Cozy Dark emerging technology began work in 2010 as a skunkworks-style engineering firm and is registered with CCR and NSPIRES.
Our early engineering & design efforts have focused on orbital debris solutions and electrodynamic tether technology.
Zach Urbina founded Cozy Dark with the cooperation of technical, research, and academic colleagues in the Southern California AeroAstro community.
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279 posts tagged science
Astronomers Watch Century-Old Broadcast of Powerful Stellar Eruption |
Astronomers are watching a delayed broadcast of a spectacular outburst from the unstable, behemoth double-star system Eta Carinae, an event initially seen on Earth nearly 170 years ago.
Dubbed the “Great Eruption,” the outburst first caught the attention of sky watchers in 1837 and was observed through 1858. But astronomers didn’t have sophisticated science instruments to accurately record the star system’s petulant activity.
Luckily for today’s astronomers, some of the light from the eruption took an indirect path to Earth and is just arriving now, providing an opportunity to analyze the outburst in detail. The wayward light was heading in a different direction, away from our planet, when it bounced off dust clouds lingering far from the turbulent stars and was rerouted to Earth, an effect called a “light echo.” Because of its longer path, the light reached Earth 170 years later than the light that arrived directly. continue reading
‘Dark Plasmons’ Transmit Energy |
Microscopic channels of gold nanoparticles have the ability to transmit electromagnetic energy that starts as light and propagates via “dark plasmons,” according to researchers at Rice University.
A new paper in the American Chemical Society journal Nano Letters shows how even disordered collections of nanoparticles in arrays as thin as 150 nanometers can be turned into waveguides and transmit signals an order of magnitude better than previous experiments were able to achieve. Efficient energy transfer on the micrometer scale may greatly improve optoelectronic devices. The Rice lab of Stephan Link, an assistant professor of chemistry and electrical and computer engineering, has developed a way to “print” fine lines of gold nanoparticles on glass. These lines of nanoparticles can transmit a signal from one nanoparticle to the next over many microns, much farther than previous attempts and roughly equivalent to results seen using gold nanowires. continue reading
Milky Way’s Black Hole Grazing On Asteroids |
The giant black hole at the center of the Milky Way may be vaporizing and devouring asteroids, which could explain the frequent flares observed, according to astronomers using data from NASA’s Chandra X-ray Observatory.
For several years Chandra has detected X-ray flares about once a day from the supermassive black hole known as Sagittarius A*, or “Sgr A*” for short. The flares last a few hours with brightness ranging from a few times to nearly one hundred times that of the black hole’s regular output. The flares also have been seen in infrared data from ESO’s Very Large Telescope in Chile.
“People have had doubts about whether asteroids could form at all in the harsh environment near a supermassive black hole,” said Kastytis Zubovas of the University of Leicester in the United Kingdom, and lead author of the report appearing in the Monthly Notices of the Royal Astronomical Society. “It’s exciting because our study suggests that a huge number of them are needed to produce these flares.” continue reading
NASA’s Solar Dynamics Observatory captured this video of swirls of darker, cooler plasma caught between competing magnetic forces over the course of 30 hours. The plasma strands rotate like tornadoes caught on magnetic field lines. It sometimes feels incredible to observe such familiar-looking fluid behavior in such unfamiliar places, but it’s just a reminder that physics works no matter where you are.
Putting the Squeeze On Planets Outside Our Solar System |
Just as graphite can transform into diamond under high pressure, liquid magmas may similarly undergo major transformations at the pressures and temperatures that exist deep inside Earth-like planets.
Using high-powered lasers, scientists at Lawrence Livermore National Laboratory and collaborators discovered that molten magnesium silicate undergoes a phase change in the liquid state, abruptly transforming to a more dense liquid with increasing pressure. The research provides insight into planet formation.
“Phase changes between different types of melts have not been taken into account in planetary evolution models,” said lead scientist Dylan Spaulding, a University of California, Berkeley graduate student who conducted most of his thesis work at the Laboratory’s Jupiter Laser Facility. “But they could have played an important role during Earth’s formation and may indicate that extra-solar ‘Super-Earth’ planets are structured differently from Earth.” continue reading
XCOR’s Doug Jones at the LA Space Salon |
Known as the Rocket Whisperer, Doug Jones is a Co-Founder and Chief Scientist at XCOR Aerospace. He handles test design and analysis of test results for the company’s liquid rocket engine development and facilitates the development and operation of rocket engine test apparatus. Before joining XCOR, Doug was responsible for sizing the fluid injector elements in Rotary Rocket Company’s (RRC) rocket engine design. Prior to RRC, Doug designed, built, and tested a 400 lb thrust nitrous oxide/propane engine, it’s test facility, and a 300,000 cubic foot balloon system for Vela Technology. Doug also flew multiple times as flight test engineer in the X-Racer rocket powered aircraft! via @SpaceVidCast
Planck All-Sky Images Show Cold Gas and Strange Haze in Milky Way Galaxy |
New images from the Planck mission show previously undiscovered islands of star formation and a mysterious haze of microwave emissions in our Milky Way galaxy. The views give scientists new treasures to mine and take them closer to understanding the secrets of our galaxy.
Planck is a European Space Agency mission with significant NASA participation.
“The images reveal two exciting aspects of the galaxy in which we live,” said Planck scientist Krzysztof M. Gorski from NASA’s Jet Propulsion Laboratory in Pasadena, Calif., and Warsaw University Observatory in Poland. “They show a haze around the center of the galaxy, and cold gas where we never saw it before.”
The new images show the entire sky, dominated by the murky band of our Milky Way galaxy. One of them shows the unexplained haze of microwave light previously hinted at in measurements by NASA’s Wilkinson Microwave Anisotropy Probe (WMAP).
“The haze comes from the region surrounding the center of our galaxy and looks like a form of light energy produced when electrons accelerate through magnetic fields,” said Davide Pietrobon, another JPL Planck scientist. continue reading
Rare Ultra-Blue Stars Found in Neighboring Galaxy’s Hub |
Peering deep inside the hub of the neighboring Andromeda galaxy, NASA’s Hubble Space Telescope has uncovered a large, rare population of hot, bright stars.
Blue is typically an indicator of hot, young stars. In this case, however, the stellar oddities are aging, Sun-like stars that have prematurely cast off their outer layers of material, exposing their extremely blue-hot cores.
Astronomers were surprised when they spotted these stars because physical models show that only an unusual type of old star can be as hot and as bright in ultraviolet light.
While Hubble has spied these ultra-blue stars before in Andromeda, the new observation covers a much broader area, revealing that these stellar misfits are scattered throughout the galaxy’s bustling center. Astronomers used Hubble’s Wide Field Camera 3 to find roughly 8,000 of the ultra-blue stars in a stellar census made in ultraviolet light, which traces the glow of the hottest stars. The study is part of the multi-year Panchromatic Hubble Andromeda Treasury survey to map stellar populations across the Andromeda galaxy.
“We were not looking for these stars. They stood out because they were bright in ultraviolet light and very different from the stars we expected to see,” said Julianne Dalcanton of the University of Washington in Seattle, leader of the Hubble survey. continue reading
