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Aleksandr-060686 [28]
3 years ago
11

Jupiter's semimajor axis is 7.78×1011 m. The mass of the Sun is 1.99×1030 kg. (a) What is the period of Jupiter's orbit in secon

ds? (b) What is the period in Earth years? Assume that one Earth year is exactly 365 days, with 24 hours in each day.
Physics
2 answers:
dedylja [7]3 years ago
7 0

Explanation:

It is given that,

Semi major axis of the Jupiter, a=7.78\times 10^{11}\ m

Mass of the sun, M=1.99\times 10^{30}\ kg

(a) Let T is the period of Jupiter's orbit. It is given by :

T^2\propto a^3

T^2=\dfrac{4\pi^2}{GM}a^3

T^2=\dfrac{4\pi^2}{6.67\times 10^{-11}\times 1.99\times 10^{30}}\times (7.78\times 10^{11})^3

T=3.74\times 10^8\ s

(b) We know that,

1\ year=3.154\times 10^7\ s

or

1\ s=3.171\times 10^{-8}\ year

3.74\times 10^8\ s={3.171\times 10^{-8}}\times {3.74\times 10^8}

T = 11.859 earth years

Hence, this is the required solution.

Tanya [424]3 years ago
6 0

Answer:

(a) 3.74 x 10^8 seconds

(b) 11.86 earth year

Explanation:

Radius, R = 7.78 x 10^11 m

mass of sun, M = 1.99 x 10^30 kg

(a) Let T be the period of Jupiter.

T=2\pi \sqrt{\frac{R^{3}}{GM}}

T=2\pi \sqrt{\frac{\left ( 7.78\times10^{11} \right )^{3}}{6.67\times10^{-11}\times1.99\times10^{30}}}

T = 3.74 x 10^8 seconds

(b) 1 year = 365 days

1 day = 24 hour

1 hour = 60 minutes

1 minute = 60 seconds

T = 11.86 earth year.

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Answer:

The percentage of its mechanical energy does the ball lose with each bounce is 23 %

Explanation:

Given data,

The tennis ball is released from the height, h = 4 m

After the third bounce it reaches height, h' = 183 cm

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The percentage of change in energy the ball retains to its original energy,

                                 \Delta E\%=\frac{1.83mg}{4mg}\times100\%

                                  ΔE % = 45 %

The ball retains only the 45% of its original energy after 3 bounces.

Therefore, the energy retains in each bounce is

                                   ∛ (0.45) = 0.77

The ball retains only the 77% of its original energy.

The energy lost to the floor is,

                                E = 100 - 77

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Hence, the percentage of its mechanical energy does the ball lose with each bounce is 23 %      

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What is the mani difference between kentic energy and potential energy
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Freeze Fracture replication

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<u>Freeze Fracture replication</u> is a technique that allows investigation of the microheterogeneity of a membrane so that one can see localized differences in different parts of the membrane.

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A stuntman sitting on a tree limb wishes to drop vertically onto a horse galloping under the tree. The constant speed of the hor
Wittaler [7]

Answer:

7.78 meters

Explanation:

So, lets just pretend we are working in a vacuum, like in (almost) all physics problems. So, we must find how much time will take to the man fall the height to the saddle to know how far away must be the saddle to be right under the limb at the right time.

So, we can use kinematics relationships. We know the for a 1D movement, with constant acceleration, the equation its:

y(t) \ = \ y_0 \ + \ v_0 \ * \ t \ +\frac{1}{2} \ a \ t^2

For our problem, the initial position its the height from which the man jumps,  

y_o \ = 2.45 \m, the final position

y(t_{fall}) must be the level of the saddle

y(t_{fall}) \ = 0 \ m,

the initial velocity must be

v_0 \ = \ 0 \ \frac{m}{s},

and the acceleration its the gravitational pull,

a \ = \ - \ g \ = \ - \ 9.8 \ \frac{m}{s^2}.

So, we get:

0\ = \ 2.45 \ m \ + \ 0 \ * \ t \ - \frac{1}{2} \ g \ t_{fall}^2

0\ = \ 2.45 \ m \ - \frac{1}{2} \ g \ t_{fall}^2

- \ 2.45 \ m \ = - \frac{1}{2} \ g \ t_{fall}^2

\ 2.45 \ m \ = \frac{1}{2} \ g \ t_{fall}^2

2 \ * \ 2.45 \ m \ = \ g \ t_{fall}^2

\frac{ 2 \ * \ 2.45 \ m}{g} \ = t_{fall}^2

\sqrt{ \frac{ 2 \ * \ 2.45 \ m}{g} } \ = \ t_{fall}

So, we can calculate this an get

t_{fall} \ = \sqrt{ \frac{ 2 \ * \ 2.45 \ m}{9.8 \frac{m}{s^2} } }

t_{fall} \ = \sqrt{ \frac{1}{2} }

Now, we know how much time will take for the man to fall to the level of the saddle. If the horse is galloping to a constant speed of

v_h \ = \ 11.0 \ \frac{m}{s},

in the time t__{fall} the horse travels a distance

d_h \ = \ v_h * t_{fall}

d_h \ = \ 11.0  \ \frac{m}{s} * \sqrt{ \frac{1}{2} }

d_h \ = \ 7.78 \ m

And this must be the distance we are looking for. So, the saddle and the limb must be at 7.78 meters when the man makes his move.

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3 years ago
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