Tuesday, December 7, 2010
Baby aspirin cuts risk for prostate cancer mortality
- When data from all eight trials are considered), patinets randomized to aspirin therapy had a statistically signifciant reduction in risk of death due to any form of cancer (odds ratio [OR] = 0.79).
- When individual patient data — available from seven of the eight trials (23 535 patients, 657 cancer deaths) — were analyzed , benefit was apparent only after 5 years’ follow-up.
- For all cancers, the hazard ratio [HR] was 0.66.
- For gastrointestinal cancers, the hazard ratio was 0·46.
- The 20-year risk of cancer death (based on 1,634 deaths in 12,659 patients in three trials) remained lower in the aspirin groups than in the control groups.
- For all solid tumors, HR = 0·80.
- For gastrointestinal cancers, HR = 0·65
- The time to evidence of an effect on deaths (the “latent period”) was about 5 years for oesophageal, pancreatic, brain, and lung cancers, but was longer for stomach, colorectal, and prostate cancers.
- The overall effect on 20-year risk of cancer death was greatest for adenocarcinomas (HR = 0·66), and the vast majority of prostate cancers areadenocarcinomas.
- The benefit of aspirin therapy was unrelated to aspirin dose (75 mg upwards), sex, or smoking, but increased with age.
- The absolute reduction in 20-year risk of cancer death was 7·08 percent (range, 2·42 to 11·74 percent) at age 65 years and older.
Sunday, December 5, 2010
Tooth decay to be a thing of the past? Enzyme responsible for dental plaque sticking to teeth deciphered
The above story is reprinted (with editorial adaptations by ScienceDaily staff) from materials provided by University of Groningen.
Wednesday, December 1, 2010
Dim Stars Triple the Universe’s Stellar Tally
There are more dim bulbs in the universe than even the most hardened pessimist might have imagined.
The profusion of stars also suggests that the early history of the cosmos may need a rewrite, perhaps doubling previous estimates of the total mass of stars in many of the universe’s first, massive galaxies. If so, those early galaxies would have forged stars at a much more prodigious rate, says Pieter van Dokkum of Yale University. He and Charlie Conroy of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass., describe their study in a paper appearing online in Nature on December 1.
Van Dokkum and Conroy set out to determine whether spiral galaxies like the Milky Way have a different mix of low-mass and high-mass stars than is found in elliptical galaxies, which tend to have an older stellar population. Such differences had long been suspected but never proven.
Because even the sharpest telescopes can’t resolve individual faint stars in galaxies millions of light-years beyond the Milky Way, the team examined light from the central portion of each of eight massive elliptical galaxies — four in the Coma cluster and four in the Virgo cluster. Such galaxies are thought to account for one-third of the stellar mass in the universe. Massive galaxies that existed during the first billion or so years of cosmic history are believed to be the early ancestors of these ellipticals.
Spectra of light from the galaxies revealed two chemical fingerprints, absorption by sodium atoms and by iron hydride, which are unusually strong in faint red dwarf stars that have less than one-third the sun’s mass. The strength of the absorption features indicates that red dwarfs account for 80 percent of the number of stars in elliptical galaxies and 60 percent of the total stellar mass in those galaxies.
“Extrapolating from the central regions of these eight galaxies to the entire universe is somewhat hazardous, but if the galaxies are typical examples of their class it may well lead to a tripling” of the total number of stars in the cosmos, van Dokkum says.
One caveat, says Richard Ellis of Caltech, is that the researchers assumed that red dwarfs in the elliptical galaxies have the same chemical composition as red dwarfs in the Milky Way. It’s possible, he notes, that the strong absorption signals don’t indicate a very large population of the dwarfs. Instead, those measurements might be explained by a smaller population of red dwarfs that happen to be richer in sodium and iron hydride than red dwarfs in the Milky Way.
Nonetheless, the study provides “the most convincing observational test” that the mix of stars — heavyweights and lightweights — varies dramatically from one type of galaxy to another, says Ellis. Instead of using the assortment of high- and low-mass stars in the Milky Way as a standard template, such differences need to be taken into account when astronomers estimate the stellar mass and star-formation rates of galaxies from the early universe, van Dokkum and Conroy note.
Images: 1) The elliptical galaxy ESO 325-G004, which may harbor 10 times as many dim stars as the Milky Way. Credit: NASA, ESA, and The Hubble Heritage Team (STScI/AURA) 2) Astronomers examined the chemical signature of small, dim stars called red dwarfs (right) in eight elliptical galaxies and found that they are much more numerous than red dwarfs in the Milky Way (left). The finding suggests that the total number of stars in the universe could be up to three times higher than previously thought. Credit: Yale University
See Also:
- Calling All Amateur Astronomers: Help Solve a Mystery
- Odds of Finding Earth-Size Exoplanets Are 1-in-4
- Early Galaxies Formed Stars Fast Because They Had More Gas
- Sharpest Image Yet of Massive Galaxy Collision
- Milky Way May Fizzle Out Sooner Than Expected
- Galaxies Discovered in Their Awkward Teen Phase
Could This Be How Stonehenge Was Actually Built?
One of the most puzzling mysteries is how Stonehenge, the prehistoric circle of stones in England, came to be. We know it was built around 4500 years ago, and the stones came from Wales, some 250km away… but how?
Of course, back then, it wasn’t so easy to transport stuff around the country – especially not 60 bluestones which are said to weigh between two and four tons each. Several theories have been bandied about over the years of how the stones were transported, including sledges; rafts along the rivers; and that Merlin himself used his magic to gather the stones there.
This week, an engineer and former BBC TV presenter, Garry Lavin, tested his theory that wicker baskets made from willows were used to roll the stones all 250kms from the quarry in Preseli Hills, Wales, to Salisbury, in Wiltshire, England. He built one himself, using willow and alder saplings, and enlisted several friends to help roll a one-ton boulder along the ground.
He thinks oxen might’ve helped roll the baskets in some parts, and that rivers could have floated them downstream. But it’s the baskets which Lavin is sure had a huge part in the formation of Stonehenge – and as he’s currently building a maxi-basket to move a five ton stone, we may soon find out the answer. Unless aliens decide to show up and show us otherwise, of course. [Daily Mail]
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Your Next Computer Chip Revolution Unveiled by IBM: Sexy Blend of Lasers, Electrons
IBM's just unveiled a new breakthrough chip tech: CMOS Integrated Silicon Nanophotonics. Confused? It's actually pretty astonishing, promising chip-sized supercomputer power in the near future. Now you're interested....
We've known for a while that optical technology is going to be the next big revolution in computing--it's simply faster than pure electronics, and means you can get even greater performance with lower power demands from similar-sized devices. The trick is about blending optical technology at a nanoscopic scale with existing silicon electronics--and this is where CMOS ISN has achieved a breakthrough. It means thanks to research at IBM's research facility, it's now possible to integrate optical computing technology and conventional electronics onto a single slice of silicon.
Optical signals can carry more information more swiftly than electronics can manage--it's why Intel's fiber-optic Light Peak connection cables may quickly supersede newcomer USB3--and the associated electronics can eat less power than normal silicon tech. This means when you mix the systems together on chips, you can get up to ten times more integration density than is possible with current chip fabrication tech. Putting a bunch of them together results in a computer that shoots data around at rates that would seem incredible compared to current designs.
IBM's trick requires no particularly hefty refits of existing CMOS production plants, and means all the nanoscopic optical equipment like modulators and photodetectors can be built right in to a more conventional chip--meaning there's no need to add in extra-special chips to access the benefits of optical tech when you're building an integrated optical computer.
Still confused? The upshot: Chips can be significantly faster, and still consume less electrical power. Enough that IBM thinks the chips could build an exascale supercomputer, roughly 1,000 times faster than the fastest machine that exists. The side effect of this, of course, will be consumer-level systems that could be as powerful as today's research supercomputers. Your laptop in several years may be driven by chips packed with frikking laser beams, people.
To read more news on this, and similar stuff, keep up with my updates by following me, Kit Eaton, on Twitter.
Tuesday, November 30, 2010
A Healthy Brain Needs a Healthy Heart
When the National Institutes of Health convened a panel of independent experts this past April on how to prevent Alzheimer’s disease, the conclusions were pretty grim. The panel determined that “no evidence of even moderate scientific quality” links anything--from herbal or nutritional supplements to prescription medications to social, economic or environmental conditions--with the slightest decrease in the risk of developing Alzheimer’s. Furthermore, the committee argued, there is little credible evidence that you can do anything to delay the kinds of memory problems that are often associated with aging. The researchers’ conclusions made headlines around the world and struck a blow at the many purveyors of “brain boosters,” “memory enhancers” and “cognitive-training software” that advertise their wares on the Web and on television. One of the panel experts later told reporters in a conference call that the group wanted to “dissuade folks from spending extraordinary amounts of money on stuff that doesn’t work.”
But did the panel overstate its case? Some memory and cognition researchers privately grumbled that the conclusions were too negative--particularly with respect to the potential benefits of not smoking, treating high blood pressure and engaging in physical activity. In late September the British Journal of Sports Medicine published a few of these criticisms. As a longtime science journalist, I suspected that this is the kind of instructive controversy--with top-level people taking opposing positions--that often occurs at the leading edge of research. As I spoke with various researchers, I realized that the disagreements signaled newly emerging views of how the brain ages. Investigators are exploring whether they need to look beyond the brain to the heart to understand what happens to nerve cells over the course of decades. In the process, they are uncovering new roles for the cardiovascular system, including ones that go beyond supplying the brain with plenty of oxygen-rich blood. The findings could suggest useful avenues for delaying dementia or less severe memory problems.