Answer:
C) scientist use experiments to test their ideas
Answer:
the answers the correct one is d
Explanation:
The speed of sound is constant so we can use the relations of uniform motion
v = x / t
x = v t
now let's calculate the distance for each person
t = 5s
x₁ = 300 5
x₁ = 1500 m
t = 6s
x₂ = 300 6
x₂ = 1800 m
therefore we have two possibilities
a) the two people are on the same side, therefore the distance between them is
Δx = x₂- x₁
Δx = 1800 - 1500
Δx = 300 m
let's reduce to km
Δx = 0.300 km
b) people are on opposite sides of the sound
Δx = x₂ + x₁
Δx = 1800 + 1500
Δx = 3300 m
Δx = 3.3 km
when checking the answers the correct one is d
Answer:
<h2>
3.94 kg</h2>
Explanation:
Given,
Force ( f ) = 30 N
Acceleration(a) = 7.6 m/s
Now, Let's find the mass of the ball
Using the Newton's second law of motion:
We get:
![force \: = mass \: \times acceleration](https://tex.z-dn.net/?f=force%20%5C%3A%20%20%3D%20mass%20%5C%3A%20%20%5Ctimes%20acceleration)
plug the value
![30 \: = m \: \times 7.6](https://tex.z-dn.net/?f=30%20%5C%3A%20%20%3D%20m%20%5C%3A%20%20%5Ctimes%207.6)
Use the commutative property to reorder the terms
![30 = 7.6 \: m](https://tex.z-dn.net/?f=%2030%20%3D%207.6%20%5C%3A%20m)
Swap the sides of the equation
![7.6m = 30](https://tex.z-dn.net/?f=7.6m%20%3D%2030)
Divide both sides of the equation by 7.6
![\frac{7.6 \: m}{7.6} = \frac{30}{7.6}](https://tex.z-dn.net/?f=%20%5Cfrac%7B7.6%20%5C%3A%20m%7D%7B7.6%7D%20%20%3D%20%20%5Cfrac%7B30%7D%7B7.6%7D%20)
Calculate
![m = 3.94 \: kg](https://tex.z-dn.net/?f=m%20%3D%203.94%20%5C%3A%20kg)
Hope this helps..
Best regards!!
We need to directly measure the spectral type in order to determine the surface temperature of a star.
<h3>How do you find the properties of a star?</h3>
Astronomers can determine the temperature of a star by looking at its color and spectrum. The apparent brightness of a star describes how luminous it looks to us. The brightness of a star tells us how bright it really is. The luminance can be determined using both the perceived brightness and the distance.
A star's luminosity, or the total amount of energy it emits each second, is determined by two factors: The stellar photosphere's "Effective Temperature," T. the star's total surface area, which is influenced by its radius, R.
Because it controls how much fuel a star has and how quickly it burns it, a star's mass is its most fundamental characteristic. The majority of a star's life is spent burning hydrogen into helium in its core, which generates energy. The star needs to achieve a balance between gravity and outward pressure in order to continue to be "alive."
To know more about stellar property visit:
brainly.com/question/14950677
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