14]
On December 7, 2021, ESA announced that the €200 million contract to build ARIEL had been awarded to Airbus Defence and Space. [15]
On December 6, 2023, ESA approved the construction of ARIEL with a targeted launch date of 2029. [16]
The design of the ARIEL spacecraft is based on that intended for the Exoplanet Characterisation Observatory (EChO) mission, and has heritage from the thermal design of Planck . [7] [17] The body of the spacecraft is split into two distinct modules known as the Service Module (SVM) and the Payload Module (PLM). The SVM is shaped as a 'sandwich' structure, consisting of three aluminium V-Grooves and three pairs of low conductivity fibreglass bipod struts supporting the PLM. [17] A basic horizontal telescope configuration is used for the PLM itself, housing all of the spacecraft's scientific instruments and its oval 1.1 m × 0.7 m (3 ft 7 in × 2 ft 4 in) primary mirror. [17] [18] At launch, the spacecraft will have a fuelled mass of 1,300 kg (2,900 lb), and will have a dry mass of 1,000 kg (2,200 lb). [18] The PLM will account for around 300 kg (660 lb) of that mass. [18]
The ARIEL telescope's assembly is an off-axis Cassegrain telescope followed by a third parabolic mirror to recollimate the beam. The telescope uses an oval 1.1 m × 0.7 m (3 ft 7 in × 2 ft 4 in) primary mirror; the imaging quality of the system is limited by diffraction for wavelengths longer than about 3 μm, and its focal ratio (f) is 13.4. [19] The system will acquire images in the visible and near-infrared spectrum. [19] The near-infrared sensor and its front-end driver board, is the same of Euclid.NISP instrument. To operate its infrared spectroscope between 1.95 μm and 7.8 μm, the telescope will be passively cooled to a temperature of 55 K (−218.2 °C; −360.7 °F). [7] [19]
The ARIEL spacecraft is expected to be launched in 2029 by Arianespace's Ariane 62 launch vehicle (currently in development [20] [21] ) together with the Comet Interceptor. [15] [3] [22] [23] It will be launched from the Centre Spatial Guyanais (CSG) in Kourou, French Guiana, [22] [23] from the "Ensemble de lancement Ariane" ELA-4 (Ariane Launch Area-4) being purpose-built for future Ariane 6 launches. [24] ARIEL will be launched to the L2 Lagrange point, in a position located at a distance of 1,500,000 km (930,000 mi) from Earth, [22] where it will encounter a very stable thermal environment that is required to detect exoplanets. [23]
The James Webb Space Telescope (JWST) is a space telescope designed to conduct infrared astronomy. As the largest telescope in space, it is equipped with high-resolution and high-sensitivity instruments, allowing it to view objects too old, distant, or faint for the Hubble Space Telescope. This enables investigations across many fields of astronomy and cosmology, such as observation of the first stars and the formation of the first galaxies, and detailed atmospheric characterization of potentially habitable exoplanets.
Venus Express (VEX) was the first Venus exploration mission of the European Space Agency (ESA). Launched in November 2005, it arrived at Venus in April 2006 and began continuously sending back science data from its polar orbit around Venus. Equipped with seven scientific instruments, the main objective of the mission was the long term observation of the Venusian atmosphere. The observation over such long periods of time had never been done in previous missions to Venus, and was key to a better understanding of the atmospheric dynamics. ESA concluded the mission in December 2014.
The Herschel Space Observatory was a space observatory built and operated by the European Space Agency (ESA). It was active from 2009 to 2013, and was the largest infrared telescope ever launched until the launch of the James Webb Space Telescope in 2021. Herschel carries a 3.5-metre (11.5 ft) mirror and instruments sensitive to the far infrared and submillimetre wavebands (55–672 μm). Herschel was the fourth and final cornerstone mission in the Horizon 2000 programme, following SOHO/Cluster II, XMM-Newton and Rosetta.
The Space Infrared Telescope for Cosmology and Astrophysics (SPICA), was a proposed infrared space telescope, follow-on to the successful Akari space observatory. It was a collaboration between European and Japanese scientists, which was selected in May 2018 by the European Space Agency (ESA) as a finalist for the next Medium class Mission 5 (M5) of the Cosmic Vision programme, to launch in 2032. At the time the other two finalists were THESEUS and EnVision, with the latter that was eventually selected for further development. SPICA would have improved on the spectral line sensitivity of previous missions, the Spitzer and Herschel space telescopes, between 30 and 230 μm by a factor of 50—100.
PLAnetary Transits and Oscillations of stars (PLATO) is a space telescope under development by the European Space Agency for launch in 2026. The mission goals are to search for planetary transits across up to one million stars, and to discover and characterize rocky extrasolar planets around yellow dwarf stars, subgiant stars, and red dwarf stars. The emphasis of the mission is on Earth-like planets in the habitable zone around Sun-like stars where water can exist in a liquid state. It is the third medium-class mission in ESA's Cosmic Vision programme and is named after the influential Greek philosopher Plato. A secondary objective of the mission is to study stellar oscillations or seismic activity in stars to measure stellar masses and evolution and enable the precise characterization of the planet host star, including its age.
The Nancy Grace Roman Space Telescope (shortened as Roman or the Roman Space Telescope, and formerly the Wide-Field Infrared Survey Telescope or WFIRST) is a NASA infrared space telescope in development and scheduled to launch to a Sun–Earth L2 orbit by May 2027. It is named after former NASA Chief of Astronomy Nancy Grace Roman.
The Exoplanet Characterisation Observatory (EChO) was a proposed space telescope as part of the Cosmic Vision roadmap of the European Space Agency, and competed with four other missions for the M3 slot in the programme. On 19 February 2014 the PLATO mission was selected in place of the other candidates in the programme, including EChO.
The Jupiter Icy Moons Explorer is an interplanetary spacecraft on its way to orbit and study three icy moons of Jupiter: Ganymede, Callisto, and Europa. These planetary-mass moons are planned to be studied because they are thought to have significant bodies of liquid water beneath their frozen surfaces, which would make them potentially habitable for extraterrestrial life.
Fast Infrared Exoplanet Spectroscopy Survey Explorer (FINESSE) was a NASA mission proposal for a space observatory operating in the Near-infrared spectrum for the Medium-Class Explorers program. The Principal Investigator was Mark Swain of the Jet Propulsion Laboratory in Pasadena, California.
CHEOPS is a European space telescope. Its objective is to determine the size of known extrasolar planets, which will allow the estimation of their mass, density, composition and their formation. Launched on 18 December 2019, it is the first Small-class mission in ESA's Cosmic Vision science programme.
The Large Ultraviolet Optical Infrared Surveyor, commonly known as LUVOIR, is a multi-wavelength space telescope concept being developed by NASA under the leadership of a Science and Technology Definition Team. It is one of four large astrophysics space mission concepts studied in preparation for the National Academy of Sciences 2020 Astronomy and Astrophysics Decadal Survey.
Giovanna Tinetti is an Italian physicist based in London. She is a Professor of Physics and Astronomy at University College London, who researches galactic planetary science, exoplanets and atmospheric science.
Contribution to ARIEL Spectroscopy of Exoplanets (CASE) is a detector subsystem contribution to an infrared spectrometer instrument for the planned European ARIEL space telescope. It is being developed by NASA as a contribution to the European Space Agency (ESA) project to add scientific capabilities to the space telescope to observe the chemical composition of the atmospheres of exoplanets, as well exoplanetary metallicities. The ARIEL spacecraft with CASE on board is planned to launch in 2029.
The Science Programme of the European Space Agency is a long-term programme of space science and space exploration missions. Managed by the agency's Directorate of Science, The programme funds the development, launch, and operation of missions led by European space agencies and institutions through generational campaigns. Horizon 2000, the programme's first campaign, facilitated the development of eight missions between 1985 and 1995 including four "cornerstone missions" – SOHO and Cluster II, XMM-Newton, Rosetta, and Herschel. Horizon 2000 Plus, the programme's second campaign, facilitated the development of Gaia, LISA Pathfinder, and BepiColombo between 1995 and 2005. The programme's current campaign since 2005, Cosmic Vision, has so far funded the development of ten missions including three flagship missions, JUICE, Athena, and LISA. The programme's upcoming fourth campaign, Voyage 2050, is currently being drafted. Collaboration with agencies and institutions outside of Europe occasionally occur in the Science Programme, including a collaboration with NASA on Cassini–Huygens and the CNSA on SMILE.
The Comet Interceptor is a robotic spacecraft mission led by the European Space Agency (ESA) planned for launch in 2029. The spacecraft will be "parked" at the Sun-Earth L2 point and wait for up to three years for a long-period comet to fly by at a reachable trajectory and speed.
Cosmic Vision is the third campaign of space science and space exploration missions in the Science Programme of the European Space Agency (ESA). Formulated in 2005 as Cosmic Vision: Space Science for Europe 2015–2025, the campaign succeeded the Horizon 2000 Plus campaign and envisioned a number of missions in the fields of astronomy and solar system exploration beyond 2015. Ten missions across four funding categories are planned to be launched under Cosmic Vision, with the first being CHEOPS in December 2019. A mission to the Galilean moons (JUICE), the first deep space mission with an opportunistic target, and one of the first gravitational-wave space observatories (LISA), are planned for launch as part of the Cosmic Vision campaign.