Astronomers see planet still growing in
its stellar womb
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[November 19, 2015]
By Irene Klotz
CAPE CANAVERAL, Fla. (Reuters) -
Astronomers have taken the first images of a planet still in formation,
a discovery expected to shed light on how giant planets manage to beef
up early in their lives, research published on Wednesday showed.
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Astronomers used a telescope in Arizona to peer at a young star
located about 450 light-years away in the constellation Taurus.
The star, known as LkCa 15, is similar to the sun, but only 2
million years old.
Unlike the 4.6 billion-year-old sun, LkCa 15 is still surrounded by
a disk of gas and dust, the raw materials for planet building.
Within the disk is a big gap, some 50 times wider than distance
between Earth and the sun.
Astronomers previously suspected that a giant planet was orbiting in
the gap. Research published in this week’s issue of the journal
Nature confirms the find with infrared images of the planet, along
with what appear to be one or two sibling planets.
Scientists also for the first time discovered the chemical
footprints of superheated hydrogen gas streaming from the dust disk
onto the planet, evidence that it is still forming, said Stephanie
Sallum, a University of Arizona astronomy graduate student who led
the team.
"This young system provides the first opportunity to study planet
formation and disk–planet interactions directly," Sallum and
colleagues wrote in Nature.
Of the nearly 2,000 confirmed planets discovered beyond the solar
system, none are still in the formation stage.
In a related commentary also published in Nature, Princeton
University astrophysicist Zhaohuan Zhu said the discovery will help
scientists hone their theories about how planets are formed.
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For example, more work is needed to explain the giant planet’s
location and why it is still growing. Scientists also cannot account
for how the planet is generating the massive magnetic fields that
are believed to be responsible for super-charging its hydrogen gas
feeding lines.
The discovery also demonstrates a technique to find other baby
planets by searching for the telltale hydrogen gas emissions.
(Editing by David Adams and Grant McCool)
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