A tidally-locked planet in its orbit around a star keeps the same face towards the star. This happens when the rotation period of the planet around its own axis becomes […]
extrasolar
On the Abundance of Circumbinary Planets
Circumbinary planets have been the subject of much recent work, providing both simulations and new discoveries. We present the first observationally based determination of the rate of occurrence of these […]
Some inconvenient truths about biosignatures involving two chemical species on Earth-like exoplanets
The detection of strong thermochemical disequilibrium in the atmosphere of an extrasolar planet is thought to be a potential biosignature. In this article we present a new kind of false […]
Prospects for Detecting Oxygen, Water, and Chlorophyll in an Exo-Earth
The goal of finding and characterizing nearby Earth-like planets is driving many NASA high-contrast flagship mission concepts, the latest of which is known as the Advanced Technology Large-Aperture Space Telescope […]
Strong Dependence of the Inner Edge of the Habitable Zone on Planetary Rotation Rate
Planetary rotation rate is a key parameter in determining atmospheric circulation and hence the spatial pattern of clouds. Since clouds can exert a dominant control on planetary radiation balance, rotation […]
Habitable Zones Around Main-Sequence Stars: Dependence on Planetary Mass
The ongoing discoveries of extrasolar planets are unveiling a wide range of terrestrial mass (size) planets around their host stars. In this letter, we present estimates of habitable zones (HZs) […]
N-body Simulations of Terrestrial Planet Formation under the Influence of a Hot Jupiter
We investigate the formation of multiple-planet systems in the presence of a hot Jupiter using extended N-body simulations that are performed simultaneously with semi-analytic calculations. Our primary aims are to […]
Earth-like Habitats in Planetary Systems
Understanding the concept of habitability is related to an evolutionary knowledge of the particular planet-in-question. Additional indications so-called “systemic aspects” of the planetary system as a whole governs a particular […]
Formation, Tidal Evolution and Habitability of the Kepler-186 System
The Kepler-186 system consists of five planets orbiting an early-M dwarf. The planets have physical radii of 1.0-1.50 R⊕ and orbital periods of 4 to 130 days. The 1.1 R⊕ Kepler-186f […]
New Rocky Planet May Have Liquid Water
San Francisco State University astronomer Stephen Kane and an international team of researchers have announced the discovery of a new rocky planet that could potentially have liquid water on its […]
