Crosses each upon their 50 Degrees, and the end of the Staff in the hollow of the Eye-bone, on the outside of the Eye, and bow the Head forward or backward, or over the one side or the other, till I see the utmost end of both the Crosses right one with the other, according as is shewn by these Lines AB and CD, as is apparent enough by the foregoing Figure; That the Sight-beams over the ends of the Crosses shall then agree with the Lines which might be drawn over the end of the Crosses, to the Point or Center at the end of the Staff, which doth agree with the Center of the Quadrant, or the beginning of the Equal Points upon which the Staff is marked. Keeping in memory such standing of the Staff, I take off the one Cross, and set the Staff again in the aforesaid manner to the Eye, and observe without any errour of the Eye.
In taking the Height of the Sun with the Cross-Staff, Men do use red or blew Glasses, for the saving and preserving the Eyes; yet it is notwithstanding a great let, and very troublesom for the Sight, especially if it be high: therefore the Quadrant and Back-Staff is much better, as will be shewed in the next Chapter.
Thus I have shewed you how to take an Observation by the Fore-Staff. The next thing that followeth in course will be to shew you how to work your Observation; which to do, take notice of these following Rules.
To Work your Observation.
IF the Sun hath North Declination, and be on the Meridian to the Southwards of you, then you must substract the Sun's Declination from your Meridian Altitude, and that Remainder is the Height of the Aequinoctial, or the Complement of the La∣titude North. But if the Sun hath South Declination, you must add the Sun's De∣clination to your Meridian Altitude, and the Sum is the Height of the Aequator, or the Complement of the Latitude North. If the Sun hath North Declination, and be on the Meridian to the Northwards, then add the Sun's Declination to his Meridian Al∣titude, and the Sum is the Height of the Aequator, or the Complement of the Latitude South, if the said Sum doth not exceed 90 deg. but if it doth exceed 90 deg. you must substract 90 deg. from the said Sum, and the Remainder is your Latitude North.
If the Sun hath South Declination, and be to the Northwards at Noon, you must then substract the Sun's Declination from his Meridian Altitude, and the Remainder is the Complement of your Latitude South. When the Sun hath no Declination, then the Meridian-Altitude is the Complement of the Latitude. If the Sun be in the Ze∣nith, and if at the same time the Sun hath no Declination, then you are under the Aequinoctial.
But if the Sun hath North Declination, and in the Zenith, then look how many Degrees and Minutes the Declination is, and that is the Latitude you be in North.
But if your Declination be South, then you are in South Latitude. If you observe the Sun or Star upon the Meridian beneath the Pole, then add your Meridian Alti∣tude to the Complement of the Sun or Stars Declination, and the Sum is the Height of the Pole.
Rules for Observation in North Latitude.
SUppose I am at Sea, and I observe the Sun's Meridian Altitude to be 39 deg. 32 min. and the same time the Sun's Declination is 15 deg. 20 min. North; I de∣mand the Latitude I am in.
|
deg. |
min. |
The Meridian Altitude |
39 |
32 |
The Declination North, subst. |
15 |
20 |
The Complement of the Lat. |
24 |
12 |
|
90 |
00 |
The Latitude I am in |
65 |
48 North. |