Results 71 to 80 of about 2,834 (210)
On the width and shape of the corotation region for low-mass planets
We study the coorbital flow for embedded, low mass planets. We provide a simple semi-analytic model for the corotation region, which is subsequently compared to high resolution numerical simulations. The model is used to derive an expression for the half-
Artymowicz +26 more
core +1 more source
Photophoresis boosts giant planet formation [PDF]
In the core accretion model of giant planet formation, a solid protoplanetary core begins to accrete gas directly from the nebula when its mass reaches about 5 earth masses.
Dodson-Robinson, Sarah E., Teiser, Jens
core +2 more sources
A Giant Impact Origin for the First Subduction on Earth
Abstract Hadean zircons provide a potential record of Earth's earliest subduction 4.3 billion years ago. It remains enigmatic how subduction could be initiated so soon after the presumably Moon‐forming giant impact (MGI). Earlier studies found an increase in Earth's core‐mantle boundary (CMB) temperature due to the accumulation of the impactor's core ...
Qian Yuan +3 more
wiley +1 more source
Wide Separation Planets in Time (WISPIT): Discovery of a Gap Hα Protoplanet WISPIT 2b with MagAO-X
Excellent (
Laird M. Close +36 more
doaj +1 more source
Accreting protoplanets in the LkCa 15 transition disk [PDF]
35 pages, 3 figures, 1 table, 9 extended data ...
Sallum, S. +16 more
openaire +3 more sources
Die Suche nach kalten, fremden Welten
Die meisten der heute bekannten extrasolaren Planeten umkreisen ihren Mutterstern auf engen Umlaufbahnen in weniger als 100 Tagen. Gesteinsplaneten mit größeren Bahnradien sind von herausragender Bedeutung für Theorien der Planetenentstehung. Die Mikrogravitationslinsenmethode bietet eine hervorragende Möglichkeit, solche Planeten zu finden – und das ...
Markus Hundertmark, Yiannis Tsapras
wiley +1 more source
SPECTRAL ENERGY DISTRIBUTIONS OF ACCRETING PROTOPLANETS [PDF]
Accepted for publication in ApJ ...
openaire +2 more sources
Dynamics and Accretion of Planetesimals
We review the basic dynamics and accretion of planetesimals by showing N-body simulations. The orbits of planetesimals evolve through two-body gravitational relaxation: viscous stirring increases the random velocity and dynamical friction realizes the ...
Ida, Shigeru, Kokubo, Eiichiro
core +1 more source
A Post‐Launch Summary of the Science of NASA's Psyche Mission
Abstract Astronomical observations indicate that asteroid (16) Psyche is a large, high‐density (likely >3,400 kg·m−3), metal‐rich (30–55 vol. %) asteroid. Psyche may be remnant core material or it could be a primordial, undifferentiated metal‐rich object.
Steven D. Dibb +15 more
wiley +1 more source
VLT/MUSE Detection of the AB Aurigae b Protoplanet with Hα Spectroscopy
We analyze high-contrast, medium-spectral-resolution H _α observations of the star AB Aurigae using the Very Large Telescope's Multi Unit Spectroscopic Explorer (MUSE).
Thayne Currie +8 more
doaj +1 more source

