A treatise of astronomy: Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
London
Printed for S. Wilmot, bookseller in Oxford; and for E. Easton, bookseller in Silver-street, Sarum
M.DCC.XXXVIII. [1738]
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| Schlagworte: | |
| Online-Zugang: | UEI01 BSB01 LCO01 SBR01 UBA01 UBG01 UBM01 UBR01 UBT01 UER01 Volltext |
| Beschreibung: | English Short Title Catalog, N53372 Reproduction of original from British Library With a final advertisement leaf |
| Beschreibung: | Online-Ressource (xx,202,[2]Seiten,plates) 8° |
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| index_date | 2024-07-03T22:37:01Z |
| indexdate | 2024-07-10T09:59:37Z |
| institution | BVB |
| language | English |
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| publishDate | 1738 |
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| publisher | Printed for S. Wilmot, bookseller in Oxford; and for E. Easton, bookseller in Silver-street, Sarum |
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| spelling | Shuttleworth, John 1670 or 71-1750 Verfasser aut A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum London Printed for S. Wilmot, bookseller in Oxford; and for E. Easton, bookseller in Silver-street, Sarum M.DCC.XXXVIII. [1738] Online-Ressource (xx,202,[2]Seiten,plates) 8° txt rdacontent c rdamedia cr rdacarrier English Short Title Catalog, N53372 Reproduction of original from British Library With a final advertisement leaf Online-Ausg Farmington Hills, Mich Cengage Gale 2009 Eighteenth Century Collections Online Electronic reproduction; Available via the World Wide Web |2009|||||||||| Astronomy Early works to 1800 http://nl.sub.uni-goettingen.de/id/1540001400?origin=/collection/nlh-ecc Verlag Volltext |
| spellingShingle | Shuttleworth, John 1670 or 71-1750 A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum Astronomy Early works to 1800 |
| title | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_auth | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_exact_search | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_exact_search_txtP | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_full | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_fullStr | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_full_unstemmed | A treatise of astronomy Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| title_short | A treatise of astronomy |
| title_sort | a treatise of astronomy wherein the diurnal motions of the heavenly bodies and the annual motion of the sun and the sun s various distances from the earth together with the inequabilities of the sun s motions throughout the year are accounted for according to the ptolemaick semi tychonick and copernican systems and particularly the third motion of the earth and the application of it in accounting for the sun s apparent motions in the copernican system is set forth by a machine described in its proper place wherein also rules founded upon known optical principles are deliver d for determining the angles of refraction of the sun moon and stars at all altitudes above the sensible horizon and wherein the sun s diurnal parallax is determined by demonstrations founded upon most authentick observations by john shuttleworth a m prebendary of sarum |
| title_sub | Wherein the diurnal motions of the heavenly bodies, and the annual motion of the sun, and the sun's various distances from the Earth, together with the inequabilities of the sun's motions throughout the year, are accounted for according to the ptolemaick, semi-tychonick and Copernican systems; and particularly the third motion of the earth, and the application of it in accounting for the sun's apparent motions in the Copernican system, is set forth by a machine described in its proper place: Wherein also rules, founded upon known optical principles, are deliver'd, for determining the angles of refraction of the sun, moon, and stars at all altitudes above the sensible horizon; and wherein the sun's diurnal parallax is determined by demonstrations, founded upon most authentick observations. By John Shuttleworth, A.M. prebendary of Sarum |
| topic | Astronomy Early works to 1800 |
| topic_facet | Astronomy Early works to 1800 |
| url | http://nl.sub.uni-goettingen.de/id/1540001400?origin=/collection/nlh-ecc |
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