Selected quad for the lemma: heaven_n

Word A	Word B	Word C	Word D	Occurrence	Frequency Band	MI	MI Band	Prominent
heaven_n	day_n	earth_n	light_n	7,461	5	6.5502	4	true

Text snippets containing the quad

ID	Title	Author	Corrected Date of Publication (TCP Date of Publication)	STC	Words	Pages
A80180	The lighting colomne or sea-mirrour containing the sea-coasts of the northern, eastern and western navigation: setting forth in divers necessarie sea-cards all the ports, rivers, bayes, roads, depths and sands ... With the discoveries of the chief countries, and on what cours and distance they lay one from another ... As also the situation of the northernly countries, as islands, the strate Davids, the isle of Ian-Mayen, Bear-Island, Old-Greenland, Spitsbergen and Nova Zembla ... Gathered out of the experience and practice of divers pilots and lovers of the famous art of navigation. By Jan van Loon. Whereunto is added a brief instruction of the art of navigation, together vvith nevv tables of the suns declination, also an almanack extending untill the yeare 1661.	Colom, Jacob Aertsz, 1599-1673.	1654 (1654)	Wing C5401A; ESTC R230954	549,120	428

THE Lighting Colomne OR SEA-MIRROUR Containing The Sea-Coasts of the Northern Eastern and Western Navigation setting forth in divers necessarie Sea-Cards all the Ports Rivers Bayes Roads Depths and Sands very curiously placed on its due Polus-heighth furnished with the discoveries of the chief Countries and on what cours and distance they lay one from another Never heretofore so clearly laid open and here and there very diligently bettered and augmented for the use of all Sea-men As also The Situation of the Northernly Countries as Island the Strate Davids the Isle of Ian-Mayen Bear-Island Old-Greenland Spitsbergen and Nova Zembla adorned with many Sea-cards and Discoveries Gathered out of the experience and practice of divers Pilots and Lovers of the famous Art of Navigation By JAN VAN LOON VVhereunto is added a brief Instruction of the Art of Navigation together vvith nevv Tables of the Suns Declination also an Almanack extending untill the yeare 1661. At AMSTERDAM Printed by JOHN JOHNSON Bookseller dwelling upon the Water in the Passe-card 1654. A SH RT Instruction in the Art of Navigation THe art of Navigation is a Science by which through certaine rules you may steere a Shipp over the Seas from one place to another and is not improperly devided into two parts to witt into ordinary and extraordinary Navigation The ordinary Navigation useth no other Instruments then the Compasse and sounding Plummet as principally consisting in experience and practice in knowledge of Lands and Corners how they are different in Points and distances and are knowne from the Sea in depths shoales qualityes of grounds the running and falling of Streames upon what point the Moone maketh high water in every severall place such like which in part are learned from the information of experienced Pilots but most out of our owne experience Extraordinary Navigation useth besides the foresayd ordinary practise divers other private Instruments and rules which must bee taken out of Astronomy and Cosmography It is therefore needfull that every Pilot who will use and practise th●s extraordinary Navigation must first of all bee well instructed in the principales of the same Arts that is that hee know and understand the proportions and devisions of the Spheare of the World the motions of the Heavens especially the eighth fourth and first together with the Fabrique of the Instruments without which knowledge its impossible to accomplish happily greate and never before sought out Voyages over the Vast Seas And seeing that such knowledge may bee attained out of good Instruction wee have here set downe in this Tractate for the benefit of young seamen who are desiruns to bee Pilots as cleare and plaine rules as the shortnesse hereof could suffer The first Point Of the Sphere and the divers motions thereof A Spheare properly is called a Ball wholly entire and round whose superficies and outside is ever● where alike distant from its center By that World Sphoera Mundi or Spheare of the World wee understand commonly the whole Ball of the Heavens with all that is therein contained and it is devided into two parts Elementary Coelestiall the Elementary part hath againe 4 parts the first is the earth which with the water as the second maketh a compleate Ball upon which wee dwell The third is the Aire encompassing the earth and the fourth is the fire which according to the opinion of Philosophers containeth the space which is betweene the Aire and the Spheare of the Moone From these Elements which are the beginning of all things which are alwayes subject to changes together with the Warmth of the Heavens arise and perish by a continuall change and alteration of the one into the other all things which wee see and find upon Earth The Celestiall part containing within in its Hollownesse the Elementaryes is pure shining Seperate and voyd of all changes is devided into 8 Speares or round Hollow Balles which are called Heavens whereof the greatest alwayes containeth one the other in manner of a Ball the seaven lowest have but every one one Starre or Plannet whereof the first next the Earth is the Heaven of the Moone the second of Mercury the third of Venus the fourth of the Sonne the fifth of Mars the sixth of Iupiter the seaventh of Saturne and the eigth of all the fixed starrs The number of these Heavens are knowne by their Courses which wee see in them round about the Poles of the Zodiaque The Moone runneth through her Heaven by her own naturall course from West to East in 27 dayes 8 howres Mercury Venus and the Sunne theirs in a yeare Mars his in two yeares Iupiter his in 12 and Saturne in 30 yeares The eighth heaven perfects its owne course according to the affirmation of Tycho Brahe in 25400 yeares These Heavens are turned about all alike in four and twenty houwres on the Poles about the Axes of the World by the ninth Heaven which is called the Primum Mobile that is the first mover by which Motion in our sight is caused Day and Night and the daily rising and falling of the heavenly lights The Second Point Of the Roundnesse of the Earth THat the Earth with the Water together maketh a round Globe appeareth not onely out of experience very clearely but also out part of the Shaddow of Earth in the Eclips of the Moone In whatsoever part of the Heaven the moon is Eclipsed or touched by the Shaddow of the earth that Shaddow seemeth alwayes round If the earth were foure square three corned or of any other forme then the Shaddow of the moone should bee also foure square three cornerd or some other forme For of what proportion any body is such also must bee the Shaddow thereof And seeing therefore that the Shaddow of the earth is alwayes and on al sides round the earth itselfe must alsoo bee necessarilly round That the Heaven is round wee marke from the eye but is most clearely perceived from the Circular motions of the heavenly lights as of the Sonne Moone and Starres The Third Point that the Earth is in the middle of the World THat the earth standeth in the middle of the World may clearely bee understood by what is hereafter spoken for if soo bee that the Globe of the earth stood not in the middle of the World but that the heaven was nearer it on one side it would come to passe that the stars in their daily courses should bee nearer on one side of the earth then on the other and by that meanes should appeare to our sight to bee greater on one side of the earth then on the other likewise if that part of the heaven next to the earth were a boveus we should then see lesse then halfe of the heaven according to instruction of the first Figure and on the contrary when that part of the heaven farthest from us were above us wee should then see more then halfe of the Heaven according to the Instruction of the second Figure But standing upon the flatt side

of the Globe wee see the Starres as well on the one side as on the other in whatsoever part of the Heaven that it is alwayes of one greatenesse and it is found by experience that wee alwayes see the one half of the Heaven and the other halfe is hidden from our eyes from thence it appeares plainly according to the expression in the third Figure That the earth stands in the middle of the World From thence is likewise to bee marked that the Globe of the earth is no more to bee likened by the Heavens then a point without thicknesse for if the earth had any thicknesse in respect of Heaven wee should standing upon the earth by that reason not see halfe of the Heaven according to Demonstration of the 4 Figure The fourth Point Of the greatnesse of the Earth ALthough the Globe of the Earth as is sayd in respect of the extraordinary widenesse of the Heaven is no more then a point neverthelesse in respect of its selfe it is a greate body having in its Compasse 5400 dutch Miles And that is knowne by this meanes If you devide the whole Circkle of the Compasse of the earth into 360 parts or degrees and wee find as well by Navigation as by measuring of Land that such a Degree or part containeth fifteene such Dutch Miles 360 such part beeing multiplyed by fifteene make out 5400 Duth miles The fifth Point Of the Axis and Poles or Axepoints of the World IN the Globe of the World is imagined to bee a Line going from one Point on the side of the Spheare as a Diameter through the Center to another Point right against it on the other side That Line is called the Axis and the outermost-ends thereof or the foresayd Points the Poles or Axepoints of the World the one towards the North and is called the Northerne Pole and the other towards the South called the Southerne Pole Upon whichs Poles it is imagined that the Spheare is upon its Axeltree daily turned The Demonstrastion THE Line A.G.B. in this Figure going from the Point A through the Center G as a Diameter to the Point B right against it sheweth the Axel of the World and the Points A and B the Poles A to the North the Northerne and B to the South the Southerne Poles The Sixth Point Of the Aequinoctiall Line IN the middest of the Heavens every where equally distant from both the Poles is imagined a greate Circle dividing the whole Spheare into two equall parts which is called the Aequinoctial because when the Sonne commeth to or under that Cirkle which commeth to passe the 21 of March and the 23 of September the day and night are in all places of the Earth of an equall length The knowledge of this Cirkle is proffitable above all things in Navigation to know thereby how farr wee goe either to the Northwards or Southwards upon Earth thereby also is reckoned the time and hower of the day the Declination of the Sonn and Starrs and more other proffitable things Demonstration IN the foregoing Figure A and B the Poles of the World C D E F is the Equinoctiall Line in the middest of the Heaven equally distant from both the Poles A and B dividing the whole Spheare A C B E into two equall parts as C A E the Northerne and C B E the Southerne part from hence is to bee noted Seeing that the whole Compasse of the Heavens is divided into 360 degrees that the Poles stand from one another 180 degrees and betweene the Poles and the Aequinoctiall remaineth every where on both sides 90 degrees This Line is marked in the Sea-cards with a red Line from east to west through the beginning of the degrees according as they are reckoned as well towards the North as to the South The Seventh Point Of the Ecliptique Line THE Ecliptique Line lyeth awry over the Equinoctiall deviding it in two points right over against one another in two equall parts and is also devided by it in two equall parts the one lyeth betweene the Equinoctiall and the North Pole the other betweene the Equinoctiall and the South Pole It s greatest Declination on both sides of the Equinoctaill towards both the Poles is 23 degree 31½ minutes and is devided into twelve equall parts and to each of them a severall signe applyed The Sonne goeth alongst this Circkle without ever going out of it and runneth through it with its owne naturall course every yeare once and even as the Poles of the World stand every where alike distant from the Equinoctiall even soo hath the Ecliptique alsoo its two Poles every were alike distant from the same Demonstration IN this Figure as before is sayd A B are the Poles of the World C D E F the Equinoctiall G D H F the Ecliptique Line cutting and dividing the Equinoctiall and its selfe alsoo into two equall parts in the points D and F which wee call the Equinoctiall the one at D the Spring Equinoctiall the other at F the Autumne Equinoctiall The one halfe D H F the northern part lyeth betweene the Equinoctiall D E F and A the North Pole at most declined towards F H 23 degrees and 31 2 minutes The other halfe F G D the Southern part lyeth betweene the Equinoctiall F C D and the South Pole B likewise at most declined as C G 23 degrees 31½ minutes The North part is devided into six signes which wee call the Northerly beginning at D with the Kimbug signes towards the North. Aries Taurus Gemini unto H. the point of the farthest declination From thence with the descending signes of the North Cancer Leo Virgo to the Equinoctiall Line in F. the Autumne Equinoctiall the southern part is also divided into six signes which wee call the Southerly beginning at F with the discending signes towards the South Libra Virgo Saggitarius untill G the Point of the sartkest Declination towards the South from thence further with klimbing signes towards the North Capricornus Aquarius Pisces as farr as till you come to the Equinoctiall line in the Spring Equinoctiall D. The Sunne runneth through the three first Northerly signes from the 21 of March new style to the 21 of June New styl the other from the 21 of Iune to the 23 of September The first 3 Southerly signes from the 23 of September to the 23 of December and the other from the 23 December till the 21 of March againe The Poles of the Ecliptique are M and N both of them standing every where alike distant from the Ecliptique G H and soo farre from the Poles of the World A and B as the Ecliptique is farthest declining from the Equinoctiall at H E and C G. The eighth Point Of the Coluri THe Coluri are two Circkles going Croswayes through both the Poles of the World dividing each other into two parts in the Poles and together with them the whole Globe Equinoctiall Zodiack or Ecliptique and all the Paralels in 4 equall parts the

houres 8 degrees which make 36 minutes it is then 13 houres 36 minutes from the noone tijde that is 1 houre 36 minut after midnight How to finde the ascension on any day in the yeere of the Sunne and the Stars we have here adjoyneth 2 tables the one of the Sunne showing from 5 dayes to 5 dayes the Sunnes ascension out of which you may easily finde the same in other dayes The other for thirtie of the primest fixed Starres both of them onely by degrees that being sufficient for this businesse The 18 Point A Table of the right ascensum of the Sunne The first number in the table shewed the day of the moneth the second of degrees of the ascension of the Sunne on that day Ianu. Febr. Mart. April May. Iuni. da. deg da. deg da. deg da. deg da. deg da. deg 5 287 5 319 5 346 5 14 5 42 5 73 10 292 10 324 10 351 10 19 10 47 10 78 15 297 15 329 15 355 15 24 15 52 15 83 20 303 20 334 20 360 20 28 20 57 20 88 25 308 25 339 25 4 25 33 15 62 25 94 31 314 28 342 31 10 30 38 31 68 31 99 Iulius Augu. Septe Octo. Nove. Dece da. deg da. deg da. deg da. deg da. deg da. eg 5 104 5 135 5 164 5 191 5 220 5 251 10 109 10 140 10 168 10 195 10 225 10 257 15 114 15 145 15 173 15 200 15 231 15 263 20 119 20 149 20 177 20 205 20 236 20 268 25 124 25 154 25 182 25 210 25 241 25 274 31 130 31 159 30 187 31 215 30 246 31 281 A Table of the right ascension of the primest Starres THe Girdle of Andromeda 12 degrees The clearest in the head of the Ram. 27 degrees Menkar the brtghtest in the mouth of the Whale 41 degr Aldebaran the south eye of the Bull. 64 degrees Capella in the left shoulder of Erichtonius 72 degrees Regel the left foot of Orion 74 degrees The Star in the left shoulder of Orion 84 degrees Syrius the great Dogge 97 degrees The North head of Gemini 180 degrees The South head of Gemini 111 degrees Procyon the little Dogge 110 degrees The brightest in the watersnake CorHydrae 137 degrees Regulns the Heart of the Lyon 147 degrees The tayle of the Lyon 172 degrees Vendemiatrix the right wing of Virgo 191 degrees Spica Virginis the eare of corne 196 degrees Arcturus the brightest in Bootes 210 degrees Arcturus the brightest in Bootes 218 degrees The South Waight 210 degrees The north Waight 224 degrees The brightest in the North Crowne 230 degrees Antares the Hart of the Scorpion 242 degrees The Head of Hercules 254 degrees The Head of Serpentarius 259 degrees The tayle of the Eagle 282 degrees Vultur the clearest in the Eagle 293 degrees The Star in the mouth of the horse Pegasus 521 degrees Formohant the brightest in the end of Aquarius 339 degr Marcab the sack or foot of Pegasus 342 degrees The uttermost in the wing of Pegasus 358 degrees The most Northerly in the Whales tayle 360 degrees The 19 Point Of the Horizon or the Circle that boundeth the sight WHere the heavens the earth or the waters seeme in our sight to meete together that is called the Horizon or the Circle bounding the sight because our sight endeth there can go no further by our Netherland Sea-farers it is also called the Kimmen This circle devideth the heavens just in two evē parts so that just the one halfe is seene by us here above and the other halfe can not be seene by us because it is hidden underneath us which happeneth in this manner The earth as in the first chapter is shewed standeth as a center in the middle of the heavens the which by reason of the unmeasurable quantitie or largenes thereof is so farre separated from the earth that the whole thicknesse of the Earth in respect of the heavens is no more then a poynt or prick or at least so little that it cannot be perceived by our sight and that which by our sight along upon the Earth or the Water we can comprehend which can not reach further then about three Dutch miles that is 10 English myles seemeth in our eyes by reason of the space so little to be no other then an halfe Globe falling perpendicular upon a plaine so that our sight falleth in the heaven as if we stood in the middle poynt of the world and saw-right compasse wise whereby it falleth out that just the halfe of the Heaven is seene by us and the other halfe is not seene by us in like manner as if a man should lay a line over the center of a Circle then the one halfe of the Circle is above and the other halfe is just under All the heavenly light as the Sunne Moone and Starres by the turning of the heavens comming above the Horizon are seene by us and going downe under it goe out of our sight The Zenith is the poynt of the heavens directly over our head and is on all sides equally distant from the Horizon it is also called the Pole of the Horizon An Explication The Horizon is too bee considered in The eye being eleva●ed above the water The visible Horizon is lower then ●he trues foote minutes 2 1 4 2 8 3 14 4 20 5 27 6 37 7 39 8 53 9 66 10 82 11 100 12 140 13 163 14 186 15 a two-fold manner according to the true and the visible the true goeth every way right waterpasse from our sight that is passeth through the Center of the Sphere as is sayd deviding it into equall parts is every way from the Zenith 90 degrees the just fourth parts of a Circle The Visible is the uttermost part of the Earth or Water that our eye can reach or see when our eye is just on the flatt or surface of the even Water then the true and Visible Horizon are one and the same but our eye lifted up above the surface of the Water the sight falleth over the Globe of the earth every where lower then water-passe and thence it followeth that the visible Horizon is lower than the true although this be not much materiall in the Art of Navigation for as much as it is recompenced by the refraction of the visible Horizon We have added this table for those that desire to be exact where men may see how much the visible differs from the true that being changed or altered by feet Example THe sight being elevated above the surface of the waters 14 feet in the 1 Columne in the 2 Columne over against it you find 4 min. which the visible Horizon is lower then the true The sight being lifted 140 feetabout the Horizon the visible wil be 13 mi. lower then the true The 20 Point Of the Meridian or Middle Circle THe Meridian is a Circle in the Heavens which we must conceive to passe through both the Poles of