Results 171 to 180 of about 828 (196)

Io's tidal response precludes a shallow magma ocean. [PDF]

Nature
Park RS, Jacobson RA, Gomez Casajus L, Nimmo F, Ermakov AI, Keane JT, McKinnon WB, Stevenson DJ, Akiba R, Idini B, Buccino DR, Magnanini A, Parisi M, Tortora P, Zannoni M, Mura A, Durante D, Iess L, Connerney JEP, Levin SM, Bolton SJ.   +20 more
europepmc   +1 more source

Understanding the Formation of Saturn's Regular Moons in the Context of Giant Planet Moons Formation Scenarios. [PDF]

Space Sci Rev
Blanc M, Crida A, Shibaike Y, Charnoz S, El Moutamid M, Estrada P, Mousis O, Salmon J, Schneeberger A, Vernazza P.   +9 more
europepmc   +1 more source

Structural evolution of liquid silicates under conditions in Super-Earth interiors. [PDF]

Nat Commun
Morard G, Hernandez JA, Pege C, Nagy C, Libon L, Lacquement A, Sokaras D, Lee HJ, Galtier E, Heimann P, Cunningham E, Glenzer SH, Vinci T, Prescher C, Boccato S, Chantel J, Merkel S, Zhang Y, Yang H, Wei X, Pandolfi S, Mao WL, Gleason AE, Shim SH, Alonso-Mori R, Ravasio A.   +25 more
europepmc   +1 more source

The importance of carbonatite lavas in outgassing Venus' modern-day atmosphere. [PDF]

Sci Adv
Trussell AR, O'Rourke JG, Williams DA, Flynn ITW, Black BA, Borrelli ME.   +5 more
europepmc   +1 more source

Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky

Gilbert E, Burt J, Barragán O, Siegel J, Mascareño AS, Silva A, Luque R, Rogers J, Lee E, Lopez E, Vanderburg A, Clement M, Youngblood A, Mamajek E, Sousa S, Cameron AC, Rodriguez J, Martin D, Arney G, Barclay T, Becker J, Colon K, Eisner N, Halverson S, Hord B, Kane S, Kreidberg L, Morley C, Mortier A, Nielsen L, Quintana E, Schlieder J, Suissa G, Triaud A, Trifonov T, Eylen VV.   +35 more
europepmc   +1 more source

The Exoplanet Orbit Database [PDF]

Publications of the Astronomical Society of the Pacific, 2011
We present a database of well-determined orbital parameters of exoplanets, and their host stars’ properties. This database comprises spectroscopic orbital elements measured for 427 planets orbiting 363 stars from radial velocity and transit measurements ...
Nikolai Piskunov, Andrew Howard
exaly   +5 more sources

Exoplanet demographics: Physical and orbital properties [PDF]

The discovery of over 5700 exoplanets has led to a boom in the field of exoplanet demographics over the past decade. Led by swaths of exoplanet discoveries from NASA\u27s Kepler space mission, astronomers have been conducting statistical studies of the ...
Ryan Cloutier
exaly   +2 more sources

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Close-Orbiting Exoplanets: Formation, Migration Mechanisms and Properties

2008
The discovery of a signal from a putative extra-solar planet around the nearby Sun-like star 51 Peg by Mayor & Queloz and the rapid confirmation by Marcy & Butler was the main starting point for the field of extrasolar planets. More than a decade later, ‘51 Peg - type planets’ or ‘hot Jupiters’ are frequently discovered and characterised by a variety ...
Hugh R. A. Jones, James S. Jenkins, John R. Barnes   +2 more
openaire   +1 more source

Formation and Migration Histories of Giant Exoplanets in Multi-stellar Systems

2017
The first planets discovered outside of our solar system were very different from the solar system planets. These discoveries raised new challenges to planet formation models, which were designed to explain the origin of the solar system planets. One particularly intriguing population, the "hot Jupiters" were some of the first planets discovered. These
openaire   +1 more source

Exoplanets in Open Clusters and Binaries: New Constraints on Planetary Migration

2016
In this dissertation, we present three complementary studies of the processes that drive planetary migration. The first is a radial-velocity survey in search of giant planets in adolescent (Gyr) open clusters. While several different mechanisms may act to drive giant planets inward, only some mechanisms will excite high eccentricities while doing so ...
openaire   +1 more source