Home
Class 11
PHYSICS
Assuming that earth and mars move in cir...

Assuming that earth and mars move in circular orbits around the sun, with the martian orbit being 1.52 times the orbital radius of the earth. The length of the martian year is days is

A

`(1.52)^(2//3)xx365`

B

`(1.52)^(3//2)xx365`

C

`(1.52)^(2)xx365`

D

`(1.52)^(3)xx365`

Text Solution

AI Generated Solution

The correct Answer is:
To find the length of the Martian year, we can use Kepler's Third Law of planetary motion, which states that the square of the orbital period (T) of a planet is directly proportional to the cube of the semi-major axis (R) of its orbit. The law can be expressed mathematically as: \[ T^2 \propto R^3 \] ### Step-by-Step Solution 1. **Identify the relationship between the orbital radii**: Given that the orbital radius of Mars (Rm) is 1.52 times the orbital radius of Earth (Re), we can write: \[ Rm = 1.52 \times Re \] 2. **Apply Kepler's Third Law**: According to Kepler's Third Law, we can write the equations for the time periods of Mars (Tm) and Earth (Te): \[ Tm^2 \propto Rm^3 \quad \text{(1)} \] \[ Te^2 \propto Re^3 \quad \text{(2)} \] 3. **Set up the ratio of the time periods**: Dividing equation (1) by equation (2): \[ \frac{Tm^2}{Te^2} = \frac{Rm^3}{Re^3} \] 4. **Substitute the relationship between Rm and Re**: Substitute \(Rm = 1.52 \times Re\) into the equation: \[ \frac{Tm^2}{Te^2} = \frac{(1.52 \times Re)^3}{Re^3} \] 5. **Simplify the equation**: This simplifies to: \[ \frac{Tm^2}{Te^2} = 1.52^3 \] 6. **Calculate \(1.52^3\)**: Calculate \(1.52^3\): \[ 1.52^3 \approx 3.51 \] 7. **Relate the time periods**: Now we can express the relationship between the time periods: \[ Tm^2 = 3.51 \times Te^2 \] 8. **Substitute \(Te\)**: Since the time period of Earth (Te) is 1 year, which is approximately 365 days: \[ Tm^2 = 3.51 \times (365)^2 \] 9. **Calculate \(Tm\)**: Now, calculate \(Tm\): \[ Tm = \sqrt{3.51 \times (365)^2} \] \[ Tm \approx \sqrt{3.51} \times 365 \approx 1.87 \times 365 \approx 683.55 \text{ days} \] 10. **Final Answer**: Therefore, the length of the Martian year is approximately: \[ Tm \approx 687 \text{ days} \]

To find the length of the Martian year, we can use Kepler's Third Law of planetary motion, which states that the square of the orbital period (T) of a planet is directly proportional to the cube of the semi-major axis (R) of its orbit. The law can be expressed mathematically as: \[ T^2 \propto R^3 \] ### Step-by-Step Solution ...
Promotional Banner

Topper's Solved these Questions

  • GRAVITATION

    NCERT FINGERTIPS|Exercise Universal Law Of Gravitations|14 Videos
  • GRAVITATION

    NCERT FINGERTIPS|Exercise The Gravitational Constant|2 Videos
  • KINETIC THEORY

    NCERT FINGERTIPS|Exercise Assertion And Reason|10 Videos

Similar Questions

Explore conceptually related problems

The planet Mars has two moons. Phobos and Delmos (i) phobos has period 7 hours, 39 minutes and an orbital radius of 9.4 xx 10^(3) km . Calculate the mass of Mars. (ii) Assume that Earth and mars move in a circular orbit around the sun, with the martian orbit being 1.52 times the orbital radius of the Earth. What is the length of the martian year in days? (G = 6.67 xx 10^(-11) Nm^(2) kg^(-2))

A planet moving in a circular orbit around the sun at a distance, 4times theaverage distance of the earth from the sun will complete one revolution in

In equilibrium, Mars emits as much radiation as it absorbs. If mars orbits the sun with an orbital radius that is 1.5 times the orbital radius of the earth about the sun, what is the approximate atmospheric temperature of mars? Assume the atmospheric temperature of earth to be 253 K -

A satellite is moving in an orbit around the earth due to

Earth completes one orbit around the sun is

Assume that Earth is in circular orbit around the Sun with kinetic energy K and potential energy U, taken to be zero for infinite separation. Then, the relationship between K and U:

A satellite of Sun is in a circular orbit around the Sun, midway between the Suna and earth. Find the period of this satellite.

In adjoining figure earth goes around the sun in eliptical orbit on which point the orbital speed is maximum :

NCERT FINGERTIPS-GRAVITATION-Assertion And Reason
  1. Assuming that earth and mars move in circular orbits around the sun, w...

    Text Solution

    |

  2. Assertion: The planet move slower when they are farther from the Sun t...

    Text Solution

    |

  3. Assertion : A central force is such that the force on the planet is al...

    Text Solution

    |

  4. Assertion: The motion of a particle under the central force is always ...

    Text Solution

    |

  5. Assertion: The time period of revolution of a satellite close to surfa...

    Text Solution

    |

  6. Assertion: When distance between bodies is doubled and also mass of ea...

    Text Solution

    |

  7. Assertion : The principle of superposition is not valid for gravitat...

    Text Solution

    |

  8. Assertion: The gravitational force on a particle inside a spherical sh...

    Text Solution

    |

  9. Assertion : Gravitational force between two masses in air is F. If the...

    Text Solution

    |

  10. Assertion: A man in a dosed cabin falling freely does not experience g...

    Text Solution

    |

  11. Assertion : For a free falling object, the next external force is just...

    Text Solution

    |

  12. Assertion: The total energy of a satellite is negative. Reason: Gra...

    Text Solution

    |

  13. Assertion : Moon has no atmosphere. Reason : The escape velocity fo...

    Text Solution

    |

  14. Assertion : The gravitational attraction of moon is much less than th...

    Text Solution

    |

  15. Assertion: A person sitting in an artificial satellite revolving aroun...

    Text Solution

    |

  16. Assertion : Geostationary satellites appear fixed from any point on ea...

    Text Solution

    |