Discovery of a large dust disk around the nearby star AU Microscopii.
نویسندگان
چکیده
We present the discovery of a circumstellar dust disk surrounding AU Microscopii (AU Mic, GJ 803, HD 197481). This young M star at 10 parsec has the same age and origin as beta Pictoris, another nearby star surrounded by a dust disk. The AU Mic disk is detected between 50 astronomical units (AU) and 210 AU radius, a region where dust lifetimes exceed the present stellar age. Thus, AU Mic is the nearest star where we directly observe the solid material required for planet formation. Because 85% of stars are M-type, the AU Mic disk provides new clues on how the majority of planetary systems might form and evolve.
منابع مشابه
Adaptive Optics Imaging of the Au Microscopii Circumstellar Disk: Evidence for Dynamical Evolution
We present anH-band image of the light scattered from circumstellar dust around the nearby (10 pc) youngM star AU Microscopii (AU Mic, GJ 803, HD 197481), obtained with the Keck adaptive optics system. We resolve the disk both vertically and radially, tracing it over 17–60 AU from the star. Our high angular resolution (0.04 or 0.4 AU per resolution element) observations thus offer the opportuni...
متن کاملRapid Dissipation of Primordial Gas from the Au Microscopii Debris Disk
The disk around AU Microscopii, an M1 star in the β Pictoris Moving Group, is extraordinarily wellsuited for comparison to the β Pic debris disk (type A5V). We use far-UV absorption spectroscopy of AU Mic to probe its edge-on disk for small amounts of H2, the primary constituent of gas giant planets. Our conservative upper limit on the line-of-sight H2 column density is 1.7 × 10 19 cm, which is...
متن کاملMass and Temperature of the Twa 7 Debris Disk
We present photometric detections of dust emission at 850 and 450 μm around the pre-main sequence M1 dwarf TWA 7 using the SCUBA camera on the James Clerk Maxwell Telescope. These data confirm the presence of a cold dust disk around TWA 7, a member of the TW Hydrae Association. Based on the 850 μm flux, we estimate the mass of the disk to be 18 Mlunar (0.2 M⊕) assuming a mass opacity of 1.7 cm ...
متن کاملThe Dynamical Influence of a Planet at Semimajor Axis 3.4 Au on the Dust around Eridani
Precise Doppler experiments suggest that a massive (m sin i 1⁄4 0:86MJ) planet orbits at semimajor axis a 1⁄4 3:4 AU around Eri, a nearby star with a massive debris disk. The dynamical perturbations from such a planet would mold the distribution of dust around this star. We numerically integrated the orbits of dust grains in this system to predict the central dust-cloud structure. For a supply ...
متن کاملSubstructure in the circumstellar disk around the young star AU Microscopii.
Keck adaptive optics imaging with a physical resolution of 0.4 astronomical units (AU) resolves the inner (15 to 80 AU) disk of AU Microscopii (AU Mic, GJ 803, HD 197481), the nearest known scattered light disk to Earth. The inner disk is asymmetric and possesses a sharp change in structure at 35 AU. The disk also shows spatially localized enhancements and deficits at 25- to 40-AU separations. ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید
ثبت ناماگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید
ورودعنوان ژورنال:
- Science
دوره 303 5666 شماره
صفحات -
تاریخ انتشار 2004