|If this is your first visit, be sure to check out the FAQ by clicking the link above. You may have to register before you can post: click the register link above to proceed. To start viewing messages, select the forum that you want to visit from the selection below.|
||Thread Tools||Display Modes|
Astronomers Discover the Nearest Young Planet-Forming Star
EMBARGOED FOR RELEASE at 2:00 p.m. EST (9:00 a.m. HST)
on Thursday, February 26, 2004, to coincide with publication
in Science Express
Dr. Michael C. Liu 1-808-956-6666
Mrs. Karen Rehbock 1-808-956-6829
Dr. Douglas Pierce-Price 1-808-969-6524
Dr. Paul Kalas, 1-510-642-828,
Astronomers Discover the Nearest Young Planet-Forming Star
A team of scientists including University of Hawaii astronomers has found
the nearest example of a young planet-forming star.
Using the telescopes on Mauna Kea, Hawaii, they have discovered a
spectacular circumstellar dust disk with indirect evidence for newly formed
planets around the star AU Microscopium (AU Mic). At a distance of only 33
light years, this is the nearest star with a visible disk, enabling
astronomers to directly observe the primordial material for making planets.
"We know that extrasolar planets are common, but understanding how they form
is an outstanding question. Because AU Mic is so near to Earth, it provides
us a special opportunity to examine planet formation in great detail," said
team member Dr. Michael Liu, an astronomer at the University of Hawaii
Institute for Astronomy.
The results will be published in this week's online Science Express, the
March print edition of Science, and an upcoming issue of the Astrophysical
Journal. The authors are Drs. Michael C. Liu and Jonathan P. Williams of the
University of Hawaii, and Drs. Paul G. Kalas and Brenda C. Matthews of the
University of California, Berkeley.
AU Mic is a dim red star, with only half the mass and one-tenth the energy
output as the Sun. Previous studies had shown that AU Mic is about 12
million years old. In comparison, our Sun is about 4.6 billion years old.
"Unfortunately, we can't go back in time and observe our own Solar System.
But by studying these very young stars, we can examine how planets are
forming around them, and thus indirectly learn about the origin of our own
Solar System," said Liu.
The team used the James Clerk Maxwell Telescope on Mauna Kea, Hawaii to
study the sub-millimeter radiation from AU Mic. This radiation, which is
invisible to the naked eye, comes from very cold dust grains orbiting the
star in the form of a disk. Such disks are believed to be the nurseries for
By analyzing the radiation, the team deduced that dust particles only
existed at large distances from the star, and were missing inside a radius
of about 17 AU. This would be slightly inside the orbit of Uranus in our own
"The dust missing from the inner regions of AU Mic is the telltale sign of
an orbiting planet. The planet sweeps away any dust in the inner regions,
keeping the dust in the outer region at bay," said Liu.
The team's visible light images of AU Mic reveal a spectacular edge-on disk,
extending out to at least 210 Astronomical Units (AU), or about 20 billion
miles. In comparison, the known edge of our Solar System is about 50 AU, or
four times smaller. AU Mic's disk is visible due to small dust particles
which reflect the light of the central star.
The images were obtained with an instrument known as a coronagraph deployed
on the with the University of Hawaii's 2.2-meter telescope. The coronagraph
blocked out the bright glare of the central star, allowing detection of the
faint edge-on disk.
"This fascinating system shows how the exceptional clarity, darkness, and
transparency of the Mauna Kea skies allow Hawaii astronomers to make
frontier discoveries," said Dr. Rolf Kudritzki, Director of the Institute
"AU Mic is a common red dwarf star, which comprise 85% for all stars. By
studying this nearby system, we might learn about how the majority of
planetary systems can form," said team member Dr. Paul Kalas, an astronomer
at the University of California, Berkeley and a Ph.D. recipient from the
University of Hawaii.
Images of disks around nearby stars are very rare, and AU Mic is the closest
dust disk found since the discovery 20 years ago of a disk around beta
Pictoris, a star about 2.5 times the mass of the sun and 65 light years
away. Though the two stars are far apart on the sky, they appear to have
been formed at the same time and are traveling together through the galaxy.
AU Mic is close enough that future imaging with the Hubble Space Telescope
or ground-based telescopes using adaptive optics can study the detailed
structure of the disk and perhaps directly image the light from any planets.
"We're waiting for the next observing season to go back and study the
physical properties of the disk. But we expect other teams to do the same
thing - there will be lots of follow-up," said Kalas.
"Astronomers will be studying AU Mic for many years to come," said Liu.
This work was supported by the National Science Foundation and the NASA
Astronomical Search for Origins program.
The Institute for Astronomy at the University of Hawaii conducts research
into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff
are also involved in astronomy education, deep space missions, and in the
development and management of the observatories on Haleakala and Mauna Kea.
Refer to http://www.ifa.hawaii.edu/ for more information about the
Color images are available at:
|Thread||Thread Starter||Forum||Replies||Last Post|
|Space Calendar - November 26, 2003||Ron Baalke||History||2||November 28th 03 09:21 AM|
|Space Calendar - November 26, 2003||Ron Baalke||Astronomy Misc||1||November 28th 03 09:21 AM|
|Space Calendar - October 24, 2003||Ron Baalke||History||0||October 24th 03 04:38 PM|
|Space Calendar - October 24, 2003||Ron Baalke||Astronomy Misc||0||October 24th 03 04:38 PM|
|Space Calendar - September 28, 2003||Ron Baalke||History||0||September 28th 03 08:00 AM|