Solar prominence

Definition and stakes

Portrait of Richard A. Proctor Richard A. Proctor,  Myths and Marvels of Astronomy

“ I have addressed hundreds of audiences in Great Britain and America on the subject of recent solar discoveries, and I have conversed with many hundreds of persons of various capacity and education, from men almost uncultured to men of the highest intellectual power; and my invariable experience has been that solar research derives its chief interest when viewed in relation to the sun's position as the mighty ruler, the steadfast sustainer, the beneficent almoner of the system of worlds to which our earth belongs. ”
Source: Gutenberg

Portrait of Robert Stawell Ball Robert Stawell Ball,  In the High Heavens (1910)

“ There seems no escape from the conclusion that the continuous loss of solar heat must still go on, so that the sun will pass through the various stages of brilliant incandescence, of glowing redness, of dull redness, until it ultimately becomes a dark and non-luminous star. In this final stage the sun will only pass into that state in which the majority of the bodies in the universe are already found. Every analogy would teach us that the dark and non-luminous bodies in the universe are far more numerous than the brilliant suns. ”
Source: Wikisource

Isaac W. Heysinger,  The Source and Mode of Solar Energy Throughout the Universe

“ What principle of conservation of energy is it possible to apply to the vast quantities of light and heat which constantly disappear in the interstellar realms of space? How to account for this enormous emission of solar energy during the long period of time requisite for the development of the earth during its past geological ages. How to explain why the moon always presents the same face to the earth. Why, if the law of gravity prevails there, there are no visible traces of atmosphere or moisture in the moon. ”
Source: Gutenberg

Get perspective with Kwize: daily news enlightened by great literature