First light for SPECULOOS
Credit: ESO/ P. Horálek
The SPECULOOS Southern Observatory (SSO) has been successfully installed at the Paranal Observatory and has obtained its first engineering and calibration images — a process known as first light. After finishing this commissioning phase, this new array of planet-hunting telescopes will begin scientific operations, starting in earnest in January 2019.
SSO is the core facility of a new exoplanet-hunting project called Search for habitable Planets EClipsing ULtra-cOOl Stars (SPECULOOS) , and consists of four telescopes equipped with 1-metre primary mirrors. The telescopes — named Io (moon), Europa (moon), Ganymede (moon) and Callisto (moon) after the four Galilean moons of Jupiter — will enjoy pristine observing conditions at the Paranal site, which is also home to ESO’s flagship brown dwarfs, whose planetary populations are still mostly unexplored. Only a few exoplanets have been found orbiting such stars, and even fewer lie within their parent star’s habitable zone . Even though these dim stars are hard to observe, they are abundant — comprising about 15% of the stars in the nearby universe. SPECULOOS is designed to explore 1000 such stars, including the nearest, brightest, and smallest, in search of Earth-sized habitable planets.
“SPECULOOS gives us an unprecedented ability to detect terrestrial planets eclipsing some of our smallest and coolest neighbouring stars,” elaborated Michaël Gillon of the University of Liège, principal investigator of the SPECULOOS project. “This is a unique opportunity to uncover the details of these nearby worlds.”
SPECULOOS will search for exoplanets using the transit method , following the example of its prototype TRAPPIST-1 planetary system. As a planet passes in front of its star it blocks some of the star’s light — essentially causing a small partial eclipse — resulting in a subtle but detectable dimming of the star. Exoplanets with smaller host stars block more of their star’s light during a transit, making these periodic eclipses much easier to detect than those associated with larger stars.
Thus far, only a small fraction of the exoplanets detected by this method have been Earth-sized or smaller. However, the small size of the SPECULOOS target stars combined with the high sensitivity of its telescopes allows detection of Earth-sized transiting planets located in the habitable zone. These planets will be ideally suited for follow-up observations with large ground- or space-based facilities.
“The telescopes are kitted out with cameras that are highly sensitive in the near-infrared,” explained Laetitia Delrez of the Cavendish Laboratory, Cambridge, a co-investigator in the SPECULOOS team. “This radiation is a little beyond what human eyes can detect, and is the primary emission from the dim stars SPECULOOS will be targeting.”
The telescopes and their brightly coloured mounts were built by the German company ASTELCO and are protected by domes made by the Italian manufacturer Gambato. The project will receive support from the two TRAPPIST 60-cm telescopes, one at ESO’s La Silla Observatory and the other in Morocco . The project will in due course also include the SPECULOOS Northern Observatory and SAINT-Ex, which are currently under construction in Tenerife, Spain, and at San Pedro Mártir, Mexico, respectively.
There is also potential for an exciting future collaboration with the Extremely Large Telescope, ESO’s future flagship telescope, currently under construction on Cerro Armazones. The ELT will be able to observe planets detected by SPECULOOS in unprecedented detail — perhaps even analysing their atmospheres.
“These new telescopes will allow us to investigate nearby Earth-like worlds in the Universe in greater detail than we could have imagined only ten years ago,” concluded Gillon. “These are tremendously exciting times for exoplanet science.”
 Speculoos, or speculaas, is a delicious type of spiced biscuit traditionally baked in Belgium and other countries for Saint Nicholas’s day on December 6. The name, with its sweet connotations, reflects the Belgian origins of the SPECULOOS project. The TRAPPIST project also has a similar Belgian namesake — it was named after Trappist beers, most of which are brewed in Belgium.
 The transit method is one of several ways exoplanets are discovered. A variety of instruments, including ESO’s planet-hunting HARPS spectrograph at the La Silla Observatory, use the radial velocity method to detect exoplanets, measuring changes in a star’s velocity due to an orbiting exoplanet.
 SSO also received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013)/ ERC grant agreement number 336480, from the Simons and MERAC Foundations, and from private sponsors.
ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It has 16 Member States: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile and with Australia as a Strategic Partner. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its world-leading Very Large Telescope Interferometer as well as two survey telescopes, VISTA working in the infrared and the visible-light VLT Survey Telescope. ESO is also a major partner in two facilities on Chajnantor, APEX and ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre Extremely Large Telescope, the ELT, which will become “the world’s biggest eye on the sky”.
The SPECULOOS Southern Observatory (SSO) is a project conducted by the University of Liège (Belgium), the Cavendish Laboratory, Cambridge (UK) and the King Abdulaziz University (Saudi Arabia), under the leadership of Michaël Gillon, research scientist and head of the group EXOplanets in Transit: Identification and Characterization (EXOTIC) at the Department of Astrophysics, Geophysics and Oceanography (AGO) of the University of Liège. SSO also involves scientists from the Universities of Bern, Birmingham, and Warwick. ESO supports SSO and hosts it at the Paranal Observatory in the Chilean Atacama Desert.
* SPECULOOS website – http://www.speculoos.uliege.be/
SPECULOOS Principal Investigator
University of Liège, Belgium
Tel: +32 4366 9743
Cell: +32 473 346 402
Email: [email protected]
SPECULOOS co-Principal Investigator , University of CambridgeUK
Tel: +44 7746 010890
Email: [email protected]
ESO Public Information Officer
Garching bei München, Germany
Tel: +49 89 3200 6655
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