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Revision: Gravitation Science English Medium Class 9 CBSE

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Definitions [20]

Definition: Gravitation

"Every particle of matter in the universe attracts every other particle with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them. The direction of the force is along the line joining the particles."

or

The force by which the Earth attracts objects towards its centre is called gravitational force.

OR

The force of mutual attraction that any two objects in the universe exert on each other, which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centres, is called the gravitational force.

Definition: Universal Law of Gravitation

"Every particle of matter attracts every other particle of matter with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between them."

Define acceleration due to gravity.

The acceleration produced in a body under the influence of the force of gravity alone is called acceleration due to gravity.

Definition: Acceleration Due to Gravity

The gravitational force due to the earth on a body results in its acceleration. This is called acceleration due to gravity and is denoted by ‘g’.

OR

When a body falls towards the Earth under gravity, then the acceleration produced in the body due to gravity is called acceleration due to gravity, which is denoted by g.

Definition: Mass

Mass is the amount of matter present in the object. The SI unit of mass is kg.

Definition: Weight

The weight of an object is defined as the force with which the earth attracts the object.

Definition: Gauge Pressure

The difference between the hydrostatic pressure (P) and the atmospheric pressure (P₀), measured by a manometer, is called gauge pressure: P − P0 = ρgh

Define thrust.

The force which produces compression is called thrust. Its S.I unit is the newton.

Definition: Density

The mass per unit volume of a substance is called density: ρ = M/V

  • SI Unit: kg/m³, Dimensions: [ML−3T0

Definition: Specific Weight or Weight Density

The weight per unit volume of a substance is called specific weight or weight density: W = mg/V

  • SI Unit: N/m³

Definition: Relative Density

The ratio of the density of a given fluid to the density of pure water at 4°C is called relative density. It is a unitless quantity.

Definition: Pressure

The thrust (Normal Force) exerted by a liquid at rest on unit area of the surface in contact is called pressure.

P = \[\frac {F_⊥​​}{A}\]

  • SI Unit: pascal (Pa) = 1 Nm⁻²
    Dimensions: [ML−1T−2]

Definition: Gauge Pressure

The difference between the absolute pressure and the atmospheric pressure at a point in a liquid is called gauge pressure.

Definition: Earth's Atmosphere

The gaseous envelope surrounding the earth is called the earth's atmosphere.

Definition: Atmospheric Pressure

The pressure exerted by the atmosphere on the earth's surface is called atmospheric pressure.

Definition: Absolute Pressure

The total pressure exerted by a fluid, which includes both the atmospheric pressure as well as any other additional pressure due to the fluid itself, is called absolute pressure.

Definition: Hydrostatic Paradox

The phenomenon in which the liquid pressure at a point is independent of the quantity of liquid and depends only upon the depth of the point below the liquid surface is called hydrostatic paradox.

What is the unit of relative density?

UNIT OF RELATIVE DENSITY: No units since it is a pure ratio.

Define the term relative density of a substance.

RELATIVE DENSITY: “is the ratio of the density of a substance to the density of water at 4° C.”
Or
RELATIVE DENSITY “is the ratio of the mass of the substance to the mass of an equal volume of water at 4° C.”

Define the term Density of a substance.

Density of a substance is defined as “Mass per Unit volume”.

Density [d]=`"mass  of the substance"/"volume of the substance"`

d=`m/v`

Formulae [5]

Formula: Gravitation

Newton’s Universal Law of Gravitation:
F = \[G\frac{m_1m_2}{r^2}\]

where:

  • F = Gravitational force between two objects
  • m1,m2 = Masses of the two objects
  • r = Distance between the centers of the two masses
  • G = Universal gravitational constant = 6.67×10−11 Nm2/kg2
Formula: Universal Law of Gravitation

The gravitational force of attraction (F) between two bodies of mass m1 and m2 separated by a distance r is:

\[\mathbf{F} = \mathbf{G}\frac{m_1 m_2}{r^2}\]
  • F: Gravitational Force of attraction (in Newtons, N).

  • \[m_1, m_2\]: Masses of the two objects (in kilograms, kg).

  • r (or d in the first part): Distance between the two objects (in meters, m).

  • G: The constant of proportionality, called the Universal gravitational constant.

    • Value in SI units: \[G=6.67\times10^{-11}\mathrm{N}\cdot\mathrm{m}^2/\mathrm{kg}^2\]

    • Dimensions: \[[G]=[\mathrm{L}^3\mathrm{M}^{-1}\mathrm{T}^{-2}]\]

Formula: Acceleration due to gravity

The value of the acceleration due to gravity (g) on the surface of the Earth is given by the formula:

\[g = \frac{G M}{R^2}\]

Where:

  • g = Acceleration due to gravity (in m/s²).
  • G = Newton's Universal Gravitational Constant (≈ 6.67 × 10⁻¹¹ N · m² / kg²).
  • M = Mass of the Earth (≈ 6 × 1024 kg).
  • R = Radius of the Earth (≈ 6.4 × 10⁶ m).
Formula: Atmospheric Pressure Value

1 atm = 1.01 × 105 Pa = 1.01 bar = 760 torr

Formula: Gauge Pressure Relation

Pgauge = Pabsolute​ − Patmospheric​

Theorems and Laws [1]

Law: Universal Law of Gravitation

Statement:

The law which states that every particle of matter attracts every other particle in the universe with a force whose magnitude is directly proportional to the product of masses and inversely proportional to the square of distance between them is called Newton's Law of Gravitation.

Derivation:

Newton's Universal Law of Gravitation states that every particle of matter attracts every other particle of matter with a force which is:

  • Directly proportional to the product of their masses: F ∝ m1 ⋅ m2
  • Inversely proportional to the square of the distance between them: F ∝ \[\frac {1}{r^2}\]

Combining both, the gravitational force is expressed as:

F = G\[\frac{m_1m_2}{r^2}\]

where G is the Universal Gravitational Constant, measured by Henry Cavendish using the Cavendish balance, with the value:

G = 6.67 × 10−11Nm2/kg2

Key Points

Key Points: Newton's Universal Law of Gravitation
  • Every object attracts every other with a gravitational force.
  • Force increases with mass — more mass means a stronger pull.
  • Force decreases with distance — doubling the distance halves the force.
  • A force acts along the line joining the centres (or centres of mass) of the two bodies.
Key Points: Free Fall
  • Free fall occurs when an object moves only under the influence of gravity, with no other forces acting on it.
  • In free fall, initial velocity (u) = 0 and acceleration = g (acceleration due to gravity).
  • The equations of motion for free fall are:
    v = gt
    s = \[\frac {1}{2}\]gt2
    v2 = 2gs
  • True free fall occurs in a vacuum, as air resistance affects motion on Earth.
  • The Moon and satellites are in free fall because they move only under Earth’s gravitational field.
 
Key Points: Variation in Acceleration due to Gravity
  • Due to Altitude: The acceleration due to gravity decreases with altitude as we move away from the surface of the Earth. As h↑, g↓.
  • Due to Depth: The acceleration due to gravity decreases as we move into the Earth's interior, i.e., with increasing depth. As d↑, g↓.
  • Due to Latitude: The acceleration due to gravity increases with latitude. At the poles (θ = 90°), g = gmax⁡​; at the equator (θ = 0°), g = gmin​.
  • Due to Shape of Earth: The equatorial radius of the Earth is greater than the polar radius. Since g ∝ \[\frac {1}{R^2}\], the acceleration due to gravity is greater at the poles compared to the equator, i.e., Requator > Rpole​ and gequator < gpole​.
Key Points: Liquid Pressure
  • Pressure exerted by a liquid column depends on height and density of the liquid column.
  • It is independent of the shape of the containing vessel or total mass of the liquid.
  • Atmospheric pressure is maximum at the surface of the earth and decreases as we move up into the atmosphere.
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