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1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Page 1: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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HNRT 228 AstrobiologyChapter 4 - Earth - Bennett & Shostak

Lecture Notes for Chapter 421 and 23 September 2015Dr. H. Geller

Page 2: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The Habitability of Earth

Geology and Life (4.1)Reconstructing the History of Earth and Life

(4.2) Rocks, radiometric dating, geological record,

fossils, geological time scale, Earth’s age

The Hadean Earth and the Dawn of Life (4.3) Atmosphere, oceans, heavy bombardments

Geology and Habitability (4.4) Earth’s interior, plate tectonics, magnetosphere

Page 3: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The Habitability of Earth

Climate Regulation and Change (4.5) Greenhouse effect, carbon cycle, ice

ages, Snowball Earth, long term habitability

The Process of Science in Action: Formation of the Moon (4.6) Sister model, capture model, spinoff

model

Page 4: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Some Guiding Questions1. What is the greenhouse effect? How does it

affect the average temperature of the Earth?2. Is the Earth completely solid inside? How can

scientists tell?3. How is it possible for entire continents to move

across the face of the Earth?4. How does our planet’s magnetic field protect life

on Earth?5. Why is Earth the only planet with an oxygen-rich

atmosphere?6. Why are prevailing winds generally from the

west over most of North America but generally from the east in Hawaii?

7. What are global warming and the “ozone hole”? Why should they concern us?

Page 5: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Telling Rocks Apart

How geologists tell apart different minerals and rocks color, luster, texture hardness test

scratching one against another• diamond is hardest

acid testusing weak hydrochloric acid to

streak testform a streak across a ceramic tile

Page 6: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Plate tectonics is involved in the formation of the three major categories of rocks Igneous Rock

cooled from molten material

Sedimentary Rock Layered eroded

material formed by the action of wind, water, or ice

Metamorphic Rock

Rock that has been altered in the solid state by extreme heat and pressure

Page 7: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The Rock Cycle

Page 8: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Rocks formed from other rocks that are heated and placed under great pressures are called

A igneous rocksB sedimentary rocksC metamorphic rocksD fault rocksE scarp rocks

Page 9: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Rocks formed from layers of fine material that have been compressed under water are calledA igneous rocksB sedimentary rocksC metamorphic rocksD fault rocksE scarp rocks

Page 10: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Rocks formed when molten material cools and solidifies are called

A igneous rocksB sedimentary rocksC metamorphic rocksD fault rocksE scarp rocks

Page 11: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Which of the following are not used to identify rocks:

A crystalline shapeB acid testC streak testD hardness testE all of the above can be used to

identify a rock

Page 12: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Surface Building Processes

Stress “stress is a force that tends to

compress, pull apart, or deform” different types of stress

compressive stresstensional stressshear stress

Strain “the adjustment to stress”

Page 13: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Stress and Strain

Page 14: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Surface Building Processes

Folds bends in

layered bedrockAnticline /\

Syncline \/

Page 15: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Surface Building Processes

Faulting formation of a crack caused by relative

movement of rock on either side of a fracture

Page 16: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Mountains

“elevated parts of the Earth’s crust that rise abruptly above the surrounding surface”

Causes folding, faulting,

volcanic activity

Page 17: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Volcanoes“hill or mountain formed by the extrusion of lava

or rock fragments from magma below”Different types

shield, cinder cone, composite (composite shown)

Page 18: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Tear-Down Processes

Weathering mechanical weathering chemical weathering

Erosion mass movement (mass wasting) running water (floodplain, delta) glacier wind (deflation and abrasion) impact cratering

Page 19: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Earthquakes

Defined as “quaking, shaking, vibrating, or upheaval of the ground”

Earthquake causes elastic rebound

theory

Intensity measure Richter Magnitude

not linear scale

Page 20: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

What is the term used to specifically define a downward fold of rock material?A scarpB erodaC foldD synclineE anticline

Page 21: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Earth’s Interior andHow We Know It

Page 22: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Earth’s Inside Story

Energy transfer in the mantle similar to that of a pot of boiling water.

Page 23: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Earth’s Interior, Then and Now

Page 24: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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What We Learn from Seismometers

The Earth’s inner and outer cores are composed of iron with some nickel and other metals mixed in

The mantle is composed of iron-rich minerals

Both temperature and pressure steadily increase with depth inside the Earth

Page 25: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Crustal Rumblings

Page 26: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker QuestionWhich of the

diagram represents the MANTLE of the Earth?

ABCDE None of the

above.

Page 27: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Which of the diagrammed sections of the Earth's interior represents the Outer Core?

ABCDE None of the

above.

Page 28: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Which of the diagrammed sections of the Earth represents the CRUST?

ABCDE None of the

above.

Page 29: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Energy transport from one region to another by the movement of material as in the mantle of the Earth is known as

A chaos.B radiance.C conduction.D differentiation.E convection.

Page 30: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

The existence of earthquake shadow zones indicates that there is an abrupt change between the properties of the mantle and those of the core. Specifically, the transverse wave shadow zone shows that the outer core must be

A solid.B liquid or semi-liquid.C gaseous.D similar to crustal material.E impossible to determine.

Page 31: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Plate Tectonics

“The theory that the Earth’s crust is made of rigid plates that float on the asthenosphere.”

Consider the scientific evidence for plate tectonics and what forced scientists to accept the theory as fact

Page 32: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Plate tectonics, or movement of the plates, is driven by convection within the asthenosphere

Molten material wells up at oceanic rifts, producing seafloor spreading, and is returned to the asthenosphere in subduction zones

As one end of a plate is subducted back into the asthenosphere, it helps to pull the rest of the plate along

Page 33: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Plate Tectonics

The Earth’s crust and a small part of its upper mantle form a rigid layer called the lithosphere.

The lithosphere is divided into huge plates that move about over the plastic layer called the asthenosphere in the upper mantle

Page 34: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Fossils across an ocean

Page 35: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The continents appear to fit together like a jigsaw puzzle

Page 36: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Development of Geologic Time

Fossilization“Reading the Rocks”

principle of uniformity principle of original horizontality principle of superposition principle of crosscutting relationships principle of faunal succession radiometric dating

Geologic Time Scale

Page 37: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Geologic Time Scale

Page 38: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Earth’s Atmosphere

Composition Nitrogen (78%), Oxygen (21%), Argon, Water

Vapor, CO2, Methane, other

Atmospheric Pressure pressure exerted by atmosphere

Warming Sun - solar constant is not really constant greenhouse effect

warming due to the transparency of a substance to radiation at visible wavelengths and opacity to infrared radiation

Page 39: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The Earth’s atmosphere has changed substantially over time

The Earth’s atmosphere differs from those of the other terrestrial planets in its chemical composition, circulation pattern, and temperature profile

The Earth’s atmosphere changed from being mostly water vapor to being rich in carbon dioxide

A strong greenhouse effect kept the Earth warm enough for water to remain liquid and to permit the evolution of life

Page 40: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The appearance of photosynthetic living organisms led to our present atmospheric composition, about four- fifths nitrogen and one-fifth oxygen

Page 41: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Structure of the Atmosphere

Page 42: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Circulation in our atmosphere results from convection and the Earth’s rotation

Because of the Earth’s rapid rotation, the circulation in its atmosphere is complex, with three circulation cells in each hemisphere

Page 43: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Winds

Local winds wind chill

factorGlobal

wind patterns

Page 44: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Weather Producers

Air MassesEvaporation

Absolute humidity Relative humidity

FrontsWaves and cyclonesStorms

thunderstorms, tornadoes, hurricanes

Page 45: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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An idealized cold front

Page 46: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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An idealized warm front

Page 47: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Weather Forecasting

Predictions based upon “characteristics, location, and rate of

movement of air masses and associated fronts and pressure systems”

Complex computer modelsLed to science of “chaos”

chaotic dynamic systems

Page 48: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Climate

“general pattern of the weather that occurs for a region over a number of years”

Major climate regions tropical temperate polar

Page 49: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The principal climate zones

Page 50: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Which of the following layers of the atmosphere is highest above the surface of the Earth?

A troposphere.B stratosphere.C thermosphere.D mesosphere.E ozone layer.

Page 51: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

What is the primary ingredient of the Earth's atmosphere?

A NitrogenB OxygenC Nitrogen and oxygen in equal partsD HydrogenE Carbon dioxide

Page 52: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

In what part of the atmosphere does weather occur?

A hydrosphereB stratosphereC ionosphereD troposphereE all of the above

Page 53: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker QuestionHow rapidly a planet loses its atmosphere depends

on the planet's I. mass II. atmospheric composition III. temperature IV. rotation period

A I & IIB III & IVC I, II, & IIID II, III, & IVE I, II, III, & IV

Page 54: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

Earth possesses few visible craters and the Moon possesses many. This is largely because

A Earth formed later than the Moon and, therefore hasn't encountered as many meteoroids.

B the Moon doesn't have an atmosphere that could burn up meteorites before impacting.

C erosion and plate tectonics have slowly removed evidence of past cratering on Earth.

D A, B and C.E Only B and C above.

Page 55: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Ocean currents influence temperatures and climates

Page 56: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The hydrologic cycle

Tidal forces help power the motion of the oceans

Page 57: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Distribution of the Water

Page 58: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Watersheds of three rivers

Page 59: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The path of groundwater

Page 60: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Oceanography

Waves and tides changes coastal structure

transport of material

long term and short term changesA Climate control mechanism

ocean conveyor beltmajor control of climate

Page 61: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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A wave passing in the open

ocean

Page 62: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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A wave becoming breaking onshore

Page 63: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Ocean Conveyor Belt -Major Climate Control

Page 64: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The Earth’s Magnetic Field

Electric currents in the liquid outer core generate a dipole magnetic field Similar to a coil of wire around an iron nail

This magnetic field produces a magnetosphere that surrounds the Earth and blocks the solar wind from hitting the atmosphere

Traps particles from the solar wind in regions Producing Van Allen Belts

Most of the particles of the solar wind are deflected around the Earth by the magnetosphere.

Page 65: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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A bow-shaped shock wave, where the supersonic solar wind is abruptly slowed to subsonic speeds, marks the outer boundary of the magnetosphere

Page 66: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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An increased flow of charged particles fromthe Sun can overload the Van Allen belts and cascade toward the Earth, producing aurorae

Some charged particles from the solar wind are trapped in two huge, doughnut-shaped rings called the Van Allen belts

Page 67: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

The presence of Earth’s magnetic field is a good indication that

A there is a large amount of magnetic material buried near the North Pole.

B there is a quantity of liquid metal swirling around in the Earth's core.

C the Earth is composed largely of iron.D the Earth is completely solid.E there are condensed gasses in the core of

the Earth.

Page 68: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Energy Sources and the Earth’s atmosphere, oceans, and surface

Page 69: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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The Greenhouse Effect Solar energy is the

energy source for the atmosphere

In the greenhouse effect, some of this energy is trapped by infrared absorbing gases in the atmosphere, raising the Earth’s surface temperature above what it would be if there was no greenhouse effect

Page 70: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Page 71: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Rising Carbon Dioxide

Page 72: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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Industrial chemicals released into the atmosphere have damaged the ozone layer in the stratosphere

Page 73: 1 HNRT 228 Astrobiology Chapter 4 - Earth - Bennett & Shostak Lecture Notes for Chapter 4 21 and 23 September 2015 Dr. H. Geller

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iClicker Question

The greenhouse effect occurs largely becauseA a gas is transparent to visible light and

opaque to infrared radiation.B a gas is transparent to infrared radiation

and opaque to ultraviolet radiation.C ozone is transparent to ultraviolet

radiation and opaque to infrared radiation.D methane is transparent to infrared

radiation and opaque to visible light.E the sun emits more infrared radiation than

ultraviolet radiation.