Embargoed until 11 A.M. EST
NSF PR 99-71 - November 29, 1999
This material is available primarily for archival
purposes. Telephone numbers or other contact information
may be out of date; please see current contact information
at media
contacts.

Astronomers Discover Six Planets Orbiting Nearby Stars
A team of astronomers searching the galaxy with powerful
telescopic instruments has found six new planets orbiting
nearby stars. This increases by more than 25 percent
the number of planets astronomers have discovered
outside our solar system, to a total of 28 planets.
All 28 have been found within the last five years.
"These scientists have added significantly to our knowledge
of planetary systems," said Morris Aizenman of the
National Science Foundation's (NSF’s) Astronomical
Sciences Division. "We’re rapidly gaining information
about Jupiter-sized planets, their orbits and orbital
distances. We hope to have enough information soon
to tell us what fraction of nearby stars have Jupiter-sized
planets, and ultimately, how many stars throughout
the galaxy have planets of any size.”
The astronomers made the discoveries as part of a long-term
project supported by NSF and NASA to survey 500 nearby
stars for orbiting planets. Steven Vogt, University
of California, Santa Cruz, Geoffrey Marcy of University
of California, Berkeley, and Paul Butler, Carnegie
Institution, along with Kevin Apps, a student at the
University of Sussex, England, used the Keck I telescope
in Hawaii outfitted with the “HIRES” spectrometer.
They will report their findings in the Astrophysical
Journal.
The six planets orbit stars that are similar in size,age,
and brightness to the sun and are at distances ranging
from 65 to 192 light years from earth. The planets
themselves range in mass from slightly smaller to
several times larger than the planet Jupiter. They
are probably also similar to Jupiter in their compositions--basically
giant balls of hydrogen and helium gas, according
to researcher Steven Vogt. Their orbits tend to be
quite eccentric, tracing oval rather than circular
paths.
"It is beginning to look like neatly stacked, circular
orbits such as we see in our own solar system are
relatively rare," said Vogt.
The presence of a planet around a star is revealed
by the variation in the star’s velocity through space
as a result of the gravitational force exerted on
it by the orbiting planet. Vogt and his coworkers
independently confirmed this method for detecting
planets recently when they were able to measure the
dimming of a star as a planet passed in front of it.
In addition to the discovery of six new planets, the
researchers gathered new data on four known planets,
whose orbits they had previously studied. Two of them
showed long-term trends in their orbits indicating
the presence of a companion, which could be an additional
planet. These findings are significant because previously
only one other system of multiple planets, around
the star Upsilon Andromedae, had been identified outside
our solar system.
For more information on the planet search, see: www.physics.sfsu.edu/~gmarcy/planetsearch/planetsearch.html
|