Results 11 to 20 of about 1,099 (180)

Characterization of exoplanets from their formation [PDF]

open access: yesAstronomy and Astrophysics, 2012
A first characterization of many exoplanets has recently been achieved by the observational determination of their radius. For some planets, a measurement of the luminosity has also been possible, with many more directly imaged planets expected in the future.
C. Mordasini   +3 more
openaire   +3 more sources

Collisional formation of massive exomoons of superterrestrial exoplanets [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT Exomoons orbiting terrestrial or superterrestrial exoplanets have not yet been discovered; their possible existence and properties are therefore still an unresolved question. Here, we explore the collisional formation of exomoons through giant planetary impacts. We make use of smooth particle hydrodynamical collision simulations
Uri Malamud   +3 more
openaire   +3 more sources

A Geologic Si‐O‐C Pathway to Incorporate Carbon in Silicates

open access: yesGeophysical Monograph Series, Page 47-54., 2020

This book is Open Access. A digital copy can be downloaded for free from Wiley Online Library.

Explores the behavior of carbon in minerals, melts, and fluids under extreme conditions

Carbon trapped in diamonds and carbonate-bearing rocks in subduction zones are examples of the continuing exchange of substantial carbon ...
Alexandra Navrotsky   +2 more
wiley  

+2 more sources

RESONANCES OF MULTIPLE EXOPLANETS AND IMPLICATIONS FOR THEIR FORMATION [PDF]

open access: yesThe Astrophysical Journal, 2014
5 pages, 5 figures, accepted for publication in ApJ ...
Xiaojia Zhang   +3 more
openaire   +2 more sources

Effect of Laboratory Reagents for Cleaning Modern Contamination on the δ<sup>15</sup>N Integrity of Nitrogen-Poor Samples. [PDF]

open access: yesRapid Commun Mass Spectrom
ABSTRACT Rationale Nitrogen isotope values have been widely used for tracing ancient biogeochemical processes, but contaminant‐sensitive materials, such as Precambrian sedimentary rocks, meteorites, or returned extraterrestrial samples, often have low nitrogen levels and are thus vulnerable to modern organic contamination.
Bubphamanee K, Schauer A, Buick R.
europepmc   +2 more sources

LkCa 15: A YOUNG EXOPLANET CAUGHT AT FORMATION? [PDF]

open access: yesThe Astrophysical Journal, 2011
Young and directly imaged exoplanets offer critical tests of planet-formation models that are not matched by RV surveys of mature stars. These targets have been extremely elusive to date, with no exoplanets younger than 10--20 Myr and only a handful of direct-imaged exoplanets at all ages.
Kraus, Adam L, Ireland, Michael
openaire   +3 more sources

Characterization of exoplanets from their formation [PDF]

open access: yesAstronomy & Astrophysics, 2017
44 pages, 26 figures (journal format). A&A in print.
Mordasini, C.   +2 more
openaire   +2 more sources

Characterization of exoplanets from their formation [PDF]

open access: yesAstronomy and Astrophysics, 2012
The research of exoplanets has entered an era in which we characterize extrasolar planets. This has become possible with measurements of radii and luminosities. Meanwhile, radial velocity surveys discover also very low-mass planets. Uniting all this observational data into one coherent picture to better understand planet formation is an important, but ...
C. Mordasini   +5 more
openaire   +3 more sources

Observational Constraints on the Formation and Evolution of Neptune-Class Exoplanets [PDF]

open access: yesSpace Science Reviews, 2020
21 pages, 6 ...
Deleuil, Magali   +4 more
openaire   +4 more sources

Understanding exoplanet formation, structure and evolution in 2010 [PDF]

open access: yesProceedings of the International Astronomical Union, 2010
AbstractIn this short review, we summarize our present understanding (and non-understanding) of exoplanet formation, structure and evolution, in the light of the most recent discoveries. Recent observations of transiting massive brown dwarfs seem to remarkably confirm the predicted theoretical mass-radius relationship in this domain.
G. Chabrier, J. Leconte, and I. Baraffe
openaire   +2 more sources

Home - About - Disclaimer - Privacy