Difference between revisions of "The Stars"

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The Stars <ref name="term_80011" />  
 
<p> Are mostly suns, but being, the nearest of them, at a distance from us more than 500,000 times our distance from the sun, are of a size we cannot estimate, but are believed to be 300 times larger than the earth; they are of unequal brightness, and are, according to this standard, classified as of the first, second, down to the sixteenth magnitude; those visible to the naked eye include stars from the first to the sixth magnitude, and number 3000, while 20,000,000 are visible by the telescope; of these in the [[Milky Way]] ( <i> q. v </i> .) alone there are 18,000,000; they are distinguished by their colours as well as their brightness, being white, orange, red, green, and blue according to their temperature and composition; they have from ancient date been grouped into constellations of the northern and the southern hemispheres and of the [[Zodiac]] ( <i> q. v </i> .), the stars in each of which being noted by the [[Greek]] letters, as [Greek: alpha], [Greek: beta], according to their brightness; they all move more or less, and some go round each other, and are called double according as there are two or more of them so revolving; besides stars singly visible there are others called Clusters Or [[Nebulæ]] ( <i> q. v </i> .). </p>
The Stars <ref name="term_80011" />
==References ==
<p> Are mostly suns, but being, the nearest of them, at a distance from us more than 500,000 times our distance from the sun, are of a size we cannot estimate, but are believed to be 300 times larger than the earth; they are of unequal brightness, and are, according to this standard, classified as of the first, second, down to the sixteenth magnitude; those visible to the naked eye include stars from the first to the sixth magnitude, and number 3000, while 20,000,000 are visible by the telescope; of these in the Milky Way ( <i> q. v </i> .) alone there are 18,000,000; they are distinguished by their colours as well as their brightness, being white, orange, red, green, and blue according to their temperature and composition; they have from ancient date been grouped into constellations of the northern and the southern hemispheres and of the [[Zodiac]] ( <i> q. v </i> .), the stars in each of which being noted by the Greek letters, as [Greek: alpha], [Greek: beta], according to their brightness; they all move more or less, and some go round each other, and are called double according as there are two or more of them so revolving; besides stars singly visible there are others called [[Clusters]] Or [[Nebulæ]] ( <i> q. v </i> .). </p>
 
== References ==
<references>
<references>
<ref name="term_80011"> [https://bibleportal.com/encyclopedia/the-nuttall-encyclopedia/stars,+the The Stars from The Nuttall Encyclopedia]</ref>
<ref name="term_80011"> [https://bibleportal.com/encyclopedia/the-nuttall-encyclopedia/stars,+the The Stars from The Nuttall Encyclopedia]</ref>
</references>
</references>

Latest revision as of 18:01, 15 October 2021

The Stars [1]

Are mostly suns, but being, the nearest of them, at a distance from us more than 500,000 times our distance from the sun, are of a size we cannot estimate, but are believed to be 300 times larger than the earth; they are of unequal brightness, and are, according to this standard, classified as of the first, second, down to the sixteenth magnitude; those visible to the naked eye include stars from the first to the sixth magnitude, and number 3000, while 20,000,000 are visible by the telescope; of these in the Milky Way ( q. v .) alone there are 18,000,000; they are distinguished by their colours as well as their brightness, being white, orange, red, green, and blue according to their temperature and composition; they have from ancient date been grouped into constellations of the northern and the southern hemispheres and of the Zodiac ( q. v .), the stars in each of which being noted by the Greek letters, as [Greek: alpha], [Greek: beta], according to their brightness; they all move more or less, and some go round each other, and are called double according as there are two or more of them so revolving; besides stars singly visible there are others called Clusters Or Nebulæ ( q. v .).

References