12CO Rovibrational Spectroscopy of AB Aurigae—A Potential Point Source Is Present
The Herbig Ae star AB Aurigae hosts a vast, low-inclination protoplanetary disk that exhibits a plethora of substructures, including the protoplanet candidate AB Aur b. We present M -band spectroscopic data taken with the NASA Infrared Telescope Facility
Janus Kozdon +6 more
doaj +1 more source
Chondrule Formation in Bow Shocks around Eccentric Planetary Embryos
Recent isotopic studies of Martian meteorites by Dauphas & Pourmond (2011) have established that large (~ 3000 km radius) planetary embryos existed in the solar nebula at the same time that chondrules - millimeter-sized igneous inclusions found in ...
Athanassiadou, Themis +3 more
core +1 more source
The Growth & Migration of Jovian Planets in Evolving Protostellar Disks with Dead Zones
The growth of Jovian mass planets during migration in their protoplanetary disks is one of the most important problems that needs to be solved in light of observations of the exosolar planets.
Andrews +43 more
core +1 more source
Evidence for Variable Accretion onto PDS 70 c and Implications for Protoplanet Detections
Understanding the processes of planet formation and accretion in young systems is essential to unraveling the initial conditions of planetary systems.
Yifan Zhou +16 more
doaj +1 more source
A pebble accretion model for the formation of the terrestrial planets in the Solar System. [PDF]
Johansen A +6 more
europepmc +1 more source
A Protoplanet Candidate in the PDS 66 Disk Indicated by Silicon Sulfide Isotopologues
Despite observational progress in planet formation, the stage in which planetesimals grow into planets remains poorly understood. During this phase, protoplanets may develop gaseous envelopes that are warmer than the surrounding disk gas, potentially ...
Tomohiro C. Yoshida +13 more
doaj +1 more source
Detailed structure of the outer disk around HD 169142 with polarized light in H-band
Coronagraphic imagery of the circumstellar disk around HD 169142 in H-band polarized intensity (PI) with Subaru/HiCIAO is presented. The emission scattered by dust particles at the disk surface in 0.2"
Abe, Lyu +61 more
core +1 more source
Silicon isotope constraints on terrestrial planet accretion. [PDF]
Onyett IJ +5 more
europepmc +1 more source
How planetary growth outperforms migration
Planetary migration is a major challenge for planet formation theories. The speed of Type I migration is proportional to the mass of a protoplanet, while the final decade of growth of a pebble-accreting planetary core takes place at a rate that scales ...
Brasser, Ramon +2 more
core +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source

