Exoplanet Measured with Remarkable Precision   
       
   August 18, 2014: Barely 30 years ago, the only planets astronomers had found   
   were located right here in our own solar system.  The Milky Way is chock-full   
   of stars, millions of them similar to our own sun.  Yet the tally of known   
   worlds in other star systems was exactly zero.   
       
   What a difference a few decades can make.   
       
   As 2014 unfolds, astronomers have not only found more than a thousand   
   "exoplanets" circling distant suns, but also they're beginning to make precise   
   measurements of them.  The old void of ignorance about exoplanets is now being   
   filled with data precise to the second decimal place.   
       
   http://www.youtube.com/watch?v=lA6MJkHJXVk&feature=youtu.be   
       
   A new ScienceCast video examines the extraordinary precision which with   
   researchers are beginning to measure exoplanets.  Play it   
       
   A team led by Sarah Ballard, a NASA Carl Sagan Fellow at the University of   
   Washington in Seattle, recently measured the diameter of a "super Earth" to   
   within an accuracy of 148 miles total or about 1 percent - remarkable accuracy   
   for an exoplanet located about 300 light years from Earth.   
       
   "It does indeed seem amazing," says Ballard. "The landscape of exoplanet   
   research has changed to an almost unrecognizable degree since I started   
   graduate school in 2007."   
       
   To size up the planet, named "Kepler 93 b," Ballard used data from NASA's   
   Kepler and Spitzer Space Telescopes.   
       
   First, Kepler discovered the planet. As seen from Earth, Kepler 93 b passes   
   directly in front of its parent star, causing the starlight to dim during the   
   transit. That dimming, which occurs once per orbit, is what allowed Kepler   
   mission scientists to find the planet in the first place.   
       
   Next, both Spitzer and Kepler recorded multiple transits at visible and   
   infrared wavelengths. Data from the observatories agreed: Kepler 93 b was   
   really a planet and not some artefact of stellar variability. Ballard then   
   knew that by looking carefully at the light curve she could calculate the size   
   of the planet relative to the star.   
       
   At that point, the only missing piece was the diameter of the star itself.   
       
   http://kepler.nasa.gov/   
       
   Click to visit the Kepler home page"The precision with which we measured the   
   size of the planet is linked directly to our measurement of the star," says   
   Ballard.  "And we measured the star using a technique called asteroseismology."   
       
   Most people have heard of "seismology," the study of seismic waves moving   
   through the Earth.  "We can learn a lot about the structure of our planet by   
   studying seismic waves," she says.   
       
   Asteroseismology is the same thing, except for stars: The outer layers of   
   stars boil like water on top of a hot stove.  Those convective motions create   
   seismic waves that bounce around inside the core, causing the star to ring   
   like an enormous bell.  Kepler can detect that "ringing," which reveals itself   
   as fluctuations in a star's brightness.   
       
   Ballard's colleague, University of Birmingham professor Bill Chaplin led the   
   asteroseismic analysis for Kepler-93 b. "By analyzing the seismic modes of the   
   star, he was able to deduce its radius and mass to an accuracy of a percent,"   
   she says.   
       
   The new measurements confirm that Kepler-93 b is a "super-Earth" sized   
   exoplanet, with a diameter about one-and-a-half times the size of our planet.   
   Previous measurements by the Keck Observatory in Hawaii had put Kepler-93 b's   
   mass at about 3.8 times that of Earth. The density of Kepler-93 b, derived   
   from its mass and newly obtained radius, suggests the planet is very likely   
   made of iron and rock, like Earth itself.   
       
   Although super-Earths are common in the galaxy, none exist in our solar   
   system. That makes them tricky to study.  Ballard's team has shown, however,   
   that it is possible to learn a lot about an exoplanet even when it is very far   
   away.   
       
   Credits:   
   Author: Dr. Tony Phillips | Production editor: Dr. Tony Phillips | Credit:   
   Science@NASA   
       
       
   Regards,   
       
   Roger   
      
   --- D'Bridge 3.99   
    * Origin: NCS BBS - Houma, LoUiSiAna (1:3828/7)