TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned
We report the measurement of the sky-projected obliquity angle λ of the warm Jovian exoplanet TOI-1670 c via the Rossiter–McLaughlin effect. We observed the transit window during UT 2023 April 20 for 7 continuous hours with NEID on the 3.5 m WIYN ...
Jack Lubin +23 more
doaj +1 more source
Observations of Extrasolar Planets During the non-Cryogenic Spitzer Space Telescope Mission [PDF]
Precision infrared photometry from Spitzer has enabled the first direct studies of light from extrasolar planets, via observations at secondary eclipse in transiting systems.
David Charbonneau +7 more
core +2 more sources
Dynamical Mass of the Exoplanet Host Star HR 8799
Abstract HR 8799 is a young A5/F0 star hosting four directly imaged giant planets at wide separations (∼16–78 au), which are undergoing orbital motion and have been continuously monitored with adaptive optics imaging since their discovery over a decade ago. We present a dynamical mass of HR 8799 using 130 epochs of relative astrometry of
Aldo G. Sepulveda, Brendan P. Bowler
openaire +2 more sources
Hydrogen sulfide and metal-enriched atmosphere for a Jupiter-mass exoplanet. [PDF]
As the closest transiting hot Jupiter to Earth, HD 189733b has been the benchmark planet for atmospheric characterization 1,2,3. It has also been the anchor point for much of our theoretical understanding of exoplanet atmospheres from composition 4 ...
Guangwei Fu +17 more
semanticscholar +1 more source
Validating AU Microscopii d with Transit Timing Variations
AU Mic is a young (22 Myr), nearby exoplanetary system that exhibits excess transit timing variations (TTVs) that cannot be accounted for by the two known transiting planets nor stellar activity.
Justin M. Wittrock +33 more
doaj +1 more source
Regular and chaotic orbits in the dynamics of exoplanets [PDF]
Many of exoplanetary systems consist of more than one planet and the study of planetary orbits with respect to their long-term stability is very interesting. Furthermore, many exoplanets seem to be locked in a mean-motion resonance (MMR), which offers a phase protection mechanism, so that, even highly eccentric planets can avoid close encounters ...
openaire +3 more sources
A New Method for Studying Exoplanet Atmospheres Using Planetary Infrared Excess [PDF]
To date, the ability for observers to reveal the composition or thermal structure of an exoplanet’s atmosphere has rested on two techniques: high-contrast direct imaging and time-series observations of transiting exoplanets.
K. Stevenson
semanticscholar +1 more source
This book is Open Access. A digital copy can be downloaded for free from Wiley Online Library.
Explores the behavior of carbon in minerals, melts, and fluids under extreme conditions
Carbon trapped in diamonds and carbonate-bearing rocks in subduction zones are examples of the continuing exchange of substantial carbon ...
wiley +1 more source
Classification of Trajectories in a Two-planet Exosystem Using the Generalized Three-body Problem
We deploy the theory of the generalized three-body problem to describe an exosystem composed of a host star, a transiting Jupiter-sized exoplanet, and an Earth-sized exoplanet.
Eman M. Moneer +5 more
doaj +1 more source
Efficient Geometric Probabilities of Multi-Transiting Exoplanetary Systems from CORBITS [PDF]
NASA's Kepler Space Telescope has successfully discovered thousands of exoplanet candidates using the transit method, including hundreds of stars with multiple transiting planets.
Brakensiek, Joshua, Ragozzine, Darin
core +3 more sources

