Results 11 to 20 of about 46,765 (196)

Exoplanet interiors and habitability [PDF]

open access: yesAdvances in Physics: X, 2019
More than 1000 exoplanets with a radius smaller than twice that of the Earth are currently known, mainly thanks to space missions dedicated to the search of exoplanets.
Tim Van Hoolst   +2 more
doaj   +2 more sources

The EBLM Project—From False Positives to Benchmark Stars and Circumbinary Exoplanets

open access: yesUniverse, 2023
The EBLM project aims to characterise very-low-mass stars that are companions to solar-type stars in eclipsing binaries. We describe the history and motivation for this project, the methodology we use to obtain the precise mass, radius, and effective ...
Pierre F. L. Maxted   +2 more
doaj   +1 more source

Imaging low-mass planets within the habitable zone of α Centauri

open access: yesNature Communications, 2021
Imaging of low-mass exoplanets can be achieved once the thermal background in the mid-infrared (MIR) wavelengths can be mitigated. Here, the authors present a ground-based MIR observing approach enabling imaging low-mass temperate exoplanets around ...
K. Wagner   +41 more
doaj   +1 more source

Heavy Metal Rules. I. Exoplanet Incidence and Metallicity

open access: yesGeosciences, 2019
The discovery of only a handful of exoplanets required establishing a correlation between giant planet occurrence and metallicity of their host stars.
Vardan Adibekyan
doaj   +1 more source

Robo-AO and SOAR High-Resolution Surveys of Exoplanet Hosting Stars

open access: yesFrontiers in Astronomy and Space Sciences, 2021
In the past decade, space-based transit surveys have delivered thousands of potential planet-hosting systems. Each of these needs to be vetted and characterized using follow-up high-resolution imaging.
Carl Ziegler   +4 more
doaj   +1 more source

Mapping Exoplanets

open access: yes, 2020
The varied surfaces and atmospheres of planets make them interesting places to live, explore, and study from afar. Unfortunately, the great distance to exoplanets makes it impossible to resolve their disk with current or near-term technology. It is still
A Shporer   +91 more
core   +1 more source

Investigation of Kepler Objects of Interest Stellar Parameters from Observed Transit Durations [PDF]

open access: yes, 2013
The Kepler mission discovery of candidate transiting exoplanets (KOIs) enables a plethora of ensemble analysis of the architecture and properties of exoplanetary systems.
Bilinski, Christopher   +2 more
core   +2 more sources

Relationship between Luminosity, Irradiance and Temperature of star on the orbital parameters of exoplanets

open access: yesEPJ Web of Conferences, 2013
For 759 exoplanets detected by radial velocities method we found that distances of exoplanets from central star comply in general Schmidt law and these distances depend on the stellar surface temperature.
Pavel Pintr
doaj   +1 more source

Follow-Up and Validation of K2 and TESS Planetary Systems With Keck NIRC2 Adaptive Optics Imaging

open access: yesFrontiers in Astronomy and Space Sciences, 2021
High resolution imaging (HRI) is a critical part of the transiting exoplanet follow-up and validation process. HRI allows previously unresolved stellar companions and background blends to be resolved, vetting false positive signals and improving the ...
Joshua E. Schlieder   +9 more
doaj   +1 more source

Muons, mutations, and planetary shielding

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Life on earth is protected from astrophysical cosmic rays by the heliospheric magnetic and slowly varying geomagnetic fields, and by collisions with oxygen and nitrogen molecules in the atmosphere.
Piet C. de Groen
doaj   +1 more source

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