All articles tagged with #near infrared
Microbes in Carlsbad Caverns toes the line between geology and biology, as cyanobacteria living on cave walls photosynthesize using near-infrared light that human eyes can’t see; the reflected light concentrates far from entrances, suggesting life could persist in ultra-dark, light-limited environments and offering clues for detecting life on other worlds, potentially guiding NASA’s future research with the James Webb Space Telescope.
MIT chemists have developed a new stable red fluorescent dye based on borenium ions that emit in the near-infrared range, potentially enabling clearer biomedical imaging of deep tissues and tumors, with applications in temperature sensing and optoelectronics.
The James Webb Space Telescope has provided a stunning new high-definition look at the supernova remnant Cassiopeia A (Cas A) in the near-infrared spectrum. The image reveals intricate details of the expanding shell of material from the exploded star, including tiny knots of gas and light echoes. The image also highlights the absence of color in certain regions, indicating the presence of ionized gas and dust. Researchers are particularly intrigued by a large, striated blob called "Baby Cas A," which appears to be a light echo located about 170 light-years behind the supernova remnant.
The James Webb Space Telescope has captured a stunning high-definition image of the supernova remnant Cassiopeia A (Cas A), revealing intricate details and hidden features. The near-infrared image showcases the expanding shell of material colliding with the gas shed by the star before it exploded. The image highlights tiny knots of gas, circular holes within the "Green Monster" (a loop of green light in Cas A's inner cavity), and light echoes from the star's explosion. The image also reveals a large, striated blob known as "Baby Cas A," which is a light echo located about 170 light-years behind the supernova remnant.
Astronomers using the Gemini North telescope have made the first detection ever of two near-infrared emission lines in the accretion disk of the galaxy III Zw 002, providing new insights into the size and behavior of these structures. Emission lines, which result from excited atoms releasing light, broaden into shallower peaks in the accretion disk due to the black hole's gravitational influence. The double-peaked profiles observed in III Zw 002's broad line region confirm the presence of an accretion disk and advance understanding of its geometry. The observations also reveal the feeding process and inner structure of the active galaxy's supermassive black hole.