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28 New Exoplanets Discovered

Jeanna Bryner
Staff Writer
SPACE.com Tue May 29, 7:01 AM ET
http://news.yahoo.com/s/space/20070529/sc_space/28newexoplanetsdiscovered;_ylt=AtQatZSRqEkptS.otRnLpduFDvII

Updated 9:30 pm Eastern

HONOLULU-Astronomers have discovered 28 new planets outside of our
solar system, increasing to 236 the number of known exoplanets,
revealing that planets can exist around a broad spectrum of stellar
types-from tiny, dim stars to giants.

"We added 12 percent to the total in the last year, and we're very
proud of that," said one of the study team members Jason Wright of the
University of California at Berkeley. "This provides new planetary
systems so that we can study their properties as an ensemble."

The planets are among 37 new objects spotted within the past year.
Seven of the objects are failed stars called brown dwarfs, with masses
that dwarf the largest, Jupiter-sized planets but too small to sustain
the nuclear reactions necessary for stellar ignition.

John Johnson of the University of California at Berkeley and his
colleagues presented the findings here today at a meeting of the
American Astronomical Society (AAS).

Astronomers don't directly spot extrasolar planets, but rather look
for stellar wobbles caused by orbiting planets. The planet's size and
distance from the parent star affect how strong or weak of a wobble,
and more sophisticated techniques for measuring the stellar wobbles
has led to an ever-lengthening list of such outer planets. Now they
can detect wobbles of a meter per second compared with the 10-meter
limit just 15 years ago.

Planet profiles

One of the exoplanets, orbiting a red M dwarf just 30 light-years from
Earth, was discovered two years ago, but recent observations have
allowed astronomers to pin down its mass, radius and density. The
ice-giant planet circles the star Gliese 436 (GJ 436) and has a radius
and density that are surprisingly similar to that of Neptune.

Weighing in at 22.4 Earth-masses, the exoplanet is the first
Neptune-sized planet observed to transit a star. The previous record
holder, dubbed HD 140926b, weighed in at 100 Earth masses, and Jupiter
is 320 Earth masses.

"[Gliese 436b] must be 50 percent rock and about 50 percent water,
with perhaps small amounts of hydrogen and helium," said head of the
planet-search team Geoffrey Marcy, also of UC Berkeley. "So this
planet has the interior structure of a hybrid super-Earth/Neptune,
with a rocky core surrounded by a significant amount of water
compressed into solid form at high pressures and temperatures."

Its 2.6-day orbit around GJ 436 means the hybrid planet circles very
close to its star, just 3 percent of the Sun-Earth distance, and
making it a hot Neptune. Unlike most giant planets found with such
close ties to their stars, this planet has an eccentric orbit. The
elongated orbit suggests the parent star could have another planetary
companion with a more distant orbit.

"I'm sure people will immediately follow up and try to measure the
atmospheric composition of this planet," Wright said.

GJ 436 is an M star and 70 percent of all stars are considered M-type
stars, so finding that these dim stars can support planets could mean
a boon for planet hunters.

Bigger is better

At least four of the newly spotted planets belong to multiple-planet
systems, supporting the idea that at least 30 percent of all
planet-parent stars have more than one planetary companion. Since
smaller planets and those outside our solar system are trickier to
detect, Wright predicts this percentage will continue to rise as
detection methods improve.

And three of the just-discovered planets circle stars that boast
masses between 1.6 and 1.9 times that of our Sun. Planets orbiting
these so-called A- and F-type stars are typically difficult to detect
because the stars rotate fast and have pulsating atmospheres.

Due to their extreme rotational velocities and high temperatures, A
and F stars only jitter slightly from orbiting planets and so surveys
can only pick up wobbles from super-massive planets and brown dwarfs
in short-period orbits around these stars.

Johnson discovered that "retired" A stars, which have nearly burned
all of their hydrogen and remain stable for a short stint, have slower
rotation rates and are not so hot. That makes it easier for
astronomers to measure their planet-caused wobbles.

Unlike planets orbiting M-type stars, these exoplanets tend to orbit
at least 0.8 astronomical units (AU) from the parent stars.

For this reason, massive stars are more likely to harbor Jupiter-sized
planets than are lower-mass stars, Johnson said. And retired A-type
stars are twice as likely to support planets compared with Sun-like
stars, which Johnson attributes to the fact that bigger stars start
out with more material in their disks to feed planet building.

So these massive stars also could represent a treasure trove for
places to spot new exoplanets, along with the M stars, Johnson said.

--
Bob.