Telescopes

Position and distance diagram of the trans-neptunian objects detected

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An article published in “The Astrophysical Journal” presents a catalog of 316 trans-neptunian objects detected by the Dark Energy Survey (DES) during the first four years of operations. A team led by Pedro Bernardinelli analyzed the data collected with a patient work to eliminate the fixed objects and then focused on the transient ones until they obtained the identification of 245 objects already known and 139 that were hitherto unknown. They’re at distances between 30 and more than 90 times the Earth’s from the Sun. Their detection will help to understand their origin and in general the Kuiper belt, where someone thinks that there may be another planet.

Artist's concept of iron rain on the exoplanet WASP-76b (Image ESO/M. Kornmesser)

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An article published in the journal “Nature” reports a study on the conditions existing on the exoplanet WASP-76b, an ultra-hot Jupiter where on the side illuminated by its star it’s so hot that metals vaporize and then condense on the dark side, where it rains iron. A team of researchers led by David Ehrenreich of the University of Geneva, Switzerland, used the ESPRESSO instrument mounted on the VLT in Chile to study the processes underway in the atmosphere of WASP-76b with the winds that carry the iron vapor across this gas giant.

Artist's concept of colliding white dwarfs (Image courtesy University of Warwick/Mark Garlick)

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An article published in the journal “Nature Astronomy” reports a study on a white dwarf out of the ordinary cataloged as WD J055134.612+413531.09, or simply WD J0551+4135. A team of astronomers coordinated by the British University of Warwick examined this white dwarf’s characteristics using data collected by ESA’s Gaia space probe and the William Herschel Telescope concluding that its atmosphere’s particular chemical composition indicates that it’s the result the merger of two medium-mass white dwarfs. WD J0551+4135 has a mass slightly higher than that of the Sun, remarkable for that type of object to the point that it was called an ultra-massive white dwarf. If it had a slightly larger mass it would probably have exploded in a supernova following the merger.

Artist's impression of K2-18b (Image courtesy Amanda Smith)

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An article published in “The Astrophysical Journal Letters” reports a study on the potential habitability conditions of the exoplanet K2-18b. A team from the British University of Cambridge led by Nikku Madhusudhan conducted a series of simulations based on the possible values of mass, size, and atmosphere data value available on it to create various models compatible with the observations. According to the conclusions, under certain conditions there may be liquid water on its surface.

The outburst region in the Ophiuchus supercluster

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An article published in “The Astrophysical Journal” reports the observation of what was called the largest explosion discovered in the universe after the Big Bang and caused by the supermassive black hole in the galaxy at the center of the Ophiuchus supercluster. A team of astronomers led by Simona Giacintucci of the Naval Research Laboratory combined X-ray observations with ESA’s XMM-Newton and NASA’s Chandra space telescopes with those at radio frequencies conducted with Murchison Widefield Array (MWA) and Giant Metrewave Radio Telescope (GMRT) radio telescopes to map the cavity generated by that cataclysmic event, about 15 times the Milky Way’s size.