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AleksandrR [38]
3 years ago
15

Please help me feel in the blanks Giving 30 points

Physics
1 answer:
maw [93]3 years ago
7 0

4:chemical properties can only be observed when a substance changes into another substance.

5: physical properties such as color and shape are easy to observe

6: in a chemical change an altered substance forms

7: cooking or baking food will result in a chemical change

8: a melting ice cube is a physical change

9: the rusting of iron is a chemical change

10: water boiling is a scientific physical change

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Fill in the blanks HELP ASAP
Alexandra [31]

checking to see if im locked out

7 0
3 years ago
Select the correct answer.
Vesna [10]

Answer:

A. continental-oceanic convergent

Explanation:

I knew it couldn't be B because it's oceanic and <em>continental</em>, not oceanic and <em>oceanic</em>.

Next, I noticed the word <em>convergent</em>, which implies "coming together" to me.

I looked it up and noticed the term <em>convergent</em> referred to a plate boundary where a plate slips under (<em>subducted</em>) another, so I knew it was A.

Hopefully, this helps you understand the question better. Have a great day!

3 0
3 years ago
What is the magnitude of the free-fall acceleration at a point that is a distance 2R above the surface of the Earth, where R is
ss7ja [257]

Answer:

g' = g/9 = 1.09 m/s²

Explanation:

The magnitude of free fall acceleration at the surface of earth is given by the following formula:

g = GM/R²   ----- equation 1

where,

g = free fall acceleration

G = Universal Gravitational Constant

M = Mass of Earth

R = Distance between the center of earth and the object

So, in our case,

R = R + 2 R = 3 R

Therefore,

g' = GM/(3R)²

g' = (1/9) GM/R²

using equation 1:

g' = g/9

g' = (9.8 m/s)/9

<u>g' = 1.09 m/s²</u>

3 0
3 years ago
a particle is moving with shm of period 8.0s and amplitude 5.0cm. find (a) the speed of particle when it is 3.0m from the centre
Fudgin [204]

Answer:

a) speed=\pi cm/s

b) v_{max}=\frac{5\pi}{4} cm/s

c) a_{max}=\frac{5\pi^{2}}{16} cm/s^{2}

Explanation:

The very first thing we must do in order to solve this problem is to find an equation for the simple harmonic motion of the given particle. Simple harmonic motion can be modeled with the following formula:

y=Asin(\omega t)

where:

A=amplitude

\omega= angular frequency

t=time

we know the amplitude is:

A=5.0cm

and the angular frequency can be found by using the following formula:

\omega=\frac{2\pi}{T}

so our angular frequency is:

\omega=\frac{2\pi}{8s}

\omega=\frac{\pi}{4}

so now we can build our equation:

y=5sin(\frac{\pi}{4} t)

we need to find the speed of the particle when it is 3m from the centre of its motion, so we need to find the time t when this will happen. We can use the equation we just found to get this value:

y=5sin(\frac{\pi}{4} t)

3=5sin(\frac{\pi}{4} t)

so we solve for t:

sin(\frac{\pi}{4} t)=\frac{3}{5}

\frac{\pi}{4} t=sin^{-1}(\frac{3}{5})

t=\frac{4}{\pi}sin^{-1}(\frac{3}{5})

you can directly use this expression as the time or its decimal representation:

t=0.81933

since we need to find the speed of the particle at that time, we will need to get the derivative of the equation that represents the particle's position, so we get:

y=5sin(\frac{\pi}{4} t)

y'=5cos(\frac{\pi}{4} t)*\frac{\pi}{4}

which simplifies to:

y' =\frac{5\pi}{4}cos(\frac{\pi}{4} t)

and we can now substitute the t-value we found previously, so we get:

y'=\frac{5\pi}{4}cos(\frac{\pi}{4} (0.81933))

y'=\pi

so its velocity at that point is \pi cm/s

b) In order to find the maximum velocity we just need to take a look at the velocity equation we just found:

y' =\frac{5\pi}{4}cos(\frac{\pi}{4} t)

its amplitude will always give us the maximum velocity of the particle, so in this case the amplitude is:

A=\frac{5\pi}{4}

so:

v_{max}=\frac{5\pi}{4} cm/s

c) we can use a similar procedure to find the maximum acceleration of the particle, we just need to find the derivative of the velocity equation and determine its amplitude. So we get:

y'= \frac{5\pi}{4}cos(\frac{\pi}{4} t)

We can use the chain rule again to find this derivative so we get:

y" =-\frac{5\pi}{4}sin(\frac{\pi}{4} t)*(\frac{pi}{4})

so when simplified we get:

y"=-\frac{5\pi^{2}}{16}sin(\frac{\pi}{4} t)

its amplitude is:

A=\frac{5\pi^{2}}{16}

so its maximum acceleration is:

a_{max}=\frac{5\pi^{2}}{16} cm/s^{2}

7 0
3 years ago
The surface temperature of a planet depends on both the distance of the planet from the Sun and on how the panet's atmosphere di
BaLLatris [955]

Answer:

Aphelion: 6404 W/m2

Perihelion: 14978 W/m2

Explanation:

The solar energy flux depends on the solar power output divided by the surface of a sphere with a radius equal to the distance to the Sun.

\Phi sol = \frac{Psol}{4 * \pi * d^2}

The distances we need are the aphelion and perihelion of Mercury.

Planetary orbits are ellipses. In an ellipse the eccentricity is related to linear eccentricity and the length of the semi major axis:

e = \frac{c}{a}

Where

e: eccentricity

c: linear eccentricity

a: semi major axis

The linear eccentricity is equal to the distance of the focus of the center of the ellipse.

c = a * c =

a = 0.39 AU = 5.83e10 m

c = 5.83e10e * 0.21 = 1.22e10 m

In planetary orbits the Sun is in one of the fucuses. With this we can calculate the prihelion and aphelion as:

Ap = a + c = 5.83e10 + 1.22e10 = 7.05e10 m

Pe = a - c = 5.83e10 - 1.22e10 = 4.61e10 m

And the solar energy fluxes will be:

\Phi Ap = \frac{4e26}{4 * \pi * 7.05e10^2} = 6404 W/m2

\Phi Pe = \frac{4e26}{4 * \pi * 4.61e10^2} = 14978 W/m2

4 0
3 years ago
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