News

This section includes scientific and technological news from the IAC and its Observatories, as well as press releases on scientific and technological results, astronomical events, educational projects, outreach activities and institutional events.

  • Result of the field test made with the copy of DRAGO on September 22nd 2021 at 08.00 local time.

    The eruption on La Palma has provided a unique scenario for testing the DRAGO instrument, the infrared camera of the Instituto de Astrofísica de Canarias (IAC) which has been observing the Canary Islands from space since January. One of the objectives for which DRAGO was designed is monitoring natural disasters, especially those which could occur in the Canaries, such as forest fires, petroleum spills, or volcanic eruptions. The role of DRAGO is to provide infrared images from space to help the management and control of these disasters. In the case of the eruption which began on September

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  • Ratio between the measured and predicted gravitational redshifts vs. cosmological redshift, zcosm. Main panel: data from the present work. Superior inset: Solar System and Milky Way data from the literature. Inferior inset: galaxy cluster data from the literature (see Figure 1 of the paper).

    We perform a new test of Einstein's Equivalence Principle which, for the first time, extends to very early cosmological epochs (we have studied its validity in 80% of the history of the Universe). The Einstein Equivalence Principle is essential for generalizing physical laws in the presence of gravity. Our test of the Equivalence Principle is based on one of Einstein's classical predictions: the gravitational redshift of photons. This test has been accurately put into practice in our Solar System and in some stars in our Galaxy (e.g. Sirius B). However, so far it has not been applied to

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  • Image taken by the Hubble Space Telescope of the Einstein ring GAL-CLUS-022058s, located in the constellation of Fornax. Credit: ESA/Hubble & NASA, S. Jha; Acknowledgment: L. Shatz

    In December 2020 a team from the European Space Agency (ESA) published an image taken by the Hubble Space Telescope (HST) of GAL-CLUS-022058s, the biggest and one of the most complete Einstein rings discovered, situated towards the southern hemisphere constellation of Fornax. Since then, those observations have been used to develop a model of gravitational lenses which has enabled the study of the physical properties of the amplified galaxies.

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  • Photometer SG-WAS. Credit: Miguel Rodríguez Alarcón (IAC).

    Completely autonomous, not invasive, and low cost. This is the new SG-WAS (SkyGlow Wireless Autonomous Sensor) which will help to measure the impact of artificial night lighting on the natural protected areas of Macaronesia.

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  • The  image shows the process of nuclear feeding of a black hole in the galaxy NGC 1566, and how the dust filaments - seen in white-blue colors- are trapped and rotating  in a spiral around the black hole  until the black hole  swallows them. Credit: ESO.

    The black holes at the centres of galaxies are the most mysterious objects in the Universe, not only because of the huge quantities of material within them, millions of times the mass of the Sun, but because of the incredibly dense concentration of matter in a volume no bigger than that of our Solar System. When they capture matter from their surroundings they become active, eventually giving rise to the ejection of huge amounts of energy. It is however difficult to detect the black hole during these capture episodes because the event is rare. We detected long and narrow dust filaments

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  • View of HH204, a Herbig-Haro object in the Orion Nebula. The left panel shows the Orion Nebula observed with the Hubble Space Telescope, picking out the area around HH204. In the right panel, we can see in detail the structure of HH204 and of its apparent companion, HH203. In this panel, the images by the Hubble Space Telescope taken during 20 years and artificially highlighted with different colours show the advance of the jets of gas through the Orion Nebula. Credit: Gabriel Pérez Díaz, SMM (IAC).

    An international team led by researchers from the Instituto de Astrofísica de Canarias (IAC) has uncovered, with an new high degree of detail, the physical and chemical effects of the impact of a protostellar jet in the interior of the Orion Nebula. The study was made using observations with the Very Large Telescope (VLT) and 20 years of images with the Hubble Space Telescope (HST). The observations show evidence of compression and heating produced by the shock front, and the destruction of dust grains, which cause a dramatic increase in the gas phase abundance of the atoms of iron, nickel

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