Advertisements
Advertisements
प्रश्न
A Saturn year is 29.5 times the earth year. How far is the Saturn from the sun if the earth is 1.50 ×108 km away from the sun?
Advertisements
उत्तर १
Distance of the Earth from the Sun, re = 1.5 × 108 km = 1.5 × 1011 m
Time period of the Earth = Te
Time period of Saturn, Ts = 29. 5 Te
Distance of Saturn from the Sun = rs
From Kepler’s third law of planetary motion, we have
T = `((4pi^2r^3)/"GM")^(1/2)`
For Saturn and Sun, we can write
`(r_s^3)/(r_e^3) = (T_s^2)/(T_e^2)`
`r_s = r_e (T_s/T_e)^(2/3)`
`=1.5 xx 10^11 ((29.5T_e)/T_e)^(2/3)`
`=1.5 xx 10^11 (29.5)^(2/3)`
`= 1.5 xx 10^11xx 9.55`
`=14.32 xx 10^11` m
Hence, the distance between Saturn and the Sun is `1.43 xx 10^(12)` m.
उत्तर २
We know that `T^2 oo R^3`
`:.(T_s^2)/(T_e^2) = (R_s^3)/(R_e^3)`
where subscript s and e refer to the Saturn and Earth respectively.
Now `T_s/T_e = 29.5`[given]; `R_e = 1.50 xx 10^8` km
`(R_s/R_e)^3 = (T_s/T_e)`
`R_s = R_exx [(29.5)^2]^(1/3)`
`= 1.50 xx 10^8 xx (870.25)^"1.3" `km
`= 1.43 xx 10^9 km = 1.43 xx 10^12` m
∴Distance of saturn from Sum `= 1.43 xx 10^(12)` m
APPEARS IN
संबंधित प्रश्न
State Kepler's law of orbit and law of equal areas.
Let us assume that our galaxy consists of 2.5 × 1011 stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution? Take the diameter of the Milky Way to be 105 ly
In the Following figure shows the elliptical path of a planet about the sun. The two shaded parts have equal area. If t1 and t2 be the time taken by the planet to go from a to b and from c to d respectively,

Answer the following question in detail.
State Kepler’s three laws of planetary motion.
Observe the given figure showing the orbit of a planet moving around the Sun and write the three laws related to it:

The orbit of a planet moving around the Sun
The orbit of a planet revolving around a star is ______.
To verify Kepler's third law graphically four students plotted graphs. Student A plotted a graph of T (period of revolution of planets) versus r (average distance of planets from the sun) and found the plot is straight line with slope 1.85. Student B plotted a graph of T2 v/s r3 and found the plot is straight line with slope 1.39 and negative Y-intercept. Student C plotted graph of log T v/s log r and found the plot is straight line with slope 1.5. Student D plotted graph of log T v/s log r and found the plot is straight line with slope 0.67 and with negative X-intercept. The correct graph is of student
Both earth and moon are subject to the gravitational force of the sun. As observed from the sun, the orbit of the moon ______.
In our solar system, the inter-planetary region has chunks of matter (much smaller in size compared to planets) called asteroids. They ______.
Supposing Newton’s law of gravitation for gravitation forces F1 and F2 between two masses m1 and m2 at positions r1 and r2 read F1 = – F2 = `- r_12/r_12^3 GM_0^2 ((m_1m_2)/M_0^2)^n` where M0 is a constant of dimension of mass r12 = r1 – r2 and n is a number. in such a case.
- the acceleration due to gravity on earth will be different for different objects.
- none of the three laws of Kepler will be valid.
- only the third law will become invalid.
- for n negative, an object lighter than water will sink in water.
What is the direction of areal velocity of the earth around the sun?
Out of aphelion and perihelion, where is the speed of the earth more and why?
The maximum and minimum distances of a comet from the Sun are 1.6 × 1012 m and 8.0 × 1010 m respectively. If the speed of the comet at the nearest point is 6 × 104 ms-1, the speed at the farthest point is ______.
lf the angular momentum of a planet of mass m, moving around the Sun in a circular orbit is L, about the center of the Sun, and its areal velocity is ______.
How can an ellipse be drawn using pins and thread?
When is a planet moving fastest in its orbit?
