Works matching Planets
Results: 5000
How the presence of a giant planet affects the outcome of terrestrial planet formation simulations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202349043
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Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities: No excess of cold Jupiters in small planet systems.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202346211
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Solid tidal friction in multi-layer planets: Application to Earth, Venus, a Super Earth and the TRAPPIST-1 planets: Potential approximation of a multi-layer planet as a homogeneous body.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 644, p. N.PAG, doi. 10.1051/0004-6361/202038204
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Connecting planet formation and astrochemistry: C/Os and N/Os of warm giant planets and Jupiter analogues.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038767
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Formation of terrestrial planets in eccentric and inclined giant planet systems.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 613, p. 1, doi. 10.1051/0004-6361/201731260
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Magnetic energy fluxes in sub-Alfvénic planet star and moon planet interactions.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 552, n. 2, p. A119, doi. 10.1051/0004-6361/201118179
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Debris disks as signposts of terrestrial planet formation II. Dependence of exoplanet architectures on giant planet and disk properties.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 541, p. 1, doi. 10.1051/0004-6361/201117049
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Interaction of free-floating planets with a star-planet pair.
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- Celestial Mechanics & Dynamical Astronomy, 2012, v. 113, n. 4, p. 387, doi. 10.1007/s10569-012-9429-8
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Orbital stability of systems of closely-spaced planets, II: configurations with coorbital planets.
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- Celestial Mechanics & Dynamical Astronomy, 2010, v. 107, n. 4, p. 487, doi. 10.1007/s10569-010-9288-0
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PLANET TOPERS: Planets, Tracing the Transfer, Origin, Preservation, and Evolution of their ReservoirS.
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- Origins of Life & Evolution of the Biosphere, 2016, v. 46, n. 4, p. 369, doi. 10.1007/s11084-016-9488-z
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Self-consistent N-body simulation of planetesimal-driven migration. I. The trajectories of single planets in the uniform background.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 6, p. 1309, doi. 10.1093/pasj/psae090
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Analytical series representing the DE431 ephemerides of the outer planets.
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- Journal of Infectious Diseases, 2017, v. 466, n. 3, p. 2675, doi. 10.1093/mnras/stw3258
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The formation of a gas giant planet in a viscously evolved protoplanetary disk within the core accretion model.
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- Astrophysics & Space Science, 2018, v. 363, n. 9, p. 1, doi. 10.1007/s10509-018-3406-y
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The ultimate cataclysm: the orbital (in)stability of terrestrial planets in exoplanet systems including planets in binaries.
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- International Journal of Astrobiology, 2009, v. 8, n. 3, p. 175, doi. 10.1017/S1473550409990164
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On the relationship of long-period comets to known and unknown planets.
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- Astronomy Letters, 2007, v. 33, n. 8, p. 562, doi. 10.1134/S1063773707080075
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Uranus and Neptune are key to understand planets with hydrogen atmospheres.
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- Experimental Astronomy, 2022, v. 54, n. 2/3, p. 1027, doi. 10.1007/s10686-021-09812-x
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Formation of the Outer Planets.
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- Space Science Reviews, 2005, v. 116, n. 1/2, p. 11, doi. 10.1007/s11214-005-1945-3
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Primordial Planets Predominantly of Dark Matter.
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- Earth, Moon & Planets, 2019, v. 122, n. 3/4, p. 115, doi. 10.1007/s11038-019-09525-4
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Explained in 60 Seconds: Why is Pluto not a Planet?
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- Communicating Astronomy with the Public Journal, 2015, n. 18, p. 4
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The Detection and Characterization of Extrasolar Planets.
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- Challenges (20781547), 2014, v. 5, n. 2, p. 296, doi. 10.3390/challe5020296
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Interior and Evolution of the Giant Planets.
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- Remote Sensing, 2023, v. 15, n. 3, p. 681, doi. 10.3390/rs15030681
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Observability of ultraviolet Ni lines in the atmosphere of transiting Earth‐like planets.
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- Astronomische Nachrichten, 2020, v. 341, n. 9, p. 879, doi. 10.1002/asna.202013842
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Probabilities of Collisions of Planetesimals from Different Regions of the Feeding Zone of the Terrestrial Planets with the Forming Planets and the Moon.
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- Solar System Research, 2019, v. 53, n. 5, p. 332, doi. 10.1134/S0038094619050046
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Homogeneous planet masses: I. Reanalysis of archival HARPS radial velocities.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2025, v. 693, p. 1, doi. 10.1051/0004-6361/202452127
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Evolution of gas envelopes and outgassed atmospheres of rocky planets that formed via pebble accretion.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451114
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Constraints on the formation history and composition of Kepler planets from their distribution of orbital period ratios.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449371
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Tidal evolution of Earth-like planets in the habitable zone of low-mass stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202348450
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Planets similar in size are often dissimilar in interior.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202347049
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Forming giant planets around late-M dwarfs: Pebble accretion and planet–planet collision.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202347664
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TOI-1416: A system with a super-Earth planet with a 1.07 d period.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202346370
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Sublimation of refractory minerals in the gas envelopes of accreting rocky planets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202245636
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Spin evolution of Venus-like planets subjected to gravitational and thermal tides.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 674, p. 1, doi. 10.1051/0004-6361/202245790
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Migration of pairs of giant planets in low-viscosity discs.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 672, p. 1, doi. 10.1051/0004-6361/202245208
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Anatomy of rocky planets formed by rapid pebble accretion: III. Partitioning of volatiles between planetary core, mantle, and atmosphere.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202142143
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Anatomy of rocky planets formed by rapid pebble accretion: II. Differentiation by accretion energy and thermal blanketing.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202142142
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Anatomy of rocky planets formed by rapid pebble accretion: I. How icy pebbles determine the core fraction and FeO contents.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202142141
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The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2022, v. 668, p. 1, doi. 10.1051/0004-6361/202244916
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Alleviating the transit timing variation bias in transit surveys: II. RIVERS: Twin resonant Earth-sized planets around Kepler-1972 recovered from a Kepler false positive.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2022, v. 661, p. 1, doi. 10.1051/0004-6361/202142822
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Constraining the properties of the potential embedded planets in the disk around HD 100546.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2021, v. 656, p. 1, doi. 10.1051/0004-6361/202141998
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Transit timing variation signature of planet migration: the case of K2-24.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 643, p. 1, doi. 10.1051/0004-6361/202039038
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Migration of gap-opening planets in 3D stellar-irradiated accretion disks.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038988
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Pebble drift and planetesimal formation in protoplanetary discs with embedded planets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 635, p. 1, doi. 10.1051/0004-6361/201937037
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Characterization of the L 98-59 multi-planetary system with HARPS: Mass characterization of a hot super-Earth, a sub-Neptune, and a mass upper limit on the third planet.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201935957
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Final spin states of eccentric ocean planets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201935905
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Planet–planet scattering as the source of the highest eccentricity exoplanets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201935744
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Carbon cycling and interior evolution of water-covered plate tectonics and stagnant-lid planets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201935091
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Formation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201834229
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NGTS-5b: a highly inflated planet offering insights into the sub-Jovian desert.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 625, p. N.PAG, doi. 10.1051/0004-6361/201935206
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Influence of general-relativity effects, dynamical tides, and collisions on planet–planet scattering close to the star.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 625, p. N.PAG, doi. 10.1051/0004-6361/201935065
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Planetesimal fragmentation and giant planet formation: II. Dependencies with planetesimal relative velocities and compositions.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 625, p. N.PAG, doi. 10.1051/0004-6361/201834168
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