Noticias y novedades sobre astronomía escritas por el periodista especializado Hernán Julio
La NASA y SpaceX continúan con sus misiones para enviar astronautas lanzándose en un cohete estadounidense desde suelo estadounidense a la Estación Espacial Internacional como parte del Programa…
Por primera vez, un equipo de astrónomos han detectado rayos X en Urano utilizando el Observatorio de Rayos X Chandra de la NASA. Este resultado podría ayudar a los…
Elliptical galaxies are generally characterized by their relatively smooth appearance when compared with spiral galaxies (one of which is to the left), which have more flocculent structures interwoven with dust lanes and spiral arms. NGC 474 is at a distance of about 100 million light-years in the constellation of Pisces. This image shows unusual structures around NGC 474 characterized as tidal tails and shell-like structures made up of hundreds of millions of stars. These features are due to recent mergers (within the last billion years) or close interactions with smaller infalling dwarf galaxies. This image is an excerpt from the Dark Energy Survey, which has released a massive, public collection of astronomical data and calibrated images from six years of work. The Dark Energy Survey is a global collaboration that includes the Department of Energy's (DOE) Fermi National Accelerator Laboratory (Fermilab), the National Center for Supercomputing Applications (NCSA), and NSF’s NOIRLab. The image was taken with the Dark Energy Camera, fabricated by DOE, on the Víctor M. Blanco 4-meter Telescope. The quality of the survey can be appreciated by diving into the zoomable version of this wider excerpt showing a background tapestry of thousands of distant galaxies.
El equipo del estudio Dark Energy Survey liberó una colección pública de datos astronómicos e imágenes calibradas que son el resultado de seis años de trabajo de esta investigación.…
Hace más de 11.000 años, una estrella supergigante masiva llegó al final de su vida. El núcleo de la estrella colapsó para formar una bola de neutrones increíblemente densa,…
Cada año, la campaña internacional de ciencia ciudadana Globe at Night crea conciencia sobre el impacto de la contaminación lumínica al invitar a los ciudadanos a ser científicos para medir…
This image was taken with the FORS2 instrument on ESO’s Very Large Telescope in late 2019, when comet 2I/Borisov passed near the Sun. Since the comet was travelling at breakneck speed, around 175 000 kilometres per hour, the background stars appeared as streaks of light as the telescope followed the comet’s trajectory. The colours in these streaks give the image some disco flair and are the result of combining observations in different wavelength bands, highlighted by the various colours in this composite image.
El cometa 2I/Borisov fue descubierto por el astrónomo aficionado Gennady Borisov en agosto de 2019 y, unas semanas más tarde, se confirmó que provenía de más allá del Sistema Solar.…
Nicknamed the Southern Pinwheel, Messier 83 (or NGC 5236) is a stunning face-on spiral galaxy located about 15 million light-years away in the southern constellation of Hydra. Its spiral arms are lined with dark lanes of dust and peppered with reddish, star-forming clouds of hydrogen gas. One of the deepest images ever taken of the Southern Pinwheel (combining more than 11 hours of exposure time), this view was captured with the Dark Energy Camera (DECam), which was built by the US Department of Energy (DOE) and is mounted on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory (CTIO), a Program of NSF’s NOIRLab. Numerous background galaxies, which lie much farther away than Messier 83, appear around the edges of the image.
Apodado el Molinillo del Sur, Messier 83 (o NGC 5236) es una impresionante galaxia espiral de cara a cara ubicada a unos 15 millones de años luz de distancia en…
Los ingenieros de la misión han informado de que el helicóptero Ingenuity ha superado sin problemas su primera gélida noche marciana. Con temperaturas que llegan a alcanzar los menos…
The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of a black hole released in 2019, has today a new view of the massive object at the centre of the Messier 87 (M87) galaxy: how it looks in polarised light. This is the first time astronomers have been able to measure polarisation, a signature of magnetic fields, this close to the edge of a black hole. This image shows the polarised view of the black hole in M87. The lines mark the orientation of polarisation, which is related to the magnetic field around the shadow of the black hole.
La colaboración EHT (Event Horizon Telescope, telescopio del horizonte de sucesos), que produjo la primera imagen de un agujero negro hecha pública en 2019, ha revelado hoy cómo se ve…
Esta semana, la misión OSIRIS-REx de la NASA le echará al asteroide Bennu un último vistazo antes de despedirse. Antes de partir hacia la Tierra el 10 de Mayo,…