Results 81 to 90 of about 14,974 (190)
Composition of giant planets: the roles of pebbles and planetesimals [PDF]
Claudia Danti +2 more
openalex +1 more source
Ferromagmatic Intrusions on Asteroid (16) Psyche May Be Magnetized
Abstract NASA's Psyche mission will arrive at the metal‐rich asteroid (16) Psyche in 2029. The mission will test whether (16) Psyche is a remnant of a melted, differentiated planetesimal that formed a molten iron metallic core. Previous studies have suggested that a molten metallic core fluid could erupt volcanically, explaining the high metal content ...
Samuel W. Courville +8 more
wiley +1 more source
The Characterization of the Dust Content in the Ring Around Sz 91: Indications of Planetesimal Formation? [PDF]
Karina Maucó +8 more
openalex +1 more source
The water content and habitability of terrestrial planets are determined during their final assembly, from perhaps a hundred 1000-km "planetary embryos" and a swarm of billions of 1-10 km "planetesimals." During this process, we assume that water-rich ...
Lunine, Jonathan I. +2 more
core +1 more source
Planet formation in slightly inclined binary systems
One of the major problems of planet formation in close binary systems, such as α Centauri AB, is the formation of planetary embryos or cores by mutual accretion of km-sized planetesimals.
Ge J., Xie J.-W., Zhou J.-L.
doaj +1 more source
Initial mass function of planetesimals formed by the streaming instability
The streaming instability is a mechanism to concentrate solid particles into overdense filaments that undergo gravitational collapse and form planetesimals.
Johansen, Anders +2 more
core +1 more source
Estimating the mass of the debris disc in HD 69830
We present a method to estimate the mass of the debris disc in the HD 69830 system, which also hosts three exoplanets with Neptune-like minimum masses. By considering the range of published stellar ages, we interpret the infrared emission from the debris
Alibert +16 more
core +1 more source
Tidal Disruption of Planetesimals from an Eccentric Debris Disk Following a White Dwarf Natal Kick
The surfaces of many white dwarfs are polluted by metals, implying a recent accretion event. The tidal disruption of planetesimals is a viable source of white dwarf pollution and offers a unique window into the composition of exoplanet systems.
Tatsuya Akiba +2 more
doaj +1 more source
Debris disks or exo-Kuiper belts, detected through their thermal or scattered emission from their dusty components, are ubiquitous around main-sequence stars.
Antranik A. Sefilian
doaj +1 more source
Silica-rich volcanism in the early solar system dated at 4.565 Ga
Achondritic meteorites can record volcanism and crust formation on planetesimals in the early Solar System. Here, the authors date the Northwest Africa 11119 meteorite with an Al-Mg age of 4564.8 ± 0.3 Ma indicating that this is the earliest evidence of ...
Poorna Srinivasan +7 more
doaj +1 more source

