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Astronomie - Cheops, ESA’s exoplanet mission -Update-3

12.03.2023

CHEOPS mission extended

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ESA

After more than three years in orbit, the mission of the CHEOPS space telescope has just been extended. Led by the University of Bern in collaboration with the University of Geneva, CHEOPS is a joint mission of the European Space Agency (ESA) and Switzerland. On March 7th, ESA’s Science Programme Committee has confirmed its continued operations to 2026 and an indicative extension to 2029, contingent upon ongoing commitments from national contributors and partners. Since its launch in December 2019, the satellite’s extremely precise measurements have contributed to several key discoveries in the field of exoplanets. The extension will make it possible to study these fascinating worlds around other stars in even more detail.

Unlike previous satellites designed to find new exoplanets – planets orbiting stars other than our Sun – by observing tens of thousands of stars simultaneously, CHEOPS has been optimized to observe a single star at a time and it targets stars already known to host exoplanets. The aim of CHEOPS is therefore to go beyond a mere census of exoplanets, and measure some of their key characteristics, in particular their size, with an exquisite precision. This precision is what allows astronomer to infer what these planets are made of: combining the CHEOPS size measurement with the previously known planet mass yields the density: dense planets like the Earth are mainly composed of rocks and metals, while planets with low densities like Jupiter are mostly made out of gas. Since these compositions are the result of the planet formation process, getting to know them opens a window to the past history of planetary systems, putting our own Solar System in context.

Observation of exoplanet properties

“In this respect, the mission has been extremely successful,” highlights Willy Benz, Professor emeritus of astrophysics at the University of Bern and head of the CHEOPS consortium, “the precision of CHEOPS has exceeded all expectations and has allowed us to determine properties of several of the most interesting exoplanets.”

For example, by closely observing how the luminosity changes as the planet WASP-103b passes in front of its star, scientists from the CHEOPS team have observed that the planet is deformed into the shape of a rugby ball due to the intense gravity of the nearby star. Such planets are so hot that CHEOPS has also been able to detect them glowing along their orbit around their stars. “The glow detected with CHEOPS for the planet WASP-189b is only a few millionth of the light emitted by the star, and is related to the temperature of the planet atmosphere and its cloud coverage. So it is clear that CHEOPS can do much more than ‘simply’ measuring planet sizes,” explains Prof. David Ehrenreich of the University of Geneva, who is co-chairing the international team of over a hundred of scientists involved in the exploitation of the mission.

More exciting discoveries with the extended mission

The primary mission of CHEOPS was planned to last for three and a half years, that is until September 2023. The outstanding quality of the science produced by the mission is attested by the publication of over fifty scientific articles based on CHEOPS data in international journals. The satellite was successfully operated amidst a global pandemic, and its health is excellent with respect to the harsh conditions of space, where it is constantly bombarded by cosmic rays and high-energy radiation. All these elements have pushed the CHEOPS team to propose extending the mission beyond 2023.

The extension of CHEOPS operations has now been confirmed by the ESA Science Programme Committee until at least 2026, provided ongoing support from national contributors and partners. The CHEOPS team members are originating from 40 institutions across Europe: in addition to ESA, 11 countries, including Switzerland in a leading role, have come together to fund and build the telescope between 2012 and 2019. “CHEOPS can continue to count on the strong support of the participating Funding Agencies, including Switzerland, for the extension of the mission, and that the Swiss lead in the CHEOPS mission (including its extended operations) is possible due to the membership of Switzerland in ESA and through its participation in the PRODEX program,” says Oliver Botta, chair of the CHEOPS Steering Committee.

With the newly approved mission extension, the CHEOPS team plans to continue using CHEOPS for what it does best while at the same time trying out new observations. “We have only scratched the surface of the capabilities of CHEOPS, there is much more science that can be done with the satellite and we look forward to exploring it during the extension,” declares Benz. “A very exciting result would be the discovery of the first exomoon,” reveals Ehrenreich. “Many planets in our Solar System have moons, so we expect to find some around exoplanets, and we are currently observing some candidates. It is challenging to detect exomoons though, because they are small, hence their signatures are faint. However, CHEOPS is precise enough to find exomoons as small as the planet Mars, which is twice the size of our Moon. If such moons exist in the systems we observe, we could find them during the extended mission.”

A unique role in the landscape of space missions

Another unique characteristic of CHEOPS is its ability to combine forces with other space missions such as the James Webb Space Telescope (JWST), which is a joint mission of NASA and ESA. CHEOPS can refine our knowledge of already known exoplanets to select the best candidates to be observed with JWST to probe the atmospheres of these planets. “Thanks to CHEOPS observations, we have been granted valuable JWST time to observe the planets in the TOI-178 system to determine their atmospheric composition, which will help to understand the dynamical history of the system,” specifies Prof. Yann Alibert of the University of Bern. Alibert is coordinating the CHEOPS program dedicated to the follow-up of multiplanetary systems discovered by NASA’s satellite TESS. “This is an example of a great synergy between CHEOPS and other missions: TESS originally found 3 planets orbiting the star TOI-178. When CHEOPS looked at this system, it discovered three more planets and revealed an outstanding and fragile orbital harmony, leading us to hypothesize that it has been unperturbed for billions of years,” explains Alibert.

“Scientists are eager to find out what surprising results CHEOPS will bring next; what is sure now is that CHEOPS will continue to make new discoveries for years to come,” concludes Benz.

After more than three years in orbit, the mission of the CHEOPS space telescope has just been extended. Led by the University of Bern in collaboration with the University of Geneva, CHEOPS is a joint mission of the European Space Agency (ESA) and Switzerland. On March 7th, ESA’s Science Programme Committee has confirmed its continued operations to 2026 and an indicative extension to 2029, contingent upon ongoing commitments from national contributors and partners. Since its launch in December 2019, the satellite’s extremely precise measurements have contributed to several key discoveries in the field of exoplanets. The extension will make it possible to study these fascinating worlds around other stars in even more detail.

Unlike previous satellites designed to find new exoplanets – planets orbiting stars other than our Sun – by observing tens of thousands of stars simultaneously, CHEOPS has been optimized to observe a single star at a time and it targets stars already known to host exoplanets. The aim of CHEOPS is therefore to go beyond a mere census of exoplanets, and measure some of their key characteristics, in particular their size, with an exquisite precision. This precision is what allows astronomer to infer what these planets are made of: combining the CHEOPS size measurement with the previously known planet mass yields the density: dense planets like the Earth are mainly composed of rocks and metals, while planets with low densities like Jupiter are mostly made out of gas. Since these compositions are the result of the planet formation process, getting to know them opens a window to the past history of planetary systems, putting our own Solar System in context.

Observation of exoplanet properties

“In this respect, the mission has been extremely successful,” highlights Willy Benz, Professor emeritus of astrophysics at the University of Bern and head of the CHEOPS consortium, “the precision of CHEOPS has exceeded all expectations and has allowed us to determine properties of several of the most interesting exoplanets.”

For example, by closely observing how the luminosity changes as the planet WASP-103b passes in front of its star, scientists from the CHEOPS team have observed that the planet is deformed into the shape of a rugby ball due to the intense gravity of the nearby star. Such planets are so hot that CHEOPS has also been able to detect them glowing along their orbit around their stars. “The glow detected with CHEOPS for the planet WASP-189b is only a few millionth of the light emitted by the star, and is related to the temperature of the planet atmosphere and its cloud coverage. So it is clear that CHEOPS can do much more than ‘simply’ measuring planet sizes,” explains Prof. David Ehrenreich of the University of Geneva, who is co-chairing the international team of over a hundred of scientists involved in the exploitation of the mission.

More exciting discoveries with the extended mission

The primary mission of CHEOPS was planned to last for three and a half years, that is until September 2023. The outstanding quality of the science produced by the mission is attested by the publication of over fifty scientific articles based on CHEOPS data in international journals. The satellite was successfully operated amidst a global pandemic, and its health is excellent with respect to the harsh conditions of space, where it is constantly bombarded by cosmic rays and high-energy radiation. All these elements have pushed the CHEOPS team to propose extending the mission beyond 2023.

The extension of CHEOPS operations has now been confirmed by the ESA Science Programme Committee until at least 2026, provided ongoing support from national contributors and partners. The CHEOPS team members are originating from 40 institutions across Europe: in addition to ESA, 11 countries, including Switzerland in a leading role, have come together to fund and build the telescope between 2012 and 2019. “CHEOPS can continue to count on the strong support of the participating Funding Agencies, including Switzerland, for the extension of the mission, and that the Swiss lead in the CHEOPS mission (including its extended operations) is possible due to the membership of Switzerland in ESA and through its participation in the PRODEX program,” says Oliver Botta, chair of the CHEOPS Steering Committee.

With the newly approved mission extension, the CHEOPS team plans to continue using CHEOPS for what it does best while at the same time trying out new observations. “We have only scratched the surface of the capabilities of CHEOPS, there is much more science that can be done with the satellite and we look forward to exploring it during the extension,” declares Benz. “A very exciting result would be the discovery of the first exomoon,” reveals Ehrenreich. “Many planets in our Solar System have moons, so we expect to find some around exoplanets, and we are currently observing some candidates. It is challenging to detect exomoons though, because they are small, hence their signatures are faint. However, CHEOPS is precise enough to find exomoons as small as the planet Mars, which is twice the size of our Moon. If such moons exist in the systems we observe, we could find them during the extended mission.”

A unique role in the landscape of space missions

Another unique characteristic of CHEOPS is its ability to combine forces with other space missions such as the James Webb Space Telescope (JWST), which is a joint mission of NASA and ESA. CHEOPS can refine our knowledge of already known exoplanets to select the best candidates to be observed with JWST to probe the atmospheres of these planets. “Thanks to CHEOPS observations, we have been granted valuable JWST time to observe the planets in the TOI-178 system to determine their atmospheric composition, which will help to understand the dynamical history of the system,” specifies Prof. Yann Alibert of the University of Bern. Alibert is coordinating the CHEOPS program dedicated to the follow-up of multiplanetary systems discovered by NASA’s satellite TESS. “This is an example of a great synergy between CHEOPS and other missions: TESS originally found 3 planets orbiting the star TOI-178. When CHEOPS looked at this system, it discovered three more planets and revealed an outstanding and fragile orbital harmony, leading us to hypothesize that it has been unperturbed for billions of years,” explains Alibert.

“Scientists are eager to find out what surprising results CHEOPS will bring next; what is sure now is that CHEOPS will continue to make new discoveries for years to come,” concludes Benz.

After more than three years in orbit, the mission of the CHEOPS space telescope has just been extended. Led by the University of Bern in collaboration with the University of Geneva, CHEOPS is a joint mission of the European Space Agency (ESA) and Switzerland. On March 7th, ESA’s Science Programme Committee has confirmed its continued operations to 2026 and an indicative extension to 2029, contingent upon ongoing commitments from national contributors and partners. Since its launch in December 2019, the satellite’s extremely precise measurements have contributed to several key discoveries in the field of exoplanets. The extension will make it possible to study these fascinating worlds around other stars in even more detail.

Unlike previous satellites designed to find new exoplanets – planets orbiting stars other than our Sun – by observing tens of thousands of stars simultaneously, CHEOPS has been optimized to observe a single star at a time and it targets stars already known to host exoplanets. The aim of CHEOPS is therefore to go beyond a mere census of exoplanets, and measure some of their key characteristics, in particular their size, with an exquisite precision. This precision is what allows astronomer to infer what these planets are made of: combining the CHEOPS size measurement with the previously known planet mass yields the density: dense planets like the Earth are mainly composed of rocks and metals, while planets with low densities like Jupiter are mostly made out of gas. Since these compositions are the result of the planet formation process, getting to know them opens a window to the past history of planetary systems, putting our own Solar System in context.

Observation of exoplanet properties

“In this respect, the mission has been extremely successful,” highlights Willy Benz, Professor emeritus of astrophysics at the University of Bern and head of the CHEOPS consortium, “the precision of CHEOPS has exceeded all expectations and has allowed us to determine properties of several of the most interesting exoplanets.”

For example, by closely observing how the luminosity changes as the planet WASP-103b passes in front of its star, scientists from the CHEOPS team have observed that the planet is deformed into the shape of a rugby ball due to the intense gravity of the nearby star. Such planets are so hot that CHEOPS has also been able to detect them glowing along their orbit around their stars. “The glow detected with CHEOPS for the planet WASP-189b is only a few millionth of the light emitted by the star, and is related to the temperature of the planet atmosphere and its cloud coverage. So it is clear that CHEOPS can do much more than ‘simply’ measuring planet sizes,” explains Prof. David Ehrenreich of the University of Geneva, who is co-chairing the international team of over a hundred of scientists involved in the exploitation of the mission.

More exciting discoveries with the extended mission

The primary mission of CHEOPS was planned to last for three and a half years, that is until September 2023. The outstanding quality of the science produced by the mission is attested by the publication of over fifty scientific articles based on CHEOPS data in international journals. The satellite was successfully operated amidst a global pandemic, and its health is excellent with respect to the harsh conditions of space, where it is constantly bombarded by cosmic rays and high-energy radiation. All these elements have pushed the CHEOPS team to propose extending the mission beyond 2023.

The extension of CHEOPS operations has now been confirmed by the ESA Science Programme Committee until at least 2026, provided ongoing support from national contributors and partners. The CHEOPS team members are originating from 40 institutions across Europe: in addition to ESA, 11 countries, including Switzerland in a leading role, have come together to fund and build the telescope between 2012 and 2019. “CHEOPS can continue to count on the strong support of the participating Funding Agencies, including Switzerland, for the extension of the mission, and that the Swiss lead in the CHEOPS mission (including its extended operations) is possible due to the membership of Switzerland in ESA and through its participation in the PRODEX program,” says Oliver Botta, chair of the CHEOPS Steering Committee.

With the newly approved mission extension, the CHEOPS team plans to continue using CHEOPS for what it does best while at the same time trying out new observations. “We have only scratched the surface of the capabilities of CHEOPS, there is much more science that can be done with the satellite and we look forward to exploring it during the extension,” declares Benz. “A very exciting result would be the discovery of the first exomoon,” reveals Ehrenreich. “Many planets in our Solar System have moons, so we expect to find some around exoplanets, and we are currently observing some candidates. It is challenging to detect exomoons though, because they are small, hence their signatures are faint. However, CHEOPS is precise enough to find exomoons as small as the planet Mars, which is twice the size of our Moon. If such moons exist in the systems we observe, we could find them during the extended mission.”

A unique role in the landscape of space missions

Another unique characteristic of CHEOPS is its ability to combine forces with other space missions such as the James Webb Space Telescope (JWST), which is a joint mission of NASA and ESA. CHEOPS can refine our knowledge of already known exoplanets to select the best candidates to be observed with JWST to probe the atmospheres of these planets. “Thanks to CHEOPS observations, we have been granted valuable JWST time to observe the planets in the TOI-178 system to determine their atmospheric composition, which will help to understand the dynamical history of the system,” specifies Prof. Yann Alibert of the University of Bern. Alibert is coordinating the CHEOPS program dedicated to the follow-up of multiplanetary systems discovered by NASA’s satellite TESS. “This is an example of a great synergy between CHEOPS and other missions: TESS originally found 3 planets orbiting the star TOI-178. When CHEOPS looked at this system, it discovered three more planets and revealed an outstanding and fragile orbital harmony, leading us to hypothesize that it has been unperturbed for billions of years,” explains Alibert.

“Scientists are eager to find out what surprising results CHEOPS will bring next; what is sure now is that CHEOPS will continue to make new discoveries for years to come,” concludes Benz.

Quelle: University of Bern

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Update: 19.03.2023

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Europe's exoplanet-hunting CHEOPS mission extended through 2026

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