Works matching Jupiter (Planet)
Results: 1222
Small impacts on the giant planet Jupiter.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 617, p. N.PAG, doi. 10.1051/0004-6361/201832689
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Hot Jupiters from secular planet-planet interactions.
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- Nature, 2011, v. 473, n. 7346, p. 187, doi. 10.1038/nature10076
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Can an Earth‐mass planet exist between Jupiter and Saturn? A numerical experiment.
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- Astronomische Nachrichten, 2023, v. 344, n. 3, p. 1, doi. 10.1002/asna.20220077
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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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An orbital period of 0.94 days for the hot-Jupiter planet WASP-18b.
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- Nature, 2009, v. 460, n. 7259, p. 1098, doi. 10.1038/nature08245
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The planet Jupiter.
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- Astronomy & Astrophysics Review, 1999, v. 9, n. 3/4
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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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Luminosity of young Jupiters revisited Massive cores make hot planets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 558, p. 1, doi. 10.1051/0004-6361/201321617
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CFBDSIR2149-0403: a 4-7 Jupiter-mass free-floating planet in the young moving group AB Doradus?
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 548, p. 1, doi. 10.1051/0004-6361/201219984
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The future of Jupiter-like planets around Sun-like stars: first steps.
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- Proceedings of the International Astronomical Union, 2021, v. 17, n. S5370, p. 275, doi. 10.1017/S1743921322003696
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Semi-Analytical Search for Sun-Synchronous and Planet Synchronous Orbits around Jupiter, Saturn, Uranus and Neptune.
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- Mathematics (2227-7390), 2022, v. 10, n. 15, p. 2684, doi. 10.3390/math10152684
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Predictions on the core mass of Jupiter and of giant planets in general.
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- Astrophysics & Space Science, 2011, v. 336, n. 1, p. 47, doi. 10.1007/s10509-011-0672-3
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OBERVATIONAL COMPLETION LIMIT OF MINOR PLANETS FROM THE ASTEROID BELT TO JUPITER TROJANS.
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- LPI Contribution, 2021, p. 1
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E. W. L. Ryves and the planet Jupiter.
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- Journal of the British Astronomical Association, 2017, v. 127, n. 5, p. 306
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The orbital evolution of the Sun–Jupiter–Saturn–Uranus–Neptune system on long time scales.
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- Astrophysics & Space Science, 2020, v. 365, n. 8, p. N.PAG, doi. 10.1007/s10509-020-03855-w
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Origin of "Bursts in Absorption" in the Jovian Decameter Radio Emission.
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- Astronomy Letters, 2024, v. 50, n. 6, p. 420, doi. 10.1134/S1063773724700257
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The Spatial Variation of Water Clouds, NH 3 , and H 2 O on Jupiter Using Keck Data at 5 Microns.
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- Remote Sensing, 2022, v. 14, n. 18, p. N.PAG, doi. 10.3390/rs14184567
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Cloud reflection modelling for impact flashes on Jupiter: A new constraint on the bulk properties of the impact objects.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202346837
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Empirical models of Jupiter's interior from Juno data Moment of inertia and tidal Love number k<sub>2</sub>.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 613, p. 1, doi. 10.1051/0004-6361/201732183
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Astrometric positions for 18 irregular satellites of giant planets from 23 years of observations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 580, p. 1, doi. 10.1051/0004-6361/201526273
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Grain opacity and the bulk composition of extrasolar planets.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 572, p. 1, doi. 10.1051/0004-6361/201423702
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Impact flux on Jupiter: From superbolides to large-scale collisions.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 560, p. 1, doi. 10.1051/0004-6361/201322216
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The occultation of HIP 107302 by Jupiter.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 556, n. 6, p. 1, doi. 10.1051/0004-6361/201321811
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Close encounters of a rotating star with planets in parabolic orbits of varying inclination and the formation of hot Jupiters.
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- Celestial Mechanics & Dynamical Astronomy, 2011, v. 111, n. 1/2, p. 51, doi. 10.1007/s10569-011-9367-x
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Close encounters of a rotating star with planets in parabolic orbits of varying inclination and the formation of hot Jupiters.
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- Celestial Mechanics & Dynamical Astronomy, 2011, v. 111, n. 1/2, p. 51, doi. 10.1007/s10569-011-9367-x
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On the Precession of Saturn.
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- Cosmic Research, 2018, v. 56, n. 4, p. 306, doi. 10.1134/S0010952518040019
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Extrasolar planets: Larger than they ought to be.
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- Nature, 2010, v. 465, n. 7296, p. 300, doi. 10.1038/465300a
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sky sights.
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- Mercury, 2014, v. 43, n. 4, p. 55
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Into Thick Air.
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- Mercury, 2002, v. 31, n. 1, p. 24
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On a collision course with Jupiter.
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- Mercury, 1993, v. 22, n. 6, p. 15
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Heavy Metal Rules. I. Exoplanet Incidence and Metallicity.
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- Geosciences (2076-3263), 2019, v. 9, n. 3, p. 105, doi. 10.3390/geosciences9030105
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Dynamo Simulations of Jupiter's Magnetic Field: The Role of Stable Stratification and a Dilute Core.
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- Journal of Geophysical Research. Planets, 2022, v. 127, n. 11, p. 1, doi. 10.1029/2022JE007479
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Dynamo Action in the Steeply Decaying Conductivity Region of Jupiter‐Like Dynamo Models.
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- Journal of Geophysical Research. Planets, 2019, v. 124, n. 3, p. 837, doi. 10.1029/2018JE005759
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Jupiter - friend or foe? III: the Oort cloud comets.
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- International Journal of Astrobiology, 2010, v. 9, n. 1, p. 1, doi. 10.1017/S1473550409990346
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Magnetic Reconnection Near the Planet as a Possible Driver of Jupiter's Mysterious Polar Auroras.
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- Journal of Geophysical Research. Space Physics, 2021, v. 126, n. 8, p. 1, doi. 10.1029/2021JA029544
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The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 643, p. 1, doi. 10.1051/0004-6361/202038856
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Layered semi-convection and tides in giant planet interiors: II. Tidal dissipation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 626, p. 1, doi. 10.1051/0004-6361/201833674
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Chemical fingerprints of hot Jupiter planet formation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 612, p. 1, doi. 10.1051/0004-6361/201732001
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Effects of an eccentric inner Jupiter on the dynamical evolution of icy body reservoirs in a planetary scattering scenario.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 605, p. 1, doi. 10.1051/0004-6361/201730411
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High-resolution imaging of young M-type stars of the solar neighbourhood: probing for companions down to the mass of Jupiter.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 539, p. 1, doi. 10.1051/0004-6361/201118223
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Water inventory from beyond the Jupiter's orbit to the terrestrial planets and the Moon.
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- Proceedings of the International Astronomical Union, 2018, v. 14, n. S345, p. 164, doi. 10.1017/S1743921319001479
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The Shape of Jupiter and Saturn Based on Atmospheric Dynamics, Radio Occultations and Gravity Measurements.
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- Geophysical Research Letters, 2023, v. 50, n. 6, p. 1, doi. 10.1029/2022GL102321
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Empirically Determined Auroral Electron Events at Mars—MAVEN Observations.
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- Geophysical Research Letters, 2022, v. 49, n. 6, p. 1, doi. 10.1029/2022GL097757
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THE JUPITR EFFECT.
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- Grain Magazine, 2018, v. 45, n. 4, p. 72
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Extraction, displacement, and focus.
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- Linguistics & Philosophy, 2014, v. 37, n. 3, p. 263, doi. 10.1007/s10988-014-9149-5
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What does displacement explain, and what do congruence effects show?
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- Linguistics & Philosophy, 2014, v. 37, n. 3, p. 269, doi. 10.1007/s10988-014-9152-x
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An attempt to build a dynamical catalog of present-day solar system co-orbitals: An attempt to build a dynamical catalog: N. Pan, T. Gallardo.
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- Celestial Mechanics & Dynamical Astronomy, 2025, v. 137, n. 1, p. 1, doi. 10.1007/s10569-024-10234-y
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Charged dust close to outer mean-motion resonances in the heliosphere.
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- Celestial Mechanics & Dynamical Astronomy, 2019, v. 131, n. 11, p. N.PAG, doi. 10.1007/s10569-019-9928-y
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Detection of Earth-mass and super-Earth Trojan planets using transit timing variation method.
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- Celestial Mechanics & Dynamical Astronomy, 2013, v. 117, n. 1, p. 75, doi. 10.1007/s10569-013-9510-y
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The Radiometric and Pointing Calibration of SECCHI COR1 on STEREO.
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- Solar Physics, 2008, v. 250, n. 2, p. 443, doi. 10.1007/s11207-008-9228-2
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