New Planets Challenge Theories
(Special Report from the 2001 American Astronomical Society meeting)
SAN DIEGO (Jan. 10, 2001) -- Two recently discovered planetary systems may challenge current theories about
how planets form, according to the astronomers who found them. One of the discoveries
may even cause theorists to reconsider the the definitions of planets and brown
dwarfs -- objects that are too large to be planets but too small to shine as
stars.
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| The newly discovered planets probably closely resemble Jupiter (shown here).
Although three of the planets are more massive than Jupiter, their stronger
gravity would compress them, so they should be no bigger than Jupiter. |
"As of a month ago, we thought we understood the lay of the land in planetary
systems," said Geoffrey Marcy, an astronomer at the University of California,
Berkeley, and leader of the world's leading team of planet hunters, during a
Tuesday press conference. "We also thought we understood the lay of the
land with regard to planetary orbits....So we were a bit cocky."
But Marcy said his team was humbled by the discoveries of a pair of two-planet
systems. One system's planets follow "resonant" orbits, while the
second system contains the largest planet-like object discovered to date. "Both
planetary systems are entirely unique, and I think a little frightening,"
he said.
Astronomers have discovered about 50 planets orbiting stars other than our
own Sun, but the new discoveries are among only a handful of systems in which
more than one planet has been found.
Home of the Whopper
One of the new systems is around HD 168433, a star similar to our own Sun, and
contains two planets or other objects. One is at least seven times as massive
as Jupiter, the largest planet in our own solar system, and orbits the star
at about three-tenths of the distance from Earth to the Sun. The second is at
least 17 times as massive as Jupiter and is about three times farther from HD
168433 than Earth is from the Sun.
"This is the whopper," said team member Paul Butler, a staff scientist
at the Carnegie Institution of Washington. "This is literally off our scale....It's
twice as massive as anything else we've ever seen."
The Marcy-Butler team has discovered almost 40 planets orbiting stars other
than the Sun. Most are as massive as Jupiter or heavier, but none approaches
the heft of the object in the HD 168433 system. Current theories say that any
object about a dozen times as massive as Jupiter or heavier should be a brown
dwarf -- a not-quite-star that can shine briefly by "fusing" the nuclei
of deuterium atoms (a form of hydrogen) in its core.
But because of its close proximity to the star, and its presence in a system
that contains a known planet, Butler said it's too early to classify their discovery
as a brown dwarf. Instead, it may be some previously known "missing link"
between planets and brown dwarfs. "I prefer to just say it's a mystery
system and hope our friends in the theoretical community will consider it a
gift," Butler said.
Planetary Reverb
The second pair of planets orbits Gliese 876, a faint, cool star known as a
red dwarf. It's one of our closest stellar neighbors, at a distance of 15 light-years.
The team had already reported the discovery of one planet in the system, but
continued observations revealed a second planet.
One planet is about one-half as massive as Jupiter, while the other is 1.8
times Jupiter's mass. What makes the system especially interesting, though,
is the planets' orbits: The innermost star orbits Gliese 876 once every 30 days,
while the other orbits every 60 days. This relationship is called a resonance,
and it suggests that the two planets act as mutual "shepherds," with
their gravitational pull keeping their orbital periods in 2-to-1 harmony.
Team member Debra Fischer of UC-Berkeley called this orbital relationship a
true "music of the spheres," and compared it to two harmonizing notes
played on a stringed musical instrument.
Similar harmonies are found in our own solar system. The planet Pluto completes
two orbits around the Sun for every three orbits of Neptune, for example. --
Damond Benningfield
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