The prime factorization is 3 x 3 x 5 x 13
Answer:
isosceles
Step-by-step explanation:
Answer:
see below for drawings and description
Step-by-step explanation:
For geometry problems involving translation, rotation, and reflection—transformations that change location, but not size ("rigid" transformations)—it might be helpful for you to trace the image onto tracing paper or clear plastic so that you can manipulate it in the desired way. Eventually, you'll be able to do this mentally, without the aid of a physical object to play with.
For the images attached here, I copied the triangle onto a piece of clear plastic so I could move it to the desired positions. The result was photographed for your pleasure.
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a. Translation means the image is moved without changing its orientation or dimensions. You are asked to copy the triangle so that the upper left vertex is moved to what is now point E. See the first attachment.
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b. Reflection means the points are copied to the same distance on the other side of the point or line of reflection. Just as an object held to a mirror has its reflection also at the mirror, any points on the line of reflection do not move. Reflection flips the image over. See the second attachment.
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c. Rotation about point D means point D stays where it is. The angle of rotation is the same as the angle at D, so the line DE gets rotated until it aligns with the line DF. The rest of the triangle maintains its shape. See the third attachment.
Given that you mention the divergence theorem, and that part (b) is asking you to find the downward flux through the disk
, I think it's same to assume that the hemisphere referred to in part (a) is the upper half of the sphere
.
a. Let
denote the hemispherical <u>c</u>ap
, parameterized by

with
and
. Take the normal vector to
to be

Then the upward flux of
through
is



b. Let
be the disk that closes off the hemisphere
, parameterized by

with
and
. Take the normal to
to be

Then the downward flux of
through
is


c. The net flux is then
.
d. By the divergence theorem, the flux of
across the closed hemisphere
with boundary
is equal to the integral of
over its interior:

We have

so the volume integral is

which is 2 times the volume of the hemisphere
, so that the net flux is
. Just to confirm, we could compute the integral in spherical coordinates:

Answer:
B. 7.9 in^2
Step-by-step explanation:
Part I.
Finding the fraction of the circle that is the sector
To start, let’s find the fraction of the circle that the sector covers. Since the measure of the central angle is 36, we get 36/360 or 1/10 of the circle.
Part II.
Finding the area of the Circle
The area of a circle is pi*r^2. Since r=5, then the area is 25pi.
Part III.
Finding the area of the sector.
Since the sector is 1/10 of the circle, its area is 1/10 of the circle’s area. So the area of the sector is 25/10*pi or (5/2)pi. This is approximately 7.9 in^2.