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Doppler imaging
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Evaporation
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Grain size and shape
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Planet and satellite: gaseous planet
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Planet-disk interactions
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Planet-star interactions
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Population synthesis
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Protoplanetary disks
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Stellar cluster
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Symplectic methods
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astronomical instrumentation
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hydrodynamics
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planet-disc interactions
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planet-star interactions
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planetary science
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planets and satellites: detections
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planets and satellites: gaseous planets
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protoplanetary discs
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telescopes
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101Published 2013“... is enhanced by gravitational focusing for giant planet satellites. In addition, impacts of interplanetary dust...”
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Doctoral Thesis -
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103
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104by Moraes, Ricardo Aparecido de [UNESP]“... of satellites formation in the low velocities regions close to the Roche lobe of a giant planet. As described...”
Published 2014
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105by J. M. Herndon“...) Composition of the Earth's inner core; (2) Giant planet internal energy production; (3) Physical impossibility...”
Published 2010-04-01
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106by Lin, Min-Kai“...Protoplanetary discs can be dynamically unstable due to structure induced by an embedded giant...”
Published 2012
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107by Quintana, Elisa V., Rowe, Jason F., Barclay, Thomas, Howell, Steve B., Ciardi, David R., Demory, Brice-Olivier, Caldwell, Douglas A., Borucki, William J., Christiansen, Jessie L., Jenkins, Jon M., Klaus, Todd C., Fulton, Benjamin J., Morris, Robert L., Sanderfer, Dwight T., Shporer, Avi, Smith, Jeffrey C., Still, Martin, Thompson, Susan E.Get fulltext
Published 2015
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108
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109by Lehmann, H., Borkovits, T., Ngo, H., Mawet, D., Csizmadia, Sz, Rappaport, Saul A., Forgacs-Dajka, E.Get fulltext
Published 2016
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110“...Abstract The weather layers of the gas giant planets, Jupiter and Saturn, comprise the shallow...”
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111by Lyra, Wladimir“... that in disks that already formed a giant planet, solid matter accumulates on the edges of the gap the planet...”
Published 2009
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Doctoral Thesis -
112The Effect of Clouds as an Additional Opacity Source on the Inferred Metallicity of Giant Exoplanets“.... Uncertainty in a giant planet’s thermal state contributes to the uncertainty in the inferred abundance...”
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113by Baldwin, Emily Clare“... produced by the hypervelocity impact of cosmic dust observed on lunar return samples, to the giant planet...”
Published 2008
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114by Husnoo, Mohammad Nawal“... period orbits, given that gas-giant planet building is supposed to take place beyond the ice-line...”
Published 2013
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115“... deposition of material for giant planet cores occurs well beyond the snow line....”
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117by Yu, Liang, Gillon, Michaël, Albrecht, Simon, Bieryla, Allyson, Dai, Fei, Delrez, Laetitia, Hillenbrand, Lynne, Holman, Matthew J., Howard, Andrew W., Huang, Chelsea X., Isaacson, Howard, Jehin, Emmanuel, Lendl, Monika, Montet, Benjamin T., Muirhead, Philip S., Sanchis-Ojeda, Roberto, Winn, Joshua Nathan, Triaud, Amaury, Rappaport, Saul AGet fulltext
Published 2016
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119by A. P. Vidmachenko“... perturbations of the outer giant planets more than 4 billion years ago. The objects of the scattered disk...”
Published 2017-12-01
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120by Dawson, Rebekah Ilene“... of upheaval, during which giant planets "migrated" from where they formed. This thesis addresses a question...”
Published 2013
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