हिंदी
कर्नाटक बोर्ड पी.यू.सी.पीयूसी विज्ञान कक्षा ११

A satellite is in an elliptic orbit around the earth with aphelion of 6R and perihelion of 2 R where R= 6400 km is the radius of the earth. - Physics

Advertisements
Advertisements

प्रश्न

A satellite is in an elliptic orbit around the earth with aphelion of 6R and perihelion of 2 R where R= 6400 km is the radius of the earth. Find eccentricity of the orbit. Find the velocity of the satellite at apogee and perigee. What should be done if this satellite has to be transferred to a circular orbit of radius 6R ?

[G = 6.67 × 10–11 SI units and M = 6 × 1024 kg]

दीर्घउत्तर
Advertisements

उत्तर

According to the diagram,

rp = radius of perigee = 2R

ra = radius of perigee = 6R

a = semi-major axis of the ellipse

Hence, we can write

`r_a = a(1 + e) = 6R`

`r_p = a(1 - e) = 2R`

`(a(1 + e))/(a(1 - e)) = (6R)/(2R)` = 3

By solving, we get eccentricity `e = 1/2`

If va and vp are the velocities of the satellite (of mass m) at aphelion and perihelion respectively, then by conservation of angular momentum

`L_("at perigee") = L_("at apogee")`

∴ `mv_pr_p = mv_ar_a` 

∴ `v_a/v_p = r_p/r_a = 1/3`

Applying conservation of energy,

The energy at perigee = Energy at apogee

`1/2 mv_p^2 - (GMm)/r_p = 1/2 mv_a^2 - (GMm)/r_a`

Where M is the mass of the earth

∴ `v_p^2 (1 - 1/9) = - 2GM (1/r_a - 1/r_p)`

= `2GM(1/r_p - 1/r_a)`  .....(By putting `v_a = v_p/3`)

`v_p = [2GM(1/r_p - 1/r_a)]^(1/2)/([1 - (v_a/v_p)^2]^(1/2)`

= `[((2GM)/R (1/2 - 1/6))/((1 - 1/9))]^(1/2)`

= `((2/3)/(8/9)  (GM)/R)^(1/2)`

= `sqrt(3/4 (GM)/R)`

= 6.85 km/s

vp = 6.885 km/s, va = 2.28 km/s

For circular orbit of radius r, 

vc = orbital velocity = `sqrt((GM)/r)`

For r = 6R, vc = `sqrt((GM)/(6R)` = 3.23 km/s.

shaalaa.com
  क्या इस प्रश्न या उत्तर में कोई त्रुटि है?
अध्याय 8: Gravitation - Exercises [पृष्ठ ६४]

APPEARS IN

एनसीईआरटी एक्झांप्लर Physics [English] Class 11
अध्याय 8 Gravitation
Exercises | Q 8.38 | पृष्ठ ६४

वीडियो ट्यूटोरियलVIEW ALL [1]

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


A comet orbits the Sun in a highly elliptical orbit. Does the comet have a constant (a) linear speed, (b) angular speed, (c) angular momentum, (d) kinetic energy, (e) potential energy, (f) total energy throughout its orbit? Neglect any mass loss of the comet when it comes very close to the Sun.


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.

State Kepler’s law of equal areas.


Write the Kepler's laws.


The third law of Kepler is also known as the Law of ______.


State Kepler’s laws.


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


If the sun and the planets carried huge amounts of opposite charges ______.

  1. all three of Kepler’s laws would still be valid.
  2. only the third law will be valid.
  3. the second law will not change.
  4. the first law will still be valid.

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.

  1. the acceleration due to gravity on earth will be different for different objects.
  2. none of the three laws of Kepler will be valid.
  3. only the third law will become invalid.
  4. for n negative, an object lighter than water will sink in water.

The centre of mass of an extended body on the surface of the earth and its centre of gravity ______.

  1. are always at the same point for any size of the body.
  2. are always at the same point only for spherical bodies.
  3. can never be at the same point.
  4. is close to each other for objects, say of sizes less than 100 m.
  5. both can change if the object is taken deep inside the earth.

Give one example each of central force and non-central force.


Draw areal velocity versus time graph for mars.


A star like the sun has several bodies moving around it at different distances. Consider that all of them are moving in circular orbits. Let r be the distance of the body from the centre of the star and let its linear velocity be v, angular velocity ω, kinetic energy K, gravitational potential energy U, total energy E and angular momentum l. As the radius r of the orbit increases, determine which of the above quantities increase and which ones decrease.


Two planets A and B of equal mass are having their period of revolutions TA and TB such that TA = 2TB. These planets are revolving in the circular orbits of radii rA and rB respectively. Which out of the following would be the correct relationship of their orbits?


When is a planet moving fastest in its orbit?


Share
Notifications

Englishहिंदीमराठी


      Forgot password?
Use app×