Results 51 to 60 of about 186,798 (170)
Highly Depleted Alkali Metals in Jupiter’s Deep Atmosphere
Water and ammonia vapors are known to be the major sources of spectral absorption at pressure levels observed by the microwave radiometer (MWR) on Juno. However, the brightness temperatures and limb darkening observed by the MWR at its longest-wavelength
Ananyo Bhattacharya +14 more
doaj +1 more source
Knudsen effusion mass spectrometry: Current and future approaches
Rationale Knudsen effusion mass spectrometry (KEMS) has been a powerful tool in physical chemistry since 1954. There are many excellent reviews of the basic principles of KEMS in the literature. In this review, we focus on the current status and potential growth areas for this instrumental technique.
Nathan S. Jacobson +4 more
wiley +1 more source
The stability of short-period extrasolar giant planets [PDF]
A three-dimensional coupled thermosphere-ionosphere model for extrasolar giant planets (EXOTIM) has been developed. This is the first such model reported in the literature.
Koskinen, T.T.
core
Planet–Planet Scattering Explains the Mass–Eccentricity Relation of Warm Jupiters
Warm Jupiters—giant planets with orbital periods of ∼10–365 days—exhibit a positive correlation between mass and eccentricity. We interpret this trend as the outcome of planet–planet scattering, representing a transition from collision-dominated ...
Jiayin Dong +5 more
doaj +1 more source
Advances in high‐temperature operatable triboelectric nanogenerator
Triboelectric nanogenerator (TENG), as a continuous, durable, and self‐sufficient power source, offers an innovative approach to effectively utilize diverse mechanical energy. This review comprehensively presents the current state and research advancements in high‐temperature operatable TENG (HTO‐TENG), providing valuable insights into future research ...
Ruirui Cao +11 more
wiley +1 more source
Small and Close-in Planets are Uncommon Around A-type Stars
The Kepler and K2 missions enabled robust calculations of planet occurrence rates around FGKM-type stars. However, these missions observed too few stars with earlier spectral types to tightly constrain the occurrence rates of planets orbiting hotter ...
Steven Giacalone, Courtney D. Dressing
doaj +1 more source
We present analysis of the atmospheres of 70 gaseous extrasolar planets via transit spectroscopy with Hubble’s Wide Field Camera 3 (WFC3). For over half of these, we statistically detect spectral modulation that our retrievals attribute to molecular ...
Billy Edwards +16 more
doaj +1 more source
Abstract Outward transport of plasma in the inner and middle magnetospheres of gas giants results from an interplay between mass loading from the inner dominant mass sources (volcanic moons), flux tube interchange in the centrifugally unstable magnetospheric plasma disk, turbulent heating of the plasma, and coupling between the equatorial plasma and ...
Marie Devinat +2 more
wiley +1 more source
Two Extrasolar Planets from the Anglo‐Australian Planet Search
We report the detection of two new extrasolar planets from the Anglo-Australian Planet Search around the stars HD 142 and HD 23079. The planet orbiting HD 142 has an orbital period of just under 1 yr, while that orbiting HD 23079 has a period of just ...
C. G. Tinney +13 more
core +1 more source
The extreme environments of transiting close-in exoplanets in highly eccentric orbits are ideal for testing exoclimate physics. Spectroscopically resolved phase curves not only allow for the characterization of their thermal response to irradiation ...
Bob Jacobs +12 more
doaj +1 more source

