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Environmental Science

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Holt Earth Science Chapter 17, Section 17.4

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Heating the Atmosphere A. What Happens to Incoming Solar Radiation? When radiation strikes an object, 3 things happen: some of the energy is absorbed by the object (converted to heat+temperature rises), some substances (water+air) are transparent to certain radiation wavelengths + transmit energy, and some radiation is bounced off the object without absorption/transmission. Reflection + scattering are responsible for redirected solar radiation. Out of the total solar radiation from the sun, 50% is absorbed by the land/sea, 20% is absorbed by the atmosphere/clouds, 5% is reflected from the land/sea surface, 5% is backscattered to space by the atmosphere, 20% is reflected by the clouds (in total, 30% is lost to space by reflection/scattering). B. Reflection and Scattering

Holt Earth Science Chapter 17, Section 17.3

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Earth-Sun Relationships The Sun is the source from almost all of the Earth?s weather and climate. Earth intercepts 12000000000 (one two-billionth) of all the energy given off by the sun (this is several hundred thousand times the energy generation of the US). Solar energy isn?t evenly distributed; the amount of energy varies with latitude, time of day, and season. Unequal heating of Earth creates winds and ocean currents, which transport heat to balance energy inequalities; the consequences of these processes are called weather. If the Sun died, global winds and currents would stop; but if the Sun shines, the winds will blow and weather will exist. Variations in solar heating are caused by the motions of the Earth relative to the Sun and variations in the Earth?s land-sea surface.

Holt Earth Science Chapter 17, Section 17.2

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Composition of the Atmosphere Air is a mixture of many discrete gases with their own physical properties in which different quantities of tiny solid/liquid particles are suspended. A. Major Components Composition of air varies depending on the time and place. If H20 Vapor, dust, and other variables were removed from the atmosphere, the makeup is very stable worldwide for an altitude of ~ 80 km. Ni and O2 make up 99% of clean, dry air. They are the most plentiful components, and important to life, but do not affect weather much. The remaining 1% is mostly Argon (0.93%) and other tiny quantities of many other gases. B. Carbon Dioxide (CO2)

Holt Earth Science Chapter 17, Section 17.1

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Vertical Structure of the Atmosphere A. Pressure Changes Atmospheric Pressure: weight of the air above - at sea level, the avg. pressure ~ 1000 millibars (mb), or ~ 1 kg/cm2 Pressure at higher altitudes is less ? of the atmosphere is below 5.6 km (3.5 mi); at 16 km (10 mi), 90% of the atmosphere has been passed, and > 100 km (62 mi), only 0.00003 % of all gases in the atmosphere remain. Rest of atmosphere merges with space vacuum. B. Temperature Changes Near Earth?s surface, air temperature drops with an increase of height. I. Troposphere (air ?turns over?) Lowermost atmosphere layer (we live in here); temperature decreases with an altitude increase. All important weather occurs here.

Holt Earth Science Chapter 12, Section 12.3

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Dating With Radioactivity It is possible to measure numerical values for the age of Earth?s geologic activities - in billions and millions of years - by using radiometric dating. A. Reviewing Basic Atomic Structure An atom has a nucleus with protons (positive) and neutrons (proton+electron combined = neutral) orbited by electrons (negative charge). Atomic Number = number of protons in the nucleus; each element?s Atomic Number differs. Atoms of the same element have the same number of protons. 99.9% of an atom?s mass is in the nucleus - electrons have hardly any mass. By adding together the number of protons and neutrons, the atomic mass of an atom is obtained. The number of neutrons varies (called isotopes; have different atomic masses).

Holt Earth Science Chapter 12, Section 12.1

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Creating a Time Scale: Relative Dating Principles A. Importance of a Time Scale Rocks record geological events + changing life forms of the past; however, many pages (especially earlier ones) are missing or incomplete. Geologiests can unravel complexity of the past Earth by studying rocks Geologic events have little meaning until put into perspective. Geologic time scale = major contribution of geology (Earth?s age = huge) B. Numerical and Relative Dates Geologists have learned that Earth is much older than people thought, and it has been changed over and over again by the same geologic principles I. Numerical Dates

Holt Earth Science Chapter 9, Section 9.5

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What Drives Plate Motions? Convection (hot rocks rise and cold rocks sink) is the ultimate driver of plate tectonics A. Forces that Drive Plate Motion The mantle consists of almost entirely solid rock, but is hot and weak enough to act like a viscous, fluid-like convective flow. The simplest type of convection is like heating a pot of water. The base, which has been heated up, becomes less dense and rises in thin sheets/blobs that spread out to the surface. As the surface cools, it densifies and the cooler water sinks back to the bottom, where it reheats, etc. This is like mantle convection. Slab pull happens when cold, dense oceanic lithosphere sinks through the less dense underlying warm asthenosphere (sink down like a rock pulled into mantle by gravity).

Holt Earth Science Chapter 9, Section 9.4

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Transform Plate Boundaries In a transform plate boundary (transform fault), plates slide horizontally past one another without producing or destroying lithosphere. They commonly connect 2 spreading centers (divergent), or less commonly 2 trenches (convergent). Mostly found on ocean floor (offset segments of oceanic ridge system, producing a steplike plate margin). Zigzag shape of Mid-Atlantic Ridge reflects shape of original shape of rifting Transform faults are part of linear breaks in seafloor (fracture zones) that include active and inactive (extensions) of the transform faults.

Holt Earth Science Chapter 9, Section 9.3

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A. Oceanic-Continental Convergence When a plate capped with continental crust converges with a slab of oceanic lithosphere, the buoyant continental block remains ?floating?; denser oceanic crust sinks into the mantle. When oceanic slab goes down about 100km, melting is triggered in the asthenosphere above it. This is because the ?wet? oceanic rock in a high-pressure place melts at a much lower temperature than ?dry? rock of the same material does. Sediments and oceanic crusts have lots of H2O, which is carried down much depth by a subducting plate. As the plate moves down, heat + pressure drive water from voids in the rock. At a depth of 100km, the wedge of rock is hot enough so that H2O from slab, when exposed, causes some melting.

Excel-steaks

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Tony had a job over spring break selling steaks door to door. For every steak he sold he earned $2.15. In our classwork file called excel please create a new spreadsheet that has the following information: Monday ? sold 25 steaks Tuesday ? sold 12 steaks Wednesday ? sold 30 steaks Thursday ? sold 16 steaks Friday ? sold 32 steaks Using an absolute cell reference please find out how much money Tony made everyday. Also give a grand total of his earnings for the week.
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