Kinematic Evidence of an Embedded Protoplanet in HD 142666 Identified by Machine Learning
Observations of protoplanetary disks have shown that forming exoplanets leave characteristic imprints on the gas and dust of the disk. In the gas, these forming exoplanets cause deviations from Keplerian motion, which can be detected through molecular ...
J. P. Terry +3 more
doaj +1 more source
Dust Size Growth and Settling in a Protoplanetary Disk
We have studied dust evolution in a quiescent or turbulent protoplanetary disk by numerically solving coagulation equation for settling dust particles, using the minimum mass solar nebular model.
Hideko Nomura +12 more
core +1 more source
On the Evolution of Dust Mineralogy, From Protoplanetary Disks to Planetary Systems [PDF]
Mineralogical studies of silicate features emitted by dust grains in protoplanetary disks and Solar System bodies can shed light on the progress of planet formation.
Beckwith +55 more
core +4 more sources
Satellites and Small Bodies With ALMA: Insights Into Solar System Formation and Evolution
Abstract Our understanding of the formation and evolution of planetary systems has made major advances in the past decade. This progress has been driven in large part by the Atacama Large Millimeter/submillimeter Array (ALMA), which has given us an unprecedented view of solar system bodies themselves, and of the structure and chemistry of forming ...
Katherine de Kleer +3 more
wiley +1 more source
Our understanding of how exoplanets form and evolve relies on analyses of both the mineralogy of protoplanetary disks and their detailed structures; however, these key complementary aspects of disks are usually studied separately.
William Grimble +9 more
doaj +1 more source
Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations
We study the dependence of protoplanetary disk evolution on stellar mass using a large sample of young stellar objects in nearby young star-forming regions. We update the protoplanetary disk fractions presented in our recent work (paper I of this series)
Bouy, Hervé +2 more
core +1 more source
The composition of the protosolar disk and the formation conditions for comets [PDF]
Conditions in the protosolar nebula have left their mark in the composition of cometary volatiles, thought to be some of the most pristine material in the solar system.
A. Dutrey +227 more
core +3 more sources
Parent body thermal metamorphism of enstatite chondrites: Disentangling the effects of shock melting
Abstract Enstatite chondrites (ECs) formed on at least two parent bodies, EH and EL. After the accretion of the EC parent bodies, EC material was subjected to varying degrees of parent body thermal metamorphism (measured by petrologic types 3–6), due to heat released by radioactive isotope decay.
Peter Mc Ardle +9 more
wiley +1 more source
Shedding Light on the Origin of the Broken Misaligned Circumtriple Disk around GW Ori
We revisit the origin of the observed misaligned rings in the circumtriple disk around GW Ori. Previous studies appeared to disagree on whether disk breaking is caused by the differential precession driven in the disk by the triple star system.
Jeremy L. Smallwood +3 more
doaj +1 more source
Resonant Relaxation in Protoplanetary Disks [PDF]
19 pages, 1 figure, LaTeX, submitted to ...
openaire +2 more sources

