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EARTH AND LIFE SCIENCE REVIEWER © angelica garcia EARTH SCIENCE all the sciences that collectively seek to understand Earth and its neighbors in space I. ASTRONOMY - the study of the universe - very useful in probing the origins of our own environment II. METEOROLOGY - study of the atmosphere and the processes that produce weather and climate III. GEOLOGY - Study of the earth - Study of solid earth, the rocks of which it is composed and the processes by which they change. A. Physical Examines the materials composing earth and the processes that operate beneath and upon its surface. B. Historical Aim to understand the origin of Earth and development of the planet through its 4.5- billion-year histor
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© angelica garcia
EARTH SCIENCE
all the sciences that collectively seek to understand Earth and its neighbors in space
I. ASTRONOMY
THE UNIVERSE
Theories on the Creation of the Universe
1. BIBLICAL CREATION - came from the bible - States that the entire cosmos was created in 6 days by a Supreme Being. 2. BIG BANG THEORY (1920) - Alexander Friedman and George Lamaitre - Universe started with a huge explosion 13.7 Billion years ago. - Explains what happened at the very beginning - “The Universe started with a cataclysm that created space and time and all the matter and energy that has ever existed in the universe” - Caused by random fluctuation in an empty void. Then there was a great explosion and expansion. Evidences:
Hubble’s Law
5. Solar-Nebular Theory - Describes the formation of our solar system from condensation of interstellar gas and dust cloud. Due to gravity , it began to condense the solar nebula, with the center becoming a protostar. As the cloud continued to shrink, rotational speed increased and became a rapidly rotating disk. The contraction converted gravitational energy into heat energy and caused the center to glow. When the temperature is sufficient enough, a nuclear reaction began at the core of the protostar and became the SUN. - The remaining gas and dust cloud form diskshaped bodies (due to rotation) called SOLAR NEBULAE. Formation of the planets involved: a. Accretion of grain-sized particles to form cm-sized particles which later grew to several km in distance b. Formation of more massive objects from coalescing planetisimals PROTOPLANETS PLANETS 6. Condensation Theory - The solar system formed a large spinning cloud of gas and dust, called the solar nebula. - Once gravity pulled it to a diameter of less than 100au, the solar nebula had become a wide rotating disc 7. Fission Theory - One day, our sun burst open , and planets, and moons shot out at high speeds and went to their respective places, then stopped, and started orbiting the sun, as the moons began orbiting the planets. 8. Capture Theory - Planets and moons were flying around, and some were captured by our sun and began circling. 9. Accretion Theory - A pile of space dust and rock chunks pushed together into our planet , and another pile pushed itself into our moon. Then the moon got close enough and began circling the earth. 10. Planetary Collision Theory - Our world collided with a small planet, and the explosion threw off rocks which became the moon and then it began orbiting us. 11. Stellar Collision Theory - Our planets, moons, and stars **spun off from the collision between stars
Our Solar System
1. The sun 2. Four terrestrial inner planets. (MVEM) - Mercury - Venus - Earth - Mars
3. Four gas giant outer planets. (JSUN) - Jupiter - Saturn - Uranus - Pluto 4. An asteroid belt composed of small rocky bodies and comets.
What is a Solar System?
The sun, its planets, and all the objects moving around them collectively Entirely dependent on the Sun and the only one which is self-luminous Rest of the planets reflect the light received from the sun
Sun
Star of the Solar System Scientific name is “Sol” Heaviest among the Solar System Ball of hot, burning gases
Nearest star to the Earth Light from the Sun takes approximately 8 minutes to reach the Earth.
Classification of Planets by Composition
1. Terrestrial Planets (Earth-like planets or Inner Planets) - Composed mostly of dense, rocky, and metallic materials - Mercury, Venus, Earth, Mars - Formed within the frost line where rocks and metals condense, and hydrogen compounds remain as gas. 2. Jovian Planets (Jupiter-like planets or Outer Planets) - Composed mostly of Hydrogen and Helium - Jupiter, Saturn, Uranus, Neptune - These planets are formed outside the frost line where light elements condense into ice.
Classification of Planets by Position Relative to the Sun
1. Inner Planets - Mercury, Venus, Earth, Mars 2. Outer Planets - Jupiter, Saturn, Uranus, Neptune
Classification of Planets by Position Relative to the Earth
1. Inferior Planets - Mercury, Venus 2. Superior Planets - Mars, Jupiter, Saturn, Uranus, Neptune
What is a Dwarf Planet?
Celestial body that has the following characteristics: a. Is in orbit around the sun b. Has sufficient mass for its self-gravity to overcome rigid body forces c. Has not cleared the neighborhood around it d. Is not a satellite Haumea, Pluto, Makemake, Eris
Properties of the Solar System
The orbits of all planets are almost in the same plane.
Asteroids
A celestial body bigger than 10m orbiting the Sun, mainly between Mars and Jupiter.
Comets
A smaller celestial body mainly composed of ice and dust. If a comet approaches the Sun it can generate a tail of gas and/or dust.
Meteoroids
Similar to an Asteroid, but significantly smaller. Mostly debris of comets, sometimes debris of asteroids.
Meteors
A bright tail of light caused by a meteoroid during its atmospheric flight, also called a shooting star or falling star. Types of meteors: a. Fireball
Meteorites
The part of a meteoroid or asteroid that survives the passage through our atmosphere and reaches the Earth’s surface.
Divides up the history of the earth based on lifeforms that have existed during specific time since the creation of the planet. Model of the history of the Earth showing the major events that occurred along the way 88% of Earth’s History (Precambrian – very little evidence of life); Other 12% (Phanerozoic – sudden development of life in the oceans, hard parts developed which increased the fossil record)
1. Eons - Longest units of time - Precambrian: Earliest Span of time - Phanerozoic: Everything since
The brightness of a star is referred to as magnitude. There are two kinds of magnitude:
a. The brightness of the star observed from the Earth is referred to as the Apparent Magnitude. b. If the star is at 10 parsecs (32.6 light years) distance from the Earth, then it would be referred to as Absolute Magnitude.
Asteroids Comets Meteoroids Meteors Meteorites
James Hutton (1726 – 1797)
Theory of Uniformitarianism
Neocatastrophism
Geologic Dating
1. Absolute - Determines how many years old something is - Know DATES - Uses Radiometric Radioactive Decay ( half-life ): occurs when the nuclei of unstable atoms break down, changing the original atoms into atoms of another element. Half-life is the amount of time it takes for half the atoms of a substance to decay into another element. Different substances have different half-life’s Ex: Uranium 238 and Carbon 14 ( Carbon 14 – date biological remains since Carbon is incorporated into the cells of living organisms and begins to decay when the organism dies; Uranium 238 – used to date rocks [larger half-life]) Half-lives of radioisotopes vary depending upon the isotope 2. Relative - Used to determine if one thing is younger or older than another - Know ORDER OF EVENTS BUT NOT DATES - Superposition, Index Fossils, Correlation of Rock layers - Comparing of rock units to decipher their age relative to one another a. Principle of Horizontal Originality b. Principle of Superposition c. Principle of Crosscutting Relationships – any feature (fault or intrusion) that cuts across rocks is younger than the youngest rock that is cut. d. Principle of Inclusion – states that objects enclosed in rock must be older than the time of rock formation.
Fossils
Remains of Ancient Plants and Animals, Evidence of Life Commonly Preserved (Hard Parts) a. Bones b. Shells c. Hard Parts of Insects d. Woody Material Rarely Preserved (Easily Decayed Parts) a. Internal Organs b. Skin c. Hair d. Feathers
Types of Fossils
1. Mold - When sediments bury an organism and the sediment hardens into rocks. - The organisms decay slowly inside the rocks leaving a cavity in the shape of the organism. 2. Cast - The cavity or mold can be filled with mud. - When the mud hardens, it takes on the shape of the organism. 3. Petrified - Permineralized fossil - Forms when minerals soak into buried remains - The materials replace the remains, changing them **to rock
Layers of the Earth:
1. Inner Core - Discovered by Inge Lehmann in 1936 - Radius of 1250 km - Solid Fe-Ni alloy - Magnetic - approximately 6000ºC - 3.6 million atm 2. Outer Core - Discovered by Richard Dixon Oldham (earth’s core as a whole) in 1906. - 2300 km thick - Lehmann discontinuity - Boundary between the inner and outer core. - Liquid Fe and Ni - Magnetic - 4000-5000ºC
Three Types: b.1 Chemical - Formed by precipitation of materials from water b.2 Biological/organic - form from the accumulation of plant and animal debris b.3 Clastic - formed from the debris due to mechanical weathering of rocks
c. Metamorphic Formed through the transformation, either by heat or pressure, of existing rocks. The original rock (protolith) can be igneous, sedimentary, and can also be metamorphic. Two major types: c.1 Foliated – metamorphic rocks that exhibited layering. It occurs during recrystallization c.2 Non- foliated – rocks that has no foliation
Geomorphic Processes
B. Endogenic Process Internal Process Reshaping the Earth’s landforms Transform the Earth from within the crust Two types: a. Volcanism Volcano – An eruption of molten rock, called magma on the surface of the Earth Magma from the mantle rises through the crust and, ultimately, unto the surface. Lava is the primary material expelled from a volcano, in addition to rocks, ash, and dust. b. Tectonic Forces The Lithosphere can be broken up into smaller parts called Tectonic plates. These plates are subjected to stress and, eventually, deformation. (Deformation is any change in the shape and size of a rock as a response to stress.) Folding Deformation: Occurs when the plates are subjected to compressional stress on both sides, causing them to fold. Faulting Deformation: Fracture or displacement of the plates along a fault plane. Three Types:
1. Normal 2. Reverse 3. Transform
Plate Movement
Geologic Hazards
1. Earthquakes – A sudden perceptible shaking of the Earth due to the sudden release of energy in the Earth’s crust or volcanic eruption. The Philippines is largely susceptible to earthquakes due to its location, which is within the pacific ring of fire. (PRoF – Major area in the pacific ocean where 90% of the earthquake occurs.) The Philippines Institute of volcanology and Seismology (PHIVOCS) overlooks the seismic and volcanic activities in the Philippines. 2. Landslides – Also known as landslips; A form of mass wasting in which a great amount of soil, rocks, and or sediments move downslope; Common cause of landslides: Earthquake, Volcano Eruption, Water (raining) 3. Tsunamis – An event caused by earthquakes, volcanic eruption and or other seismic activities that affect bodies of water, thus, also known as seismic sea wave; Generated by a large displacement of water; The Philippines is susceptible to tsunami due to its location.
Other Subsystems:
2. Atmosphere - layer of gases, such as nitrogen and oxygen, that surrounds the planet. - Came from the greek word “atmos” (vapour) and “sphaira" (sphere). - Four layers: a. Troposphere The lowest part of the Atmosphere; The layer that we live in Contains all of the weather Colder as the distance from sea level increase (due to decreased pressure). Contains 75% of all the air in the atmosphere
Boundary layer: lowest part of the troposphere. Tropopause: boundary between troposphere and stratosphere. Poles: 7-10 km Equator: 17-18 km
b. Stratosphere Area between the tropopause to about 50 km above sea level. It contains most of the ozone (O3) in the atmosphere. The temperature increase with height due to the absorption of Ultraviolet (UV) light by the ozone. Stratopause: boundary between stratosphere and mesosphere.