The Sun and solar phenomena
A star modest in appearance, gigantic in reality
The Sun is classified as a yellow dwarf, but its size and mass make it a colossal star. During the formation of the Solar System, it alone captured 99.86% of the total mass from the primordial nebula. This concentration of matter shaped its evolution and determined the dynamics of the entire Solar System.
An uneven distribution of matter
After the Sun, Jupiter is the body that took the largest share of the remaining material, about 71% of what had not been absorbed by the nascent star. The other planets, much smaller, formed from the residue of this gravitational evolution, giving rise to a diversity of rocky, gaseous, and icy worlds.
An energy engine with spectacular phenomena
The Sun is not only a source of light and heat: it is also the site of dynamic phenomena such as solar flares, sunspots, coronal mass ejections, and variations in the solar wind. These manifestations influence the space environment and can even affect Earth, reminding us of the power of the star that governs our Solar System.
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Stability and Chaos: Limits of the Solar System’s Orbital Harmony
Where Does the Sun's Energy Come From?
The Grand Tour: The Hidden Secrets of the Planets in Our Stellar Neighborhood
The Sounds of Space: When Data Sings
The Three-Body Problem: Three Celestial Bodies, One Law, Infinite Destinies
Lagrange Points: The Illusion of Stable Gravitational Oases
Nemesis: The Theory of the Sun's Companion Star
Solar System vs. Stellar Systems: A Comparison of Planetary Systems
The Faint Young Sun Paradox: Why Wasn't Early Earth Frozen?
380 billion billion megawatts: The Solar Energy Excess
The Ecliptic or the Apparent Orbit of the Sun
Solar maximum and minimum
How to weigh the sun?
The Sun: When the Yellow Star Turns Blue
Understanding the Sun's Figure-8 Curve: The Analemma Explained
Frost Line: The Boundary That Shaped the Planets
Tourist trip in the solar system
Sunspots and the Solar Cycle: From Minimum to Maximum
The infernal journey of the photon or random walk
Dynamics of Solar Cycles and Physical Mechanisms of Solar Flares
Baily grains in a solar eclipse
Birth, Life and Death of the Sun: Chronicle of an Average Star
Grains of Baily or pearls of light
Sunlight and wavelengths
The chaotic formation of the solar system
Solar Storms and Catastrophic Scenarios
Solar Prominences: Filaments of Matter in the Solar Atmosphere
Why Does the Sun Rotate So Slowly? The Mystery of the Missing Angular Momentum
Solar Winds: A Key Phenomenon of Interplanetary Space
Heliosphere: At the Borders of the Solar System
Chaos and sensitivity to initial conditions