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11. Our solar system
| 11.3 |
Our star (the sun) |
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| The Sun is the only star near enough to us to be observed as more than simply a point of light. Although stars vary greatly in size, the Sun is typical of many, and is identical in size, brightness and ergon output to countless others in the universe. It is the source of all our ergon particles and essential to the survival of human and all other life forms. Around it, in various orbits, move the nine planets in our solar system and a huge number of asteroids, meteors and comets- all of them under the Sun's gravitational attraction. | ||
| 11.3.1 | The Sun's vital statistics | |
| In terms of temperature and brightness, the Sun is a typical star. However its size is small compared with some stars that are up to 300 times its diameter. It's mass is made up of (at high-temperature) 24% helium and 74% hydrogen, together with a small proportion (about 2 per cent) of other heavier elements. The temperature at the core of the Sun is much higher (about 20 million K) than its surface (around 5,000K) . The Sun's gravity at its surface is 27 times that of Earth and, were it not for the enormous energis reactions of giant particle fields returning inwards and outwards from its core, the Sun would collapse inwards under the force of its own gravity. | ||
| The Sun's energis high pressure environment is derived from continuous nuclear fusion reactions from protons, through to electrons fused into more complex structures. The strongest particle to particle reaction is single protons being fused into pairs ( Helium proton cores). | ||
| The Sun is about 1.44 million km in diameter- more than 100 times that of the Earth. As it is composed mainly of light gases, its average density is, however much less than that of Earth- only about one quarter. The average distance of the Sun from the Earth is about 150 million km. Most of its energy is given off in the form of ultraviolet radiation, but the Sun also radiates all other wavelengths in the electro magnetic spectrum including very short gamma rays and x-rays and the longer wavelength microwaves and radio waves. | ||
| Similar to what we now understand from Chapter 10, the particles radiated from the Sun in large part constitute massive particle fields that effectively "hold together" the framework of the Solar system. | ||
| We also understand from Chapter 10, that the Suns cycles of input-output balance of particle fields corresponds a period of higher attraction (higher input) than output= and a period of higher output than input. | ||
| We also understand that this cycle means a period of around one to two years at the end of one cycle whereby input (inbound energis particles) and output (outbound energis particles) are at there most unbalanced. | ||
| 11.3.2 | The particles discharged from the Sun |  |
| Our Sun, consistent with other self-luminous stars, produces an array of different particles, with most types reaching Earth. It emits around 7 million tonnes of material per second. However contrary to contemporary science, the Sun also attracts back (via its powerful ergon particle fields) a similar but not equal amount. | ||
| Consistent with real life analysis in Chapter 7 and 8 of this book, all particles from the Sun are fused together into naturally corresponding "packets" in the Chromosphere of the Sun. These packaged particle groups travel across space and are either reflected or absorbed by the Earth's atmosphere. | ||
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