Results 21 to 30 of about 21,733,950 (248)
The formation and subsequent migration of gas giants could significantly affect the material mixing in the solar system. In this study, we use N -body simulations to investigate how much water is transported into the region of the terrestrial planet ...
Masahiro Ogihara +2 more
doaj +1 more source
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
A Large Double-ring Disk Around the Taurus M Dwarf J04124068+2438157
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
Summary of the Second International Planetary Dunes Workshop: Planetary Analogs — Integrating Models, Remote Sensing, and Field Data, Alamosa, Colorado, USA, May 18–21, 2010 [PDF]
The Second International Planetary Dunes Workshop took place in Alamosa, Colorado, USA from May 18–21, 2010. The workshop brought together researchers from diverse backgrounds to foster discussion and collaboration regarding terrestrial and extra ...
Tirsch, D. +31 more
core +1 more source
The planetary system around HD 190622 (TOI-1054)
Context. Giant planets are known to dominate the long-term stability of planetary systems due to their prevailing gravitational interactions, but they are also thought to play an important role in planet formation.
Ragazzoni, R. +109 more
core +1 more source
Let’s Sweep: The Effect of Evolving J 2 on the Resonant Structure of a Three-planet System
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
New Dynamical State and Habitability of the HD 45364 Planetary System [PDF]
Planetary systems with multiple giant planets provide important opportunities to study planetary formation and evolution. The HD 45364 system hosts two giant planets that reside within the Habitable Zone (HZ) of their host star and was the first system ...
Kane, Stephen R. +4 more
core +1 more source
Habitable Planet Formation in Binary Planetary Systems [PDF]
27 pages, 11 figures, submitted for ...
Haghighipour, Nader, Raymond, Sean N.
openaire +2 more sources
Planet formation with envelope enrichment: new insights on planetary diversity [PDF]
Aims. We compute for the first time self-consistent models of planet growth that include the effect of envelope enrichment. The change in envelope metallicity is assumed to be the result of planetesimal disruption or icy pebble sublimation. Methods.
Alibert, Yann +2 more
core +2 more sources
Implications of Differentiated Late Accretion for the Volatile Inventory of the Bulk Silicate Earth
Earth is believed to have acquired its highly siderophile element (HSE) inventory through the late accretion of ∼0.3%–0.5% of its mass in chondrite-like materials, following the main stage of its growth. Late accretion, particularly if it originated from
Damanveer S. Grewal, Varun Manilal
doaj +1 more source

