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Transit Zones of the Solar System Planets [PDF]
The detection of thousands of extrasolar planets by the transit method naturally raises the question of whether potential extrasolar observers could detect the transits of the Solar System planets.
Heller, R. +12 more
core +7 more sources
Simultaneous formation of solar system giant planets [PDF]
Context. In the last few years, the so-called “Nice model” has become increasingly significant for studying the formation and evolution of the solar system.
O. M. Guilera +11 more
core +6 more sources
Microlensing search for extra solar planets [PDF]
Gravitational microlensing may be used to probe distant stars for planetary companions. The presence of a planet in the vicinity of a star acting as the lens may cause a short lived anomaly in the observed lightcurve of the lensing event.
Tsapras, Yiannis
core +2 more sources
Is There a Tenth Planet in the Solar System? [PDF]
WE have been analysing the longitudinal residuals of Neptune (N), partly from sheer interest aroused by the discordance between the pre-discovery position of N and its currently accepted orbit1 and because colleagues (already conducting a photographic hunt for a hypothetical tenth planet) sought our assistance in narrowing the field of search by using ...
D. RAWLINS, M. HAMMERTON
openaire +1 more source
Chemical Convection and Stratification in the Earth's Outer Core
Convection in the Earth's outer core is driven by buoyancy sources of both thermal and compositional origin. The thermal and compositional molecular diffusivities differ by several orders of magnitude, which can affect the dynamics in various ways.
Mathieu Bouffard +3 more
doaj +1 more source
Weather conditions and weather forecast on the planets of the solar system based on the behavior of Rossby waves [PDF]
Out of all atmospheric processes on the planets of the Solar System, special attention will be devoted here to leading circulation of planetary or global scales, known as Rossby waves.
Gavrilov Milivoj B. +2 more
doaj +1 more source
Electrification represents a fundamental process in planetary atmospheres, widespread in the Solar System. The atmospheres of the terrestrial planets (Venus, Earth, and Mars) range from thin to thick are rich in heavier gases and gaseous compounds, such ...
Marija Radmilović-Radjenović +2 more
doaj +1 more source
Solar System Planets and Exoplanets
Solar System planets have been studied for centuries, but the observation of exoplanets is only a few decades old. Consequently, knowledge of exoplanets is considerably more limited than Solar System planets. This chapter reviews the essential characteristics of Solar System planets and associated data derived from a variety of observational approaches.
openaire +3 more sources
Penerapan Teknologi Augmented Reality sebagai Media Pembelajaran Interaktif Tata Surya
Learning the solar system through books has been a major choice over time. This learning is considered monotonous because of the limited interaction of students with the delivery of material.
Meisye Putri Azizah +1 more
doaj +1 more source
SPECIFICATION OF LIMITS OF POSSIBLE EXISTENCE OF SATELLITES IN THE GRAVITATIONAL FIELD OF PLANETS
It is known that the satellites of the planets may exist in the area, which is bounded on one side by Rocha limit, on the other – Hill sphere. The article deals with the determination of the Rocha limits and Hill sphere of satellites of some planets in ...
S. O. Yasenev, K. O. Radchenko
doaj +1 more source

