Alnilam is the brightest star
Absolute brightness is how bright the star actually is. Apparent brightness is how bright the star looks.
Factors that influence how bright a star looks is distance. The fact that Alnilam has the same apparent brightness of the other two stars even though it is farther away, means that it is brighter.
Answer: -31.36 m/s
Explanation:
This is a problem of motion in one direction (specifically vertical motion), and the equation that best fulfills this approach is:
(1)
Where:
is the final velocity of the supply bag
is the initial velocity of the supply bag (we know it is zero because we are told it was "dropped", this means it goes to ground in free fall)
is the acceleration due gravity (the negtive sign indicates the gravity is downwards, in the direction of the center of the Earth)
is the time
Knowing this, let's solve (1):
(2)
Finally:
Note the negative sign is because the direction of the bag is downwards as well.
Answer:
what r the questions i can’t see them
Explanation:
Answer:
i dont know
Explanation:
i dont know since you didn't provide something to base off of
Answer:
![Ep=-2.3*10^{-19}J](https://tex.z-dn.net/?f=Ep%3D-2.3%2A10%5E%7B-19%7DJ)
Explanation:
The change in potential energy can be expressed as:
![Ep=K.\frac{q1.q2}{r}](https://tex.z-dn.net/?f=Ep%3DK.%5Cfrac%7Bq1.q2%7D%7Br%7D)
where K is a constant with a value of
, q1 and q2 are the charges of the proton and the electron and r is the distance between them.
The charge for the proton is
and the charge for the electron is
.
Converting r=1.0nm to m:
![1.0nm*\frac{1*10^{-9}m}{1.0nm}=1*10^{-9}m](https://tex.z-dn.net/?f=1.0nm%2A%5Cfrac%7B1%2A10%5E%7B-9%7Dm%7D%7B1.0nm%7D%3D1%2A10%5E%7B-9%7Dm)
Replacing values:
![Ep=9*10^{9}\frac{N.m^{2}}{C^{2}}.\frac{(+1.6*10^{-19}C).(-1.6*10^{-19}C)}{1*10^{-9}m}](https://tex.z-dn.net/?f=Ep%3D9%2A10%5E%7B9%7D%5Cfrac%7BN.m%5E%7B2%7D%7D%7BC%5E%7B2%7D%7D.%5Cfrac%7B%28%2B1.6%2A10%5E%7B-19%7DC%29.%28-1.6%2A10%5E%7B-19%7DC%29%7D%7B1%2A10%5E%7B-9%7Dm%7D)
![Ep=-2.3*10^{-19}J](https://tex.z-dn.net/?f=Ep%3D-2.3%2A10%5E%7B-19%7DJ)