CARMENES discovers two planetary systems made of (super-)Earths

June 30th 2021portada

The CARMENES instrument at the Calar Alto observatory 3.5-meter telescope finds one exo-Earth and two super-Earths around two red dwarf stars, confirming the ubiquity of rocky planets around such tiny stars, whose violent flares may complicate and even prevent the detection of exoplanets.

Since 1995, over 4000 planets have been discovered out of our Solar System. The ample variety of these exoplanets has demonstrated that the structure of the Solar System, with rocky (or terrestrial) planets in the inner regions and gaseous and icy ones in the outer parts, is not so typical as believed. Other configurations, such as gas giant planets very close to their stars or systems with several super-Earths around dwarf stars, appear more common. In this context, a new detection of two planetary systems by the CARMENES instrument, operating at Spanish Calar Alto Observatory (CAHA, Almeria), reinforces the idea that dwarf stars tend to harbor rocky planets.

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OPTICON-RadioNet PILOT (ORP), the largest astronomy network in Europe, is born


April 15th 2021

Two astronomy networks come together to form the largest collaborative terrestrial astronomy network in Europe. The French CNRS will be responsible for coordinating the ORP project, which has 15 million euros of funding from the European Union through the H2020 program. Observing time on Calar Alto telescopes will be available through ORP every semester.

To date, Europe has had two major collaborative networks for ground-based astronomy, OPTICON and RadioNet, operating respectively in optical and radio. Now, these networks have come together to form the largest collaborative network for ground-based astronomy in Europe. The new network, called OPTICON-RadioNet PILOT (ORP), aims to harmonize observing methods and tools and to provide access to a wider range of astronomical facilities. Calar Alto Observatory (CAHA) and the Institute of Astrophysics of Andalusia (IAA-CSIC) participate in the project, which will be coordinated by the French National Centre for Scientific Research (CNRS), together with the University of Cambridge (UK) and the Max-Planck Institute for Radio Astronomy (Germany).

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Discovery of a super-Earth ideal for testing planetary atmospheric models

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March 4th 2021

An international team of astronomers has discovered a hot super-Earth around the Gliese 486 star, only 26 light-years away from our Sun. This exoplanet, detected by the CARMENES instrument at the Calar Alto observatory 3.5 meter telescope, might be the Rosetta Stone for the study of the atmospheres of rocky planets.

During the last quarter of century, astronomers have discovered an ample variety of exoplanets made of rock, ice or gas. The commissioning of new astronomical instruments, like the CARMENES spectrograph at Calar Alto Observatory (Almeria, Spain), specialized in planet hunting, has allowed us to detect several thousands of new worlds out of the Solar System. Among all of them, only a handful are similar to our Earth, like the Teegarden b exoplanet found at Calar Alto.

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Star formation in gravitationally perturbed galaxies


December 31st 2020

An international team has studied the rates of star formation in galaxies from the CALIFA survey and has found subtle differences between galaxies influenced by neighbors, and those unperturbed. Gravitational interaction between galaxies could enhance the star formation in the inner regions of perturbed ones.

Galaxies are huge assemblies of billions of stars as well as tons of dust and gas. Stars were and are born from this gas, when it collapses by gravitation into “big balls of plasma”, so hot that nuclear reactions of fusion start in their cores. Then, stars live for millions to billions of years in a pretty stable state, converting hydrogen into helium -- and more complex atoms -- while releasing their heat and light, like our Sun does. Stars eventually die, in more or less violent explosions, rejecting their “recycled” material (richer in complex chemical elements) back to their host galaxy. New generations of stars can then be formed from this richer gas and dust.

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