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How to Determine Longitudinal DIstances By Hersius Introduction These articles have continually promoted the believability of the fictional world that John Norman created for the Gor series. Part of the insistence on the verisimilitude of the fictional planet Gor is negative - the refutation of the distortion of distance found on many online maps. For example, the Tahari is not a miniscule blob hugging a supposed crook in the Voltai chain; the rainforests likewise do not comprise a small geographic inconvenience; and Torvaldsland does not span halfway across the northern forests. The other part is positive - the promotion of the simple ideas that when you have a planet of ballpark-definable size, then (1) you have only a set amount of territory in which to locate the places in the books; (2) the placements have constraints based on climate; (3) Norman’s climate-based geography is, in general terms, discoverable; (4) the placements have constraints based on their locales relative to each other; and (5) typographical errors in the texts do not nullify a self-consistent geographic scheme. One starts, then, with an idea of the size of Gor. Gor is smaller than Earth, so you have less overall space on which to project places. In the March 2003 TGV I argued for the comparison to therefore be made with Venus, since the diameter of Venus is 95% that of Earth. You can pick a size either slightly larger or slightly smaller than Venus to conceptualize the size of Gor. For these articles, I chose a size narrowly smaller so that I would have a figure, expressed in pasangs, that was easy to work with mathematically. This allows for the imposition of longitude and latitude grids and so prepares the blueprint. Next, since Gor is an Earth-like planet not in an ice age, the climate-based geography of Gor must correspond in general to the climate-based geography of Earth. In the February 2003 TGV I presented a latitude-based climate comparison of Gor and Earth based on information that would have been available to Norman at the outset of his creation of the Gor books. The comparison chart shown in the article strengthens the idea that Norman based his planetary geology on latitude-based climate ideas. This only makes since: the Tahari would not be expected to be found at polar latitudes, nor would a Vosk River that freezes in places in the winter be expected to be found in tropical locales. Once climate zones can be placed on the planet, then specific places can be projected relative to each other. City A is southwest of City B; Town C is west of Town D; and, if we are lucky, Place E is 400 pasangs from Place F. When you take into account that a planet has a curved surface, you then realize with a wince that you must use geometry to construct distances between planetary points. These articles have proposed distances and longitude - latitude coordinates for places using assumptions that have been openly held from the beginning. This month, you get to see the math and the resulting tables behind those projections.
The Formula The formula for longitudinal distance is: 1 degree = 2 x pi x Radius x cosine of latitude / 360 Notice that 2 x pi x Radius is the circumference and that the circumference divided by 360 gives 1 degree around the circle. As a sphere or spheroid approaches a pole, the circle gets smaller. The circumferences of the smaller circles are found by introducing the cosine of the latitude into the equation. As shown in the February TGV article, one degree of longitude at the equator of Venus is roughly 90 pasangs. I chose 85 pasangs to be the measure of one degree of longitude at the equator of Gor. Whatever distance is chosen determines the attributed distances from that time onward. As long has one has a starting point, one can derive distances, so not only can your mileage actually vary but you can determine by how much it varies! Choosing 85 pasangs as the measure of one degree of longitude at the equator yields a planetary radius of 4,868 pasangs at the equator. Rounding pi to 3.14 or using actual pi gives the final staple for the formula. A cosine table provides the final tool. Here is an example problem to be solved: The solution:
Application Here are the tables used in these articles to determine longitudinal distances at different latitudes. If you prefer different starter numbers you can create your own similar tables using the above formula. Down = Latitude, Across = Longitude So, by this table, 60 degrees of longitude covers a whopping 5100 pasangs at the equator but only a mere 440 pasangs near the north and south poles at 85 degrees latitude. At the equator, that same 44o pasangs spans just over 5 degrees of longitude. |