Formation and detection of Earth mass planets around low mass stars

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Formation and Detection of Earth Mass Planets around Low Mass Stars

We investigate an in-situ formation scenario for Earth-mass terrestrial planets in short-period, potentially habitable orbits around low-mass stars (M∗ < 0.3M⊙). We then investigate the feasibility of detecting these Earth-sized planets. We find that such objects can feasibly be detected by a ground-based transit survey if their formation frequency is high and if correlated noise can be control...

متن کامل

Detecting Planets around Very Low Mass Stars with the Radial Velocity Method

The detection of planets around very low-mass stars with the radial velocity method is hampered by the fact that these stars are very faint at optical wavelengths where the most high-precision spectrometers operate. We investigate the precision that can be achieved in radial velocity measurements of low mass stars in the near infrared (nIR) Y -, J-, and H-bands, and we compare it to the precisi...

متن کامل

Induced Formation of Primordial Low-Mass Stars

We show that the explosion of the first pair-unstable supernovae can trigger lowmass star formation via gravitational fragmentation of the supernova-driven gas shell. The necessary conditions for such instability are: (i) the mean density of the ambient medium is 14 cm < n0 < 790 cm ; (ii) the explosion energy ESN > 3 × 10 52 erg (i.e. core-collapse supernovae are not suitable triggers). The ty...

متن کامل

Spectral fingerprints of Earth-like planets around FGK stars.

We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK stars with effective temperatures ranging from Teff=4250 K to Teff=7000 K in 250 K intervals. We have modeled the remotely detectable spectra of Earth-like planets for clear and cloudy atmospheres at the 1 AU equivalent distance from the VIS to IR (0.4 to 20 μm) to compare detectability of featur...

متن کامل

Mass loss and dust formation around oxygen - rich evolved stars

Infrared spectra of a number of evolved O-rich stars have been obtained with the Short and Long Wavelength spectrometers on board the Infrared Space Observatory. The very broad wavelength coverage (2.4–197μm) obtained by combining observations made with the two spectrometers includes practically all of the flux emitted by the sources, and allows us to determine the emission and absorption featu...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Icarus

سال: 2009

ISSN: 0019-1035

DOI: 10.1016/j.icarus.2009.02.035