Dibrugarh University B.Sc. Geology Major 2025 Question Paper (PYQ) with Answers 1st Semester
View the Dibrugarh University B.Sc. Geology Major Previous Year (2025) question paper for Semester 1 with answers and explanations to help with exam preparation and revision.
Time: 2 hours
Total Marks:45
Unit 1 (Universe And Solar System)
Question 1. Fill in the blanks:
(a) The heliocentric model was proposed by _________.
Ans: The heliocentric model was proposed by Nicolaus Copernicus.
(b) ________ is regarded as the father of modern astronomy.
Ans: Galileo Galilei (or Nicolaus Copernicus) is regarded as the father of modern astronomy.
(c) The largest meteorite ever found on the earth is the _________.
Ans: The largest meteorite ever found on the earth is the Hoba meteorite.
(d) The earth formed over 4.6 billion years ago out of a mixture of ________ and ________.
Ans: The earth formed over 4.6 billion years ago out of a mixture of dust and gas.
(e) The Himalayan Mountain range began forming during the ________ Era.
Ans: The Himalayan Mountain range began forming during the Cenozoic Era.
Question 2. Describe about the nebular hypothesis and its drawbacks.
Ans: The Nebular Hypothesis
The Nebular Hypothesis, initially proposed by Immanuel Kant (1755) and mathematically formulated by Pierre-Simon Laplace (1796), is a widely accepted model explaining the formation of the solar system.
Process:
The solar system began as a giant, rotating cloud of interstellar gas and dust called the solar nebula.
Due to a disruptive event (like a nearby supernova) or gravitational instability, the nebula began to collapse under its own gravity.
As it collapsed, the conservation of angular momentum caused the nebula to spin faster, flattening it into a protoplanetary disk.
The majority of the mass concentrated in the center, heating up to form the proto-Sun.
In the cooler outer regions of the disk, matter collided and accreted to form planetesimals, which eventually aggregated into the planets.
Drawbacks of the Classical Nebular Hypothesis
Despite its strengths, the original Kant-Laplace hypothesis faced significant criticisms, leading to modern modifications:
Angular Momentum Distribution: The most critical drawback is the distribution of angular momentum. The Sun contains about 99.8% of the solar system's mass but possesses only about 2% of its angular momentum. The planets, comprising merely 0.2% of the mass, hold 98% of the angular momentum. The classical hypothesis could not explain how the central proto-Sun transferred its angular momentum to the outer planets.
Formation of Rings vs. Planets: Laplace suggested that the shrinking nebula left behind discrete rings of matter that condensed into planets. However, physicists like James Clerk Maxwell demonstrated that a ring of gaseous material would not condense into a single planet due to gravitational dispersion forces; instead, it would remain as a ring of small particles.
Note: Modern variations of this theory involve magnetic braking and solar wind to explain the angular momentum transfer.
Question 3. Write short notes on any two of the following:
Note: Solutions for all three options are provided below for comprehensive study.
(a) Iron meteorite
Ans: Iron meteorites are a major class of meteorites composed overwhelmingly of an iron-nickel alloy, primarily the minerals kamacite and taenite.
Origin: They are believed to be the fragmented cores of larger, ancient asteroids that underwent planetary differentiation (melting and separation into a metallic core and a rocky mantle) before being destroyed by collisions.
Characteristics: They have an extremely high density. When cut, polished, and etched with weak acid, most iron meteorites display a distinct, intersecting crystalline structure known as the Widmanstätten pattern, which indicates an extremely slow cooling rate over millions of years within the parent body's core.
Significance: They provide direct analogues for the composition of Earth's own metallic core. The Hoba meteorite in Namibia is the largest known example on Earth.
(b) Geological timescale
Ans: The Geological Timescale (GTS) is a system of chronological dating that classifies geological strata (stratigraphy) in time. It is used by geologists, paleontologists, and other Earth scientists to describe the timing and relationships of events that have occurred during Earth's history.
Hierarchy: The GTS is broken down into a hierarchical sequence of time units. In descending order of duration, these are: Eons, Eras, Periods, Epochs, and Ages.
Basis: The divisions are primarily based on major geological and evolutionary events recorded in the rock and fossil records, such as mass extinctions (e.g., the Permian-Triassic extinction boundary) or the sudden appearance of new life forms.
Modern Calibration: While historically based on relative dating principles (Steno's Laws, Faunal Succession), the modern GTS is continuously refined with absolute ages using radiometric dating (chronostratigraphy) coordinated by the International Commission on Stratigraphy (ICS).
(c) Types of asteroid
Ans: Asteroids are small, rocky remnants left over from the early formation of our solar system. They are classified into three primary types based on their spectral characteristics, which reflect their surface composition (albedo) and corresponding mineralogy:
C-type (Carbonaceous): These are the most abundant type, making up over 75% of known asteroids. They are very dark (low albedo) and composed of clay and silicate rocks, containing a high percentage of carbon. They are some of the oldest objects in the solar system.
S-type (Silicate/Stony): Accounting for about 17% of asteroids, these are relatively bright. They are composed mostly of silicate materials and nickel-iron, lacking significant carbon content. They dominate the inner asteroid belt.
M-type (Metallic): These are moderately bright and are primarily composed of metallic iron and nickel. They are believed to be the exposed cores of early, differentiated planetesimals that were shattered by impacts.
Unit - 2 : Earth System
Question 4. Answer all the questions:
(a) What is the shape of the earth?
Ans: The shape of the Earth is an oblate spheroid (or oblate ellipsoid), meaning it is mostly spherical but slightly flattened at the poles and bulging at the equator due to its rotation.
(b) What is the mass of the earth?
Ans: The mass of the Earth is approximately 5.97 × 1024 kg.
(c) Which is the largest terrestrial planet of our solar system?
Ans: Earth is the largest terrestrial planet in our solar system.
(d) Give two examples of Jovian planets.
Ans: Two examples of Jovian planets are Jupiter and Saturn (Uranus and Neptune are also correct).
(e) Define magnetosphere.
Ans: The magnetosphere is the region of space surrounding an astronomical object, such as Earth, in which charged particles (like those from the solar wind) are controlled and deflected by that object's magnetic field.
Question 5. Write short notes on any two of the following:
Note: Solutions for all three options are provided below for comprehensive study.
(a) Lithosphere
Ans: The lithosphere is the rigid, outermost rocky shell of the Earth.
Composition and Depth: It consists of the crust and the uppermost part of the solid mantle. It extends from the Earth's surface to a depth of approximately 100 km, though it can be thicker under old cratons and thinner at mid-ocean ridges.
Tectonic Significance: Based on its mechanical properties, the lithosphere behaves as a brittle, rigid solid over geological timescales. It is fragmented into tectonic plates (both oceanic and continental lithosphere) that glide over the hotter, more ductile asthenosphere below.
Dynamics: The creation, destruction, and movement of the lithosphere govern the principles of plate tectonics, driving earthquakes, volcanism, and mountain building.
(b) Gravitational field of the earth
Ans: The Earth's gravitational field is the field of attractive force surrounding the Earth, pulling objects toward its center of mass.
Mechanism: Governed by Newton's law of universal gravitation, the acceleration due to gravity on the Earth's surface averages about 9.8 m/s2.
Variations: The field is not perfectly uniform. It varies across the Earth's surface due to two main factors:
Centrifugal Force: Earth's rotation causes a slight outward centrifugal force that counters gravity, making the gravitational pull slightly weaker at the equator than at the poles.
Mass Distribution: Uneven distribution of mass in the crust and mantle (e.g., mountains, dense ore bodies, ocean trenches) creates localized gravity anomalies.
Measurement: These anomalies are measured using gravimeters and are mapped as the geoid, which is the shape the ocean surface would take under the influence of gravity and rotation alone.
(c) Cryosphere
Ans: The cryosphere encompasses all the regions of the Earth's surface where water is in a solid form.
Components: This includes continental ice sheets (Greenland and Antarctica), mountain glaciers, ice caps, sea ice, lake and river ice, snow cover, and permafrost (frozen ground).
Role in Earth System: The cryosphere is a crucial component of the global climate system. It heavily influences the Earth's surface albedo (reflectivity); ice and snow reflect a significant amount of solar radiation back into space, helping to cool the planet.
Significance: It serves as the largest reservoir of freshwater on Earth. Fluctuations in the volume of the cryosphere directly control global eustatic sea levels and ocean circulation patterns.
Question 6. Define discontinuity. Describe the internal structure of the earth with suitable diagram. (1+3=4)
Ans:
Definition of Discontinuity: In seismology and geology, a discontinuity is a boundary or interface within the Earth's interior where there is a sudden and distinct change in the velocity of seismic waves (P-waves and S-waves). These abrupt shifts indicate a fundamental change in the chemical composition, density, or physical state (solid/liquid) of the earth's internal materials.
Internal Structure of the Earth: Based on chemical composition and seismic evidence, the Earth is divided into three primary concentric layers:
The Crust: The outermost, thinnest solid skin of the Earth. It is divided into:
Continental Crust: Thicker (average 30–50 km), less dense, and composed largely of granitic (felsic) rocks rich in silica and aluminum (Sial).
Oceanic Crust: Thinner (average 5–10 km), denser, and composed of basaltic (mafic) rocks rich in silica and magnesium (Sima).
The Mantle: The thickest layer, extending from the base of the crust to a depth of 2,900 km. It is composed of solid, dense, ultramafic rock (peridotite).
Upper Mantle: Includes the rigid lithospheric mantle and the underlying ductile asthenosphere, which allows for plate tectonic movement.
Lower Mantle (Mesosphere): Solid due to extreme pressure, despite high temperatures.
The Core: The innermost layer, composed primarily of an iron-nickel alloy (Nife). It is divided into two distinct parts based on physical state:
Outer Core (2900–5150 km): Liquid state. The convection of this liquid metallic layer generates the Earth's magnetic field.
Inner Core (5150–6371 km): Solid state due to immense pressure, despite possessing the highest temperatures in the Earth's interior.
Major Discontinuities separating these layers:
Mohorovičić Discontinuity (Moho): Separates the crust from the underlying mantle.
Gutenberg Discontinuity: Separates the lower mantle from the liquid outer core at 2,900 km depth. P-wave velocities drop sharply, and S-waves disappear entirely.
Lehmann Discontinuity: Separates the liquid outer core from the solid inner core at approximately 5,150 km.
Diagram Required: Internal Structure of the Earth.
Description: The student should draw a pie-slice or a cross-section of the Earth from the surface to the center.
Labels required:
Layers: Crust (Continental and Oceanic), Lithosphere, Asthenosphere, Lower Mantle, Outer Core, Inner Core.
Depths: 0 km (surface), ~35 km (Moho), 2900 km (Gutenberg Discontinuity), 5150 km (Lehmann Discontinuity), 6371 km (Center).
State: Label Outer core as "Liquid" and Inner core as "Solid".
Unit - 3 : Introduction to Geology
Question 7. Fill in the blanks:
(a) The process in which rocks and minerals on the earth's surface are broken down into smaller pieces is called ________.
Ans: The process in which rocks and minerals on the earth's surface are broken down into smaller pieces is called weathering.
(b) ________ refers to the rate at which the temperature increases with depth in the earth's crust.
Ans: Geothermal gradient refers to the rate at which the temperature increases with depth in the earth's crust.
(c) S-waves travel only through ________.
Ans: S-waves travel only through solids.
(d) The theory of uniformitarianism was primarily proposed by ________.
Ans: The theory of uniformitarianism was primarily proposed by James Hutton (and later popularized by Charles Lyell).
(e) The earth's inner core is primarily composed of ________ and ________.
Ans: The earth's inner core is primarily composed of iron and nickel.
Question 8. Write short notes on any three of the following:
Note: Solutions for all five options are provided below for comprehensive study.
(a) Coriolis effect
Ans: The Coriolis effect is an apparent inertial force resulting from the Earth's rotation, causing moving objects or fluids to deflect from a straight path.
Mechanism: Because the Earth rotates eastward, and rotational velocity is higher at the equator than at the poles, moving masses of air or water are deflected.
Direction of Deflection: Objects are deflected to the right in the Northern Hemisphere and to the left in the Southern Hemisphere.
Significance in Earth Sciences: It is a fundamental control on global atmospheric circulation (creating the trade winds and westerlies) and drives the major surface currents (gyres) in the world's oceans. It is also responsible for the rotation of cyclonic weather systems.
(b) Soil profile
Ans: A soil profile is a vertical cross-section of the soil that exposes its various horizons, extending from the ground surface down to the unweathered parent bedrock.
Horizons: A mature soil profile consists of distinct layers, typically labelled from top to bottom:
O Horizon: Surface litter and organic matter.
A Horizon (Topsoil): Rich in humus and minerals; a zone of intense biological activity.
E Horizon: Zone of eluviation (leaching) where minerals and clays are washed downward.
B Horizon (Subsoil): Zone of illuviation where leached minerals (like iron, clay, and calcium carbonate) accumulate.
C Horizon: Partially weathered parent rock material.
R Horizon: Unweathered bedrock.
Fig: Soil Profile
Significance: The profile reflects the geologic, climatic, and biological processes of weathering over time and dictates the soil's fertility and drainage capacity.
(c) Land-air-sea interactions
Ans: Land-air-sea interactions refer to the complex and dynamic exchanges of energy (heat), matter (water, gases, aerosols), and momentum among the lithosphere, atmosphere, and hydrosphere.
Processes: These interactions are driven primarily by solar radiation. Examples include the evaporation of seawater adding moisture to the air, which precipitates over land, weathers rocks, and returns to the sea via rivers (the hydrological cycle).
Thermal Dynamics: Land surfaces heat up and cool down much faster than oceans due to differing specific heat capacities. This differential heating drives regional atmospheric circulation.
Geological/Climatic Significance: These interactions generate massive climatic phenomena like the Asian Monsoon, the El Niño-Southern Oscillation (ENSO), and coastal breezes, profoundly influencing global climate regulation and geomorphic erosion rates.
(d) Lateral continuity
Ans: The Principle of Lateral Continuity is one of the foundational laws of stratigraphy, originally formulated by Nicolas Steno in 1669.
Definition: It states that layers of sedimentary rock are initially deposited as continuous, laterally extensive sheets in all directions within a basin.
Application: If a sequence of identical sedimentary beds is now found separated by an erosional feature, such as a river valley or a canyon, a geologist can safely assume that the layers were once continuous.
Geological Significance: This principle is crucial for stratigraphic correlation, allowing geologists to map and connect isolated rock outcrops across broad regions to reconstruct ancient sedimentary environments.
(e) Post-glacial landforms
Ans: Post-glacial landforms are topographical features created by the depositional work of glaciers or by the actions of glacial meltwater (glaciofluvial processes) as a glacier retreats after a period of glaciation.
Depositional Landforms (Till): These consist of unsorted glacial sediments dropped directly by melting ice. The most prominent examples are moraines (terminal, lateral, and ground moraines) which form ridges of debris, and drumlins, which are streamlined, asymmetrical hills of till.
Glaciofluvial Landforms (Meltwater): Formed by flowing meltwater, these feature sorted sediments. Examples include eskers (sinuous ridges of sand and gravel deposited by subglacial streams), kames (irregular mounds of sediment), and outwash plains.
Depressional Features: Blocks of dead ice buried in outwash can melt to form depressions called kettle lakes.
Question 9. Define mobile belt. Describe the geomorphic divisions of Indian subcontinent. (1+5=6)
Ans:
Mobile Belt: A mobile belt is a long, relatively narrow, and structurally unstable region of the Earth's crust that is currently experiencing, or has recently experienced, significant tectonic activity. This activity includes severe deformation, folding, faulting, metamorphism, and igneous intrusion (magmatism). These regions are synonymous with orogenic (mountain-building) belts and typically form at convergent plate boundaries.
Geomorphic Divisions of the Indian Subcontinent: The Indian subcontinent displays vast diversity in its geology and topography. It is broadly divided into four major geomorphic/physiographic divisions based on tectonic history, stratigraphy, and relief:
1. The Peninsular Shield (The Peninsular Plateau)
Characteristics: This is the oldest and most stable landmass of the subcontinent, forming part of the ancient Gondwanaland. It has been virtually untouched by significant crustal deformation since the Precambrian, except for block faulting.
Features: It consists of ancient igneous and metamorphic rocks (cratons). The topography is highly dissected and dominated by relict mountains, broad and shallow valleys, and rounded hills.
Key Sub-divisions: The Central Highlands, the Deccan Plateau, the Western Ghats, and the Eastern Ghats. It also hosts the Deccan Traps (massive flood basalts).
2. The Extra-Peninsular Region (The Northern Mountains / Himalayas)
Characteristics: This represents a young, tectonically active mobile belt formed by the Cenozoic collision between the Indian Plate and the Eurasian Plate.
Features: It contains the highest mountain peaks in the world, deep gorges, and active thrust faults. The rocks here are highly compressed, folded, and faulted marine sediments of the Tethys Sea.
Key Sub-divisions: It includes the Greater Himalayas (Himadri), the Lesser Himalayas (Himachal), and the Sub-Himalayas (Shiwaliks), extending from the Indus gorge to the Brahmaputra gorge.
3. The Indo-Gangetic-Brahmaputra Plains
Characteristics: This is a vast, flat aggradational plain situated between the Peninsular Shield and the Himalayas. It is a foredeep tectonic depression formed during the Himalayan uplift.
Features: The depression was subsequently filled by thousands of meters of Quaternary alluvium brought down by the Indus, Ganga, and Brahmaputra river systems. It is highly fertile and geologically very young.
4. The Coastal Plains and Islands
Coastal Plains: Narrow strips of land bordering the Peninsular plateau along the Arabian Sea (Western Coastal Plains— narrow and submerged) and the Bay of Bengal (Eastern Coastal Plains— broader, marked by large river deltas).
Islands:
Andaman and Nicobar Islands: Located in the Bay of Bengal, these represent an elevated portion of a submarine volcanic ridge/tectonic arc.
Lakshadweep Islands: Located in the Arabian Sea, these are entirely coral atolls built on submarine ridges.
Additional 15 marks for 2023 Batch
Question 10. Define any three of the following: (1x3=3)
Note: Solutions for all four options are provided below for comprehensive study.
(a) Comet
Ans: A comet is a relatively small, icy planetary body orbiting the Sun. When it approaches the inner solar system, solar radiation and solar wind cause its volatile ice content to sublimate (outgas), producing a visible, glowing atmosphere (coma) and often two distinct tails (an ion tail and a dust tail) that always point away from the Sun.
(b) Heliopause
Ans: The heliopause is the theoretical boundary in space where the Sun's solar wind is completely stopped by the pressure of the interstellar medium (the background gas and dust of the Milky Way galaxy). It marks the outermost edge of the heliosphere, effectively defining the magnetic boundary of the solar system.
(c) Unconformity
Ans: An unconformity is a buried erosional or non-depositional surface separating two rock masses or strata of different ages, indicating that sediment deposition was not continuous. It represents a significant hiatus, or missing gap in the geological rock record, resulting from a period of tectonic uplift and erosion before subsidence and renewed deposition occurred.
(d) Eustasy
Ans: Eustasy (or eustatic sea-level change) refers to global, uniform changes in sea level that are independent of local land movements (isostasy). These changes are primarily caused by variations in the absolute volume of water in the global oceans (such as from the melting or growth of continental ice sheets during glacial cycles) or changes in the volumetric capacity of ocean basins (due to seafloor spreading rates).
Question 11. Write short notes on any three of the following: (4x3=12)
Note: Solutions for all five options are provided below for comprehensive study.
(a) Big Bang Theory
Ans: The Big Bang Theory is the leading cosmological model explaining the origin and evolution of the observable universe.
Concept: The theory postulates that approximately 13.8 billion years ago, all matter, energy, space, and time in the universe were concentrated into a single point of infinite density and temperature known as a singularity.
Process: This singularity underwent a rapid, massive expansion (inflation), not an explosion in space, but an expansion of space itself. As the universe expanded, it cooled, allowing subatomic particles to form, followed by simple atoms (hydrogen and helium). Over billions of years, gravity pulled these gases together to form the first stars and galaxies.
Evidence: The theory is supported by three major observational pillars:
Hubble's Law: The observation that galaxies are moving away from Earth at speeds proportional to their distance (redshift), proving the universe is expanding.
Cosmic Microwave Background (CMB): The detection of pervasive, uniform relic radiation left over from the initial hot state of the universe.
Primordial Abundance of Elements: The predicted ratio of light elements (Hydrogen, Helium, Lithium) matches observable reality.
(b) Hydrosphere and Biosphere
Ans: The Hydrosphere and Biosphere are two of the Earth's four fundamental, interacting subsystems.
Hydrosphere: This represents the discontinuous layer of water at or near Earth's surface. It encompasses all liquid and frozen surface waters (oceans, rivers, lakes, glaciers, sea ice), groundwater in soil and rock voids, and atmospheric water vapor. The oceans account for over 97% of the hydrosphere. It is highly dynamic, constantly circulating through the hydrological cycle driven by solar energy.
Biosphere: This is the global sum of all ecosystems. It is the zone of life on Earth, extending from deep ocean trenches to the lower atmosphere. It integrates all living organisms (plants, animals, microbes) and their interactions with the physical environment.
Interactions: The biosphere cannot exist without the hydrosphere, as water is the universal solvent essential for biological functions. Conversely, the biosphere drastically alters the hydrosphere by regulating water chemistry, transpiration rates, and the global carbon cycle.
(c) Continental Drift
Ans: Continental Drift is the pioneering geological hypothesis proposed primarily by the German meteorologist Alfred Wegener in 1912.
Hypothesis: Wegener proposed that the Earth's continents are not fixed in place but move across the Earth's surface over geologic time. He suggested that all landmasses were once joined together in a single supercontinent called Pangea (surrounded by a superocean, Panthalassa) during the late Paleozoic and early Mesozoic eras before breaking apart and drifting to their current positions.
Evidence Used by Wegener:
Geometrical Fit: The jigsaw-puzzle fit of the opposing coastlines of the Atlantic Ocean (South America and Africa).
Paleontological Evidence: Identical terrestrial fossil species (e.g., the reptile Mesosaurus and the fern Glossopteris) found on widely separated continents.
Geological Matching: Continuous mountain belts and identical rock sequences terminating at the coast of one continent and reappearing on another.
Paleoclimatic Evidence: Evidence of ancient glaciations (tillites) found in regions that are currently tropical (India, Africa).
Legacy: The theory was initially rejected because Wegener could not provide a viable physical mechanism for the movement. However, it laid the foundational groundwork for the modern, comprehensive theory of Plate Tectonics developed in the 1960s.
(d) Earth's heat budget
Ans: The Earth's heat budget (or energy balance) refers to the perfect balance between the incoming shortwave solar radiation from the Sun and the outgoing longwave terrestrial radiation lost to space. This equilibrium maintains the Earth's relatively stable global average temperature.
Incoming Energy: Assuming 100 units of solar radiation reach the top of the atmosphere:
Roughly 30 units are immediately reflected back to space by clouds, atmospheric dust, and the Earth's surface (ice, snow). This reflectivity is known as the Earth's albedo.
About 19 units are absorbed by the atmosphere (water vapor, ozone, clouds).
The remaining 51 units reach and are absorbed by the Earth's surface (land and oceans), heating it.
Outgoing Energy: To maintain thermal equilibrium, the Earth's surface radiates those absorbed 51 units back as longwave infrared radiation. Much of this is temporarily absorbed by greenhouse gases in the atmosphere, creating the natural greenhouse effect, before eventually escaping into space along with the energy absorbed by the atmosphere. Over a long period, incoming energy precisely equals outgoing energy.
(e) Types of volcano
Ans: Volcanoes are classified into several distinct types based on their eruptive style, the viscosity of their magma, and their resulting structural morphology. The three primary types are:
1. Shield Volcanoes:
Characteristics: These are the largest volcanoes on Earth by volume. They have very broad, gently sloping profiles resembling a warrior's shield.
Formation: Formed by highly fluid, low-viscosity basaltic lava that flows over great distances before cooling. Eruptions are typically non-explosive and effusive.
Examples: Mauna Loa and Kilauea in Hawaii.
2. Stratovolcanoes (Composite Volcanoes):
Characteristics: Classic, tall, symmetrical cone-shaped mountains with steep flanks.
Formation: Built from alternating layers (strata) of viscous, intermediate-to-felsic lava flows (andesite, rhyolite), volcanic ash, and pyroclastic debris. Their high-viscosity magma traps gases, leading to highly explosive and dangerous eruptions.
Examples: Mount Fuji (Japan), Mount Vesuvius (Italy), Mount St. Helens (USA).
3. Cinder Cones (Pyroclastic Cones):
Characteristics: The smallest and most common type. They are steep-sided, highly symmetrical cones often featuring a distinct crater at the summit.
Formation: Built entirely from loose, airborne volcanic fragments (cinders/scoria) that are ejected from a single vent and fall back down around it. They are typically formed during single, short-lived eruptive episodes.
Examples: Parícutin (Mexico).