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Kaylis [27]
3 years ago
13

By using kepler's 3rd law we find that ___________.

Physics
2 answers:
tangare [24]3 years ago
8 0

Answer;

By using kepler's 3rd law we find that;

-A year on Earth is shorter than a year on Saturn.

Explanation;

-Kepler’s 3rd law states that the square of a planet’s orbital period is proportional to the cube of its average distance from the Sun (semi-major axis), which tells us that more distant planets move more slowly in their orbits.

-In other words, if you square the 'year' of each planet, and divide it by the cube of its distance to the Sun, you get the same number, for all planets. The law captures the relationship between the distance of planets from the Sun, and their orbital periods.

maw [93]3 years ago
3 0

By using Kepler's 3rd law we find that A year on Earth is shorter than a year on Saturn (d)

<h3>Further explanation</h3>

Kepler's law is based on the orbits of planets around the sun.

There are 3 laws issued by Kepler

  • 1. Kepler Law 1

the inner planet's orbit around the sun is based on an elliptical path and the sun is the center

  • 2. Kepler Law 2

Imaginary lines are drawn from planets to the sun cover the same area at the same time interval.

  • 3. Kepler Law 3

The square of the orbital period of a planet is proportional to the cube of its average distance to the sun

General formula:

\large{\boxed{\bold{\frac{T_1^2}{r_1^3} =\frac{T_2^2}{r_2^3} }}}

There are choices of questions that need to be completed from the questions above:

a. A day on Earth is shorter than a day on Saturn.

b. A year on Earth is longer than a year on Saturn.

c. A day on Earth is longer than a day on Saturn.

d. A year on Earth is shorter than a year on Saturn.

If we use Kepler 3's Law to see the answer choices then:

  • 1. the length of days of a planet depends on the rotation of each planet

Kepler 3's law is based only on the period of the planet, in this case, the planet's revolution against the sun.

So the determination of the length of the day can not be determined using Kepler 3 Law

So answers a and c do not meet the area of ​​Kepler 3 law

  • 2. Long or short years of a planet based on the planet's revolution against the sun

One year is counted one revolution = one cycle = one orbit

The longer the planet's distance from the sun, the longer it will get one rotation so that the longer the year from the planet

The planets that circle the sun in sequence from the closest are: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune

From this sequence shows that the distance of the planet Saturn is further than that of the planet Earth so

A year on Earth is shorter than a year on Saturn (d)

<h3>Learn more</h3>

The Sun has more gravity than the other plans in our solar system

brainly.com/question/3252750

weight and mass used synonymously on Earth

brainly.com/question/5956881

the Earth has more gravitation pull than the moon

brainly.com/question/1513912

Keywords: Kepler law 3, sun, revolution, earth, Saturn, rotation, year, day

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frez [133]

Answer:

r_f=137493m

v=8638940m/s

Explanation:

During this process the mass M=2\times10^{30}Kg will be considered constant. We start from a radius r_i=7\times10^8m and a period T_i=30\ days=(30)(24)(60)(60)s=2592000s. The final period is T_f=0.1s.

Angular momentum <em>L</em> is conserved in this process. We can use the formula L=I\omega, where I is the momentum of inertia (which for a solid sphere is I=\frac{2mr^2}{5}) and \omega=\frac{2\pi }{T} is the angular velocity, so we can write the star's angular momentum as:

L=I\omega=\frac{2mr^2}{5}\frac{2\pi }{T}=\frac{4\pi mr^2 }{5T}

Since L_f=L_i we have:

\frac{4\pi mr_f^2 }{5T_f}=\frac{4\pi mr_i^2 }{5T_i}

Which can be simplified as:

\frac{r_f^2 }{T_f}=\frac{r_i^2 }{T_i}

Which means:

r_f=\sqrt{\frac{r_i^2 T_f}{T_i}}=r_i \sqrt{\frac{T_f}{T_i}}

Which for our values is:

r_f=r_i \sqrt{\frac{T_f}{T_i}}=(7\times10^8m) \sqrt{\frac{0.1s}{2592000s}}=137493m

And we calculate the speed of a point on the equator by dividing the final circumference over the final period:

v=\frac{C_f}{T_f}=\frac{2\pi r_f}{T_f}=\frac{2\pi (137493m)}{(0.1s)}=8638940m/s

3 0
4 years ago
Calculate the frequency of the 3rd normal mode of a guitar string of length 40.0cm and mass 0.5g when stretched with a tension o
Alexandra [31]

Answer:

Explanation:

For third normal mode of vibration

l = \frac{3\lambda}{2}  , λ is wavelength , l is length of string .

.4 = \frac{3\lambda}{2}

λ = .267 m

velocity = \sqrt{\frac{T}{m} }

T is tension and m is mass unit length

m = .5 x 10⁻³ / 40 x 10⁻²

= .00125 kg / m

Putting the values

velocity = \sqrt{\frac{80}{.00125} }

= 253 m /s

frequency

= velocity / λ

= 253 / .267

= 947.5 Hz .

7 0
3 years ago
The wavelength of light visible to the human eye is on the order of 5 x 10-7 m. if the speed of light in air is 3 x 108 m/s, fin
juin [17]

The frequency of light wave is 0.6*10^15 Hz.

The relation between the speed of light, frequency, and wavelength is given as

c=λν

Plugging the values in the above equation

3*10^8=5*10^(-7)*ν

ν=0.6*10^15 Hz.

Therefore the frequency of the light wave is 0.6*10^15 Hz.

6 0
4 years ago
The annoying sound from a mosquito is produced when it beats its wings at the average rate of 600. wingbeats per second. What is
jok3333 [9.3K]
The frequency is exactly the rate at which the bug beats its wings.
If that "600" that you mentioned is 600 beats per second, then
THAT's the frequency . . . 600 per second. (600 Hz) 
3 0
4 years ago
When thermal energy is added to an object what happens to the motion of the particles
Juli2301 [7.4K]

Answer:

The movement of thermal energy from a substance at a higher temperature to one at a lower temperature is called heat. When a substance is heated, it gains thermal energy. Therefore, its particles move faster and its temperature rises.

Explanation:

5 0
3 years ago
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