Tutorial 0: Finding your way around CurvedLand
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| Curved Space View | 
The blue circle at the center of the screen represents the curved space that 
you are occupying. The space illustrated by the CurvedLand applet is space of
constant positive curvature; this is mathematically equivalent to the surface
of a sphere. For more information about this model, click
here. 
For the purposes of analysis, we will always assume that
you are at the North Pole on the surface of a sphere. The default for the 
applet is to show 90 degrees of the 
surface of the sphere in either direction; this means that you would be able to
 see all the way to
 the equator from the North Pole. You can adjust this visible angle by 
adjusting the slider labeled view size. 
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| Shape Selection | 
Adjusting the view size will not do much until you have something drawn in your space. You can draw shapes in the space by selecting a type of shape using the radio buttons at the left side of the applet, and clicking and dragging in the space. You will notice that there are two types of shapes: true shapes and apparent shapes. True shapes are shapes defined according to the geometrical definitions in curved space; true lines are lines that follow great circles, or the geodesics in this type of space (to learn more about geodesics, read 
Tutorial 1), and true circles consist of all of the points equidistant
 from a center point. Apparent shapes are shapes that appear to be 
flat-space true shapes from your current perspective. The screen can be cleared
 of all of the shapes by pressing the erase button, or by pressing the center 
key on the numerical keypad when Num Lock is turned off. 
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| Navigation Buttons | 
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| Navigation Controls | 
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| Trail Controls | 
Once you have drawn shapes, you can move around in the space and watch how 
those shapes start to distort from your perspective. To move, use the 
navigation arrows in the upper right-hand corner of the applet. It is also 
possible to move using the arrow keys on the keyboard, or the arrow keys on the
 numerical keypad (usually found on the right side of PC keyboards for desktop
 computers). In order to make the arrow keys on the numerical keypad work 
properly, ensure that Num Lock is turned off. Notice that you can also 
rotate using the buttons in the upper 
corners of the navigation button panel; another way to achieve rotation is by 
using the
 upper corner keys on the keyboard's numerical keypad. 
To control the size of the steps 
you take each time you press a step button, adjust the step-size slider. You 
can also control the angle that you rotate through each time you press the 
rotate button by adjusting the rotation angle slider. In addition to this, the
total distance you have traveled will be displayed on the right-hand side of 
the applet. You can reset this distance to 0 by pressing the reset button. You
 can also make a trail appear behind you showing where you have been; to do 
this, click the trail on button in the top left-hand corner of the applet. Next
 to this button is a clear trail button; this allows you to erase the trail 
(clear it from memory). 
General relativity states that space-time is curved, yet we experience 
space-time as flat. When we draw a triangle, the angles add up to 180 degrees,
 and when we draw a circle, the ratio between circumference and diameter is pi.
 If we live in curved space-time, how can these things still be true? The key 
here is that, on a local level, curved space-time (or space) can be 
approximated by flat space-time; in other words, if you zoom in far enough, 
curved space looks flat. Try exploring this in the applet: zoom in to the 
smallest view size, and be sure to adjust the step-size slider as well so that 
steps remain inside the same view. Try drawing shapes and watching how they 
react as you move through the space. Compare this to how you expect shapes to 
change as you move through flat space. 
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| Viewing 360 Degrees | 
Next, try taking the view size to the other extreme. If you zoom all the way 
out by adjusting the view size slider so it is at its maximum value, the 
curvature of the space becomes very apparent (to move around, you may also 
want to increase the step size). The view size value should now be 360 degrees;
 this means that you can see 360 degrees around the sphere in either direction.
 Essentially, what you see in this view is all the way around the sphere and 
back to yourself. Turn the trail on; you should see a green circle that goes 
all the way around the edge of the visible space. This green circle represents 
you. If you were actually in this space, and you could see this far in every 
direction, then you would just see yourself. 
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| Sight Lines on an Embedding Diagram | 
Think of yourself as being at the 
North Pole; if you draw a shape 
that crosses the South Pole then you will also see that shape in all 
directions (represented as a yellow circle at 180 degrees from the center).
Draw some shapes in the space; each shape you draw should show up twice 
(although the two versions may look different from one another). This is 
because you will see each shape once before the South Pole, and once after the
 South Pole; if you think about your sight lines as rays reaching outward from
 the North Pole, those sight lines will first pass through all of the shapes 
on their way down to the South Pole, and then they will pass through all of 
the shapes again on their way back up to the North Pole (where you are).
To see this example in an even more extreme form, you can increase the maximum
 view size allowed by the slider and increase your view size to see even more 
of the space. To do this, click on the "Reset Maximum Zoom" button. Then
 enter a new maximum zoom value; it might be useful to start with multiples of
 180 degrees. If you enter 720 degrees, and you adjust the view size to 720 
using the slider, how images of each shape will you see? At what angles will 
you see yourself? At what angles will you see a spot at the South Pole? What if
 you increase your maximum view size to 1440 degrees? 
A summary of the controls mentioned in this document is 
here. 
You can also display this summary inside the applet by clicking and dragging
the bar at the bottom to expand it. 
Copyright (C) 2010 Stephanie Erickson, Gary Felder
 
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