Astronomers discover an ultra-light and super-fast sub-Earth orbiting a red dwarf

An artist's simulation of the subterrestrial planet GJ 367 b. Credit: DLR
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Exoplanets and Astrobiology

The search for life in the universe has been driven by recent discoveries of planets around other stars (known as exoplanets), becoming one of the most active fields in modern astrophysics. The growing number of new exoplanets discovered in recent years and the recent advance on the study of their atmospheres are not only providing new valuable

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Helio and Astero-Seismology and Exoplanets Search

The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars, 3) to search for extrasolar planets using photometric methods (primarily by transits of their host stars) and their characterization (using radial velocity information) and 4) the study of the planetary

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V1298 Tau

An international team of scientists, in which researchers from the Instituto de Astrofísica de Canarias (IAC) participate together with other institutions from Spain, Italy, Germany, Belgium, UK, and Mexico, has been able to measure the masses of the giant planets of the V1298 Tau system, just 20 million year old. Masses for such young giant planets had not been obtained previously, and this is the first evidence that these objects have already reached their final size at very early stages of their evolution. For this study they have used radial velocity measurements from the HARPS-N

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María Rosa Zapatero Osorio at EWASS 2015. Credits: Iván Jiménez / IAC.

By IVÁN JIMÉNEZ Twenty years ago an exceptional discovery blurred forever the boundary between what we call stars and what we call planets. A star is characterized by producing nuclear reactions in its interior. However in 1995 a group of researchers of the Instituto de Astrofísica de Canarias (IAC), among them Maria Rosa Zapatero Osorio (now at the Centre for Astrobiology (CAB-CSIC-INTA) discovered an object which appeared to be a star, but without sufficient mass to produce significant nuclear reactions. Although it was given the name Teide-1, the scientists had in fact found a type of

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