Are WASP-107-like Systems Consistent with High-eccentricity Migration?
WASP-107 b seems to be a poster child of the long-suspected high-eccentricity migration scenario. It is on a 5.7 day, polar orbit. The planet is Jupiter-like in radius but Neptune-like in mass with exceptionally low density.
Hang Yu, Fei Dai
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The discovery of exoplanets: towards understanding planet formation
Abstract The discovery of exoplanets has opened a new, very rich field in modern astronomy, allowing a much better insight into the characteristics of planets and the mechanisms for their formation than possible from only the observation of the Solar System.
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The case for a rectangular format space telescope for finding exoplanets
We suggest that rectangular primary-mirror telescopes provide a clearer path to discovering habitable worlds than other designs currently being pursued. We show that a simple infrared (λ∼10 μm) telescope design with a rectangular mirror 20 m in length and 1 m in width, combined with technology already developed for JWST, can discover ∼11 habitable ...
Heidi Jo Newberg +6 more
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No Strong Associations between Eccentricity and Orbital Architecture in Kepler Compact Multis
The dynamical history of a planetary system is recorded in the present day architecture of its constituent planets’ sizes, orbital periods, and eccentricities.
Gregory J. Gilbert +2 more
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TOWARD THE FORMATION OF CARBONACEOUS REFRACTORY MATTER IN HIGH TEMPERATURE HYDROCARBON-RICH ATMOSPHERES OF EXOPLANETS UPON MICROMETEOROID IMPACT [PDF]
Beni B. Dangi +4 more
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Characterization of exoplanets from their formation II. The planetary mass-radius relationship [PDF]
C. Mordasini +5 more
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The accretion of material from disks onto weakly magnetized objects invariably involves its traversal through a material surface, known as the boundary layer (BL).
Zhihao Fu, Shunquan Huang, Cong Yu
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Understanding the Planetary Formation and Evolution in Star Clusters (UPiC). I. Evidence of Hot Giant Exoplanets Formation Timescales [PDF]
Yuan-Zhe Dai +3 more
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Understanding the orbits of giant planets is critical for testing planet formation models, particularly at wide separations (>10 au) where traditional core accretion becomes inefficient.
Vidya Venkatesan +101 more
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Magma Ocean Interactions Can Explain JWST Observations of the Sub-Neptune TOI-270 d
Sub-Neptunes with substantial atmospheres may possess magma oceans in contact with the overlying gas, with chemical interactions between the atmosphere and magma playing an important role in shaping atmospheric composition.
Matthew C. Nixon +11 more
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