Extrasolar Planets


Circumbinary Exoplanets And Brown Dwarfs With LISA

Circumbinary Exoplanets And Brown Dwarfs With LISA

We explore here the prospects for detection of both giant circumbinary exoplanets, and brown dwarfs orbiting Galactic double white dwarfs binaries (DWDs) with the LISA mission.


Wavefront Error Tolerancing For Direct Imaging Of Exo-Earths With A Large Segmented Telescope In Space

Wavefront Error Tolerancing For Direct Imaging Of Exo-Earths With A Large Segmented Telescope In Space

Direct imaging of exo-Earths and search for life is one of the most exciting and challenging objectives for future space observatories.


A Virtual Planet Simulator for Modeling Distant Worlds Across Time

A Virtual Planet Simulator for Modeling Distant Worlds Across Time

University of Washington astrobiologist Rory Barnes has created software that simulates multiple aspects of planetary evolution across billions of years, with an eye toward finding and studying potentially habitable worlds.


Energy Budgets for Terrestrial Extrasolar Planets

Energy Budgets for Terrestrial Extrasolar Planets

The pathways through which incoming energy is distributed between the surface and atmosphere has been analyzed for the Earth. However, the effect of the spectral energy distribution of a host star on the energy budget of an orbiting planet may be significant given the wavelength-dependent absorption properties of atmospheric CO2 and water vapor, and surface ice and snow.


An Automated Method to Detect Transiting Circumbinary Planets

An Automated Method to Detect Transiting Circumbinary Planets

To date a dozen transiting "Tatooines" or circumbinary planets (CBPs) have been discovered, by eye, in the data from the Kepler mission; by contrast, thousands of confirmed circumstellar planets orbiting around single stars have been detected using automated algorithms.


How Many Earth-like Planets Are Around Sun-like Stars?

How Many Earth-like Planets Are Around Sun-like Stars?

A new study provides the most accurate estimate of the frequency that planets that are similar to Earth in size and in distance from their host star occur around stars similar to our Sun.


Red Dots: A Temperate 1.5 Earth-mass Planet In A Compact Multi-terrestrial Planet System Around GJ1061

Red Dots: A Temperate 1.5 Earth-mass Planet In A Compact Multi-terrestrial Planet System Around GJ1061

Small low-mass stars are favourable targets for the detection of rocky habitable planets. In particular, planetary systems in the solar neighbourhood are interesting and suitable for precise characterisation. The Red Dots campaigns seek to discover rocky planets orbiting nearby low-mass stars.


Identifying Atmospheres on Rocky Exoplanets Through Inferred High Albedo

Identifying Atmospheres on Rocky Exoplanets Through Inferred High Albedo

The upcoming launch of the James Webb Space Telescope (JWST) means that we will soon have the capability to characterize the atmospheres of rocky exoplanets.


A Scaling Theory for Atmospheric Heat Redistribution on Rocky Exoplanets

A Scaling Theory for Atmospheric Heat Redistribution on Rocky Exoplanets

Atmospheric heat redistribution shapes the remote appearance of rocky exoplanets but there is currently no easy way to predict a planet's heat redistribution from its physical properties.


Two Earth-like Planets Discovered Near Teegarden's Star

Two Earth-like Planets Discovered Near Teegarden's Star

An international research team led by the University of Göttingen has discovered two new Earth-like planets near one of our closest neighboring stars.


Frequency of Planets Orbiting M dwarfs in the Solar Neighbourhood

Frequency of Planets Orbiting M dwarfs in the Solar Neighbourhood

The most abundant stars in the Galaxy, M dwarfs, are very commonly hosts to diverse systems of low-mass planets. Their abundancy implies that the general occurrence rate of planets is dominated by their occurrence rate around such M dwarfs.


Signatures of a Planet-planet Impacts Phase in Exoplanetary Systems Hosting Giant Planets

Signatures of a Planet-planet Impacts Phase in Exoplanetary Systems Hosting Giant Planets

Exoplanetary systems host giant planets on substantially non-circular, close-in orbits.


Exomoons May Be Home To Extraterrestrial Life

Exomoons May Be Home To Extraterrestrial Life

Moons orbiting planets outside our solar system could offer another clue about the pool of worlds that may be home to extra-terrestrial life, according to an astrophysicist at the University of Lincoln.


Characterization of the L 98-59 multi-planetary System with HARPS

Characterization of the L 98-59 multi-planetary System with HARPS

L 98-59 (TIC 307210830, TOI-175) is a nearby M3 dwarf around which TESS revealed three terrestrial-sized transiting planets (0.80, 1.35, 1.57 Earth radii) in a compact configuration with orbital periods shorter than 7.5 days.


Discovery and Characterization of Kepler-36b

Discovery and Characterization of Kepler-36b

We describe the circumstances that led to the discovery of Kepler-36b, and the subsequent characterization of its host planetary system.


Validation of a Temperate Fourth Planet in the K2-133 Multi-planet System

Validation of a Temperate Fourth Planet in the K2-133 Multi-planet System

We present follow-up observations of the K2-133 multi-planet system. Previously, we announced that K2-133 contained three super-Earths orbiting an M1.5V host star - with tentative evidence of a fourth outer-planet orbiting at the edge of the temperate zone.


How to Find a Planet from Transit Variations

How to Find a Planet from Transit Variations

Here we describe a story behind the discovery of Kepler-46, which was the first exoplanetary system detected and characterized from a method known as the transit timing variations (TTVs).


Unexpectedly Strong Effect of Supergranulation on the Detectability of Earth Twins Orbiting Sun-like Stars With Radial Velocities

Unexpectedly Strong Effect of Supergranulation on the Detectability of Earth Twins Orbiting Sun-like Stars With Radial Velocities

Magnetic activity and surface flows at different scales pertub radial velocity measurements.


Life Could Be Evolving Right Now on Nearest Exoplanets

Life Could Be Evolving Right Now on Nearest Exoplanets

Rocky, Earth-like planets orbiting our closest stars could host life, according to a new study that raises the excitement about exoplanets.


Exoplanetary Atmospheres: Key Insights, Challenges and Prospects

Exoplanetary Atmospheres: Key Insights, Challenges and Prospects

Exoplanetary science is on the verge of an unprecedented revolution. The thousands of exoplanets discovered over the past decade have most recently been supplemented by discoveries of potentially habitable planets around nearby low-mass stars.



Top stories from October.