| Non-Rationalised Geography NCERT Notes, Solutions and Extra Q & A (Class 6th to 12th) | |||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 6th | 7th | 8th | 9th | 10th | 11th | 12th | |||||||||||||||||||||
Class 11th Geography NCERT Notes, NCERT Question Solutions and Extra Q & A (Non-Rationalised)
Fundamentals of Physical Geography
1. Geography As A Discipline
This introductory chapter establishes geography as a scientific and interdisciplinary field that studies the Earth's surface, its features, inhabitants, and phenomena. It moves beyond simply locating places, asking the core questions of "what is where, and why is it there?". The chapter explores the dualism within the discipline, such as the debate between a systematic approach (studying one phenomenon across the globe) and a regional approach (studying all phenomena within a specific area). It outlines the main branches of geography, including physical geography (studying the natural environment like landforms, climate, and ecosystems) and human geography (studying human-environment interactions, population, and settlements). The chapter emphasizes geography's crucial role in understanding spatial patterns, environmental systems, and the complex relationship between humans and their environment, providing a foundational framework for all subsequent geographical studies.
2. The Origin And Evolution Of The Earth
This chapter journeys back in time to explore the scientific theories explaining the origin and evolution of the Earth and the cosmos. It begins with the universally accepted Big Bang Theory, which describes the origin of the universe from a singular point of infinite density about 13.7 billion years ago. It then discusses theories on the formation of stars and planets, including the early Nebular Hypothesis by Kant and Laplace. The chapter details the stages of Earth's formation, from a hot, barren planet to its present state. This includes the process of differentiation, which led to the formation of the Earth's layered structure (crust, mantle, and core), and the evolution of the lithosphere, atmosphere, and hydrosphere through processes like degassing and condensation. Finally, it touches upon the origin of life, providing a cosmic and geological context for our planet's existence.
3. Interior Of The Earth
This chapter delves into the mysterious interior of the Earth, a region inaccessible to direct observation. It explains how our knowledge is derived from direct sources (like mining and drilling) and, more importantly, indirect sources, with a focus on seismic waves (P-waves and S-waves) from earthquakes. The behaviour of these waves—their velocity, reflection, and refraction as they travel through the Earth—reveals the properties and boundaries of its different layers. The chapter provides a detailed description of the Earth's concentric structure: the crust (the thin, solid outer layer), the mantle (a thick, semi-molten layer containing the asthenosphere on which tectonic plates float), and the core (the extremely hot, dense centre, with a liquid outer core and a solid inner core). Understanding this layered structure is fundamental to explaining major geological phenomena.
4. Distribution Of Oceans And Continents
This chapter explains the dynamic nature of the Earth's surface by exploring theories about the distribution of oceans and continents. It starts with Alfred Wegener's groundbreaking Continental Drift Theory, which proposed that continents were once joined together in a supercontinent called Pangaea and have since drifted apart. Wegener supported his theory with compelling evidence like the jigsaw fit of coastlines, fossil distribution, and geological similarities across continents. The chapter then transitions to the more comprehensive and modern theory of Plate Tectonics. This theory explains that the Earth's lithosphere is divided into several major and minor plates that are constantly in motion. The interaction at the plate boundaries (convergent, divergent, and transform) is responsible for most of the world's earthquakes, volcanic eruptions, and the formation of major landforms like the Himalayas, which were formed by the collision of the Indian and Eurasian plates.
5. Minerals And Rocks
This chapter focuses on the fundamental components of the Earth's lithosphere: minerals and rocks. A mineral is defined as a naturally occurring inorganic substance with an orderly atomic structure and a definite chemical composition. The chapter discusses common rock-forming minerals like feldspar and quartz. A rock is an aggregate of one or more minerals. The chapter provides a detailed classification of rocks into three major families based on their mode of formation. Igneous rocks are formed from the cooling and solidification of magma or lava. Sedimentary rocks are formed from the accumulation, compaction, and cementation of sediments over a long period. Metamorphic rocks are formed when existing igneous or sedimentary rocks are changed by heat, pressure, or chemical action. The chapter concludes with the concept of the Rock Cycle, illustrating the continuous process through which rocks are transformed from one type into another.
6. Geomorphic Processes
This chapter focuses on the various geomorphic processes that continuously shape and modify the Earth's surface. These processes are broadly classified into two categories. Endogenic forces, which originate from within the Earth's interior, are the 'land-building' forces. They include diastrophism (slow movements like mountain building) and sudden movements like earthquakes and volcanism. In contrast, exogenic forces originate from the atmosphere and are the 'land-wearing' forces. These forces, powered by solar energy, lead to denudation—the overall lowering of the Earth's surface through processes like weathering (the breakdown of rocks in situ), mass wasting (movement of material down a slope due to gravity), and erosion (the acquisition and transportation of rock debris by agents like running water, wind, and glaciers). The interplay between these internal and external forces creates the diverse landscapes we see on Earth.
7. Landforms And Their Evolution
Building on the previous chapter, this one examines the specific landforms created by different exogenic agents and their evolution over time. It details the work of running water (fluvial processes), which creates features like V-shaped valleys, waterfalls, meanders, and deltas. It explores the action of glaciers (glacial processes), which carve out U-shaped valleys, cirques, and deposit moraines. The chapter also discusses the work of wind in arid regions (aeolian processes), which forms landforms like sand dunes and mushroom rocks, the work of groundwater which creates unique karst topography (like stalactites and stalagmites) in limestone regions, and the action of sea waves on coastlines. It illustrates how these landforms evolve through stages of youth, maturity, and old age, following a conceptual "cycle of erosion," which helps in understanding the dynamic history of any landscape.
8. Composition And Structure Of Atmosphere
This chapter introduces the Earth's atmosphere, the protective blanket of gases essential for life. It begins with the composition of the atmosphere, detailing the major gases: Nitrogen (78.08%) and Oxygen (20.95%), along with minor gases like Argon, Carbon Dioxide, and trace gases, as well as variable components like water vapour and dust particles. The chapter then explains the vertical structure of the atmosphere, which is divided into five distinct layers based on temperature profiles. These layers are: the Troposphere (where all weather phenomena occur and temperature decreases with height), the Stratosphere (which contains the vital ozone layer that protects us from harmful UV radiation), the Mesosphere (where meteors burn up), the Thermosphere (containing the ionosphere, which aids in radio communication), and the outermost Exosphere.
9. Solar Radiation, Heat Balance And Temperature
This chapter explains the energy dynamics of the Earth's climate system, starting with solar radiation, or insolation, which is the primary source of energy. It discusses how this energy heats the Earth's surface and atmosphere. A key concept explained is the Earth's heat balance or heat budget, which details how the Earth maintains a stable average temperature by balancing the amount of incoming solar radiation with the amount of outgoing terrestrial radiation. The chapter also explores the factors that influence the distribution of temperature across the globe, such as latitude (angle of the sun's rays), altitude (height above sea level), distance from the sea (continentality), prevailing winds, and ocean currents. It introduces the concept of temperature inversion and the use of isotherms to map temperature distribution.
10. Atmospheric Circulation And Weather Systems
This chapter explores the large-scale movement of air, known as atmospheric circulation, which distributes heat around the globe and creates our weather. It explains the relationship between air pressure and wind, detailing the formation of global pressure belts and the resulting permanent wind systems, including the Trade Winds, Westerlies, and Polar Easterlies, all influenced by the Coriolis force. The chapter then delves into various weather systems, explaining the formation of air masses and fronts. It provides a detailed look at cyclones, distinguishing between Tropical Cyclones (like hurricanes and typhoons) which form over warm oceans, and Extra-Tropical (Temperate) Cyclones which form in the mid-latitudes along the polar front.
11. Water In The Atmosphere
This chapter focuses on the crucial role of water in the atmosphere and the processes of the hydrological cycle. It begins by explaining the concepts of evaporation and humidity (the amount of water vapour in the air), distinguishing between absolute and relative humidity. It then details the process of condensation, which occurs when air cools to its dew point, leading to the formation of clouds, dew, fog, and frost. The chapter classifies different types of clouds based on their form (cirrus, cumulus, stratus) and altitude. Finally, it explains precipitation, which is any form of water that falls from the atmosphere to the Earth's surface. It discusses the different forms of precipitation (rain, snow, sleet, hail) and the three main types of rainfall: convectional, orographic (relief), and cyclonic (frontal), which are essential for understanding rainfall patterns worldwide.
12. World Climate And Climate Change
This chapter synthesizes previous concepts to classify and describe the major climate types of the world. It introduces empirical classification systems, with a focus on Koppen's classification scheme, which categorizes world climates into groups and types based on annual and monthly averages of temperature and precipitation. The second part of the chapter addresses the urgent global issue of climate change. It discusses the evidence for climate change, such as rising global temperatures and melting glaciers. It explains the causes, distinguishing between natural factors and anthropogenic (human-induced) causes, primarily the enhancement of the greenhouse effect due to the emission of greenhouse gases from burning fossil fuels. The chapter highlights the potential impacts of global warming and underscores the international efforts needed to mitigate this profound environmental challenge.
13. Water (Oceans)
This chapter shifts focus to the hydrosphere, exploring the vast and vital bodies of saline water known as oceans. It covers the basics of oceanography, including the distribution of oceans and seas and the hydrological cycle. Key characteristics of ocean water, such as temperature and salinity, are discussed, along with the factors that cause their variation both horizontally and vertically (thermocline). The chapter provides a detailed description of the relief of the ocean floor, outlining its major divisions: the continental shelf (shallow, submerged extension of a continent), the continental slope (the steep drop-off), the deep sea plain or abyssal plain (vast, flat areas), and spectacular features like mid-oceanic ridges and oceanic deeps or trenches. This provides a foundational understanding of the marine environment.
14. Movements Of Ocean Water
This chapter examines the three primary types of dynamic movements of ocean water. First, it discusses waves, which are the oscillatory movements of surface water, primarily generated by wind. Second, it explains tides, the periodic and predictable rise and fall of sea level, caused mainly by the gravitational pull of the Moon and the Sun. It distinguishes between spring tides (higher range, during full and new moon) and neap tides (lower range, during quarter moons). Third, it details ocean currents, which are like large rivers flowing within the oceans. These currents, driven by factors like wind, temperature, and salinity differences, are classified as warm or cold currents and play a crucial role in redistributing heat across the globe, thereby significantly influencing regional climates, especially in coastal areas.
15. Life On The Earth
This chapter introduces the ecological perspective in geography, focusing on life on Earth within the Biosphere. It defines an ecosystem as a community of living organisms (biotic components) interacting with each other and their physical environment (abiotic components). The chapter explains the fundamental processes that sustain ecosystems: the one-way flow of energy from the sun through different trophic levels via food chains and food webs, and the cyclical movement of chemical nutrients, known as biogeochemical cycles (e.g., the water cycle, carbon cycle, and nitrogen cycle). It also discusses ecological balance and the concept of biomes—large ecosystems with distinct vegetation and wildlife, like tropical rainforests or deserts.
16. Biodiversity And Conservation
This chapter introduces the concept of biodiversity, defined as the variety and variability of life on Earth. It explains that biodiversity exists at three levels: genetic diversity, species diversity, and ecosystem diversity. The chapter highlights the immense value of biodiversity for human survival, providing essential ecosystem services and resources. It then discusses the alarming rate of biodiversity loss due to human activities, identifying major threats like habitat destruction, over-exploitation, pollution, and climate change, leading to species becoming endangered or extinct. Finally, it explores the critical need for conservation, outlining the two main strategies: in-situ (on-site) conservation, which involves protecting species in their natural habitats (e.g., national parks, biosphere reserves), and ex-situ (off-site) conservation, which involves protecting them outside their natural habitats (e.g., zoos, seed banks). India, as a mega-diverse country, plays a significant role in these global conservation efforts.
India Physical Environment
1. India — Location
This chapter provides a precise geographical context for India's location and its strategic importance. It details India's position in the Northern Hemisphere, specifying its latitudinal extent from 8°4' N to 37°6' N and its longitudinal extent from 68°7' E to 97°25' E. It highlights key geographical lines, including the Tropic of Cancer (23°30’ N), which passes through the middle of the country, and the Standard Meridian of India (82°30' E), which is used to determine the Indian Standard Time (IST). The chapter emphasizes India's peninsular shape and its long coastline, which gives it a dominant position at the head of the Indian Ocean. This strategic location has historically facilitated trade, cultural exchange, and maritime connectivity, making India a crucial link between the East and the West.
2. Structure And Physiography
This chapter explores the geological structure that forms the basis of India's varied relief and its major physiographic divisions. Based on geological history, it identifies three main structural units: the ancient and stable Peninsular Block (part of the Gondwana landmass), the geologically young and unstable Himalayan mountain chain, and the Indo-Ganga-Brahmaputra Plain (a geosynclinal depression filled with sediments). Building on this structure, the chapter details India's six major physiographic divisions: The Northern and North-eastern Mountains (The Himalayas), The Northern Plain, The Peninsular Plateau, The Indian Desert, The Coastal Plains, and The Islands. Each division's unique characteristics, formation, and resource base are described, showcasing the immense physical diversity of the Indian subcontinent.
3. Drainage System
This chapter provides a comprehensive analysis of the drainage system of India, which encompasses the network of its rivers. It classifies the river systems based on their origin into two major groups. The Himalayan rivers are perennial, fed by melting glaciers and rainfall, and include three major systems: the Indus, the Ganga, and the Brahmaputra. The Peninsular rivers are generally seasonal and rain-fed. These are further divided into east-flowing rivers (like the Mahanadi, Godavari, Krishna, and Kaveri), which form large deltas, and west-flowing rivers (like the Narmada and Tapi), which flow through rift valleys and form estuaries. The chapter describes the different drainage patterns and highlights the vital role these river systems play in providing water for irrigation, domestic use, and generating hydroelectric power across India.
4. Climate
This chapter offers a detailed examination of the climate of India, which is characterized as a tropical monsoon climate. It delves into the factors that control India's climate, including its latitudinal location, the presence of the Himalayas as a climatic barrier, and the influence of the surrounding oceans. A key focus is on the mechanism of the Indian monsoon, explaining the seasonal reversal of winds due to the differential heating of land and sea, and the role of phenomena like the Jet Stream and El Niño. The chapter describes the four distinct seasons: the cold weather season (winter), the hot weather season (summer), the advancing southwest monsoon (rainy season), and the retreating monsoon. It also highlights the regional variations in climate and the critical importance of the monsoon for India's agriculture-based economy.
5. Natural Vegetation
This chapter explores the rich and diverse natural vegetation of India, which is closely linked to the country's varied climatic and relief conditions. It classifies India's forests into five major types: Tropical Evergreen and Semi-Evergreen Forests (found in high rainfall areas like the Western Ghats), Tropical Deciduous Forests (the most widespread type, also known as monsoon forests, with valuable trees like Teak and Sal), Tropical Thorn Forests (in arid and semi-arid regions), Montane Forests (found in mountainous regions with varying vegetation based on altitude), and Littoral and Swamp Forests (including the unique Mangrove Forests of the Sunderbans). The chapter discusses the characteristics and distribution of these forest types and emphasizes their ecological and economic importance, as well as the need for forest conservation in India.
6. Soils
This chapter provides a detailed study of soils in India, a vital natural resource for agriculture. It begins by explaining the process of soil formation (pedogenesis) and the factors that influence it, including parent material, climate, relief, and time. The chapter then describes the major types of soil found in India based on the classification by the Indian Council of Agricultural Research (ICAR). These include Alluvial soils (most widespread and fertile), Black soils (ideal for cotton), Red and Yellow soils, Laterite soils, Arid soils, and Forest soils. For each type, their characteristics, distribution, and suitability for different crops are discussed. The chapter concludes by addressing the serious problem of soil erosion and the various methods for soil conservation.
7. Natural Hazards And Disasters
This chapter addresses the critical issue of natural hazards and disasters prevalent in India. It explains the difference between a hazard (a potential threat) and a disaster (an actual event causing widespread damage). The chapter details the causes, consequences, and distribution of major natural disasters affecting India, including earthquakes (Himalayan region), floods (Ganga and Brahmaputra plains), droughts (parts of the Peninsular Plateau), cyclones (eastern coast), and landslides (Himalayan and Western Ghats regions). A significant focus is on disaster management, outlining the four stages of the disaster management cycle: mitigation (prevention), preparedness, response, and recovery. It highlights the role of national agencies like the NDMA in creating a more disaster-resilient India.
Practical Word in Geography
1. Introduction To Maps
This chapter serves as a fundamental introduction to maps, defining them as a two-dimensional representation of the Earth's three-dimensional surface, drawn to a scale. It explains the indispensable role of maps in geography for visualizing and analyzing spatial information. The chapter classifies maps into different types based on scale (large-scale and small-scale) and function (physical and cultural/thematic maps). It also introduces the essential components or 'language' of a map: the title, scale, direction, legend (key), and coordinate system, which are crucial for accurate map reading and interpretation. The history of map-making is also briefly touched upon.
2. Map Scale
This practical chapter focuses entirely on the crucial concept of map scale. It defines scale as the ratio between the distance on a map and the corresponding distance on the ground. The chapter details the three primary methods of representing scale: (1) Statement of Scale, a simple verbal description (e.g., '1 cm to 10 km'); (2) Representative Fraction (RF), a universal ratio or fraction (e.g., 1:1,000,000) that is independent of any unit of measurement; and (3) Graphical or Linear Scale, a drawn line subdivided to show map distances. The chapter provides practical exercises on converting between these scale types and using them to accurately measure distances on a map.
3. Latitude, Longitude And Time
This chapter explains the global grid system used for precise location. It defines latitude as the angular distance of a point north or south of the Equator, measured in degrees, with lines of latitude being called parallels. It defines longitude as the angular distance of a point east or west of the Prime Meridian, with lines of longitude being called meridians. The chapter then establishes the critical relationship between longitude and time. It explains how the Earth's 360° rotation in 24 hours means that every 15° of longitude corresponds to a one-hour time difference. This leads to the concept of time zones and the necessity of a Standard Time for each country, like the Indian Standard Time (IST) based on the 82°30' E meridian, and the International Date Line.
4. Map Projections
This chapter deals with the technical challenge of representing the spherical Earth on a flat map, a process known as map projection. It explains that this transformation inevitably causes distortions in one or more properties: shape, area, distance, or direction. The chapter classifies projections based on the developable surface used (cylindrical, conical, and planar/azimuthal) and the property they preserve (e.g., equal-area, conformal). It discusses the uses, advantages, and limitations of different projections, helping students understand why there is no single "perfect" map and why the choice of projection depends on the specific purpose of the map.
5. Topographical Maps
This chapter provides a detailed guide to reading and interpreting topographical maps (or 'topo sheets'), which are large-scale maps showing both natural and man-made features in great detail. It focuses on the key feature of these maps: the representation of relief (elevation and shape of the land) using contour lines. A contour line is an imaginary line connecting points of equal elevation. The chapter explains how to interpret contour patterns to identify landforms like hills, valleys, plateaus, and steep or gentle slopes. It also covers the conventional signs and symbols used to represent various features like settlements, transport networks, and vegetation, making it a vital skill for fieldwork and geographical analysis.
6. Introduction To Aerial Photographs
This chapter introduces aerial photographs as a valuable source of geographical data. It defines them as photographs of the Earth's surface taken from an airborne platform, like an aircraft. The chapter distinguishes between different types, mainly vertical and oblique photographs, and discusses their geometric properties. It highlights the advantages of aerial photos, such as providing a bird's-eye view and capturing data from inaccessible areas. The chapter introduces the basics of photo interpretation, explaining how to identify objects and features based on elements like size, shape, tone, texture, and pattern, and also touches upon the concept of stereoscopic vision for 3D viewing.
7. Introduction To Remote Sensing
This chapter introduces the modern technology of remote sensing, defining it as the science of acquiring information about the Earth's surface without being in physical contact with it. It explains the basic principles, showing how sensors on platforms like satellites or aircraft collect data by recording the energy reflected or emitted from the Earth's surface across different parts of the electromagnetic spectrum. The chapter discusses the stages of remote sensing, from data acquisition to processing and analysis. It highlights the various applications of this powerful technology in fields like resource management, land use mapping, environmental monitoring, and disaster management, noting the significant contributions of organizations like the Indian Space Research Organisation (ISRO) in this domain.
8. Weather Instruments, Maps And Charts
This practical chapter focuses on the tools used to study weather. It introduces a range of weather instruments and their functions for measuring key atmospheric elements: the thermometer for temperature, the barometer for air pressure, the wind vane for wind direction, the anemometer for wind speed, and the rain gauge for measuring rainfall. The chapter then explains how this data is represented on weather maps and charts. It teaches how to read and interpret these maps, which use internationally recognized symbols to depict weather conditions and isolines (lines connecting points of equal value), such as isobars (for pressure) and isotherms (for temperature), to visualize weather patterns.