The purpose of this test is to revise the concepts that you have learned throughout your schooling and get you to think critically about some of the concepts that we will encounter in the next few weeks.
Do send me the solutions once you are done! Have fun, take as much time as you need. Note that you are allowed to use calculators and any other resources you wish (just don’t look up the answers! If you do that, you are only harming your progress and understanding of the subject)
Suppose you are given two equations, $a_1 x + b_1y = c_1$ and $a_2x+b_2y = c_2$. Here $x,y$ are unknowns and $a_2,a_2, b_1, b_2, c_1 , c_2$ are constants. Can you find the values of $x$ and $y$ in terms of these constants using the process of elimination?
Can you extend the process of elimination to the following system of three equations? Again, $x,y,z$ are variables all others are constants.
$$ \begin{align*}
a_1x + b_1 y + c_1 z &= d_1 \\ a_2x + b_2 y + c_2 z &= d_2 \\ a_3x + b_3 y + c_3 z &= d_3 \\
\end{align*} $$
Can you find the solution to the following equation $x^4 + ax^2 + b = 0$ in terms of $a$ and $b$?
Suppose you are given two finite sets $A$ and $B$. What is the condition for these two sets to be equal?
Prove the basic trigonometric identities :
$$ \begin{align*}
&\sin^2 x + \cos^2 x = 1 \\ &\cot^2 x + 1 = \csc^2 x \\ &\tan^2x + 1 = \sec^2x
\end{align*} $$
How would you prove that two triangles are congruent without using the congruence test? What does it mean for triangles to be congruent?
We will now see how you can calculate the circumference of earth (at the equator) using just basic trigonometry. The following method is the simplified method that Eratosthenes (~240 BC in Ancient Greece).
The assumption of this method are as following,
Here’s the process (and a bit of history) — Eratosthenes travelled between two cities, the city of Alexandria (which we call point B) and the city of Syene (which we call point A for simplicity). He knew exactly at what time of the day the sun was directly overhead in Syene, thus casting no shadow, this was noon. He then went to Alexandria and calculated the angle at of sun’s elevation.
He did this by keeping a stick vertically upright (assume the length of the stick was 1 meter) and then measuring the shadow cast by the sun rays of the stick. This is depicted in the following figure,
Now, suppose the distance between Syene and Alexandria was 800 km. In other words, going from Alexandria to Syene causes a change of about $7^\circ$ in the angle of incidence of the sun rays. So how much fraction of the earth’s circumference would you have travelled to achieve this difference of $7^\circ$ ?
Based on this can you calculate the circumference of the earth? As a corollary, also find the diameter of earth.