Astronomers have unveiled a new atlas of the inner regions of the Milky Way - that's our home galaxy, if you're from someplace else - and it's peppered with thousands of previously undiscovered dense knots of cold cosmic dust, the potential birthplaces of new stars. Using observations from the APEX telescope in Chile, this survey is the largest map of cold dust so far.
This new guide for astronomers, known as the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) shows the Milky Way in submillimetre-wavelength light (between infrared light and radio waves. Images of the cosmos at these wavelengths are vital for studying the birthplaces of new stars and the structure of the crowded galactic core.
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NASA's Lunar Reconnaissance Orbiter has transmitted its first images since reaching the moon on June 23. The spacecraft's two cameras, collectively known as the Lunar Reconnaissance Orbiter Camera, or LROC, were activated June 30. The cameras are working well and have returned images of a region in the lunar highlands south of Mare Nubium (Sea of Clouds).
As the moon rotates beneath LRO, LROC gradually will build up photographic maps of the lunar surface.
As the moon rotates beneath LRO, LROC gradually will build up photographic maps of the lunar surface.
Astronomers using ESA’s XMM-Newton X-ray observatory have discovered a black hole they labeled HLX-1 (Hyper-Luminous X-ray source 1), which lies towards the outskirts of the galaxy ESO 243-49, approximately 290 million light-years from Earth and weighs more than 500 solar masses, making it a 'missing link' between lighter stellar-mass and heavier supermassive black holes. This discovery is the best detection to date of a new class that has long been searched for: intermediate mass black holes.
The discovery has been made by an international team of researchers working with XMM-Newton data, led by Sean Farrell from the Centre d’Etude Spatiale des Rayonnements, now based at the University of Leicester.
The discovery has been made by an international team of researchers working with XMM-Newton data, led by Sean Farrell from the Centre d’Etude Spatiale des Rayonnements, now based at the University of Leicester.
Researchers have completed the largest ever survey for very distant clusters of galaxies.
Named the Spitzer Adaptation of the Red-sequence Cluster Survey, "SpARCS" detects galaxy clusters using deep ground-based optical observations from the CTIO 4m and CFHT 3.6m telescopes, combined with Spitzer Space Telescope infrared observations.
SpARCS is designed to find clusters as they appeared lwhen the universe was 6 billion years old or younger. Astronomers believe the universe was formed 13.7 billion years ago.
Named the Spitzer Adaptation of the Red-sequence Cluster Survey, "SpARCS" detects galaxy clusters using deep ground-based optical observations from the CTIO 4m and CFHT 3.6m telescopes, combined with Spitzer Space Telescope infrared observations.
SpARCS is designed to find clusters as they appeared lwhen the universe was 6 billion years old or younger. Astronomers believe the universe was formed 13.7 billion years ago.
Why did our Milky Way galaxy survive while others failed? Ill-defined, convenient catch-all dark matter gets the credit, according to a new paper. Dark matter is thought to make up 85 per cent of the Universe’s mass and it may also be one of the building blocks of galaxy formation.
The researchers say that the early Milky Way, which had begun forming stars, held on to the raw gaseous material from which further stars would be made. This material would otherwise have been evaporated by the high temperatures generated by the “ignition” of the Universe about half-a-billion years after the Big Bang.
The researchers say that the early Milky Way, which had begun forming stars, held on to the raw gaseous material from which further stars would be made. This material would otherwise have been evaporated by the high temperatures generated by the “ignition” of the Universe about half-a-billion years after the Big Bang.
In a few days, scores of Italian post-doctoral researchers in experimental particle physics will get tested on their knowledge of the matter, without any promise of a position, but just to get one further "stamp" on their curriculum, testifying that they are competent enough to be worth offering a temporary position by INFN, the Italian Institute for (sub)Nuclear Physics. So this is a national exam, with the sole purpose of giving a green light to be admitted to two-year positions , which are typically paid less than 1400 euros a month, and which are so far not available. Frankly, I feel ashamed, since I myself work for INFN, and I strongly disagree with its current recruitment policies.
Dolphins, whales and porpoises are perfectly adapted for maximum aquatic agility. We know why that is - biologists expect that as a result of evolution - but to-date no one in physics had ever successfully analyzed how the animals' flippers interact with water; the hydrodynamic lift that they generate, the drag that they experience and their hydrodynamic efficiency.
Laurens Howle and Paul Weber from Duke University teamed up with Mark Murray from the United States Naval Academy and Frank Fish from West Chester University to find out more about the hydrodynamics of whale and dolphin flippers. Their findings; some dolphins' fins generate lift in the same way as delta wing aircraft.
Laurens Howle and Paul Weber from Duke University teamed up with Mark Murray from the United States Naval Academy and Frank Fish from West Chester University to find out more about the hydrodynamics of whale and dolphin flippers. Their findings; some dolphins' fins generate lift in the same way as delta wing aircraft.
From Prof. Chad Orzel's Graduation Speech:
Science isn't a body of facts, science is a process for figuring out how the world works: you see something interesting, come up with an idea of why that might happen, and test you're idea to see if you're right. You repeat this process until you figure out why things happen the way they do, and then you use that knowledge to explain new things, or to do things that you couldn't do before.
If you have followed this blog for long enough, dear readers, the words "multi-muons", "anomalous muons", or even "lepton jets" are not foreign to you. They all refer to a paper appeared on the ArXiv on the evening of Halloween last year. In the paper the CDF collaboration published the results of a detailed analysis which described how a component of collider data containing two or more muons could not be explained by known Standard Model processes.
NASA watch seems to have been first in noticing the way-cool Star-Trek Style NASA poster, cheerfully shown here in all its glory. Yes, this is not your parent's NASA... no, wait, it is. Star Trek also dates from the 60s.

It's a well-done poster, with great poses all around. That's the crew for shuttle Expedition 21. Until we build Star Fleet, I figure these people qualify.

It's a well-done poster, with great poses all around. That's the crew for shuttle Expedition 21. Until we build Star Fleet, I figure these people qualify.
In a few days italian post-docs working in high-energy physics will be asked to gather for a nasty exam, held by the INFN -the italian institute for nuclear physics- to qualify valiant researchers for future hiring in the institute.
The exam generated a wave of outrage among the very pool of people at which it is aimed: the scores of "precari" (temporary workers) who are spending the best years of their life to try and make a career in particle physics. Let me explain why that is so.
The exam generated a wave of outrage among the very pool of people at which it is aimed: the scores of "precari" (temporary workers) who are spending the best years of their life to try and make a career in particle physics. Let me explain why that is so.
An enormous plume of water spurts in giant jets from the south pole of Saturn's moon Enceladus and a report published in Nature provides evidence that this magnificent plume is fed by a salty ocean.
The Cassini spacecraft made a surprising discovery about Saturn's sixth largest moon, Enceladus, on its exploration of the giant ringed planet in 2005. Enceladus ejects water vapor, gas and tiny grains of ice into space hundreds of kilometres above the moon's surface.
The Cassini spacecraft made a surprising discovery about Saturn's sixth largest moon, Enceladus, on its exploration of the giant ringed planet in 2005. Enceladus ejects water vapor, gas and tiny grains of ice into space hundreds of kilometres above the moon's surface.
At the quantum level, the atoms that make up matter and the photons that make up light behave in seemingly bizarre ways.
Particles can exist in "superposition," in more than one state at the same time (don't look!), a situation that permitted Schrödinger's famed cat to be simultaneously alive and dead. Matter can also be entangled', what Albert Einstein called "spooky action at a distance" in such a way that one thing influences another, regardless of how far apart the two are.
Particles can exist in "superposition," in more than one state at the same time (don't look!), a situation that permitted Schrödinger's famed cat to be simultaneously alive and dead. Matter can also be entangled', what Albert Einstein called "spooky action at a distance" in such a way that one thing influences another, regardless of how far apart the two are.
Not all job rejections are equal. Being turned down from the 'Wally the Whale' fish sandwich stop at age 17, for example, was probably a blessing in disguise. Also humorous, as it was my first 'overqualified' experience-- I'd had 2 year's work at a seafood market prior.
That said, some jobs you just want more than others. I'm only a few weeks into my attempt at transitioning to a salaried science writing/web gig. So far the news is mixed. And mixed, as all job-hunters know, means either 'indetermined' or 'bad'.
Having just gotten the 'call of doom' from the first off my "really want" job list, though, I must say there are many bright sides to this. Here's my top 5 list on why job hunting rocks!
That said, some jobs you just want more than others. I'm only a few weeks into my attempt at transitioning to a salaried science writing/web gig. So far the news is mixed. And mixed, as all job-hunters know, means either 'indetermined' or 'bad'.
Having just gotten the 'call of doom' from the first off my "really want" job list, though, I must say there are many bright sides to this. Here's my top 5 list on why job hunting rocks!
For a long time, recreational computer users all over the world have benefitted from improvements to computing systems that were invented in order to facilitate research in fundamental physics. The foremost example is, of course, the World Wide Web which you are using to read this.
Now the time has come for the gamers to give back to physics. Of course, nobody would buy that as a moral argument, but money talks louder than most ethicists, and the market for games consoles and graphics cards has become huge and strongly driven by increases in computational performance, leading to ever faster graphics processors being developed to please the gamers. If you have a moderately recent desktop computer, odds are that the graphics card has more computational power than the CPU.
Now the time has come for the gamers to give back to physics. Of course, nobody would buy that as a moral argument, but money talks louder than most ethicists, and the market for games consoles and graphics cards has become huge and strongly driven by increases in computational performance, leading to ever faster graphics processors being developed to please the gamers. If you have a moderately recent desktop computer, odds are that the graphics card has more computational power than the CPU.
Century Old Materials Mystery Solved: Grain Boundary Formation Shows Similarities Of Metal And Glass
Stress and strain research got a boost thanks to research from NIST, where scientists have recently found evidence of an important similarity between the behavior of polycrystalline materials, like metals and ceramics, and glasses.
Most metals and ceramics used in manufacturing are polycrystals. The steel in a bridge girder is formed from innumerable tiny metal crystals that grew together in a patchwork as the molten steel cooled and solidified. Each crystal, or “grain,” is highly ordered on the inside, but in the thin boundaries it shares with the grains around it, the molecules are quite disorderly.
Most metals and ceramics used in manufacturing are polycrystals. The steel in a bridge girder is formed from innumerable tiny metal crystals that grew together in a patchwork as the molten steel cooled and solidified. Each crystal, or “grain,” is highly ordered on the inside, but in the thin boundaries it shares with the grains around it, the molecules are quite disorderly.
A new National Institute of Standards and Technology (NIST) assay using a “glow or no glow” technique may soon help the U.S. Department of Homeland Security (DHS) defend the nation against a spectrum of biological weapons that could be used in a terrorist attack.
One very dangerous toxin on the list is ricin, a protein derived from castor beans that is lethal in doses as small as 500 micrograms—about the size of a grain of salt.
One very dangerous toxin on the list is ricin, a protein derived from castor beans that is lethal in doses as small as 500 micrograms—about the size of a grain of salt.
Below I offer a preview of the slides I will show tomorrow at an invited seminar on the rather technical topic of "The b-jet energy calibration with Z-->bb decays", which I have come to CERN to give at a meeting of the LHCb collaboration. As I mentioned already in the first part of this two-part article, the topic is rather technical, and I do not expect a large audience -but I will nonetheless make an attempt at explaining the meaning of the slides pasted below. Then, of course, I am available to provide some additional light on any specific issue among those dealt below which you may want to understand more about.
Can you fly a house with balloons? The recent Pixar movie "Up" does, but it's animated. In the "Up" production notes, Steve May, the film's supervising technical director, writes
"It was important to the film to have fairly realistic balloon simulations. The balloons behave in a realistic way, although the notion of being able to fly a hosue with balloons is pretty preposterous. We're not physicists but one of our technical directors calculated that it would take on the order of 20 to 30 million balloons to actually life Carl's house. We ended up using [...] 20,622 when it actually lifts off."
Prologue


