Results 31 to 40 of about 4,018,158 (274)

Isotopic evolution of planetary crusts by hypervelocity impacts evidenced by Fe in microtektites

open access: yesNature Communications, 2021
Fe isotopic composition of the distal ejecta of a terrestrial impact crater records both evaporation and condensation, refining the nature of the isotopic fractionation taking place during hypervelocity impacts in the Solar System.
S. M. Chernonozhkin   +12 more
doaj   +1 more source

Why do more massive stars host larger planets? [PDF]

open access: yesA&A 652, A110 (2021), 2021
It has been suggested that planetary radii increase with the stellar mass, for planets below 6 R$_{\oplus}$ and host below 1 M$_\odot$. In this study, we explore whether this inferred relation between planetary size and the host star's mass can be explained by a larger planetary mass among planets orbiting more massive stars, inflation of the planetary
arxiv   +1 more source

Planetary mass–radius relations across the galaxy [PDF]

open access: yesAstronomy & Astrophysics, 2020
Context. Planet formation theory suggests that planet bulk compositions are likely to reflect the chemical abundance ratios of their host star’s photosphere.
A. Michel   +3 more
semanticscholar   +1 more source

A Theoretical Framework for the Mass Distribution of Gas Giant Planets forming through the Core Accretion Paradigm [PDF]

open access: yes, 2021
This paper constructs a theoretical framework for calculating the distribution of masses for gas giant planets forming via the core accretion paradigm. Starting with known properties of circumstellar disks, we present models for the planetary mass distribution over the range $0.1M_J < M_{\rm p} < 10M_J$.
arxiv   +1 more source

The New Generation Planetary Population Synthesis (NGPPS). IV. Planetary systems around low-mass stars [PDF]

open access: yesAstronomy & Astrophysics, 2021
Previous work concerning planet formation around low-mass stars has often been limited to large planets and individual systems. As current surveys routinely detect planets down to terrestrial size in these systems, a more holistic approach that reflects ...
R. Burn   +7 more
semanticscholar   +1 more source

Natural Products Containing ‘Rare’ Organophosphorus Functional Groups

open access: yesMolecules, 2019
Phosphorous-containing molecules are essential constituents of all living cells. While the phosphate functional group is very common in small molecule natural products, nucleic acids, and as chemical modification in protein and peptides, phosphorous can ...
Janusz J. Petkowski   +2 more
doaj   +1 more source

Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70 [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Young circumstellar disks are the birthplaces of planets. Their study is of prime interest to understand the physical and chemical conditions under which planet formation takes place.
M. Keppler   +135 more
semanticscholar   +1 more source

Impact of Changing Stellar and Planetary Magnetic Fields on (Exo)planetary Environments and Atmospheric Mass Loss

open access: yesThe Astrophysical Journal, 2023
The magnetic activity of a star—which modulates the stellar wind outflow—shapes the immediate environments of orbiting (exo)planets and induces atmospheric loss, thereby impacting their habitability.
Sakshi Gupta   +2 more
doaj   +1 more source

Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10−4 Planets from the First 4 yr Survey

open access: yesThe Astronomical Journal, 2023
We present the analysis of seven microlensing planetary events with planet/host mass ratios q < 10 ^−4 : KMT-2017-BLG-1194, KMT-2017-BLG-0428, KMT-2019-BLG-1806, KMT-2017-BLG-1003, KMT-2019-BLG-1367, OGLE-2017-BLG-1806, and KMT-2016-BLG-1105.
Weicheng Zang   +42 more
doaj   +1 more source

Cloud Atlas: Rotational Spectral Modulations and Potential Sulfide Clouds in the Planetary-mass, Late T-type Companion Ross 458C [PDF]

open access: yesAstrophysical Journal, 2019
Measurements of photometric variability at different wavelengths provide insights into the vertical cloud structure of brown dwarfs and planetary-mass objects.
E. Manjavacas   +13 more
semanticscholar   +1 more source

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