Impulse is just the product of mass and speed!
I = 1700 * 22.5 = 38,250 kg m/s
It does not have any special name for its units :(
You must observe the object twice.
-- Look at it the first time, and make a mark where it is.
-- After some time has passed, look at the object again, and
make another mark at the place where it is.
-- At your convenience, take out your ruler, and measure the
distance between the two marks.
What you'll have is the object's "displacement" during that period
of time ... the distance between the start-point and end-point.
Technically, you won't know the actual distance it has traveled
during that time, because you don't know the route it took.
Explanation:
Let
and ![\textbf{B} = 2\hat{\textbf{i}} - 2\hat{\textbf{j}} + 3\hat{\textbf{k}}](https://tex.z-dn.net/?f=%5Ctextbf%7BB%7D%20%3D%202%5Chat%7B%5Ctextbf%7Bi%7D%7D%20-%202%5Chat%7B%5Ctextbf%7Bj%7D%7D%20%2B%203%5Chat%7B%5Ctextbf%7Bk%7D%7D)
The sum of the two vectors is
![\textbf{A + B} = (6 + 2)\hat{\textbf{i}} + (4 - 2)\hat{\textbf{j}} + (-2 + 3)\hat{\textbf{k}}](https://tex.z-dn.net/?f=%5Ctextbf%7BA%20%2B%20B%7D%20%3D%20%286%20%2B%202%29%5Chat%7B%5Ctextbf%7Bi%7D%7D%20%2B%20%284%20-%202%29%5Chat%7B%5Ctextbf%7Bj%7D%7D%20%2B%20%28-2%20%2B%203%29%5Chat%7B%5Ctextbf%7Bk%7D%7D)
![= 8\hat{\textbf{i}} + 2\hat{\textbf{j}} + \hat{\textbf{k}}](https://tex.z-dn.net/?f=%20%3D%208%5Chat%7B%5Ctextbf%7Bi%7D%7D%20%2B%202%5Chat%7B%5Ctextbf%7Bj%7D%7D%20%2B%20%5Chat%7B%5Ctextbf%7Bk%7D%7D)
The difference between the two vectors can be written as
![\textbf{A - B} = (6 - 2)\hat{\textbf{i}} + (4 - (-2))\hat{\textbf{j}} + (-2 - 3)\hat{\textbf{k}}](https://tex.z-dn.net/?f=%5Ctextbf%7BA%20-%20B%7D%20%3D%20%286%20-%202%29%5Chat%7B%5Ctextbf%7Bi%7D%7D%20%2B%20%284%20-%20%28-2%29%29%5Chat%7B%5Ctextbf%7Bj%7D%7D%20%2B%20%28-2%20-%203%29%5Chat%7B%5Ctextbf%7Bk%7D%7D)
![= 4\hat{\textbf{i}} + 6\hat{\textbf{j}} - 5\hat{\textbf{k}}](https://tex.z-dn.net/?f=%3D%204%5Chat%7B%5Ctextbf%7Bi%7D%7D%20%2B%206%5Chat%7B%5Ctextbf%7Bj%7D%7D%20-%205%5Chat%7B%5Ctextbf%7Bk%7D%7D)
Answer: The younger elliptical and lenticular galaxies had results similar to spiral galaxies like the Milky Way. The researchers found that the older galaxies have a larger fraction of low-mass stars than their younger counterparts.
Explanation: