Results 141 to 150 of about 404,312 (236)
Due to the unprecedented signal strengths offered by the newest high-resolution spectrographs on 10 m class telescopes, exploring the 3D nature of exoplanets is possible with an unprecedented level of precision.
Aurora Y. Kesseli+3 more
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The Orbital Geometries and Stellar Obliquities of Exoplanet-Hosting Multi-Star Systems [PDF]
The current orbital geometries of exoplanet systems offer a fossilized record of the systems' dynamical histories. A particularly rich set of dynamical mechanisms is available to exoplanets residing in multi-star systems, which may have their evolution shaped by the gravitational influence of bound stellar companions. In this work, we examine the joint
arxiv
Carving Out the Inner Edge of the Period Ratio Distribution through Giant Impacts
The distribution of orbital period ratios between adjacent observed exoplanets is approximately uniform, but exhibits a strong falloff toward close orbital separations.
Kaitlyn Chen+5 more
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Before the launch of the Kepler Space Telescope, models of low-mass planet formation predicted that convergent type I migration would often produce systems of low-mass planets in low-order mean-motion resonances.
Jacob H. Hamer, Kevin C. Schlaufman
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Observational Signatures of a Previous Dynamical Instability in Multi-planet M-dwarf Systems
We identify observational signatures suggesting a history of dynamical instability in 26 out of 34 M-dwarf multi-planet systems containing no large planets.
Anna C. Childs+4 more
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An Obliquity Measurement of the Hot Neptune TOI-1694b
We present spectral observations of the multiplanet host TOI-1694 during the transit of TOI-1694b, a 26.1 M _⊕ hot Neptune with a 3.77 day orbit. By analyzing radial velocities obtained from the Keck Planet Finder, we modeled the Rossiter–McLaughlin ...
Luke B. Handley+12 more
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The orbital eccentricity distribution of planets orbiting M dwarfs. [PDF]
Sagear S, Ballard S.
europepmc +1 more source
Salty ice and the dilemma of ocean exoplanet habitability. [PDF]
Journaux B.
europepmc +1 more source
Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings. [PDF]
Way MJ+11 more
europepmc +1 more source
A Larger Sample Confirms Small Planets around Hot Stars Are Misaligned
The distribution of stellar obliquities provides critical insight into the formation and evolution pathways of exoplanets. In the past decade, it was found that hot stars hosting hot Jupiters are more likely to have high obliquities than cool stars, but ...
Emma M. Louden+9 more
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