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182                                                                                    PHYSICS

                                        velocities taken relative to the centre of mass. Remember  ′ =r  r  – R ; rest of the
                                                                                            i   i
                                        notation is the standard notation used in the chapter. Note  ′ L   and  M ×R V  can
                                        be said to be angular momenta, respectively, about and of the centre of mass of
                                        the system of particles.
                                              d ′        d ′
                                                          p
                                               L
                                     (d) Show    = ∑  r i ′ ×
                                              dt         dt
                                        Further, show that
                                        d ′
                                          L
                                            = ′ ττ
                                         dt    ext
                                        where  ′ τ ττ τ ext   is the sum of all external torques acting on the system about the
                                        centre of mass.
                                        (Hint : Use the definition of centre of mass and third law of motion. Assume the
                                        internal forces between any two particles act along the line joining the particles.)



                                                      Pluto - A Dwarf Planet


                          The International Astronomical Union (IAU) at the IAU 2006 General Assembly
                          held on August 24, 2006, in Prague in Czech Republic, adopted a new
                          definition of planets in our Solar System. According to the new definition,
                          Pluto is no longer a planet. This means that the Solar System consists of
                          eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and
                          Neptune. According to the IAU usage, the ‘planet’ and ‘other bodies’ in our
                          Solar System, except satellites, are to be defined into three distinct categories
                          of celestial objects in the following way:
                          1. A ‘planet’ is a celestial body that (a) is in orbit around the Sun, (b) has
                              sufficient mass for its self-gravity to overcome rigid body forces so that it
                              assumes a hydrostatic equilibrium (nearly round) shape, and (c) has
                              cleared the neighbourhood around its orbit.
                          2. A ‘dwarf planet’ is a celestial body that (a) is in orbit around the Sun,
                              (b) has sufficient mass for its self-gravity to overcome rigid body forces so
                              that it assumes a hydrostatic equilibrium (nearly round) shape, (c) has
                              not cleared the neighbourhood around its orbit, and (d) is not a satellite.

                          3. All ‘other objects’, except satellites, orbiting the Sun, shall be referred to
                              collectively as ‘Small Solar-System Bodies’.

                              Unlike other eight planets in the Solar System, Pluto’s orbital path overlaps
                          with ‘other objects’ and the planet Neptune. The ‘other objects’ currently
                          include most of the Solar System asteroids, most of the Trans-Neptunian
                          Objects (TNOs), comets, and other small bodies.
                              Pluto is a ‘dwarf planet’ by the above definition and is recognised as the
                          prototype of a new category of Trans-Neptunian Objects.












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