In the Second Part, being GENE∣RAL [ 40] GEOGRAPHY.
Treats of the Affections of the Places of the Earth, depending on the apparent Motion of the Stars.
Chap. 22.—Folio 203. [ 50]
TReats of Things necessary to be fore∣known in Geography.
Chap. 23.—Folio 207.
OF the LATITVDE of Places, and the Elevation of the Pole. Shewing, that the Latitude of a place in the Superficies of the Earth is the distance of the same from the Aequator. That [ 60] the Elevation of the Pole of any place, or above the Horizon of any place, is called the Arch of the Coelestial Meridian of that place intercepted between one and the other Coelestial Pole, and the Horizon of that place. The place being given in the Superficies of the Globe, so to constitute the Globe, that the Wooden Horizon may be the Horizon of that place. A place being given in the Superficies of the Globe, or the Latitude of any place being given, to shew all the places of the Earth, which may have the same Latitude, or Distance from the Aequator, or Elevation of the Pole; or to find all the places of the Earth, which may have the distance given from the Aequator. How to find the Meridian, and Point of the North and South in the given place of the Earth. To place a Globe, so that the Car∣dines of the same, may respect the Cardines of the Earth, that is, that the Brazen Meridian may be seated in the true Meridian of the Place. To find the Latitude of the place from the Hea∣ven, or the Elevation of the Pole above the Ho∣rizon of any place by the benefit of the Stars. The places of the Earth (under the Aequator) have no Latitude, but both Poles lye in their Horizon. The places under the Poles have the Latitude of 90 Degrees; viz. the Pole in the Vertex, and the Aequator in the Horizon. The places between the Poles and the Aequator, have a less Latitude than 90 Degrees.
Chap. 24.—Folio 213.
TReats of the Division of the Earth into ZONES; and the Caelestial Appearances in the divers Zones; Shewing, that from the proper or Annual Motion of the Sun, there ari∣seth a certain Division of the Superficies of the Earth into five Zones, as already treated of; and that the Aequator of the Earth passeth through these places there taken notice of. In the places that lye in the Tropicks, the Sun once a Year is only vertical on the Meridies, or Noon∣stead; but in places under the Torrid Zone he is vertical twice a Year, viz. two Days, which are equally distant from the longest Day. But in places without the Torrid Zone, and seated with∣out the Tropicks, the Sun never in any Day of the Year is vertical. To Places seated in either of the Frigid Zones, the Sun every Year (some Day or other) setteth not, and so many Days riseth not; and that so many Days the more, by how much those Days are nigh the Poles; so that in a whole place of the Pole for six Months it setteth not, and riseth not to another. But in places in the Artick and Antartick Circle the Sun setteth not one Day in the Year, and one Day riseth not; but other Days it sets and riseth. That in Places seated without the Frigid Zone, that is, in the Temperate, or Torrid Zones, the Sun every Day riseth and setteth.
Chap. 25.—Folio 220.
TReats of the LONGITVDE of the Days in divers places of the Earth; and of the Division of the Earth into Climates, which proceed from them. That in two Days of the Year are the Aequinoxes, or the Night is equal to the Day in all places of the Earth. In places seated in the Aequator, the Days and Nights are always equal: In the places of the Poles there is only one Day and one Night in the whole Year: Now the Day is longer than the Night in