A research team using the ChemCam instrument onboard NASA’s Curiosity rover discovered higher-than-usual amounts of manganese in lakebed rocks within Gale Crater on Mars, which indicates that the sediments were formed in a river, delta, or near the shoreline of an ancient lake. The results were published today in Journal of Geophysical Research: Planets.
Researchers at The Ohio State University played a major role in analyzing the first year of data from the Dark Energy Spectroscopic Instrument’s survey into the history of the universe.
Vera C. Rubin Observatory's successfully coats 8.4-meter primary/tertiary mirror in on-site coating chamber
Meadors' new role comes with some historic significance as she is the first African American and first female space grant director for the state of Arkansas as well as the first African American female space grant director in the United States.
Computer simulations by astronomers support the idea that dark matter – matter that no one has yet directly detected but which many physicists think must be there to explain several aspects of the observable universe – exists, according to the researchers, who include those at the University of California, Irvine.
Utilizando el telescopio de Gemini Sur, ubicado en la Región de Coquimbo en Chile, un equipo de astrónomos confirmó por primera vez que las diferencias observadas en las estrellas binarias se deben a las diferencias químicas en la nube de material estelar de la cual se formaron. Los resultados ayudan a explicar por qué las estrellas que nacieron de la misma nube molecular pueden tener una composición química distinta y sistemas planetarios tan diferentes, además de plantear nuevos retos a los modelos actuales de formación estelar y planetaria.
Using the Gemini South telescope a team of astronomers have confirmed for the first time that differences in binary stars’ composition can originate from chemical variations in the cloud of stellar material from which they formed.
Using the Gemini South telescope a team of astronomers have confirmed for the first time that differences in binary stars’ composition can originate from chemical variations in the cloud of stellar material from which they formed.
Utilizando el telescopio de Gemini Sur, ubicado en la Región de Coquimbo en Chile, un equipo de astrónomos confirmó por primera vez que las diferencias observadas en las estrellas binarias se deben a las diferencias químicas en la nube de material estelar de la cual se formaron. Los resultados ayudan a explicar por qué las estrellas que nacieron de la misma nube molecular pueden tener una composición química distinta y sistemas planetarios tan diferentes, además de plantear nuevos retos a los modelos actuales de formación estelar y planetaria.
An unusual group of stars in the Orion constellation have revealed their secrets. FU Orionis, a double star system, first caught astronomers’ attention in 1936 when the central star suddenly became 1,000 times brighter than usual.
Samples reveal evidence of changes experienced by the surface of asteroid Ryugu, some probably due to micrometeoroid bombardment.
Researchers at the University of Minnesota Twin Cities College of Science and Engineering co-led a new study by an international team that will improve the detection of gravitational waves—ripples in space and time.
Scientists at the Department of Energy’s Oak Ridge National Laboratory have developed a method that demonstrates how fiber-reinforced polymer composite materials used in the automotive, aerospace and renewable energy industries can be made stronger and tougher to better withstand mechanical or structural stresses over time.
Eagle-eyed, armchair astronomers have almost certainly made a number of thrilling discoveries, including two possible Jupiter-sized ‘exoplanets’ – planets outside our solar system – in an international, citizen-science project run out of a UK university.
To celebrate Hubble’s 34th launch anniversary, NASA released the telescope’s new observation of the Little Dumbbell Nebula. Also known as Messier 76, or M76, it is composed of a ring, seen edge-on as the central bar structure, where a central red giant star burned out, and two lobes of gas and dust that are on either opening of the ring.
En un abrir y cerrar de ojos, el dispositivo de carga acoplada revolucionó la astronomía, modificando radicalmente nuestra forma de explorar el cosmos y haciendo avanzar muchos otros campos de la ciencia y la tecnología. ¿Qué sigue ahora?
In a flash the charge-coupled device ignited a revolution in astronomy, fundamentally altering our approach to exploring the cosmos while advancing many other areas of science and technology. What’s next?
Gamma-ray bursts (GRBs) are intense bursts of gamma radiation, typically generating more energy in a few seconds than the Sun will produce over its ten-billion-year lifetime.
Gracias a las imágenes que podrán ser obtenidas con seis filtros distintos montados en la cámara más grande construida para la astronomía, el Observatorio Vera C. Rubin estará en condiciones de descubrir los efectos de la interacción de la materia oscura con corrientes estelares nunca antes vistos en la Vía Láctea.
Gracias a las imágenes que podrán ser obtenidas con seis filtros distintos montados en la cámara más grande construida para la astronomía, el Observatorio Vera C. Rubin estará en condiciones de descubrir los efectos de la interacción de la materia oscura con corrientes estelares nunca antes vistos en la Vía Láctea.
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