The increasing number of Extrasolar planets observed in the last years makes important to define, as soon as possible, a mass – radius relationship, and so, we adjusted an planetary constitution independent experimental equation. Using the latest database of Extrasolar planets, a bi-logarithmic graphic was plotted that represents the mass - radius relationship where we adjusted a polynomial equation, which better suited the sample of Extrasolar planets at current time
Context. The radius of an exoplanet may be affected by various factors, including irradiation receiv...
Astronomik cisimlerin en önemli salt parametrelerinden ikisi kütle ve yarıçaptır. Giderek artan yeni...
Context. The research of extrasolar planets has entered an era in which we characterize ex...
The masses and radii of exoplanets are fundamental quantities needed for their characterisation. Stu...
The masses and radii of exoplanets are fundamental quantities needed for their characterisation. Stu...
Transit observations, and radial velocity measurements, have begun to populate the mass radius diagr...
Context. Mass and radius are two fundamental properties for characterising exoplanets, but only for ...
Today, with the large number of detected exoplanets and improved measurements, we can reach the next...
Thanks to CoRoT and Kepler space telescope, the thousand of exoplanets have been discovered. Th...
In many cases, astronomers can measure the radius of a planet, but not its mass. Our models of Earth...
For planets other than Earth, particularly exoplanets, interpretation of the composition and structu...
Transiting planet surveys like Kepler have provided a wealth of information on the distribution of p...
International audienceMost transit exoplanets (85%) were discovered with the Kepler space telescope....
Context. Planet formation theory suggests that planet bulk compositions are likely to reflect the ch...
We employ planetary evolution modeling to reproduce the MR distribution of the 198 so far detected p...
Context. The radius of an exoplanet may be affected by various factors, including irradiation receiv...
Astronomik cisimlerin en önemli salt parametrelerinden ikisi kütle ve yarıçaptır. Giderek artan yeni...
Context. The research of extrasolar planets has entered an era in which we characterize ex...
The masses and radii of exoplanets are fundamental quantities needed for their characterisation. Stu...
The masses and radii of exoplanets are fundamental quantities needed for their characterisation. Stu...
Transit observations, and radial velocity measurements, have begun to populate the mass radius diagr...
Context. Mass and radius are two fundamental properties for characterising exoplanets, but only for ...
Today, with the large number of detected exoplanets and improved measurements, we can reach the next...
Thanks to CoRoT and Kepler space telescope, the thousand of exoplanets have been discovered. Th...
In many cases, astronomers can measure the radius of a planet, but not its mass. Our models of Earth...
For planets other than Earth, particularly exoplanets, interpretation of the composition and structu...
Transiting planet surveys like Kepler have provided a wealth of information on the distribution of p...
International audienceMost transit exoplanets (85%) were discovered with the Kepler space telescope....
Context. Planet formation theory suggests that planet bulk compositions are likely to reflect the ch...
We employ planetary evolution modeling to reproduce the MR distribution of the 198 so far detected p...
Context. The radius of an exoplanet may be affected by various factors, including irradiation receiv...
Astronomik cisimlerin en önemli salt parametrelerinden ikisi kütle ve yarıçaptır. Giderek artan yeni...
Context. The research of extrasolar planets has entered an era in which we characterize ex...