BASICS OF BASICS
BASIC DEFINITIONS
1. Speed (scalar) • At instant Ø Equal to velocity at instant • Average over period of time Ø ����� = Ø Distance rigorously speaking requires curve length integral calculation 2. Velocity (vector) • At instant Ø Magnitude is equal to speed at instant • Average over period of time Ø �������� = Ø Displacement = change in position vector. 3. Mechanical energy • Kinetic energy + potential energy
� = � + �
GRAVITY
NEWTON’S LAW OF UNIVERSAL GRAVITATION
NEWTON’S LAW OF UNIVERSAL GRAVITATION
1. Any two bodies in universe attract each other with force that follows: � � � = � � �� � �� � ��� �������� ������ ����: � = = � � + ℎ
• � , � measured in kg • � is distance between � ��� � (Usually point approximation is used, i.e. r is distance between centres of � & � , this is reasonably valid when distance between mass is large compared to size of objects) • G is gravitational constant: � ≈ 6.67 ∗ 10 �� �� (this is quite small, i.e. only significantly heavy objects will exert significant forces)
• � ⃗ measured in N. When acted on one of object in pair, it points towards other object
2. Alternative Forms: Universal Law of Gravitation can be rewritten in below forms relating to exact mass one is referring to (these are useful when calculating integrals, i.e. for potential): • Below are all quite confusing, best method is to just remember gravity is attractive, & consider specific cases accordingly. • ����� �� � : � ⃗ = � �̂, �ℎ��� �̂ ������ ���� � �� � • �����������: ����� �� � : � ⃗ = −� �̂, �ℎ��� �̂ ������ ���� � �� � (this is just reversal of �̂ from former) • ����� �� � can be derived from above by adding negative sign in front of equation, since by Third Law force is equal & opposite in direction. 3. Shell Theorem: • spherical empty shell of mass with uniform distribution exerts gravitational force to objects outside it as if all mass in shell is concentrated at its centre • Solid sphere case: If solid sphere can be separated into layers of empty uniform shells as mentioned above, then clearly repetitive application of shell theorem show that sphere exerts gravity to objects outside it as if all its mass is concentrated in its centre. • Shell Theorem as Approximation for celestial bodies: planets, stars, etc. generally have layered mass structure that is similar to ideal shell theorem shell layer scenario, consequently, their gravitational force can usually be approximated using solid sphere case aforementioned. 4. Inverse square law (for gravity) 1 � ∝ (������� �� �ℎ� ��� �������� ����������) � • Applies also for other forces, i.e. Coulomb’s force (electrostatic force) • visualization of why such effect occurs (of course, this is theory, & not universal clearly for all forces): FREEVCENOTES . COM
SEVERAL GRAVITATIONAL SYSTEMS COM 1. Solar system . • Overwhelming mass of sun maintains stability (other planets, due to mutual attraction, causes sun to ‘wobble’, but their effects are minimal due to its large mass & thus less acceleration relatively speaking wrt planets) 2. Earth-moon system • Earth less acceleration, same reason as why sun relatively less acceleration in solar system wrt to planets. • Nevertheless, moon’s gravitational force has effects on Earth, i.e. tides (hence term tidal forces)
MEASURING GRAVITATIONAL CONSTANT, G VIA TORSION BALANCE
1. Torsion balances measure very small twisting forces 2. Henry Cavendish’s experiment in 1798 had design of torsion balance that could measure forces smaller than 1 ��. He used to it measure force exerted by lead balls held small distance apart, which in turn may be used to calculate value of G.
WEIGHT
1. Refers to gravitational force object experiences, not mass like people treat it in daily life, i.e.:
����ℎ� = � • ����ℎ� = �� ( formula used in Unit 2) is just special case of general Universal Gravitation Law where object is on surface of earth. • � �� ������� �� ����ℎ (acceleration due to gravity) is generally taken as 9.8 (�� 9.81) �� � �� � = = � � 2. Apparent weightlessness: (though in text, this term is not part of stud. design., but likely examined via alternate terminology) • Sample response from 2018 Exam rep. Ø ‘zero gravity experience’ is due to the lack of a contact or normal force () o More detailed (personal addition): due to the lack of a contact/normal force arising from the approximate equivalence in acceleration between the object and its surroundings • Refers to gravitational force ‘felt’ Ø normal reaction force acting against gravity to an object to cancel unequal acceleration between objects (usually what Phys 34 seeks for) Ø Tidal forces may used to detect gravity, but they really aren’t what you typically associate with ‘weight’ Ø May well be no real acceleration due to gravity, but weight may be perceived (e.g. centrifuge, artificial gravity) • Cases where apparent weight is different from weight: Ø Orbit Ø Freefall FREEVCENOTESØ Accelerating lift • Note that true weightlessness is when gravitational force is 0, whereas apparent weightlessness is just what one feels is 0.
OTHER
1. Gravity ‘drives universe’ • force that first caused particles to coalesce into atoms, & atoms to congregate into nebulas/planets/stars
GRAVITATIONAL FIELDS
GRAVITATIONAL FIELDS
1. Proposed in 18th century, to simplify effects of forces 2. Mental constructs initially (though now though to be legitimate entities that may say carry energy) 3. Refer to region where gravitational force exerted on all matter within 4. Every physical object of mass has accompanying gravitational field 5. Special in that field strength = acceleration (equivalence principle)
INVERSE SQUARE LAW 1. Applies to many forces 1 � ∝ � 2. A intuitive visualization
COM .
NEPTUNE DICOVERY
1. Discovered through its gravitational effect on other planets. 2. Uranus orbit appeared different from those calculated from Sun’s gravity & other known planets’ gravity → possibly unknown planet caused this, which led to discovery of Neptune
REPRESENTING GRAVITATIONAL FIELDS
1. Field lines: shows direction of field intensity, i.e. gravitational acceleration in region of space 2. Closely spaced arrows: strong field 3. Widely spaced arrows: weaker field 4. Parallel arrows: same direction (if spaced out equally, then would also imply constant field strength, so uniform field) 5. Field lines can never cross 6. Infinite number of field lines can be drawn, only few are chosen to represent to rest
GRAVITATIONAL FIELD STRENGTH
1. Gravitational fields theoretically extend infinitely out into space 2. By inverse square law, gravitational field strength is decrease by distance 3. Formula for gravitational field strength:
� �� GM g = = = (M often denotes source mass) FREEVCENOTES� � r 4. Gravitational field strength is equivalent to gravitational acceleration by equivalence principle (gravitational mass is equal to inertial mass) 5. Unit of field strength: N kg (note acceleration unit is m s , which is equivalent)
VARIATIONS IN GRAVITATIONAL FIELD STRENGTH OF EARTH