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|Hilo, Hawaii – February 8, 2008: A team of Japanese astronomers has resolved a circumstellar disk around the young lightweight star FN Tau. The diminutive star is located in a star-forming region toward the Constellation Taurus at a distance 460 light years from Earth. This research group used the Coronagraphic Imager with Adaptive Optics (CIAO) at the Subaru Telescope to directly image FN Tau and|
the lightweight disk of planet-forming material surrounding it.
This star is merely 100 thousand years old and weighs only one tenth of the Sun.
A circumstellar disk is a mixture of gas and dust around a young newly formed star. The disk accompanies almost most, if not all, sun-like star formation processes, and planets commonly form in this disk. The disk can also be referred to as a protoplanetary disk because the solid particles inside the disk collide and stick together and grow into planetesimals, which then crash into each other eventually accumulating enough mass to be stabilized as planets. In response to this scenario, the study of youthful stars and their surrounding structures provide details into the formation of planetary systems, and the search for planets outside our solar system motivates much of modern astronomy. Although hundreds have been found through indirect methods, being the first to directly image an extrasolar planet is one of the primary goals of Subaru. The findings at FN Tau show that Subaru is on the right path toward planet discovery.
Observation of protoplanetary disks is not simple because they are small and fainter than their central stars.
FN Tau captured by CIAO instrument mounted on Subaru Telescope.
This infrared image taken at 1.6 micron shows an almost face-on circular disk structure.
The light from the central star FN Tau itself is blocked by the coronagraph mask.
Somewhat symmetrical darker areas are the blocking by the secondary mirror support.
Image: © Subaru Telescope, National Astronomical Observatory of Japan
To date, there are only a few examples that were resolved to show the structures of disks,
and only two of them are for Sun-like single stars.
Thus far, the
has pointed toward more massive disks around stars heavier than the Sun.
The FN Tau researchers pointed the telescope toward
this least massive star trying to detect lightweight disks.
The previous record of the direct imaging of lowest mass disks was around star TW Hya,
which is seven times heavier than the FN Tau disk.
The small size in this study is a big jump in knowledge
about planet formation around lowest mass stars.
The FN Tau study found a thick, compact, and roughly circular protoplanetary disk,
meaning astronomers were observing it nearly face-on.
Its radius is 260 times the Earth-Sun distance,
similar to other disks observed previously.
The disk is rather featureless,
and does not have any anomalies or asymmetries,
such as rings, spirals, or arms.
The mass of the disk was estimated to be 6% of the central FN Tau star,
and by far the least massive one directly detected.
In result, the current finding is the combination
of the most lightweight protoplanetary disk around the least massive star.
One of the questions to come out during the study was what kind of planets can be formed from the disk around FN Tau ?
To date, astronomers worldwide have found 270 extrasolar planets using the indirect detection method, and all are primarily Jupiter-like giant
the least massive exoplanet is still 5 times heavier than Earth.
Because it surrounds a smaller star, the disk about FN Tau
was believed to more likely contain Earth-like planets.
The best-fit model used during this study shows
that the lightweight disk around FN Tau
could only produce Earth-like planets.
The planetary system formation theory also predicted that the disk
is able to form planets lighter than the Earth within 30 AU,
the distance where we find planets in our Solar System.
The lack of heavier objects, such as a Jupiter-size planet,
in the FN Tau disk system is consistent with the astronomersí theoretical expectation.
For the future, the newly commissioned instrument HiCIAO at Subaru will boost the approach of this team. The high dynamic range instrument also will have powerful reinforcement with Subaruís new generation AO system with 188 elements and a laser guide star. The astronomers are hoping to resolve the detailed structure of disks and analyze the size and composition of the dust within. The team will narrow their targets before observations start at ALMA (Atacama Large Millimeter Array) or the next generation large telescopes.
Second Generation Coronagraphic Imager HiCIAO Commissioned On Subaru Telescope, Dec 2007.
Subaru Telescope Adds Laser Guide Star Adaptive Optics System, Nov 2006.
First Light For Subaru Telescope's Adaptive Optics, Dec 2000.
T. Kudo, M. Tamura, Y. Kitamura, M. Hayashi, E. Kokubo, M. Fukagawa, S. S. Hayashi, M. Ishii, Y. Itoh,
S. Mayama, M. Momose, J. Morino, Y. Oasa, T.-S. Pyo and H. Suto,
"Discovery of a Scattering Disk around the Low-Mass T Tauri Star FN Tauri," Ap. J. Lett. 673, L67–L70 (2008)
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