The gravitational constant (also known as the universal gravitational constant, the Newtonian constant of gravity, or the Cavendish gravitational constant), denoted by the letter G, is an empirical physical constant that is defined in Sir Isaac Newton’s law of universal gravitational effects. included in the calculation. In Gravity and Albert Einstein’s General Theory of Relativity.
Each measurement has two parts. The first one is a number (n) and the next one is a unit (u). Q = no. For example, length of an object = 40 cm. A number expressing the magnitude of a physical quantity is inversely proportional to the chosen unit.
Understanding the concepts of Units and Dimensions, as well as Gravitation, is fundamental in physics. Here are some reputable resources that provide comprehensive notes on these topics, available for download in PDF format:
Units and Dimensions:
-
Career Point Kota – Units and Dimensions:
- This material offers an in-depth overview of different units of physical quantities, the concept of dimensions, and their applications in physics.
- Access the PDF here:
-
Resonance – Units & Dimensions:
- This document provides detailed explanations of fundamental quantities, derived quantities, and the importance of dimensional analysis in physics.
- Access the PDF here:
Gravitation:
-
Vedantu – Class 11 Physics Chapter 8: Gravitation:
- These revision notes cover topics such as Newton’s law of universal gravitation, gravitational potential energy, and the motion of planets and satellites.
- Access the PDF here:
-
MasterJEE Classes – Gravitation:
- This resource delves into Newton’s law of gravitation, gravitational field intensity, and potential, providing a thorough understanding of the subject.
- Access the PDF here:
These resources should assist you in gaining a comprehensive understanding of Units and Dimensions, as well as Gravitation, enhancing your physics studies.
Physics Unit and Dimension Gravitation Notes Pdf Download
Physics Notes Class 11 CHAPTER 8 GRAVITATION
Unit dimensions and Measurement
Physics_Unit & Dimension.p65
01 Units and Measurements
GRAVITATION
gravitation.pdf
1. Units and Dimensions
A. Introduction
- Physical Quantity: A property that can be measured (e.g., length, mass, time).
- Units: Standard measurement of a physical quantity (e.g., meter, kilogram, second).
- Dimensions: Express physical quantity in terms of fundamental quantities (M, L, T).
B. Fundamental Quantities & Units
| Quantity | Symbol | SI Unit |
|---|---|---|
| Length | L | meter (m) |
| Mass | M | kilogram (kg) |
| Time | T | second (s) |
| Electric Current | I | ampere (A) |
| Temperature | θ | kelvin (K) |
| Luminous Intensity | Iv | candela (cd) |
| Amount of Substance | N | mole (mol) |
C. Derived Quantities
- Expressed as a combination of fundamental quantities
- Examples:
- Velocity: [v]=LT−1[v] = L T^{-1}[v]=LT−1
- Acceleration: [a]=LT−2[a] = L T^{-2}[a]=LT−2
- Force: [F]=MLT−2[F] = M L T^{-2}[F]=MLT−2
D. Dimensional Formula & Equations
- Dimensional formula: Represents physical quantity in terms of M, L, T, etc.
- Dimensional equation: Relates physical quantities mathematically using their dimensions.
- Applications: Checking correctness of equations, deriving relations, converting units
2. Gravitation
A. Universal Law of Gravitation
- Newton’s Law of Gravitation: Every particle attracts every other particle with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
- Equation:
F=Gm1m2r2F = G \frac{m_1 m_2}{r^2}F=Gr2m1m2
where G=6.67×10−11 Nm²/kg²G = 6.67 \times 10^{-11} \, \text{Nm²/kg²}G=6.67×10−11Nm²/kg²
B. Acceleration Due to Gravity
- At the surface of Earth:
g=GMR2g = \frac{G M}{R^2}g=R2GM
- Variation of g with height (h) and depth (d)
gh=g(1−2hR),gd=g(1−dR)g_h = g \left(1 – \frac{2h}{R}\right), \quad g_d = g \left(1 – \frac{d}{R}\right)gh=g(1−R2h),gd=g(1−Rd)
C. Gravitational Potential Energy
- Formula: U=−Gm1m2rU = – \frac{G m_1 m_2}{r}U=−rGm1m2
- Negative sign indicates bound system
D. Escape Velocity
- Minimum velocity to escape Earth’s gravity:
ve=2GMR=2gRv_e = \sqrt{\frac{2GM}{R}} = \sqrt{2 g R}ve=R2GM=2gR
E. Orbital Motion
- Orbital velocity: v=GMrv = \sqrt{\frac{GM}{r}}v=rGM
- Satellite period: T=2πr3GMT = 2 \pi \sqrt{\frac{r^3}{GM}}T=2πGMr3
F. Important Notes
- Weight is the force due to gravity: W=mgW = mgW=mg
- Free fall is motion under gravity only, ignoring air resistance
- Kepler’s Laws of Planetary Motion often applied in Gravitation problems
3. Tips for Using the Notes
- Memorize key formulas for G, g, escape velocity, and orbital motion.
- Practice numerical problems regularly.
- Use dimensional analysis to check equations in mechanics.
- Draw diagrams for better understanding of orbits and forces.
