Planet Detection Capabilities of the Eddington Mission
Eddington is a space mission for extrasolar planet finding and for asteroseismic observations. It has been selected by ESA as
239 indexed results
Eddington is a space mission for extrasolar planet finding and for asteroseismic observations. It has been selected by ESA as
We consider several processes operating during the late stages of planet formation that can affect observed orbital elements. Disk-planet interactions,
Due to their extremely small luminosity compared to the stars they orbit, planets outside our own Solar System are extraordinarily
A planetary system may undergo significant radial rearrangement during the early part of its lifetime. Planet migration can come about
Extragalactic astronomy with photons ends at ~0.1 PeV, but we know there are astrophysical sources for seven more decades of
Three transits of the planet orbiting the solar type star HD209458 were observed in the far UV at the wavelength
We present an overview of our ongoing systematic search for wide (sub)stellar companions around the stars known to host rad-vel
Most young low-mass stars are born as binary systems, and circumstellar disks have recently been observed around the individual components
The N2K consortium is carrying out a distributed observing campaign with the Keck, Magellan and Subaru telescopes, as well as
We are setting up a new search for transiting extrasolar planets using the 0.5m Automated Patrol Telescope at Siding Spring
We have measured radial velocities of a star, OGLE-TR-56, which shows a 1.2-day transit-like light curve found photometrically by Udalski
We report the detection of a low-mass companion orbiting the solar-type star HD178911B, the distant component of the stellar triple
A 4MJ planet with a 15.8day orbital period has been detected from very precise radial velocity measurements with the CORALIE
The core-accretion mechanism for gas giant formation may be too slow to create all observed gas giant planets during reasonable
The quest for life in the Universe is often affected by the free use of extrapolations of our phenomenological geocentric
The past five years has seen a surge in research and innovative ideas for the imaging of extrasolar planets, particular
How do planets form from circumstellar disks of gas and dust? What physical processes are responsible for determining the final
Over two hundred years ago Capt. James Cook sailed up Whitsunday Passage, just a few miles where we now sit,
We present the chemical analysis of a new set of stars known to harbor low mass companions, namely HD 1237,
The Space Interferometry Mission (SIM) will make precise astrometric measurements that can be used to detect planets around nearby stars.
The dust disk around Beta Pic must be produced by collision or by evaporation of orbiting Kuiper belt-like objects. Here
I attempt to piece together a consistent scenario based on current estimates of the evolution of the star formation rate
We report the first detection of a planetary transit by spectroscopic measurements. We have detected the distortion of the stellar
We explore here the idea, reminiscent in some respect of Von Weizsacker's (1944) and Alfven's (1976) outmoded cosmogonies, that long-lived