SlideShare a Scribd company logo
1 of 56
 You will receive a list of unit vocabulary at the top of 
every unit note packet! 
 How you choose to complete the vocabulary is up to 
you! 
 It should be completed in your science notebook or 
stored in your binder and will be checked for 
completion on the day it is due. [10 points] 
 Expect a vocabulary test approximately 1 week after 
you receive the list.
Unit 1 
The study of stars and space. 
Big Bang
• The universe is expanding 
o How do we know this? 
• In the late 1920’s, Edwin Hubble 
discovered that All galaxies were “red-shifted” 
when viewed from Earth. 
• This meant that all galaxies were moving 
away from Earth and each other, and thus, 
the universe must be expanding. 
• Learn to annotate!
• All matter and energy in the universe was once 
condensed into a single point 
• 13.8 bya 
• Moments after the Big Bang, the universe was very 
hot and dense 
o Protons, neutrons, and electrons formed 
o Hydrogen formed 
o There was enough energy to start nuclear fusion 
 Helium formed
• Evidence 
o Background radiation 
 Space is...space! 
o There should be no heat at all (0K) 
o Scientists have measured space; 3K (Background 
radiation exists) 
o Composition of matter in the universe 
 74% hydrogen 
 24% helium 
Expansion of the Universe
A. Electromagnetic Energy 
1. The sun is the major energy 
source for weather changes in 
the atmosphere and many of the 
changes occurring at Earth’s 
surface. 
2. Energy from the sun comes in 
many different wavelengths.
 Each element or 
compound in its 
gaseous form 
produce a unique 
set of spectral 
lines. 
 Spectral lines act as 
“FINGERPRINTS” 
as they identify 
elements present in 
the 
STARS/GALAXIES 
. 
Example: The SUN has thousands of dark lines & 
more than 60 elements have been identified by 
matching these lines with those elements known on 
Earth!
• The Doppler Effect 
o The change in frequency of a wave an observer relative to its motion 
o Moving toward you: Waves are 
compressed together 
o Moving away: Waves are stretched
• Redshift 
o When the light of a distant object (star, 
planet, etc.) is viewed through a prism, 
the spectrum is not continuous 
o Black lines appear: Absorption lines 
 Determine which elements are present 
o When the object is moving away from 
us, the absorption lines are shifted 
toward the red end of the spectrum 
(stretched): Redshift!
Using the spectroscope, astronomers can determine 
whether a particular object is moving toward Earth or 
away from Earth
• Our sun is just one of billions of stars in the Milky 
Way galaxy. 
• Only star whose surface we can study. 
• Through spectroscopic analysis of the sun, scientists 
know that most of the known elements are found in 
the sun 
o Hydrogen makes up 74%of the sun’s mass 
o Helium makes up 24%
• Sunspots: “Dark” areas 
on the sun 
o “Cool” areas 
o The magnetic field 
breaks through the 
surface, causing a 
disruption in heat 
transfer 
o The number of 
sunspots varies every 
11 years. This is known 
as the solar cycle.
• The core 
o Nuclear fusion
Life Cycles of Stars
• A Star is Born
• A star’s “life cycle” can last billions of years. 
• The following slides describe the general phases in 
stellar evolution
Nebula 
• Dark, cool clouds of 
interstellar gas and 
dust. 
• Often referred to as 
“stellar nurseries.” 
• Stars begin to form 
as gas and dust 
collide.
Protostar 
• Developing star 
• Not yet hot enough 
for fusion reactions 
(10x106 K) 
http://seethaler.net/space/protostar.jpeg
Main Sequence Star 
• Hydrogen to Helium 
fusion has begun! 
• The hotter, larger 
stars burn H2 
fastest. 
• This stage makes 
up 90% of a star’s 
“life.” 
http://content4.bestthinking.com/s/1/topics/500/images/3e6daf0-40a3-495c-8006-5da9e7e9b069_972.jpeg
Earth’s Place in the Universe
Universe 
Our Milky Way 
Galaxy is one of 
billions of galaxies in 
an expanding 
universe
Milky Way Galaxy 
• Our Sun/solar 
system is one of 
an estimated 
180 billion stars 
making up this 
spiral galaxy
Our Solar System 
Earth – a small dense rocky planet, one of 8 planets 
that orbit the sun 
AND – the only one we know of that has LIFE as 
we know it……
So…. What Keeps Us Going? 
Newton’s Laws of Gravity 
Gravity and Inertia
Newton’s Law of Inertia 
States that a body in forward motion will continue in forward 
motion unless acted on by an outside force. 
Inertia 
Gravity 
Stable Orbit
 Inertia – causes a 
planet to move in a 
straight line. 
 Gravity – pulls a 
planet toward the 
sun.
Rotation 
• The spinning of a 
celestial body (Earth) 
on an imaginary axis
Rotation 
A. Earth’s Direction of Rotation: 
WEST to EAST 
2. Angular Rate of Rotation: 
THINK – one complete rotation 
360 degrees 
24 hours 
Rate = 3600/24 hours = 150/hour
B. Effects of Earth’s Rotation 
1. Day and Night
B. Effects of Earth’s Rotation 
2. Apparent daily motion 
of the sun 
a. Earth rotates from 
WEST to EAST 
b. Sun “appears” to move in 
an arc from EAST to 
WEST
Earth is NOT a perfect sphere. 
It is an oblate spheroid – 
slightly wider across the 
equator (due to its rotational 
spin) 
Earth‘s axis is not stable. It 
moves/wobbles (like a top). 
This is known as precession. 
It’s very slow - 26,000 years to 
complete one cycle. 
Within the precession are 
additional motions known as 
nutations. These are 
smaller motions back and forth 
as the precession occurs.
V. Revolution 
• The orbiting of one celestial body around another 
celestial body. 
A. Earth’s Angular Rate of Revolution 
1. 360 degrees 
2. 365 days 
3. Rate = 3600/365 days ~ = 10/day
B. Effects of Earth’s 
Revolution 
1. Nighttime constellations 
change in a yearly cycle. 
2. Constellation – groups 
of stars that form 
patterns of imaginary 
things such as animals, 
legendary heroes, and 
mythological gods
3. Seasons – a yearly cycle
5. Seasons of the Year 
A. Causes: 
1. Revolution - Earth revolves around the sun 
2. TILT - Earth is tilted/inclined on axis 23 1/2o 
3. Parallelism of Axis - Earth’s axis always points in the 
same direction.
B. Earth’s axis is tilted 23.50 relative to the plane 
of it’s orbit. 
• Draw and label 
your diagram 
according to the 
diagram at the 
right. Be sure to 
name the 
equator, the 
Tropic of Cancer 
and Capricorn 
and note where 
we live.
C. The apparent path of the sun changes with the 
seasons and with latitude. 
N.C. 35.5 degrees North Latitude
D. Length of Daylight (duration of daylight) – 
changes with seasons and with latitude.
E. Factors affecting Insolation 
1. Shape of the Earth (spherical) 
2. As latitude 
increases, the 
angle of 
insolation 
decreases, and 
the intensity of 
insolation 
decreases.
C. Season of the Year 
a. As Earth travels along its orbital path around the sun, 
the angle of insolation at a given latitude changes with 
the seasons. This depends on how far a given latitude 
is from the direct rays of the sun. The direct rays 
migrate between the Tropic of Cancer (north) and 
the Tropic of Capricorn (south).
4. Time of Day 
a. The angle of 
insolation 
changes in the 
course of one 
day. Maximum 
intensity occurs at 
Noon.
b. Looking South 
• The shadow of a vertical pole indicates how the angle of insolation 
changes during the day. The higher/greater the angle of insolation, 
the shorter the shadow, and the greater the intensity of 
insolation.
VI The Moon 
A.The moon is a natural 
satellite of Earth.
B. Physical Properties of the Moon 
1. Size 
a. Diameter: 2160 
miles 
b. Compared to Earth 
Diameter of Moon = 2160 = 1 
Earth 8000 4 
2. Gravity 
a. 1/6 the gravity of Earth 
b. This is because the Moon 
has – less mass
2. Atmosphere 
a) The Moon has No atmosphere, 
so radiation from sun strong 
b) Gravity too weak so gases 
escape into space. 
c) Without an atmosphere radiation 
from the sun is INTENSE! 
d) Frozen water may exist at the 
Moon’s polar regions, but none 
in liquid form
3. Phases of the Moon - 
Period of Revolution = 1 month OR 29.5 days 
a. The phases of the moon are caused by the moon’s 
revolution around Earth. 
b. Our Earth view of the changing illuminated part of the 
moon’s surface that face’s Earth.
c. Waning moon - the decrease 
in light (on the left), away 
from being a full moon to new 
moon, is called a.
d. waxing moon - as the moon 
increases towards becoming 
a full moon.
4. Moon Rotation 
b. Does that mean the 
moon doesn't 
rotate? 
c. YES it does --one 
rotation for each 
revolution around 
Earth!
5. Lunar Eclipse 
a. An eclipse of the Moon can only take place 
at full moon and only if the Moon passes 
through some portion of the earth’s 
shadow. The shadow is actually composed 
of two (2) cone-shaped components, one 
inside the other. The outer or penumbra 
shadow is a zone where some portion of 
the sun’s rays are blocked. In contrast, the 
inner or umbra shadow is a region devoid 
of all direct sunlight.
6. Solar Eclipse 
a. A solar eclipse 
occurs when the 
moon passes 
directly between 
the Earth and 
sun. 
b. New Moon are 
the only time 
solar eclipses can 
occur.
10. Tides 
a. Tides are the alternate 
rising and falling of the 
sea. 
b. This is caused by the 
Moon’s gravitational pull. 
c. The rising of tides is 
affected by the position and 
distance of moon! 
d. The period from high tide to 
high tide is 12 hours and 12 
minutes. 
e. Tides are a CYCLIC 
change.

More Related Content

What's hot

Earth dynamics
Earth dynamicsEarth dynamics
Earth dynamicsbeaduro
 
The Dynamic Earth
The Dynamic EarthThe Dynamic Earth
The Dynamic Earthduncanpatti
 
Ii. e. history of the earth
Ii. e. history of the earthIi. e. history of the earth
Ii. e. history of the earthMarian Santos
 
C:\Users\Lisa Knight\Desktop\A Scientific Revolution Begins
C:\Users\Lisa Knight\Desktop\A Scientific Revolution BeginsC:\Users\Lisa Knight\Desktop\A Scientific Revolution Begins
C:\Users\Lisa Knight\Desktop\A Scientific Revolution Beginsknightsnc
 
Ii. d. deformation of the crust
Ii. d. deformation of the crustIi. d. deformation of the crust
Ii. d. deformation of the crustMarian Santos
 
Science Review Semester Final
Science Review Semester FinalScience Review Semester Final
Science Review Semester FinalManuel S. Herrera
 
Unit 9 Internal dynamics of the earth
Unit 9  Internal dynamics of the earthUnit 9  Internal dynamics of the earth
Unit 9 Internal dynamics of the earthmihayedo
 
UNIT 2 EARTH'S INTERNAL ENERGY
UNIT 2 EARTH'S INTERNAL ENERGYUNIT 2 EARTH'S INTERNAL ENERGY
UNIT 2 EARTH'S INTERNAL ENERGYbeabio75
 
2012 updated plate tectonics new one use this one backup
2012 updated plate tectonics new one use this one backup2012 updated plate tectonics new one use this one backup
2012 updated plate tectonics new one use this one backupharvey09
 
Unit 8: The Earth's internal energy
Unit 8: The Earth's internal energyUnit 8: The Earth's internal energy
Unit 8: The Earth's internal energyMónica
 
UNIT 2 EARTH'S INTERNAL ENERGY.
UNIT 2 EARTH'S INTERNAL ENERGY.UNIT 2 EARTH'S INTERNAL ENERGY.
UNIT 2 EARTH'S INTERNAL ENERGY.beabio75
 
212_zer nola( irene leire nagore).doc.doc
212_zer nola( irene leire nagore).doc.doc212_zer nola( irene leire nagore).doc.doc
212_zer nola( irene leire nagore).doc.docElhuyarOlinpiada
 
Plate Tectonics
Plate TectonicsPlate Tectonics
Plate Tectonicswindyridge
 

What's hot (20)

Unit 5 - Disaster Management
Unit 5 - Disaster ManagementUnit 5 - Disaster Management
Unit 5 - Disaster Management
 
Earth dynamics
Earth dynamicsEarth dynamics
Earth dynamics
 
The Dynamic Earth
The Dynamic EarthThe Dynamic Earth
The Dynamic Earth
 
Ii. e. history of the earth
Ii. e. history of the earthIi. e. history of the earth
Ii. e. history of the earth
 
C:\Users\Lisa Knight\Desktop\A Scientific Revolution Begins
C:\Users\Lisa Knight\Desktop\A Scientific Revolution BeginsC:\Users\Lisa Knight\Desktop\A Scientific Revolution Begins
C:\Users\Lisa Knight\Desktop\A Scientific Revolution Begins
 
Ii. d. deformation of the crust
Ii. d. deformation of the crustIi. d. deformation of the crust
Ii. d. deformation of the crust
 
Science Review Semester Final
Science Review Semester FinalScience Review Semester Final
Science Review Semester Final
 
Module 2 intro
Module 2 introModule 2 intro
Module 2 intro
 
Unit 9 Internal dynamics of the earth
Unit 9  Internal dynamics of the earthUnit 9  Internal dynamics of the earth
Unit 9 Internal dynamics of the earth
 
UNIT 2 EARTH'S INTERNAL ENERGY
UNIT 2 EARTH'S INTERNAL ENERGYUNIT 2 EARTH'S INTERNAL ENERGY
UNIT 2 EARTH'S INTERNAL ENERGY
 
2012 updated plate tectonics new one use this one backup
2012 updated plate tectonics new one use this one backup2012 updated plate tectonics new one use this one backup
2012 updated plate tectonics new one use this one backup
 
Unit 8: The Earth's internal energy
Unit 8: The Earth's internal energyUnit 8: The Earth's internal energy
Unit 8: The Earth's internal energy
 
Ch19 building the earths surface
Ch19 building the earths surfaceCh19 building the earths surface
Ch19 building the earths surface
 
UNIT 2 EARTH'S INTERNAL ENERGY.
UNIT 2 EARTH'S INTERNAL ENERGY.UNIT 2 EARTH'S INTERNAL ENERGY.
UNIT 2 EARTH'S INTERNAL ENERGY.
 
212_zer nola( irene leire nagore).doc.doc
212_zer nola( irene leire nagore).doc.doc212_zer nola( irene leire nagore).doc.doc
212_zer nola( irene leire nagore).doc.doc
 
Plate Tectonics
Plate TectonicsPlate Tectonics
Plate Tectonics
 
Module 1 intro
Module 1 introModule 1 intro
Module 1 intro
 
Geology 2º ESO
Geology 2º ESOGeology 2º ESO
Geology 2º ESO
 
Geology 2 eso
Geology 2 esoGeology 2 eso
Geology 2 eso
 
Arnychap05 earth
Arnychap05   earthArnychap05   earth
Arnychap05 earth
 

Viewers also liked

Unit 1, lesson 2
Unit 1, lesson 2Unit 1, lesson 2
Unit 1, lesson 2hschiesher
 
Makeup of the earth, lesson 2
Makeup of the earth, lesson 2Makeup of the earth, lesson 2
Makeup of the earth, lesson 2hschiesher
 
Sailor Story2
Sailor Story2Sailor Story2
Sailor Story2medvele
 
Meteorologists
MeteorologistsMeteorologists
Meteorologistshschiesher
 
Makeup of the earth, lesson 1
Makeup of the earth, lesson 1Makeup of the earth, lesson 1
Makeup of the earth, lesson 1hschiesher
 
Unit C, Lesson 1
Unit C, Lesson 1Unit C, Lesson 1
Unit C, Lesson 1hschiesher
 

Viewers also liked (7)

Unit 1, lesson 2
Unit 1, lesson 2Unit 1, lesson 2
Unit 1, lesson 2
 
Makeup of the earth, lesson 2
Makeup of the earth, lesson 2Makeup of the earth, lesson 2
Makeup of the earth, lesson 2
 
Sailor Story2
Sailor Story2Sailor Story2
Sailor Story2
 
Meteorologists
MeteorologistsMeteorologists
Meteorologists
 
Makeup of the earth, lesson 1
Makeup of the earth, lesson 1Makeup of the earth, lesson 1
Makeup of the earth, lesson 1
 
Unit C, Lesson 1
Unit C, Lesson 1Unit C, Lesson 1
Unit C, Lesson 1
 
Meteorology
MeteorologyMeteorology
Meteorology
 

Similar to Astronomy nc 2014

Chapter 20 planetary motion
Chapter 20   planetary motionChapter 20   planetary motion
Chapter 20 planetary motionAnnie cox
 
Apes earth systems
Apes  earth systemsApes  earth systems
Apes earth systemsBobby Lewis
 
Review#14 astronomy
Review#14 astronomyReview#14 astronomy
Review#14 astronomyLexume1
 
Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6Don R. Mueller, Ph.D.
 
New astronomy presentation
New astronomy presentationNew astronomy presentation
New astronomy presentationkshukla
 
T1. solar system 3, plates, orbits, periods, light,
T1. solar system 3, plates, orbits, periods, light,T1. solar system 3, plates, orbits, periods, light,
T1. solar system 3, plates, orbits, periods, light,jaume2014
 
8. universe and earth ana
8. universe and earth ana8. universe and earth ana
8. universe and earth anaanaruperez
 
Earth's Motions
Earth's MotionsEarth's Motions
Earth's Motionsjmkale
 
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02Laurie Mccauley-Holland
 
Fy12 astronomy
Fy12 astronomyFy12 astronomy
Fy12 astronomybionioncle
 
218087672 mokgopa.sun&earth presentation
218087672 mokgopa.sun&earth presentation218087672 mokgopa.sun&earth presentation
218087672 mokgopa.sun&earth presentationTsiamo Mokgopa
 

Similar to Astronomy nc 2014 (20)

Astronomy NC 2014
Astronomy NC 2014Astronomy NC 2014
Astronomy NC 2014
 
Chapter 20 planetary motion
Chapter 20   planetary motionChapter 20   planetary motion
Chapter 20 planetary motion
 
Astronomy - Notes
Astronomy - NotesAstronomy - Notes
Astronomy - Notes
 
Unit1.Planet Earth
Unit1.Planet EarthUnit1.Planet Earth
Unit1.Planet Earth
 
Solar system
Solar systemSolar system
Solar system
 
Apes earth systems
Apes  earth systemsApes  earth systems
Apes earth systems
 
Review#14 astronomy
Review#14 astronomyReview#14 astronomy
Review#14 astronomy
 
Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6Astonishing Astronomy 101 - Chapter 6
Astonishing Astronomy 101 - Chapter 6
 
New astronomy presentation
New astronomy presentationNew astronomy presentation
New astronomy presentation
 
Astronomy
AstronomyAstronomy
Astronomy
 
Chapter 13 universe
Chapter 13   universeChapter 13   universe
Chapter 13 universe
 
UNIT 2 ASTRONOMY.pptx
UNIT 2 ASTRONOMY.pptxUNIT 2 ASTRONOMY.pptx
UNIT 2 ASTRONOMY.pptx
 
sun properties.ppt
sun properties.pptsun properties.ppt
sun properties.ppt
 
T1. solar system 3, plates, orbits, periods, light,
T1. solar system 3, plates, orbits, periods, light,T1. solar system 3, plates, orbits, periods, light,
T1. solar system 3, plates, orbits, periods, light,
 
8. universe and earth ana
8. universe and earth ana8. universe and earth ana
8. universe and earth ana
 
Earth's Motions
Earth's MotionsEarth's Motions
Earth's Motions
 
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
Planetarymotionhistoricalpeopleinastronomy 131204162554-phpapp02
 
Fy12 astronomy
Fy12 astronomyFy12 astronomy
Fy12 astronomy
 
218087672 mokgopa.sun&earth presentation
218087672 mokgopa.sun&earth presentation218087672 mokgopa.sun&earth presentation
218087672 mokgopa.sun&earth presentation
 
Astronomy
AstronomyAstronomy
Astronomy
 

More from lorizimmerman

Models and dimensions of earth
Models and dimensions of earthModels and dimensions of earth
Models and dimensions of earthlorizimmerman
 
Energy resources ppt
Energy resources pptEnergy resources ppt
Energy resources pptlorizimmerman
 
NC Human Impact Unit
NC Human Impact UnitNC Human Impact Unit
NC Human Impact Unitlorizimmerman
 
Energy intro activity
Energy intro activityEnergy intro activity
Energy intro activitylorizimmerman
 
Energy resources unit powerpoint
Energy resources unit powerpointEnergy resources unit powerpoint
Energy resources unit powerpointlorizimmerman
 
Weathering, Erosion and Soils
Weathering, Erosion and SoilsWeathering, Erosion and Soils
Weathering, Erosion and Soilslorizimmerman
 
Mountain building ppt nc 13
Mountain building ppt nc 13Mountain building ppt nc 13
Mountain building ppt nc 13lorizimmerman
 
Geologic history academic
Geologic history academicGeologic history academic
Geologic history academiclorizimmerman
 
Earth history nc honors 13
Earth history nc honors 13Earth history nc honors 13
Earth history nc honors 13lorizimmerman
 
Models and dimensions of earth
Models and dimensions of earthModels and dimensions of earth
Models and dimensions of earthlorizimmerman
 
Earth/Environmental - Introduction
Earth/Environmental - IntroductionEarth/Environmental - Introduction
Earth/Environmental - Introductionlorizimmerman
 

More from lorizimmerman (17)

Gel 111 intro ppt
Gel 111 intro pptGel 111 intro ppt
Gel 111 intro ppt
 
8 oceanography ppt
8  oceanography ppt8  oceanography ppt
8 oceanography ppt
 
Astronomy jeopardy
Astronomy jeopardyAstronomy jeopardy
Astronomy jeopardy
 
Models and dimensions of earth
Models and dimensions of earthModels and dimensions of earth
Models and dimensions of earth
 
Energy resources ppt
Energy resources pptEnergy resources ppt
Energy resources ppt
 
NC Human Impact Unit
NC Human Impact UnitNC Human Impact Unit
NC Human Impact Unit
 
GHHS Oceanography
GHHS Oceanography GHHS Oceanography
GHHS Oceanography
 
Freshwater
Freshwater Freshwater
Freshwater
 
Energy intro activity
Energy intro activityEnergy intro activity
Energy intro activity
 
Energy resources unit powerpoint
Energy resources unit powerpointEnergy resources unit powerpoint
Energy resources unit powerpoint
 
Weathering, Erosion and Soils
Weathering, Erosion and SoilsWeathering, Erosion and Soils
Weathering, Erosion and Soils
 
Rocks & minerals
Rocks & mineralsRocks & minerals
Rocks & minerals
 
Mountain building ppt nc 13
Mountain building ppt nc 13Mountain building ppt nc 13
Mountain building ppt nc 13
 
Geologic history academic
Geologic history academicGeologic history academic
Geologic history academic
 
Earth history nc honors 13
Earth history nc honors 13Earth history nc honors 13
Earth history nc honors 13
 
Models and dimensions of earth
Models and dimensions of earthModels and dimensions of earth
Models and dimensions of earth
 
Earth/Environmental - Introduction
Earth/Environmental - IntroductionEarth/Environmental - Introduction
Earth/Environmental - Introduction
 

Recently uploaded

Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactdawncurless
 
Employee wellbeing at the workplace.pptx
Employee wellbeing at the workplace.pptxEmployee wellbeing at the workplace.pptx
Employee wellbeing at the workplace.pptxNirmalaLoungPoorunde1
 
Concept of Vouching. B.Com(Hons) /B.Compdf
Concept of Vouching. B.Com(Hons) /B.CompdfConcept of Vouching. B.Com(Hons) /B.Compdf
Concept of Vouching. B.Com(Hons) /B.CompdfUmakantAnnand
 
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...EduSkills OECD
 
microwave assisted reaction. General introduction
microwave assisted reaction. General introductionmicrowave assisted reaction. General introduction
microwave assisted reaction. General introductionMaksud Ahmed
 
Crayon Activity Handout For the Crayon A
Crayon Activity Handout For the Crayon ACrayon Activity Handout For the Crayon A
Crayon Activity Handout For the Crayon AUnboundStockton
 
_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting Data_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting DataJhengPantaleon
 
Presiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha electionsPresiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha electionsanshu789521
 
18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf
18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf
18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdfssuser54595a
 
CARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptxCARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptxGaneshChakor2
 
Class 11 Legal Studies Ch-1 Concept of State .pdf
Class 11 Legal Studies Ch-1 Concept of State .pdfClass 11 Legal Studies Ch-1 Concept of State .pdf
Class 11 Legal Studies Ch-1 Concept of State .pdfakmcokerachita
 
Sanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdfSanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdfsanyamsingh5019
 
A Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy ReformA Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy ReformChameera Dedduwage
 
SOCIAL AND HISTORICAL CONTEXT - LFTVD.pptx
SOCIAL AND HISTORICAL CONTEXT - LFTVD.pptxSOCIAL AND HISTORICAL CONTEXT - LFTVD.pptx
SOCIAL AND HISTORICAL CONTEXT - LFTVD.pptxiammrhaywood
 
Call Girls in Dwarka Mor Delhi Contact Us 9654467111
Call Girls in Dwarka Mor Delhi Contact Us 9654467111Call Girls in Dwarka Mor Delhi Contact Us 9654467111
Call Girls in Dwarka Mor Delhi Contact Us 9654467111Sapana Sha
 
Paris 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activityParis 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activityGeoBlogs
 
Alper Gobel In Media Res Media Component
Alper Gobel In Media Res Media ComponentAlper Gobel In Media Res Media Component
Alper Gobel In Media Res Media ComponentInMediaRes1
 
Interactive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communicationInteractive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communicationnomboosow
 

Recently uploaded (20)

Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impact
 
Employee wellbeing at the workplace.pptx
Employee wellbeing at the workplace.pptxEmployee wellbeing at the workplace.pptx
Employee wellbeing at the workplace.pptx
 
Concept of Vouching. B.Com(Hons) /B.Compdf
Concept of Vouching. B.Com(Hons) /B.CompdfConcept of Vouching. B.Com(Hons) /B.Compdf
Concept of Vouching. B.Com(Hons) /B.Compdf
 
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
Presentation by Andreas Schleicher Tackling the School Absenteeism Crisis 30 ...
 
microwave assisted reaction. General introduction
microwave assisted reaction. General introductionmicrowave assisted reaction. General introduction
microwave assisted reaction. General introduction
 
TataKelola dan KamSiber Kecerdasan Buatan v022.pdf
TataKelola dan KamSiber Kecerdasan Buatan v022.pdfTataKelola dan KamSiber Kecerdasan Buatan v022.pdf
TataKelola dan KamSiber Kecerdasan Buatan v022.pdf
 
Crayon Activity Handout For the Crayon A
Crayon Activity Handout For the Crayon ACrayon Activity Handout For the Crayon A
Crayon Activity Handout For the Crayon A
 
_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting Data_Math 4-Q4 Week 5.pptx Steps in Collecting Data
_Math 4-Q4 Week 5.pptx Steps in Collecting Data
 
Presiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha electionsPresiding Officer Training module 2024 lok sabha elections
Presiding Officer Training module 2024 lok sabha elections
 
18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf
18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf
18-04-UA_REPORT_MEDIALITERAСY_INDEX-DM_23-1-final-eng.pdf
 
CARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptxCARE OF CHILD IN INCUBATOR..........pptx
CARE OF CHILD IN INCUBATOR..........pptx
 
Class 11 Legal Studies Ch-1 Concept of State .pdf
Class 11 Legal Studies Ch-1 Concept of State .pdfClass 11 Legal Studies Ch-1 Concept of State .pdf
Class 11 Legal Studies Ch-1 Concept of State .pdf
 
Model Call Girl in Tilak Nagar Delhi reach out to us at 🔝9953056974🔝
Model Call Girl in Tilak Nagar Delhi reach out to us at 🔝9953056974🔝Model Call Girl in Tilak Nagar Delhi reach out to us at 🔝9953056974🔝
Model Call Girl in Tilak Nagar Delhi reach out to us at 🔝9953056974🔝
 
Sanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdfSanyam Choudhary Chemistry practical.pdf
Sanyam Choudhary Chemistry practical.pdf
 
A Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy ReformA Critique of the Proposed National Education Policy Reform
A Critique of the Proposed National Education Policy Reform
 
SOCIAL AND HISTORICAL CONTEXT - LFTVD.pptx
SOCIAL AND HISTORICAL CONTEXT - LFTVD.pptxSOCIAL AND HISTORICAL CONTEXT - LFTVD.pptx
SOCIAL AND HISTORICAL CONTEXT - LFTVD.pptx
 
Call Girls in Dwarka Mor Delhi Contact Us 9654467111
Call Girls in Dwarka Mor Delhi Contact Us 9654467111Call Girls in Dwarka Mor Delhi Contact Us 9654467111
Call Girls in Dwarka Mor Delhi Contact Us 9654467111
 
Paris 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activityParis 2024 Olympic Geographies - an activity
Paris 2024 Olympic Geographies - an activity
 
Alper Gobel In Media Res Media Component
Alper Gobel In Media Res Media ComponentAlper Gobel In Media Res Media Component
Alper Gobel In Media Res Media Component
 
Interactive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communicationInteractive Powerpoint_How to Master effective communication
Interactive Powerpoint_How to Master effective communication
 

Astronomy nc 2014

  • 1.  You will receive a list of unit vocabulary at the top of every unit note packet!  How you choose to complete the vocabulary is up to you!  It should be completed in your science notebook or stored in your binder and will be checked for completion on the day it is due. [10 points]  Expect a vocabulary test approximately 1 week after you receive the list.
  • 2. Unit 1 The study of stars and space. Big Bang
  • 3. • The universe is expanding o How do we know this? • In the late 1920’s, Edwin Hubble discovered that All galaxies were “red-shifted” when viewed from Earth. • This meant that all galaxies were moving away from Earth and each other, and thus, the universe must be expanding. • Learn to annotate!
  • 4. • All matter and energy in the universe was once condensed into a single point • 13.8 bya • Moments after the Big Bang, the universe was very hot and dense o Protons, neutrons, and electrons formed o Hydrogen formed o There was enough energy to start nuclear fusion  Helium formed
  • 5. • Evidence o Background radiation  Space is...space! o There should be no heat at all (0K) o Scientists have measured space; 3K (Background radiation exists) o Composition of matter in the universe  74% hydrogen  24% helium Expansion of the Universe
  • 6. A. Electromagnetic Energy 1. The sun is the major energy source for weather changes in the atmosphere and many of the changes occurring at Earth’s surface. 2. Energy from the sun comes in many different wavelengths.
  • 7.
  • 8.  Each element or compound in its gaseous form produce a unique set of spectral lines.  Spectral lines act as “FINGERPRINTS” as they identify elements present in the STARS/GALAXIES . Example: The SUN has thousands of dark lines & more than 60 elements have been identified by matching these lines with those elements known on Earth!
  • 9. • The Doppler Effect o The change in frequency of a wave an observer relative to its motion o Moving toward you: Waves are compressed together o Moving away: Waves are stretched
  • 10.
  • 11. • Redshift o When the light of a distant object (star, planet, etc.) is viewed through a prism, the spectrum is not continuous o Black lines appear: Absorption lines  Determine which elements are present o When the object is moving away from us, the absorption lines are shifted toward the red end of the spectrum (stretched): Redshift!
  • 12. Using the spectroscope, astronomers can determine whether a particular object is moving toward Earth or away from Earth
  • 13. • Our sun is just one of billions of stars in the Milky Way galaxy. • Only star whose surface we can study. • Through spectroscopic analysis of the sun, scientists know that most of the known elements are found in the sun o Hydrogen makes up 74%of the sun’s mass o Helium makes up 24%
  • 14. • Sunspots: “Dark” areas on the sun o “Cool” areas o The magnetic field breaks through the surface, causing a disruption in heat transfer o The number of sunspots varies every 11 years. This is known as the solar cycle.
  • 15. • The core o Nuclear fusion
  • 16. Life Cycles of Stars
  • 17. • A Star is Born
  • 18. • A star’s “life cycle” can last billions of years. • The following slides describe the general phases in stellar evolution
  • 19. Nebula • Dark, cool clouds of interstellar gas and dust. • Often referred to as “stellar nurseries.” • Stars begin to form as gas and dust collide.
  • 20. Protostar • Developing star • Not yet hot enough for fusion reactions (10x106 K) http://seethaler.net/space/protostar.jpeg
  • 21. Main Sequence Star • Hydrogen to Helium fusion has begun! • The hotter, larger stars burn H2 fastest. • This stage makes up 90% of a star’s “life.” http://content4.bestthinking.com/s/1/topics/500/images/3e6daf0-40a3-495c-8006-5da9e7e9b069_972.jpeg
  • 22. Earth’s Place in the Universe
  • 23. Universe Our Milky Way Galaxy is one of billions of galaxies in an expanding universe
  • 24. Milky Way Galaxy • Our Sun/solar system is one of an estimated 180 billion stars making up this spiral galaxy
  • 25. Our Solar System Earth – a small dense rocky planet, one of 8 planets that orbit the sun AND – the only one we know of that has LIFE as we know it……
  • 26. So…. What Keeps Us Going? Newton’s Laws of Gravity Gravity and Inertia
  • 27.
  • 28. Newton’s Law of Inertia States that a body in forward motion will continue in forward motion unless acted on by an outside force. Inertia Gravity Stable Orbit
  • 29.  Inertia – causes a planet to move in a straight line.  Gravity – pulls a planet toward the sun.
  • 30. Rotation • The spinning of a celestial body (Earth) on an imaginary axis
  • 31. Rotation A. Earth’s Direction of Rotation: WEST to EAST 2. Angular Rate of Rotation: THINK – one complete rotation 360 degrees 24 hours Rate = 3600/24 hours = 150/hour
  • 32. B. Effects of Earth’s Rotation 1. Day and Night
  • 33. B. Effects of Earth’s Rotation 2. Apparent daily motion of the sun a. Earth rotates from WEST to EAST b. Sun “appears” to move in an arc from EAST to WEST
  • 34. Earth is NOT a perfect sphere. It is an oblate spheroid – slightly wider across the equator (due to its rotational spin) Earth‘s axis is not stable. It moves/wobbles (like a top). This is known as precession. It’s very slow - 26,000 years to complete one cycle. Within the precession are additional motions known as nutations. These are smaller motions back and forth as the precession occurs.
  • 35. V. Revolution • The orbiting of one celestial body around another celestial body. A. Earth’s Angular Rate of Revolution 1. 360 degrees 2. 365 days 3. Rate = 3600/365 days ~ = 10/day
  • 36. B. Effects of Earth’s Revolution 1. Nighttime constellations change in a yearly cycle. 2. Constellation – groups of stars that form patterns of imaginary things such as animals, legendary heroes, and mythological gods
  • 37. 3. Seasons – a yearly cycle
  • 38. 5. Seasons of the Year A. Causes: 1. Revolution - Earth revolves around the sun 2. TILT - Earth is tilted/inclined on axis 23 1/2o 3. Parallelism of Axis - Earth’s axis always points in the same direction.
  • 39. B. Earth’s axis is tilted 23.50 relative to the plane of it’s orbit. • Draw and label your diagram according to the diagram at the right. Be sure to name the equator, the Tropic of Cancer and Capricorn and note where we live.
  • 40. C. The apparent path of the sun changes with the seasons and with latitude. N.C. 35.5 degrees North Latitude
  • 41. D. Length of Daylight (duration of daylight) – changes with seasons and with latitude.
  • 42. E. Factors affecting Insolation 1. Shape of the Earth (spherical) 2. As latitude increases, the angle of insolation decreases, and the intensity of insolation decreases.
  • 43. C. Season of the Year a. As Earth travels along its orbital path around the sun, the angle of insolation at a given latitude changes with the seasons. This depends on how far a given latitude is from the direct rays of the sun. The direct rays migrate between the Tropic of Cancer (north) and the Tropic of Capricorn (south).
  • 44. 4. Time of Day a. The angle of insolation changes in the course of one day. Maximum intensity occurs at Noon.
  • 45. b. Looking South • The shadow of a vertical pole indicates how the angle of insolation changes during the day. The higher/greater the angle of insolation, the shorter the shadow, and the greater the intensity of insolation.
  • 46. VI The Moon A.The moon is a natural satellite of Earth.
  • 47. B. Physical Properties of the Moon 1. Size a. Diameter: 2160 miles b. Compared to Earth Diameter of Moon = 2160 = 1 Earth 8000 4 2. Gravity a. 1/6 the gravity of Earth b. This is because the Moon has – less mass
  • 48. 2. Atmosphere a) The Moon has No atmosphere, so radiation from sun strong b) Gravity too weak so gases escape into space. c) Without an atmosphere radiation from the sun is INTENSE! d) Frozen water may exist at the Moon’s polar regions, but none in liquid form
  • 49. 3. Phases of the Moon - Period of Revolution = 1 month OR 29.5 days a. The phases of the moon are caused by the moon’s revolution around Earth. b. Our Earth view of the changing illuminated part of the moon’s surface that face’s Earth.
  • 50. c. Waning moon - the decrease in light (on the left), away from being a full moon to new moon, is called a.
  • 51. d. waxing moon - as the moon increases towards becoming a full moon.
  • 52.
  • 53. 4. Moon Rotation b. Does that mean the moon doesn't rotate? c. YES it does --one rotation for each revolution around Earth!
  • 54. 5. Lunar Eclipse a. An eclipse of the Moon can only take place at full moon and only if the Moon passes through some portion of the earth’s shadow. The shadow is actually composed of two (2) cone-shaped components, one inside the other. The outer or penumbra shadow is a zone where some portion of the sun’s rays are blocked. In contrast, the inner or umbra shadow is a region devoid of all direct sunlight.
  • 55. 6. Solar Eclipse a. A solar eclipse occurs when the moon passes directly between the Earth and sun. b. New Moon are the only time solar eclipses can occur.
  • 56. 10. Tides a. Tides are the alternate rising and falling of the sea. b. This is caused by the Moon’s gravitational pull. c. The rising of tides is affected by the position and distance of moon! d. The period from high tide to high tide is 12 hours and 12 minutes. e. Tides are a CYCLIC change.