From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl
From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl
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In our eReader you can find the full English version of the book. Read From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl
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Their distribution, so different from that of all other ob- jects, may be considered to show that they have no unity with the rest; but there are other bodies, the stars of Type M for in- stance, which remain indifferent to galactic influence. Indeed, the mere fact that spiral nebulae shun the galaxy may indicate that they are influenced by it. The alternative view is that, lying altogether outside our system, those that happen to be in low galactic latitudes are blotted out by great tracts of ...absorbing mat- ter similar to those which form the dark spaces of the Milky Way.
If the spiral nebulae are within the stellar system, we have no notion what their nature may be. That hypothesis leads to a full stop. It is true that according to one theory the solar system was evolved from a spiral nebula, but the term is here used only by a remote analogy with such objects as those depicted in the Plate. The spirals to which we are referring are, at any rate, too vast to give birth to a solar system, nor could they arise from the disruptive approach of two stars; we must at least credit them as capable of generating a star cluster.
What to read after From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl?
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To quickly assess the difficulty of the text, read a short excerpt:
Their distribution, so different from that of all other ob- jects, may be considered to show that they have no unity with the rest; but there are other bodies, the stars of Type M for in- stance, which remain indifferent to galactic influence. Indeed, the mere fact that spiral nebulae shun the galaxy may indicate that they are influenced by it. The alternative view is that, lying altogether outside our system, those that happen to be in low galactic latitudes are blotted out by great tracts of ...absorbing mat- ter similar to those which form the dark spaces of the Milky Way.
If the spiral nebulae are within the stellar system, we have no notion what their nature may be. That hypothesis leads to a full stop. It is true that according to one theory the solar system was evolved from a spiral nebula, but the term is here used only by a remote analogy with such objects as those depicted in the Plate. The spirals to which we are referring are, at any rate, too vast to give birth to a solar system, nor could they arise from the disruptive approach of two stars; we must at least credit them as capable of generating a star cluster.
What to read after From Nebula to Nebula Or the Dynamics of the Heavens Containing a Broad Outl?
You can find similar books in the "Read Also" column, or choose other free books by George Henry Lepper to read onlineMoreLess
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