Results 61 to 70 of about 54,418 (256)
Exoplanets in physics and astronomy teaching
This article aims to investigate Physics teaching and scientific dissemination activities with the main theme being the study of exoplanets, planets belonging to a star system distinct from our solar system.
Ryan Nepomuceno Montemor+1 more
doaj +1 more source
The Observational Case for Jupiter Being a Typical Massive Planet
We identify a subsample of the recently detected extrasolar planets that is minimally affected by the selection effects of the Doppler detection method.
Grether, Daniel, Lineweaver, Charles H.
core +1 more source
HELIOS-Retrieval: An Open-source, Nested Sampling Atmospheric Retrieval Code, Application to the HR 8799 Exoplanets and Inferred Constraints for Planet Formation [PDF]
We present an open-source retrieval code named HELIOS-Retrieval (hereafter HELIOS-R), designed to obtain chemical abundances and temperature-pressure profiles from inverting the measured spectra of exoplanetary atmospheres. In the current implementation,
Bonnefoy, Mickaël+9 more
core +3 more sources
Tools for Learning—Promoting Reflection for Student Teachers' Development of PCK
ABSTRACT This paper investigates how the coherent integration of three different tools for reflection during a science methods course can contribute to student teachers' planning and enactment of science teaching, that is, their development of pedagogical content knowledge (PCK).
Pernilla Nilsson+1 more
wiley +1 more source
We review the recent progress in understanding the jet structures on exoplanets as well as on and inside the Sun. The emphasis is on the more robust aspects of observation and numerical modeling that relate directly to jets. For the exoplanets, the primary focus is on hot-Jupiters since many more observations are available for them presently than other
Woosok Moon+6 more
openaire +3 more sources
Exoplanets Torqued by the Combined Tides of a Moon and Parent Star [PDF]
In recent years, there has been interest in Earth-like exoplanets in the habitable zones of low mass stars ($\sim0.1-0.6\,M_\odot$). Furthermore, it has been argued that a large moon may be important for stabilizing conditions on a planet for life. If these two features are combined, then an exoplanet can feel a similar tidal influence from both its ...
arxiv +1 more source
On homogeneous statistical distributions exoplanets for their dynamic parameters
Correct distributions of extrasolar systems for their orbital parameters (semi-major axes, period, eccentricity) and physical characteristics (mass, spectral type of parent star) are received. Orbital resonances in extrasolar systems are considered.
A. Burrows+4 more
core +1 more source
Rational speculation about biological evolution on other worlds is one of the outstanding challenges in astrobiology. With the growing confirmation that multiplanetary systems abound in the universe, the prospect that life occurs redundantly throughout ...
Louis N. Irwin+3 more
doaj +1 more source
Habitability of Super-Earths: Gliese 581c and 581d
The unexpected diversity of exoplanets includes a growing number of super-Earth planets, i.e., exoplanets with masses smaller than 10 Earth masses. Unlike the larger exoplanets previously found, these smaller planets are more likely to have a similar ...
C. Bounama+5 more
core +1 more source
Tidal effects arise from differential and inelastic deformation of a planet by a perturbing body. The continuous action of tides modify the rotation of the planet together with its orbit until an equilibrium situation is reached. It is often believed that synchronous motion is the most probable outcome of the tidal evolution process, since synchronous ...
Correia, Alexandre C. M.+1 more
openaire +7 more sources