Saturday, April 27, 2013

National survey highlights perceived importance of dietary protein to prevent weight gain

Apr. 26, 2013 ? Atkins Diet, Zone Diet, South Beach Diet, etc., etc., etc. Chances are you have known someone who has tried a high protein diet. In fact, according to the International Food Information Council Foundation, 50% of consumers were interested in including more protein in their diets and 37% believed protein helps with weight loss. In a new study released in the May/June 2013 issue of the Journal of Nutrition Education and Behavior, researchers found a relatively high proportion of women who reported using the practice of ''eating more protein'' to prevent weight gain, which was associated with reported weight loss.

Among a national sample, researchers from the University of Minnesota surveyed 1,824 midlife women (40-60 years old) to (1) describe perceptions about protein sources and requirements, (2) identify the reported frequency of using the ''eating more protein'' practice to prevent weight gain, and (3) compare reported protein intake to reported frequency of using the ''eating more protein'' practice to prevent weight gain.

Most women correctly identified good protein sources, and the majority could indicate the daily percent of dietary energy recommended from protein. ''Eating more protein'' to prevent weight gain was reported by 43% of women (and more than half of obese women) as a practice to prevent weight gain. Reported use of this practice was related to self-reported weight loss over two years. Two factors associated with effective use of this practice included the level of protein intake and self-efficacy toward weight management.

According to Noel Aldrich, lead author, those participants' who had reported weight loss with "eating more protein" had a protein intake that was consistent with the focus on protein suggested by the 2010 Dietary Guidelines Advisory Committee. He said, "Education regarding dietary protein requirements may enhance the use of this practice. Women may need more information regarding protein energy content and effective selection of protein sources to enhance protein intake as a weight management strategy. Given that the majority of Americans are overweight, identifying the most effective practices and related factors surrounding successful weight loss and prevention of weight gain are important."

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The above story is reprinted from materials provided by Elsevier Health Sciences, via EurekAlert!, a service of AAAS.

Note: Materials may be edited for content and length. For further information, please contact the source cited above.


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Disclaimer: This article is not intended to provide medical advice, diagnosis or treatment. Views expressed here do not necessarily reflect those of ScienceDaily or its staff.

Source: http://feeds.sciencedaily.com/~r/sciencedaily/~3/jvEwSUw8gvw/130426115618.htm

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Astronomer studies far-off worlds through 'characterization by proxy'

Apr. 25, 2013 ? A University of Washington astronomer is using Earth's interstellar neighbors to learn the nature of certain stars too far away to be directly measured or observed, and the planets they may host.

"Characterization by proxy" is the technique used by Sarah Ballard, a post-doctoral researcher at the UW, to infer the properties of small, relatively cool stars too distant for measurement, by comparing them to closer stars that now can be directly observed.

Ballard is lead author of a study accepted for publication in The Astrophysical Journal that used this method and observations from the Kepler Space Telescope to learn the nature of the distant star Kepler-61.

Our understanding of the size and temperature of planets depends crucially on the size and temperature of the stars they orbit. Astronomers already have a robust way to discern the physical properties of solar-type stars -- those like the sun -- by measuring the light they emit at different wavelengths and matching that to synthetically created spectra.

"The challenge is that small stars are incredibly difficult to characterize," Ballard said. Those theoretical methods don't work well for what are called M-dwarf stars, lower-mass stars about half the size of the sun and smaller -- which is too bad, because such stars make up about three-quarters of the universe.

Ballard is using the characterization by proxy method to try to fill this knowledge gap. She is building on what she calls "truly remarkable" work by astronomer Tabetha Boyajian, now at Yale University, who uses a near-infrared interferometer -- an array of telescopes working in unison studying light wavelengths a bit longer than visible light -- to resolve the physical size of relatively nearby stars.

Ballard said her characterization by proxy method takes "full advantage that there now exists this precious sample" of relatively nearby stars that have been directly measured. You could say the method borrows a bit from Greek mathematician Euclid, whose first "common notion" held that things that equal the same thing must necessarily also equal each other.

In the new paper, Ballard and co-authors used this reasoning to learn about Kepler-61b, a planet orbiting near the inner edge of the habitable zone of the distant, low-mass star Kepler-61, about 900 light-years away in the Cygnus Constellation. A star's habitable zone is that swath of space just right for an orbiting planet's surface water to be in liquid form, thus giving life a chance.

She did this by comparing it to temperature size averages from four spectroscopically similar stars between 12 and 25 light-years away in the Ursa Major and Cygnus constellations. A light-year is about 6 trillion miles.

A funny thing also happened along the way: Kepler-61 turned out to be bigger and hotter than expected, which in turn recalibrated planet Kepler-61b's relative size upward as well -- meaning it, too, would be hotter than previously thought and no longer a resident of the star's habitable zone.

All of this caused Ballard to informally subtitle the paper, "How Nearby Stars Bumped a Planet out of the Habitable Zone."

Funding for the research came from NASA and its Jet Propulsion Laboratory at the California Institute of Technology.

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The above story is reprinted from materials provided by University of Washington. The original article was written by Peter Kelley.

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Source: http://feeds.sciencedaily.com/~r/sciencedaily/space_time/nasa/~3/Pqnj7kUN2vI/130426114641.htm

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