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Appendix

Important proofs and derivations

Product Rule

log a x y = log a x + log a y

Proof:

Let m = log a x and n = log a y .

Write in exponent form.

x = a m and y = a n .

Multiply.

x y = a m a n = a m + n

a m + n = x y log a ( x y ) = m + n = log a x + log b y

Change of Base Rule

log a b = log c b log c a log a b = 1 log b a

where x and y are positive, and a > 0 , a 1.

Proof:

Let x = log a b .

Write in exponent form.

a x = b

Take the log c of both sides.

log c a x = log c b x log c a = log c b x = log c b log c a log a b = log c b log a b

When c = b ,

log a b = log b b log b a = 1 log b a

Heron’s Formula

A = s ( s a ) ( s b ) ( s c )

where s = a + b + c 2

Proof:

Let a , b , and c be the sides of a triangle, and h be the height.

A triangle with sides labeled: a, b and c.  A line runs through the center of the triangle, bisecting the top angle; this line is labeled: h.

So s = a + b + c 2 .

We can further name the parts of the base in each triangle established by the height such that p + q = c .

A triangle with sides labeled: a, b, and c.  A line runs through the center of the triangle bisecting the angle at the top; this line is labeled: h. The two new line segments on the base of the triangle are labeled: p and q.

Using the Pythagorean Theorem, h 2 + p 2 = a 2 and h 2 + q 2 = b 2 .

Since q = c p , then q 2 = ( c p ) 2 . Expanding, we find that q 2 = c 2 2 c p + p 2 .

We can then add h 2 to each side of the equation to get h 2 + q 2 = h 2 + c 2 2 c p + p 2 .

Substitute this result into the equation h 2 + q 2 = b 2 yields b 2 = h 2 + c 2 2 c p + p 2 .

Then replacing h 2 + p 2 with a 2 gives b 2 = a 2 2 c p + c 2 .

Solve for p to get

p = a 2 + b 2 c 2 2 c

Since h 2 = a 2 p 2 , we get an expression in terms of a , b , and c .

h 2 = a 2 p 2 = ( a + p ) ( a p ) = [ a + ( a 2 + c 2 b 2 ) 2 c ] [ a ( a 2 + c 2 b 2 ) 2 c ] = ( 2 a c + a 2 + c 2 b 2 ) ( 2 a c a 2 c 2 + b 2 ) 4 c 2 = ( ( a + c ) 2 b 2 ) ( b 2 ( a c ) 2 ) 4 c 2 = ( a + b + c ) ( a + c b ) ( b + a c ) ( b a + c ) 4 c 2 = ( a + b + c ) ( a + b + c ) ( a b + c ) ( a + b c ) 4 c 2 = 2 s ( 2 s a ) ( 2 s b ) ( 2 s c ) 4 c 2

Therefore,

h 2 = 4 s ( s a ) ( s b ) ( s c ) c 2 h = 2 s ( s a ) ( s b ) ( s c ) c

And since A = 1 2 c h , then

A = 1 2 c 2 s ( s a ) ( s b ) ( s c ) c = s ( s a ) ( s b ) ( s c )

Properties of the Dot Product

u · v = v · u

Proof:

u · v = u 1 , u 2 , ... u n · v 1 , v 2 , ... v n = u 1 v 1 + u 2 v 2 + ... + u n v n = v 1 u 1 + v 2 u 2 + ... + v n v n = v 1 , v 2 , ... v n · u 1 , u 2 , ... u n = v · u

u · ( v + w ) = u · v + u · w

Proof:

u · ( v + w ) = u 1 , u 2 , ... u n · ( v 1 , v 2 , ... v n + w 1 , w 2 , ... w n ) = u 1 , u 2 , ... u n · v 1 + w 1 , v 2 + w 2 , ... v n + w n = u 1 ( v 1 + w 1 ) , u 2 ( v 2 + w 2 ) , ... u n ( v n + w n ) = u 1 v 1 + u 1 w 1 , u 2 v 2 + u 2 w 2 , ... u n v n + u n w n = u 1 v 1 , u 2 v 2 , ... , u n v n + u 1 w 1 , u 2 w 2 , ... , u n w n = u 1 , u 2 , ... u n · v 1 , v 2 , ... v n + u 1 , u 2 , ... u n · w 1 , w 2 , ... w n = u · v + u · w

u · u = | u | 2

Proof:

u · u = u 1 , u 2 , ... u n · u 1 , u 2 , ... u n = u 1 u 1 + u 2 u 2 + ... + u n u n = u 1 2 + u 2 2 + ... + u n 2 = | u 1 , u 2 , ... u n | 2 = v · u

Standard Form of the Ellipse centered at the Origin

1 = x 2 a 2 + y 2 b 2

Derivation

An ellipse consists of all the points for which the sum of distances from two foci is constant:

( x ( c ) ) 2 + ( y 0 ) 2 + ( x c ) 2 + ( y 0 ) 2 = constant

An ellipse centered at the origin on an x, y-coordinate plane.  Points C1 and C2 are plotted at the points (0, b) and (0, -b) respectively; these points appear on the ellipse.  Points V1 and V2 are plotted at the points (-a, 0) and (a, 0) respectively; these points appear on the ellipse.  Points F1 and F2 are plotted at the points (-c, 0) and (c, 0) respectively; these points appear on the x-axis, but not the ellipse. The point (x, y) appears on the ellipse in the first quadrant.  Dotted lines extend from F1 and F2 to the point (x, y).

Consider a vertex.

An ellipse centered at the origin.  The points C1 and C2 are plotted at the points (0, b) and (0, -b) respectively; these points are on the ellipse.  The points V1 and V2 are plotted at the points (-a, 0) and (a, 0) respectively; these points are on the ellipse.  The points F1 and F2 are plotted at the points (-c, 0) and (c, 0) respectively; these points are on the x-axis and not on the ellipse.  A line extends from the point F1 to a point (x, y) which is at the point (a, 0).  A line extends from the point F2 to the point (x, y) as well.

Then, ( x ( c ) ) 2 + ( y 0 ) 2 + ( x c ) 2 + ( y 0 ) 2 = 2 a

Consider a covertex.

An ellipse centered at the origin.  The points C1 and C2 are plotted at the points (0, b) and (0, -b) respectively; these points are on the ellipse.  The points V1 and V2 are plotted at the points (-a, 0) and (a, 0) respectively; these points are on the ellipse.  The points F1 and F2 are plotted at the points (-c, 0) and (c, 0) respectively; these points are on the x-axis and not on the ellipse.  There is a point (x, y) which is plotted at (0, b). A line extends from the origin to the point (c, 0), this line is labeled: c.  A line extends from the origin to the point (x, y), this line is labeled: b.  A line extends from the point (c, 0) to the point (x, y); this line is labeled: (1/2)(2a)=a.  A dotted line extends from the point (-c, 0) to the point (x, y); this line is labeled: (1/2)(2a)=a.

Then b 2 + c 2 = a 2 .

( x ( c ) ) 2 + ( y 0 ) 2 + ( x c ) 2 + ( y 0 ) 2 = 2 a ( x + c ) 2 + y 2 = 2 a ( x c ) 2 + y 2 ( x + c ) 2 + y 2 = ( 2 a ( x c ) 2 + y 2 ) 2 x 2 + 2 c x + c 2 + y 2 = 4 a 2 4 a ( x c ) 2 + y 2 + ( x c ) 2 + y 2 x 2 + 2 c x + c 2 + y 2 = 4 a 2 4 a ( x c ) 2 + y 2 + x 2 2 c x + y 2 2 c x = 4 a 2 4 a ( x c ) 2 + y 2 2 c x 4 c x 4 a 2 = 4 a ( x c ) 2 + y 2 1 4 a ( 4 c x 4 a 2 ) = ( x c ) 2 + y 2 a c a x = ( x c ) 2 + y 2 a 2 2 x c + c 2 a 2 x 2 = ( x c ) 2 + y 2 a 2 2 x c + c 2 a 2 x 2 = x 2 2 x c + c 2 + y 2 a 2 + c 2 a 2 x 2 = x 2 + c 2 + y 2 a 2 + c 2 a 2 x 2 = x 2 + c 2 + y 2 a 2 c 2 = x 2 c 2 a 2 x 2 + y 2 a 2 c 2 = x 2 ( 1 c 2 a 2 ) + y 2

Let 1 = a 2 a 2 .

a 2 c 2 = x 2 ( a 2 c 2 a 2 ) + y 2 1 = x 2 a 2 + y 2 a 2 c 2

Because b 2 + c 2 = a 2 , then b 2 = a 2 c 2 .

1 = x 2 a 2 + y 2 a 2 c 2 1 = x 2 a 2 + y 2 b 2

Standard Form of the Hyperbola

1 = x 2 a 2 y 2 b 2

Derivation

A hyperbola is the set of all points in a plane such that the absolute value of the difference of the distances between two fixed points is constant.

Side-by-side graphs of hyperbole.  In Diagram 1: The foci F’ and F are labeled and can be found a little in front of the opening of the hyperbola.  A point P at (x,y) on the right curve is labeled.  A line extends from the F’ focus to the point P labeled: D1.  A line extends from the F focus to the point P labeled: D2.  In Diagram 2:  The foci F’ and F are labeled and can be found a little in front of the opening of the hyperbola.  A point V is labeled at the vertex of the right hyperbola.  A line extends from the F’ focus to the point V labeled: D1.  A line extends from the F focus to the point V labeled: D2.

Diagram 1: The difference of the distances from Point P to the foci is constant:

( x ( c ) ) 2 + ( y 0 ) 2 ( x c ) 2 + ( y 0 ) 2 = constant

Diagram 2: When the point is a vertex, the difference is 2 a .

( x ( c ) ) 2 + ( y 0 ) 2 ( x c ) 2 + ( y 0 ) 2 = 2 a

( x ( c ) ) 2 + ( y 0 ) 2 ( x c ) 2 + ( y 0 ) 2 = 2 a ( x + c ) 2 + y 2 ( x c ) 2 + y 2 = 2 a ( x + c ) 2 + y 2 = 2 a + ( x c ) 2 + y 2 ( x + c ) 2 + y 2 = ( 2 a + ( x c ) 2 + y 2 ) x 2 + 2 c x + c 2 + y 2 = 4 a 2 + 4 a ( x c ) 2 + y 2 x 2 + 2 c x + c 2 + y 2 = 4 a 2 + 4 a ( x c ) 2 + y 2 + x 2 2 c x + y 2 2 c x = 4 a 2 + 4 a ( x c ) 2 + y 2 2 c x 4 c x 4 a 2 = 4 a ( x c ) 2 + y 2 c x a 2 = a ( x c ) 2 + y 2 ( c x a 2 ) 2 = a 2 ( ( x c ) 2 + y 2 ) c 2 x 2 2 a 2 c 2 x 2 + a 4 = a 2 x 2 2 a 2 c 2 x 2 + a 2 c 2 + a 2 y 2 c 2 x 2 + a 4 = a 2 x 2 + a 2 c 2 + a 2 y 2 a 4 a 2 c 2 = a 2 x 2 c 2 x 2 + a 2 y 2 a 2 ( a 2 c 2 ) = ( a 2 c 2 ) x 2 + a 2 y 2 a 2 ( a 2 c 2 ) = ( c 2 a 2 ) x 2 a 2 y 2

Define b as a positive number such that b 2 = c 2 a 2 .

a 2 b 2 = b 2 x 2 a 2 y 2 a 2 b 2 a 2 b 2 = b 2 x 2 a 2 b 2 a 2 y 2 a 2 b 2 1 = x 2 a 2 y 2 b 2

Trigonometric identities

Pythagorean Identity cos 2 t + sin 2 t = 1 1 + tan 2 t = sec 2 t 1 + cot 2 t = csc 2 t
Even-Odd Identities cos ( t ) = c o s t sec ( t ) = sec t sin ( t ) = sin t tan ( t ) = tan t csc ( t ) = csc t cot ( t ) = cot t
Cofunction Identities cos t = sin ( π 2 t ) sin t = cos ( π 2 t ) tan t = cot ( π 2 t ) cot t = tan ( π 2 t ) sec t = csc ( π 2 t ) csc t = sec ( π 2 t )
Fundamental Identities tan t = sin t cos t sec t = 1 cos t csc t = 1 sin t c o t t = 1 tan t = cos t sin t
Sum and Difference Identities cos ( α + β ) = cos α cos β sin α sin β cos ( α β ) = cos α cos β + sin α sin β sin ( α + β ) = sin α cos β + cos α sin β sin ( α β ) = sin α cos β cos α sin β tan ( α + β ) = tan α + tan β 1 tan α tan β tan ( α β ) = tan α tan β 1 + tan α tan β
Double-Angle Formulas sin ( 2 θ ) = 2 sin θ cos θ cos ( 2 θ ) = cos 2 θ sin 2 θ cos ( 2 θ ) = 1 2 sin 2 θ cos ( 2 θ ) = 2 cos 2 θ 1 tan ( 2 θ ) = 2 tan θ 1 tan 2 θ
Half-Angle Formulas sin α 2 = ± 1 cos α 2 cos α 2 = ± 1 + cos α 2 tan α 2 = ± 1 cos α 1 + cos α tan α 2 = sin α 1 + cos α tan α 2 = 1 cos α sin α
Reduction Formulas sin 2 θ = 1 cos ( 2 θ ) 2 cos 2 θ = 1 + cos ( 2 θ ) 2 tan 2 θ = 1 cos ( 2 θ ) 1 + cos ( 2 θ )
Product-to-Sum Formulas cos α cos β = 1 2 [ cos ( α β ) + cos ( α + β ) ] sin α cos β = 1 2 [ sin ( α + β ) + sin ( α β ) ] sin α sin β = 1 2 [ cos ( α β ) cos ( α + β ) ] cos α sin β = 1 2 [ sin ( α + β ) sin ( α β ) ]
Sum-to-Product Formulas sin α + sin β = 2 sin ( α + β 2 ) cos ( α β 2 ) sin α sin β = 2 sin ( α β 2 ) cos ( α + β 2 ) cos α cos β = 2 sin ( α + β 2 ) sin ( α β 2 ) cos α + cos β = 2 cos ( α + β 2 ) cos ( α β 2 )
Law of Sines sin α a = sin β b = sin γ c a sin α = b sin β = c sin γ
Law of Cosines a 2 = b 2 + c 2 2 b c cos α b 2 = a 2 + c 2 2 a c cos β c 2 = a 2 + b 2 2 a b cos γ

Toolkit functions

Three graphs side-by-side. From left to right, graph of the identify function, square function, and square root function. All three graphs extend from -4 to 4 on each axis.
Three graphs side-by-side. From left to right, graph of the cubic function, cube root function, and reciprocal function. All three graphs extend from -4 to 4 on each axis.
Three graphs side-by-side. From left to right, graph of the absolute value function, exponential function, and natural logarithm function. All three graphs extend from -4 to 4 on each axis.

Trigonometric functions

Unit Circle

Graph of unit circle with angles in degrees, angles in radians, and points along the circle inscribed.
Angle 0 π 6 , or 30 ° π 4 , or 45 ° π 3 , or 60 ° π 2 , or 90 °
Cosine 1 3 2 2 2 1 2 0
Sine 0 1 2 2 2 3 2 1
Tangent 0 3 3 1 3 Undefined
Secant 1 2 3 3 2 2 Undefined
Cosecant Undefined 2 2 2 3 3 1
Cotangent Undefined 3 1 3 3 0

Questions & Answers

how does the planets on our solar system orbit
cheten Reply
how many Messier objects are there in space
satish Reply
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Richard Reply
what are astronomy
Issan Reply
Astronomy (from Ancient Greek ἀστρονομία (astronomía) 'science that studies the laws of the stars') is a natural science that studies celestial objects and phenomena. It uses mathematics, physics, and chemistry in order to explain their origin and evolution.
Rafael
vjuvu
Elgoog
what is big bang theory?
Rosemary
what type of activity astronomer do?
Rosemary
No
Richard
the big bang theory is a theory which states that all matter was compressed together in one place the matter got so unstable it exploded releasing All its contents in the form of hydrogen
Roaul
I want to be an astronomer. That's my dream
Astrit
Who named the the whole galaxy?
Shola Reply
solar Univers
GPOWER
what is space
Richard
what is the dark matter
Richard
what are the factors upon which the atmosphere is stratified
Nicholas Reply
is the big bang the sun
Folakemi Reply
no
Sokak
bigbang is the beginning of the universe
Sokak
but thats just a theory
Sokak
nothing will happen, don't worry brother.
Vansh
what does comet means
GANGAIN Reply
these are Rocky substances between mars and jupiter
GANGAIN
Comets are cosmic snowballs of frozen gases , rock and dust that orbit the sun. They are mostly found between the orbits of Venus and Mercury.
Aarya
hllo
John
hi
John
qt rrt
John
r u there
John
hey can anyone guide me abt international astronomy olympiad
sahil
how can we learn right and true ?
Govinda Reply
why the moon is always appear in an elliptical shape
Gatjuol Reply
Because when astroid hit the Earth then a piece of elliptical shape of the earth was separated which is now called moon.
Hemen
what's see level?
lidiya Reply
Did you mean eye sight or sea level
Minal
oh sorry it's sea level
lidiya
according to the theory of astronomers why the moon is always appear in an elliptical orbit?
Gatjuol
hi !!! I am new in astronomy.... I have so many questions in mind .... all of scientists of the word they just give opinion only. but they never think true or false ... i respect all of them... I believes whole universe depending on true ...থিউরি
Govinda
hello
Jackson
hi
Elyana
we're all stars and galaxies a part of sun. how can science prove thx with respect old ancient times picture or books..or anything with respect to present time .but we r a part of that universe
w astronomy and cosmology!
Michele
another theory of universe except big ban
Albash Reply
how was universe born
Asmit Reply
there many theory to born universe but what is the reality of big bang theory to born universe
Asmit
what is the exact value of π?
Nagalakshmi
by big bang
universal
there are many theories regarding this it's on you believe any theory that you think is true ex. eternal inflation theory, oscillation model theory, multiple universe theory the big bang theory etc.
Aarya
I think after Big Bang!
Michele
from where on earth could u observe all the stars during the during the course of an year
Karuna Reply
I think it couldn't possible on earth
Nagalakshmi
in this time i don't Know
Michele
is that so. the question was in the end of this chapter
Karuna
in theory, you could see them all from the equator (though over the course of a year, not at pne time). stars are measured in "declination", which is how far N or S of the equator (90* to -90*). Polaris is the North star, and is ALMOST 90* (+89*). So it would just barely creep over the horizon.
Christopher
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Source:  OpenStax, Algebra and trigonometry. OpenStax CNX. Nov 14, 2016 Download for free at https://legacy.cnx.org/content/col11758/1.6
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