Results 301 to 310 of about 22,046,683 (361)

Adapting the Planetary Health Report Card for Graduate Medical Training Programs. [PDF]

open access: yesJ Grad Med Educ
Schear S   +4 more
europepmc   +1 more source

Percolative sulfide core formation in oxidized planetary bodies. [PDF]

open access: yesNat Commun
Crossley SD   +9 more
europepmc   +1 more source

PlanetTXT: A Text-based Planetary System Simulation Interface for Astronomy Edutainment

International Conference on E-Education, E-Business, E-Management, and E-Learning, 2023
Planetary systems represent a set of gravitationally bounded non-stellar objects in or out of orbit around a star or star system. However, existing works for simulating exoplanetary systems other than the solar system are still limited. In this paper, we
Wanwan Li
semanticscholar   +1 more source

Planetary System

, 1982
Maciej Konacki   +2 more
semanticscholar   +2 more sources

Planetary Systems Now

2022
Planetary Systems Now offers a broad, interdisciplinary perspective and introduction to the latest results from leading experts in each field. It offers an unusually wide range of research on topics both inside and outside of the solar system, as well as the most recent results from ongoing ground- and space-based investigations. Experts in their field
Lara, Luisa María, Jewitt David
openaire   +2 more sources

Tides in Planetary Systems

2013
The Solar system is the seat of many interactions between the Sun, the planets and their natural satellites. Moreover, since 1995, a large number of extrasolar planetary systems has been discovered where planets orbit around other stars, sometimes very close to them. Therefore, in such systems, tidal interactions are one of the key mechanisms that must
Mathis, Stéphane   +2 more
openaire   +4 more sources

Planetary nebulae in planetary and binary systems

Astrophysics and Space Science, 1981
The problem of the survival of a low-mass secondary orbiting a primary that becomes a planetary nebula is studied. The values of the mass of the primary are 1.0, 1.5, and 2.0M ⊙; the values of the mass of the secondary 0.001M ⊙, 0.01M ⊙ and 0.1M ⊡.
Kyu H. Choi, Samuel C. Vila
openaire   +2 more sources

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