Argali (Ovis ammon) 500 Tugriks...
Figure Eight Dragon $2 2oz .999 pure silver coin, antique finish. This...
Star Wars - The Return of the Jedi $2 1oz silver coin. This limited...
Colourful Creatures - The Wolf Glow in the Dark 3€ Cu-Ni coin. Attention...
Box for 1 coin 38.61mm + capsule = 45mm. Weight: 150g Size: 90x90x28mm...
Box for 5 coins 38.61mm + capsule = 45mm. Weight: 340g Size:...
Murrine Millefiori Glass Art $5 .999 pure silver coin. Beautiful...
Source of Life 1000 CFA Francs 1oz...
Source of Life 1000 CFA Francs 1oz .999 pure silver coin.
This amazing coin is dedicated to the Sun, our strongest energy supplier and the source of life on Earth. The coin has a gold plated centre with digital black. Glowing Image Of The Sun! First Coin With The Centre Of Our Planetary System!
Mintage: 2,000 pieces worldwide. With luxury box and COA.
1 Item Items
Warning: Last items in stock!
|Face Value :||1,000 CFA Francs|
|Metal :||.999 Fine silver|
|Weight :||1 oz|
|Size :||40.00 mm|
|Mintage :||2,000 pcs. worldwide|
|Certificate of Authenticity :||Yes|
|Original ETUI box/case :||Yes|
The Sun is the star at the center of the Solar System. It is a nearly perfect sphere of hot plasma, with internal convective motion that generates a magnetic field via a dynamo process. It is by far the most important source of energy for life on Earth. Its diameter is about 109 times that of Earth, and its mass is about 330,000 times that of Earth, accounting for about 99.86% of the total mass of the Solar System. About three quarters of the Sun's mass consists of hydrogen (~73%); the rest is mostly helium (~25%), with much smaller quantities of heavier elements, including oxygen, carbon, neon, and iron.
The Sun is a G-type main-sequence star (G2V) based on its spectral class, and is informally referred to as a yellow dwarf. It formed approximately 4.6 billion years ago from the gravitational collapse of matter within a region of a large molecular cloud. Most of this matter gathered in the center, whereas the rest flattened into an orbiting disk that became the Solar System. The central mass became so hot and dense that it eventually initiated nuclear fusion in its core. It is thought that almost all stars form by this process.
The Sun is roughly middle-aged; it has not changed dramatically for more than four billion years, and will remain fairly stable for more than another five billion years. After hydrogen fusion in its core has diminished to the point at which it is no longer in hydrostatic equilibrium, the core of the Sun will experience a marked increase in density and temperature while its outer layers expand to eventually become a red giant. It is calculated that the Sun will become sufficiently large enough to engulf the current orbits of Mercury, Venus, and probably Earth.
No customer reviews for the moment.