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Nokesh
SATELLITE   by   Prabhakar
Satellite:- revolves around planet,
            Uniform velocity,
             fixed orbit
 Satellite are of two types:-

  1.Artificial satellite
  •Ex-polar satellite

  2.Natural satellite
  •Ex-moon
Natural Satellite:-           A Natural Satellite is a
                               Natural Body which revolves
around(orbits) a Planet .It is usually called moon and is
large and ball shaped.

There are 177 natural satellite in our solar system.


  Mercury-0
  Venus-0
  Earth-1
  Jupiter-67
  Saturn-62
  Uranus-27
  Neptune-13
  Mars-2
  Pluto-5
Artificial Satellite:-A Artificial Satellite is an
                    object which has been placed
into orbit by human endeavour.

Sputnik 1 –launched by Soviet union in 1957.

Artificial Satellite is of two types :-

1..Geostationary Satellite

2. Polar Satellite.
Geostationary Satellite
1.Rotates around the Earth over equator
2.Fixed over a particular place
3.40,000 km above the Earth surface
4.Time period is 24 hours
5.Used in telecommunication
Polar Satellite
1.Rotates around the Earth from pole to pole
2.Rotate around the Earth 8-10 times per day
3.Only 300-400 km above the earth surface
4.Time period is 2-3 hours
5.Used in weather broadcasting ,remote sensing and G.p.s
Escape Velocity of a Satellite:- maximum
speed to which a object is projected so that it
moves out of gravitational field .

Luna 1
The escape velocity of a satellite is




          with                            with
Locatio                         Locatio
          respect       Ve[2]             respect       Ve[2]
n                               n
          to                              to

on        the
                     617.5 k
the Sun   Sun's
                        m/s
,         gravity:

        Mercury                 at      the
on Merc              4.3 km/                        67.7 km
        's                      Mercury Sun's
ury,                       s                              /s
        gravity:                ,       gravity:
the                    at the
                        11.2 km/              the Sun's   42.1 km/
on Earth,   Earth's                Earth/Mo
                               s              gravity:           s
            gravity:               on,


on          the                               the
                                   at the
the Moon    Moon's      2.4 km/s              Earth's     1.4 km/s
                                   Moon,
,           gravity:                          gravity:



            Mars'                             the Sun's   34.1 km/
on Mars,                5.0 km/s   at Mars,
            gravity:                          gravity:           s




on Jupite   Jupiter's   59.5 km/   at         the Sun's   18.5 km/
r,          gravity:           s   Jupiter,   gravity:           s
on Satur    Saturn's   35.6 km               at        the Sun's   13.6 km
n,          gravity:         /s              Saturn,   gravity:          /s


on Uran     Uranus'    21.2 km               at        the Sun's   9.6 km/
us,         gravity:         /s              Uranus,   gravity:          s


            Neptune'                         at
on Nept                23.6 km                       the Sun's
            s                                Neptune               7.7 km/
une,                         /s                      gravity:
            gravity:                         ,


on Pluto,                 Pluto's gravity:                         1.2 km/s

                          the Milky Way's
in the Solar System,                                          ≥ 525 km/s[3]
                          gravity:

                          a black hole's
on the event horizon,                                      = 299,792 km/s
                          gravity:
Orbital Velocity:- velocity at which an
satellite rotates around a planet.



Orbital velocity of a satellite

                     =√gr
Relation between orbital velocity and Escape
velocity
Time Period of a satellite:- time
taken by a satellite for 1 revolution.

The time period of a satellite




     T=2∏r×√r
       √GM
Height of a satellite:- the
expression to find out height of
satellite is
Total Energy of a satellite :-
Kinetic energy of a satellite=
                                   GMm
                                    2r
Potential energy of a satellite=
                                  -GMm
                                     r
Total energy of a satellite= K.E-P.E
       =GMm - GMm
         2r    r
         =-GMm
            2r
Kepler‘s law of Elliptical orbit

According to kepler’s 1st law the orbits of all planets
are elliptical and sun remains at one of the focus
Kepler’s law of aerial velocity

According to kepler’s 2nd law , a planet
covers equal area in equal interval of time.
Kepler’s law of time period
According to kepler’s 3rd law ,square of the
time period is directly proportional to the
cube of the semi-major axis.

        T²          r³

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Satellite

  • 1. Nokesh SATELLITE by Prabhakar
  • 2. Satellite:- revolves around planet, Uniform velocity, fixed orbit Satellite are of two types:- 1.Artificial satellite •Ex-polar satellite 2.Natural satellite •Ex-moon
  • 3. Natural Satellite:- A Natural Satellite is a Natural Body which revolves around(orbits) a Planet .It is usually called moon and is large and ball shaped. There are 177 natural satellite in our solar system. Mercury-0 Venus-0 Earth-1 Jupiter-67 Saturn-62 Uranus-27 Neptune-13 Mars-2 Pluto-5
  • 4. Artificial Satellite:-A Artificial Satellite is an object which has been placed into orbit by human endeavour. Sputnik 1 –launched by Soviet union in 1957. Artificial Satellite is of two types :- 1..Geostationary Satellite 2. Polar Satellite.
  • 5.
  • 6. Geostationary Satellite 1.Rotates around the Earth over equator 2.Fixed over a particular place 3.40,000 km above the Earth surface 4.Time period is 24 hours 5.Used in telecommunication
  • 7.
  • 8. Polar Satellite 1.Rotates around the Earth from pole to pole 2.Rotate around the Earth 8-10 times per day 3.Only 300-400 km above the earth surface 4.Time period is 2-3 hours 5.Used in weather broadcasting ,remote sensing and G.p.s
  • 9.
  • 10. Escape Velocity of a Satellite:- maximum speed to which a object is projected so that it moves out of gravitational field . Luna 1
  • 11. The escape velocity of a satellite is with with Locatio Locatio respect Ve[2] respect Ve[2] n n to to on the 617.5 k the Sun Sun's m/s , gravity: Mercury at the on Merc 4.3 km/ 67.7 km 's Mercury Sun's ury, s /s gravity: , gravity:
  • 12. the at the 11.2 km/ the Sun's 42.1 km/ on Earth, Earth's Earth/Mo s gravity: s gravity: on, on the the at the the Moon Moon's 2.4 km/s Earth's 1.4 km/s Moon, , gravity: gravity: Mars' the Sun's 34.1 km/ on Mars, 5.0 km/s at Mars, gravity: gravity: s on Jupite Jupiter's 59.5 km/ at the Sun's 18.5 km/ r, gravity: s Jupiter, gravity: s
  • 13. on Satur Saturn's 35.6 km at the Sun's 13.6 km n, gravity: /s Saturn, gravity: /s on Uran Uranus' 21.2 km at the Sun's 9.6 km/ us, gravity: /s Uranus, gravity: s Neptune' at on Nept 23.6 km the Sun's s Neptune 7.7 km/ une, /s gravity: gravity: , on Pluto, Pluto's gravity: 1.2 km/s the Milky Way's in the Solar System, ≥ 525 km/s[3] gravity: a black hole's on the event horizon, = 299,792 km/s gravity:
  • 14. Orbital Velocity:- velocity at which an satellite rotates around a planet. Orbital velocity of a satellite =√gr Relation between orbital velocity and Escape velocity
  • 15.
  • 16. Time Period of a satellite:- time taken by a satellite for 1 revolution. The time period of a satellite T=2∏r×√r √GM
  • 17. Height of a satellite:- the expression to find out height of satellite is
  • 18. Total Energy of a satellite :- Kinetic energy of a satellite= GMm 2r Potential energy of a satellite= -GMm r Total energy of a satellite= K.E-P.E =GMm - GMm 2r r =-GMm 2r
  • 19. Kepler‘s law of Elliptical orbit According to kepler’s 1st law the orbits of all planets are elliptical and sun remains at one of the focus
  • 20. Kepler’s law of aerial velocity According to kepler’s 2nd law , a planet covers equal area in equal interval of time.
  • 21. Kepler’s law of time period According to kepler’s 3rd law ,square of the time period is directly proportional to the cube of the semi-major axis. T² r³