We know that the planets in our solar system were born from a dusty  disk surrounding the sun billions of years ago;wouldn't it be amazing  if we could see another star system going through the birthing throes of this protoplanetary phase?
  Today, a team of astronomers using the awesome power of the twin 10-meter Keck Telescopes atop Mauna Kea, Hawaii, have announced just that. 
Environment-Clean-Generations
For the first time they have directly imaged a baby world forming  close to its parent star inside an empty track of a larger disk of dust.  This makes it a record-breaker -- the proto(exo?)planet is five-times  younger than the youngest exoplanet discovered to date.
The baby world -- called LkCa 15 b -- orbits LkCa 15, a T Tauri star located 450 light-years from Earth that is already known to possess a dusty circumstellar disk. 
T Tauri stars are very luminous, young, variable stars. In astronomical  timescales, they've recently formed from a cloud of gas under  gravitational collapse. The gravitational energy released is what  provides the energy to power the star, a phase before nuclear fusion is  ignited in their cores.  
So, when we observe LkCa 15, we know we are looking at a star that's  just starting out, potentially with a whole system of worlds that might  form from its protoplanetary disk.
  And now we know that there will be at least one world, LkCa 15 b, that Keck can see slowly forming.
  "LkCa 15 b is the youngest planet ever found, about 5 times younger  than the previous record holder," said astronomer Adam Kraus of the  University of Hawaii's Institute for Astronomy. "This young gas giant is  being built out of the dust and gas. In the past, you couldn't measure  this kind of phenomenon because it's happening so close to the star.  But, for the first time, we've been able to directly measure the planet  itself as well as the dusty matter around it."
Using a clever trick, Kraus and co-investigator Michael Ireland, of  Macquarie University and the Australian Astronomical Observatory, were  able to tease out the light being emitted by the dust surrounding the  newborn star. They combined the power of Keck's Adaptive Optics with a  technique called aperture mask interferometry to manipulate the  starlight after it is received by the telescope.
  "It's like we have an array of small mirrors," said Kraus. "We can  manipulate the light and cancel out distortions." By doing this, the  bright light emitted by the star can be canceled out, resolving the  faint disks and gaps therein where baby worlds may be hiding. In one of  those gaps, LkCa 15 b resides.
"We realized we had uncovered a super Jupiter-sized gas planet, but  that we could also measure the dust and gas surrounding it. We’d found a  planet, perhaps even a future solar system at its very beginning," he  adds.
  Kraus and Ireland intend to continue surveying other nearby stars to  see if similar worlds are forming in the ultimate hope of understanding  the planetary formation processes that built our own solar system.
by "environment clean generations"

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