The astronomy of comets: In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Bury St. Edmund's
printed by P. Gedge, for J. Murray, No 32, Fleet-Street, London; and sold by all the booksellers
MDCCLXXXVI. [1786]
|
| Schlagworte: | |
| Online-Zugang: | UEI01 BSB01 LCO01 SBR01 UBA01 UBG01 UBM01 UBR01 UBT01 UER01 Volltext |
| Beschreibung: | English Short Title Catalog, T110886 Reproduction of original from British Library With a list of subscribers |
| Beschreibung: | Online-Ressource (xvi,90Seiten,plate) 8° |
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| illustrated | Not Illustrated |
| index_date | 2024-07-03T22:34:57Z |
| indexdate | 2024-07-10T09:56:20Z |
| institution | BVB |
| language | English |
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| physical | Online-Ressource (xvi,90Seiten,plate) 8° |
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| publishDate | 1786 |
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| publisher | printed by P. Gedge, for J. Murray, No 32, Fleet-Street, London; and sold by all the booksellers |
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| spelling | Hancock, Blyth 1721 or 2-1795 Verfasser aut The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics Bury St. Edmund's printed by P. Gedge, for J. Murray, No 32, Fleet-Street, London; and sold by all the booksellers MDCCLXXXVI. [1786] Online-Ressource (xvi,90Seiten,plate) 8° txt rdacontent c rdamedia cr rdacarrier English Short Title Catalog, T110886 Reproduction of original from British Library With a list of subscribers Online-Ausg Farmington Hills, Mich Cengage Gale 2009 Eighteenth Century Collections Online Electronic reproduction; Available via the World Wide Web |2009|||||||||| Comets Early works to 1800 Solar system / Early works to 1800 http://nl.sub.uni-goettingen.de/id/0034600900?origin=/collection/nlh-ecc Verlag Volltext |
| spellingShingle | Hancock, Blyth 1721 or 2-1795 The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics Comets Early works to 1800 |
| title | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_auth | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_exact_search | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_exact_search_txtP | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_full | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_fullStr | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_full_unstemmed | The astronomy of comets In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| title_short | The astronomy of comets |
| title_sort | the astronomy of comets in two parts part i containing a physical account of the solar system the whole theory of comets with the rationale or physical causes of these phoenomena from the earliest ages to the present time part ii containing the practical methods of calculation first by the properties of the parabola without tables and secondly by tables prefixed to the work with the construction of the tables whereby the place and distance of comet from the earth together with its latitude and longitude in the ecliptic may for any time be known by any one who has but a common skill in plane trigonometry the whole process of calculation exemplified in the comet which is expected to make its appearance in the year 1789 by blyth hancock teacher of the mathematics |
| title_sub | In two parts. Part I. Containing a physical account of the solar system; the whole Theory of Comets, with the Rationale, or Physical Causes of these Phoenomena, from the earliest Ages to the present Time. Part II. Containing the practical methods of calculation. First, by the Properties of the Parabola without Tables; and secondly, by Tables prefixed to the Work, with the Construction of the Tables, whereby the Place and Distance of Comet from the Earth, together with its Latitude and Longitude in the Ecliptic, may, for any Time, be known, by any one who has but a common Skill in Plane Trigonometry. The whole Process of Calculation exemplified in the Comet which is expected to make its Appearance in the Year 1789. By Blyth Hancock, Teacher of the Mathematics |
| topic | Comets Early works to 1800 |
| topic_facet | Comets Early works to 1800 |
| url | http://nl.sub.uni-goettingen.de/id/0034600900?origin=/collection/nlh-ecc |
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