WALLSTREETJOURNAL.COM - Astronomers have spotted what they believe is a planet in the violent
process of being born in another solar system, an event that may shed
light on how planets come into being.
An international team of researchers
said the so-called protoplanet has a mass that appears to be at least
the size of Jupiter, and perhaps two to three times its size. It is
located about 335 light years from Earth, within the Milky Way. That
isn't too far in cosmic terms; the Milky Way itself is about 100,000
light years across.
"If we are correct, this is the first
time we are seeing a planet forming inside its natal environment," said
Sascha Quanz, an astronomer at the Swiss university ETH Zurich and
leader of the team. The findings are reported in Astrophysical Journal
Letters, a scientific publication.
There are two leading theories of planet
formation. Under one, small dust grains circling around a parent star
collide, get larger and larger, and under the force of gravity develop
into a much larger object. Over hundreds of thousands of years, this
object accumulates enough material to become a planet. That is how the
planets of our solar system most likely formed.
Another theory suggests that material surrounding a young star can
undergo gravitational collapse under its own mass. This causes debris to
clump together, creating a planet in just a few thousand years. It
isn't clear how the latest suspected protoplanet is being formed.
If it holds up, the latest finding
would be one of the first direct observations of the very early stages
of a planet's birth. Dr. Quanz and colleagues based their discovery on
observations by a high-resolution infrared camera linked to a telescope
located in Chile's Atacama Desert.
The telescope was pointed at a young
star, HD 100546, about 2.5-times the size of our sun. Astronomers were
interested in the star because the disk of materials around it showed
certain asymmetries. "It's a good indication that something might be
hiding or forming in the disk," said Dr. Quanz.
The infrared imagery revealed a little
bright blob in the disk, suggesting an entity emitting radiation. When
the picture of the blob was laid over an image of the asymmetry, they
coincided perfectly. The conclusion: The blob was an object embedded in
the material around the star, suggesting a nascent planet.