The Astrophysical Journal, 2023 Constraining the physical and chemical structure of young embedded disks is crucial for understanding the earliest stages of planet formation. As part of the Early Planet Formation in Embedded Disks Atacama Large Millimeter/submillimeter Array Large ...
Yoshihide Yamato +30 more
doaj +1 more source
Early formation of planetary building blocks inferred from Pb isotopic ages of chondrules [PDF]
Science Advances, 2017 Age dating of meteorite inclusions suggests rapid formation of the building blocks of terrestrial planets within 1 My of the Sun. The most abundant components of primitive meteorites (chondrites) are millimeter-sized glassy spherical chondrules formed by
J. Bollard +8 more
semanticscholar +1 more source
Mass and Eccentricity Constraints in the WASP-47 Planetary System from a Simultaneous Analysis of Radial Velocities & Transit Timing Variations [PDF]
, 2016 Measuring precise planet masses, densities, and orbital dynamics in individual planetary systems is an important pathway toward understanding planet formation. The WASP-47 system has an unusual architecture that invites a complex formation theory.
L. Weiss +11 more
semanticscholar +1 more source
A Large Double-ring Disk Around the Taurus M Dwarf J04124068+2438157
The Astrophysical Journal, 2023 Planet formation imprints signatures on the physical structures of disks. In this paper, we present high-resolution (∼50 mas, 8 au) Atacama Large Millimeter/submillimeter Array observations of 1.3 mm dust continuum and CO line emission toward the disk ...
Feng Long +25 more
doaj +1 more source
Let’s Sweep: The Effect of Evolving J 2 on the Resonant Structure of a Three-planet System
The Astrophysical Journal, 2023 Short and ultrashort period planets are peculiar types of exoplanets with periods as short as a few days or less. Although it is challenging to detect them, already several have been observed, with many additional candidates.
Thea H. Faridani +3 more
doaj +1 more source
Consequences of planetary migration on the minor bodies of the early solar system [PDF]
Astronomy & Astrophysics, 2019 Pebble accretion is an efficient mechanism that is able to build up the core of the giant planets within the lifetime of the protoplanetary disc gas-phase. The core grows via this process until the protoplanet reaches its pebble isolation mass and starts
S. Pirani +4 more
semanticscholar +1 more source
Habitable Planet Formation in Binary Planetary Systems [PDF]
The Astrophysical Journal, 2007 27 pages, 11 figures, submitted for ...
Haghighipour, Nader, Raymond, Sean N.
openaire +2 more sources
Implications of the interstellar object 1I/'Oumuamua for planetary dynamics and planetesimal formation [PDF]
, 2017 'Oumuamua, the first bona-fide interstellar planetesimal, was discovered passing through our Solar System on a hyperbolic orbit. This object was likely dynamically ejected from an extrasolar planetary system after a series of close encounters with gas ...
S. Raymond +4 more
semanticscholar +1 more source
Making the Planetary Material Diversity during the Early Assembling of the Solar System [PDF]
Astrophysical Journal, 2018 Chondritic meteorites, the building blocks of terrestrial planets, are made of an out-of-equilibrium assemblage of solids formed at high and low temperatures, either in our Solar system or previous generations of stars. For decades this was considered to
F. Pignatale +3 more
semanticscholar +1 more source
Planetary system disruption by Galactic perturbations to wide binary stars [PDF]
Nature, 2013 Nearly half the exoplanets found within binary star systems reside in very wide binaries with average stellar separations greater than 1,000 astronomical units (one astronomical unit (au) being the Earth–Sun distance), yet the influence of such distant ...
N. Kaib, S. Raymond, M. Duncan
semanticscholar +1 more source