Europe's new exoplanet-spotting space telescope has observed its first alien worlds.
The probe, called the Characterizing Exoplanet Satellite (CHEOPS), launched into Earth's orbit last December and has just completed a three-month commissioning phase. During that time, the European Space Agency (ESA) tested out CHEOPS' instruments and even used the telescope to observe a few exoplanets, or planets that orbit stars beyond our solar system. The space observatory is now ready to begin routine science observations, which should begin at the end of April, ESA officials said in a statement.
While other exoplanet missions like NASA's Kepler Space Telescope and the Transiting Exoplanet Survey Satellite (TESS) were designed to search for planets around other stars, CHEOPS will spend its time honing in on known exoplanets to measure their sizes with unprecedented accuracy and precision. Combined with data on each exoplanet's mass, which can be calculated from their orbits, the size measurements will allow astronomers to determine each exoplanet's density, thus revealing more clues about the composition of these worlds — and whether they could sustain life.
Video: Europe's new exoplanet hunter begins star observations
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CHEOPS performed a series of in-flight tests between January and February to make sure its instruments were functioning and calibrated properly. The spacecraft took its first images in February, featuring blurry views of star systems. Those fuzzy images were no accident.
"The deliberate defocusing is at the core of the mission's observing strategy, which improves the measurement precision by spreading the light coming from distant stars over many pixels of its detector," ESA said in the statement.
In March, the new space telescope began looking at well-known star systems. CHEOPS "first needed to observe stars whose properties are well known, stars that are well-behaved — hand-picked to be very stable, with no signs of activity," CHEOPS project scientist Kate Isaak said in the statement. This allowed the CHEOPS team on Earth to verify that the satellite's instruments are precise and stable enough for observations.
"We were thrilled when we realised that all the systems worked as expected or even better than expected," CHEOPS instrument scientist Andrea Fortier said in the same statement.
CHEOPS spent the last two weeks of in-orbit commissioning observing two stars that are known to host exoplanets. Specifically, the telescope practiced watching as exoplanets transited their stars. During a transit, an exoplanet crosses in front of the star, blocking a tiny bit of starlight and causing the star to dim slightly. While TESS uses the "transit method" to search for alien worlds, CHEOPS will use transits to take precise measurements of exoplanets.
One of the exoplanets that CHEOPS observed during this practice one is a puffy, gaseous world known as KELT-11b. The exoplanet orbits a subgiant star called HD 93396, which is located 320 light-years away from Earth. HD 93396 is three times larger than our sun, and KELT-11b is about 30% larger than Jupiter, but the gas giant orbits closer to its host star than Mercury is to the sun.
Using data CHEOPS gathered during that transit, scientists measured that KELT-11b is 112,800 miles (181,600 kilometers) wide. This measurement is five times more accurate than what can be done using Earth-based telescopes, ESA officials said in the statement.
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ESA held a formal review of the satellite's performance and ground operations on March 25, and CHEOPS passed it with flying colors. "The in-orbit commissioning phase was an exciting period, and we are pleased we were able to meet all requirements," said Nicola Rando, CHEOPS project manager at ESA. "The satellite platform and instrument performed remarkably, and both the Mission and Science Operation Centres supported operations impeccably."
While the mission's science phase has not yet officially begun, CHEOPS is already taking a peek at some of its early targets, which include the exoplanets 55 Cancri e (a hot 'super-Earth' with a lava ocean) and GJ 436b, a so-called 'warm Neptune' that is losing its atmosphere.
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Email Hanneke Weitering at email@example.com or follow her @hannekescience. Follow us on Twitter @Spacedotcom and on Facebook.
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Good diameter measurement reported. Other reports I read show close to 1.3 Jupiter radii, given the diameter in km, I calculated about 1.27 Jupiter radii. Did not see a rotation rate but if similar to Jupiter, spinning near 16 km/s at its equator. I had some notes on this exoplanet in my home database. KELT-11b: A Highly Inflated Sub-Saturn Exoplanet Transiting the V = 8 Subgiant HD 93396