Category Astronomy/Space

Mysterious Infrared Light from Space Resolved Perfectly

60 percent of them have corresponding optical/infrared galaxies, whereas the remaining 40 percent are invisible in other wavelength. Credit: ALMA (ESO/NAOJ/NRAO), NAOJ, Fujimoto et al.

60 percent of them have corresponding optical/infrared galaxies, whereas the remaining 40 percent are invisible in other wavelength. Credit: ALMA (ESO/NAOJ/NRAO), NAOJ, Fujimoto et al.

A research team using ALMA has detected the faintest millimeter-wave source ever observed. By accumulating millimeter-waves from faint objects like this throughout the Universe, the team finally determined that such objects are 100% responsible for the enigmatic infrared background light filling the Universe. By comparing these to optical and infrared images, the team found that 60% of them are faint galaxies, whereas the rest have no corresponding objects in optical/infrared wavelengths and their nature is still unknown.

The Universe looks dark in the parts between stars and galaxies...

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Using “Nanoantennae” to Manipulate Light Beams

Complete control of light waves would allow the miniaturization of traditional optical components, such as lenses, polarizers or beam-splitters, to nanoscale sizes while dramatically increasing their performance and resolution. Credit: Copyright Agency for Science, Technology and Research (A*STAR)

Complete control of light waves would allow the miniaturization of traditional optical components, such as lenses, polarizers or beam-splitters, to nanoscale sizes while dramatically increasing their performance and resolution. Credit: Copyright Agency for Science, Technology and Research (A*STAR)

This may lead to new light-based technologies. Complete control of some of the key properties of light waves – polarisation and phase – at the nanoscale is of major interest for light-based technologies such as display screens, and in energy harvesting and data transmission. It would allow, for example, the miniaturization of traditional optical components, such as lenses, polarizers or beam-splitters, to nanoscale sizes...

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Sticky, Stony and Sizzling Science launching to ISS

This is a small handheld gecko grippers and associated test hardware. Credit: NASA

This is a small handheld gecko grippers and associated test hardware. Credit: NASA

Orbital ATK CRS-6 will deliver investigations to the space station to study fire, meteors, regolith, adhesion, and 3-D printing in microgravity. NASA’s commercial partner plans to launch its Cygnus spacecraft into orbit on March 22, 2016 atop a United Launch Alliance Atlas V rocket for its fifth contracted resupply mission to the International Space Station. The Spacecraft Fire Experiment-I (Saffire-I) intentionally lights a large-scale fire inside an empty Cygnus resupply vehicle after it leaves the space station and before it re-enters Earth’s atmosphere.

In the decades of research into combustion and fire processes in reduced gravity, few experiments have directly studied spacecraft fire safety under lo...

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Dark Matter Satellites Trigger Massive Birth of Stars

This is a dwarf galaxy with a starburst. Credit: UC Riverside

This is a dwarf galaxy with a starburst. Credit: UC Riverside

Astronomers use computer simulations based on theoretical models to explain massive star formation observed in dwarf galaxies. One of the main predictions of the current model of the creation of structures in the universe, known at the Lambda Cold Dark Mattermodel, is that galaxies are embedded in very extended and massive halos of dark matter surrounded by many thousands of smaller sub-halos also made from dark matter.

Around large galaxies, eg Milky Way, these dark matter sub-halos are large enough to host enough gas and dust to form small galaxies on their own, and some of these galactic companions, known as satellite galaxies, can be observed...

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