Tag Archive for 'IR'

Artist’s impression of diamond dust. Image credit: S. Dagnello.

Astronomers Find Rapidly Spinning Nanodiamonds in Dust Disks around Young Stars

Jun 12, 2018 by News Staff

A faint and mysterious stream of microwaves emanating from young star systems far out in the Milky Way Galaxy could be caused by nanodiamonds about 1.5-2.2 nm...

An artist’s impression of WASP-107b. Image credit: NASA / ESA / Hubble / M. Kornmesser.

Helium Detected in Atmosphere of Exoplanet for First Time

May 3, 2018 by News Staff

An international team of astronomers has detected helium — the second-most abundant element in the Universe after hydrogen — in the atmosphere...

Xu et al achieved a breakthrough, inventing a stretchy new material modeled after both squid skin and Hollywood dinosaurs with remarkable properties. Image credit: Xu et al, doi: 10.1126/science.aar5191.

Scientists Create Infrared Camouflage Material

Apr 2, 2018 by News Staff

Thermal vision cameras detect differences in temperature by sensing infrared wavelengths. If a coating could be developed that showed dynamic tuning of...

A new high-resolution map of the magnetic field lines in gas and dust swirling around Milky Way’s central black. Image credit: Roche et al, doi: 10.1093/mnras/sty129.

Clearest Infrared Image of Milky Way’s Central Region Unveiled

Feb 28, 2018 by News Staff

Using data from the CanariCam infrared camera on the Gran Telescopio Canarias, astronomers have created a high resolution map of the magnetic field lines...

This illustration depicts a hypothetical uneven ring of dust orbiting KIC 8462852. Image credit: NASA / JPL-Caltech.

Mysterious Long-Term Dimming of KIC 8462852 May Be Caused by Dust, Astronomers Say

Oct 9, 2017 by News Staff

University of Arizona astronomer Huan Meng and co-authors have found the long-term dimming of KIC 8462852 — a main-sequence F-type star located in...

This image combines two products from the first pointing at Phobos by Mars Odyssey’s THEMIS camera. Surface-temperature information from observation in thermal-infrared wavelengths is overlaid on a more detailed image from a visible-light observation. The left edge of the small moon was in darkness, and the right edge in morning sunlight. The distance to Phobos from Mars Odyssey during the observation was about 3,424 miles (5,511 km). Researchers will analyze the surface-temperature information from this observation and possible future THEMIS observations to learn how quickly the surface warms after sunup or cools after sundown. That could provide information about surface materials, because larger rocks heat or cool more slowly than smaller particles do. The thermal information in this image is from merging observations made in four thermal-infrared wavelength bands, centered from 11.04 microns to 14.88 microns. Image credit: NASA / JPL-Caltech / Arizona State University.

Mars Odyssey Captures Phobos in Infrared Light

Oct 5, 2017 by News Staff

The Thermal Emission Imaging System (THEMIS) camera on NASA’s Mars Odyssey spacecraft observed Phobos — the larger and inner of the two natural...

An all-sky image of the Milky Way Galaxy, as observed by ESA’s Planck Space Observatory in IR. The data contained in this image were used in this research and were essential in calculating the distribution of the light energy of the Galaxy. Image credit: ESA / HFI / LFI consortia.

Researchers Map Light Energy Distribution in Milky Way Galaxy

Jul 31, 2017 by News Staff

An international team of scientists has used data from ESA’s Planck Space Observatory and other telescopes to map the distribution of all light energy...

This composite, false-color infrared image of Jupiter reveals haze particles over a range of altitudes, as seen in reflected sunlight. It was taken using the Gemini North telescope’s Near-InfraRed Imager (NIRI) on May 18, 2017. The multiple filters corresponding to each color used in the image cover wavelengths between 1.69 microns and 2.275 microns. Jupiter’s Great Red Spot (GRS) appears as the brightest (white) region at these wavelengths, which are primarily sensitive to high-altitude clouds and hazes near and above the top of Jupiter's convective region. The GRS is one of the highest-altitude features in Jupiter’s atmosphere. Narrow spiral streaks that appear to lead into it or out of it from surrounding regions probably represent atmospheric features being stretched by the intense winds within the GRS, such as the hook-like structure on its western edge (left side). Some are being swept off its eastern edge (right side) and into an extensive wave-like flow pattern, and there is even a trace of flow from its northern edge. Other features near the GRS include the dark block and dark oval to the south and the north of the eastern flow pattern, respectively, indicating a lower density of cloud and haze particles in those locations. Both are long-lived cyclonic circulations, rotating clockwise -- in the opposite direction as the counterclockwise rotation of the GRS. A prominent wave pattern is evident north of the equator, along with two bright ovals, which are anticyclones that appeared in January 2017. Both the wave pattern and the ovals may be associated with an impressive upsurge in stormy activity that has been observed in these latitudes this year. Another bright anticyclonic oval is seen further north. High hazes are evident over both polar regions with much spatial structure not previously been seen quite so clearly in ground-based images. Image credit: Gemini Observatory / AURA / NASA / JPL-Caltech.

Infrared Images of Jupiter from Subaru and Gemini Telescopes to Enhance Juno Flyby

Jul 4, 2017 by News Staff

High-resolution imaging of Jupiter and its Great Red Spot by the Subaru Telescope and the Gemini North telescope, both on Hawaii’s Mauna Kea peak, is...

This VISTA image of the Small Magellanic Cloud shows millions of stars. Image credit: ESO / VISTA / VMC.

VISTA Telescope Takes Biggest Infrared Image Ever of Small Magellanic Cloud

May 3, 2017 by News Staff

This enormous image (zoomable version), captured with ESO’s Visible and Infrared Survey Telescope (VISTA), is the largest infrared image (43,223 x 38,236...

This is a three-color composite image of Saturn and its rings taken January 23, 2008 with the COMICS instrument on the Subaru Telescope. The Cassini Division and the C ring appear bright. Color differences reflect the temperatures; the warmer part is blue, the cooler part is red. Image credit: NAOJ.

Researchers Measure Brightness, Temperatures of Saturn’s Main Rings

Mar 2, 2017 by Enrico de Lazaro

Using mid-infrared data from the 8.2-m Subaru Telescope, a research team led by Dr. Hideaki Fujiwara, Subaru scientist at the National Astronomical Observatory...

Hubble Captures Stunning Image of LEDA 52270

Jan 2, 2017 by News Staff

The NASA/ESA Hubble Space Telescope has taken a picture of LEDA 52270, a combination of two gas-rich spiral galaxies. This image, taken with the Advanced...

Blazars are the most common sources detected by NASA’s Fermi Gamma-ray Space Telescope. As matter falls toward the supermassive black hole at the galaxy’s center, some of it is accelerated outward at nearly the speed of light along jets pointed in opposite directions. When one of the jets happens to be aimed in the direction of Earth, as illustrated here, the galaxy appears especially bright and is classified as a blazar. Image credit: M. Weiss / CfA.

NASA Space Telescopes Reveal Unexpected Blazar Connection

Aug 24, 2016 by News Staff

Astronomers studying black-hole-powered galaxies called blazars have uncovered a surprising link between two very different wavelengths of the light these...

Security screening area. Image credit: Dan Paluska / CC0 1.0.

Real-Time, Hand-Held Scanner to Revolutionize Airport Security

Jul 20, 2016 by News Staff

A real-time, hand-held chemical scanner with stand-off detection capabilities has been unveiled by a team of researchers and engineers from nine European...

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