SlideShare ist ein Scribd-Unternehmen logo
1 von 32
presents
a                               production
    INTRODUCTION TO
      THE UNIVERSE
    based on the IB Astrophysics option


                                          1
INTRODUCTION TO
  THE UNIVERSE
  What is there in the Universe?
      Asteroids and comets
              Moons
             Planets
              Stars
             Nebulae
         Stellar clusters
            Galaxies
        Galactic clusters
The Solar System
RELATIVE SIZES: if Sun = 100, Earth =1 ...
... and the distance between them is 10 000




  They all orbit the Sun on elliptical paths
The Sun
Mass: 1.99 x 1030 kg

Radius:6.96 x 108 m

Surface temperature: 5800 K
Planets Data                             (and Pluto)
Planet    Picture   Distance to the   Radius (km)     Orbital     Orbital      Surface   Density/   Satellite
                       Sun (km)                       period      period      day temp    g/cm3        s
                                                    around its                  (ºC)     water=1
Mercury               58 million       4 878 km        axis
                                                     59 days      88 days       167        5,43        0


Venus                108 million      12 104 km     -243 days    225 days       464       5,24         0


 Earth              149,6 million     12 756 km      23, 93 h      365,2        15        5,52         1
                                                                   days

 Mars                228 million       6 794 km     24h 37min    687 days       -65       3,04         2


Jupiter              778 million      142 800 km    9h 50min     12 years       -110      1,32        +63
                                                       30s

Saturn               1 427 million    120 000 km    10h 14min    29,5 years     -140      0,69        +56


Uranus               2 870 million    51 800 km     16h 18min    84 years       -195      1,27         27


Neptune              4 497 million    49 500 km     15h 48min    164 years      -200      1,77         13


 Pluto               5 900 million     2 400 km      6 days      248 years      -225        2          1
Mercury and Venus
The rocky planets closest to the Sun
Earth and Moon




                         Mariner 10


Many planets have moons which orbit
the planet (which orbits the Sun)
Mars
The fourth of the inner planets




Spirit Rover: Mars’ West Valley
Asteroid Belt
                       Ceres (480km):
                       it was the first
                       asteroid to be
                       seen. Now it’s a
                       dwarf planet.



                          Mathilde
                          (52km)




                    Eros
                (13x13x33km)
Jupiter
            The largest gas giant, 5 times more
            distant from the Sun than the Earth




Jupiter and its moons: Io,    Approximate size comparison
Europa, Ganymede and Callisto of Earth and Jupiter
Saturn
         Nearly twice as far from the Sun as Jupiter




A rough comparison of the sizes
of Saturn and Earth
Uranus
Twice as far from the Sun as Saturn




                        Size comparison
                        of Earth and
                        Uranus
Neptune
         Nearly twice as far from the Sun as Uranus
                (30 times further than Earth)




Size comparison of Neptune and
Earth.
Astronomical units of distance
The Astronomical Unit (AU) – this is the average
distance between the Earth and the Sun.
        1 AU = 150 000 000 km = 1.5x1011m
Astronomical distances
The light year (ly) – this is the distance travelled by light in
one year.

        c = 3x108 m/s
        t = 1 year = 365.25 x 24 x 60 x 60= 3.16 x 107 s

        Speed =Distance / Time

        Distance = Speed x Time
        
        = 3x108 x 3.16 x 107 = 9.46 x 1015 m

                    1 ly = 9.46x1015 m
Relative distances

        The Moon is 1.3 light seconds from the Earth


        The Earth is 500 light seconds from the Sun


    The nearest star to the Sun is about 4 light years away


   The diameter of a galaxy is about 100 000 light years


The distance between galaxies is about 1 000 000 light years
Galaxies
   A galaxy is a collection of a very large number of stars
(around 100 thousand million) mutually attracting each other
through the gravitational force and staying together. The
number of stars varies between a few million and hundreds
of billions. There are approximately 100 thousand million
galaxies in the observable universe.
  There are three types of galaxies:
  
   - Spiral (Milky Way)
  
   - Elliptical (M49)
  
   - Irregular (Magellanic Clouds)
Spiral Galaxies
  Spiral galaxies consist of a rotating disk of stars
along with a central bulge of generally older stars.
Extending outward from the bulge are relatively bright
arms. There is a supermassive black hole at the
centre. The dark patches in the picture is interstellar
dust.




              Milky Way
Spiral Galaxies
Andromeda galaxy is the closest large galaxy to Earth. It covers
about the same area of the night sky as the Moon but is much
dimmer.
Spiral Galaxies




         Sombrero Galaxy
Elliptical Galaxies




    M49                          ESO 325-G004

Elliptical cross-section and no spiral arms.
They range in shape from nearly spherical to highly flattened
ellipsoids and in size from hundreds of millions to over one
trillion stars.
In the outer regions, many stars are grouped into globular
clusters.
Irregular Galaxies
  Irregular galaxies have no specific structure. The
Large and Small Magellanic Clouds, the nearest
galaxies, are an example of irregular galaxies.




   Small Magellanic Cloud   Hoag's Object, a ring galaxy.
Stellar cluster
   A group of stars within
a galaxy which are close
to each other, probably
held together by
gravitational attraction.
They are all in the same
direction from Earth and
the same distance away.
A stellar cluster can
contain from hundreds
to millions of stars.
              Messier 69 a globular cluster, part of the Milky
              Way is 30 000 ly distant and 42 ly across.
Constellations
  A group of stars in a
recognizable pattern that
appear to be near each
other in space. They are in
the same direction from
Earth but are not
necessarily the same
distance away.



                    Orion includes Bellatrix (250 ly);
                    Betelgeuse (640 ly); Rigel (860 ly)
Polaris
The North star
How the stars seem to move
                                    The night sky seems
                                    to rotate around a
                                    point above the
                                    Earth’s axis of
                                    rotation. In 24
                                    hours, it completes
                                    a full circle.


Over the course of a year, the stars are in a slightly different
position each night due to the Earth’s tilt.

Stars which are closer to the Earth also move relative to the
background of more distant stars due to the Earth’s orbit
around the Sun.
Nebulae
                  Nebulous means ‘cloud-like’
Originally, ‘nebula’ was a general name for any extended
astronomical object (the Andromeda Galaxy was referred to as
the Andromeda Nebula before galaxies were discovered by
Edwin Hubble). Nowadays, several different astronomical
objects are known as ‘nebulae’.

A nebula can be an interstellar cloud of dust, hydrogen gas and
plasma. These nebulae are often star-forming regions, such as
the Eagle nebula.

A nebula can also refer to the remains of a dying star, a
planetary nebula (eg Cat’s Eye nebula).

Or it can be a supernova remnant (eg Crab nebula).
Nebulae




Eagle Nebula and the Cone nebula:
       star-forming regions
Supernova remnants


                                  Crab Nebula - supernova remnant




Eta Carinae - supernova remnant
Cat’s Eye Nebula




Planetary nebulae are nebulae that form from the gaseous
shells that are ejected from low-mass giant stars when they
transform into white dwarfs.
Eskimo nebula
Planetary nebula 3000 ly from Earth,
discovered by William Herschel in 1787
a                                                 production


                  MUCH MORE AT
        http://nothingnerdy.wikispaces.com
    http://nothingnerdy.wikispaces.com/E1+INTRODUCTION+TO+THE+UNIVERSE




                                                             32

Weitere ähnliche Inhalte

Was ist angesagt?

Stars galaxies powerpoint
Stars galaxies powerpointStars galaxies powerpoint
Stars galaxies powerpoint
reddonna
 
Dark Matter And Dark Energy
Dark Matter And Dark EnergyDark Matter And Dark Energy
Dark Matter And Dark Energy
Google
 
Moon Formation and Structure
Moon Formation and StructureMoon Formation and Structure
Moon Formation and Structure
Teach5ch
 
Stars & The Solar System
Stars & The Solar SystemStars & The Solar System
Stars & The Solar System
itutor
 

Was ist angesagt? (20)

Gravitational Waves
Gravitational WavesGravitational Waves
Gravitational Waves
 
Gravitation ppt
Gravitation pptGravitation ppt
Gravitation ppt
 
Stars galaxies powerpoint
Stars galaxies powerpointStars galaxies powerpoint
Stars galaxies powerpoint
 
THE UNIVERSE
THE UNIVERSETHE UNIVERSE
THE UNIVERSE
 
Galaxies
GalaxiesGalaxies
Galaxies
 
Formation of the moon
Formation of the moonFormation of the moon
Formation of the moon
 
Galaxy presentation
Galaxy presentationGalaxy presentation
Galaxy presentation
 
Space and time
Space and timeSpace and time
Space and time
 
Dark Matter And Dark Energy
Dark Matter And Dark EnergyDark Matter And Dark Energy
Dark Matter And Dark Energy
 
Moon Formation and Structure
Moon Formation and StructureMoon Formation and Structure
Moon Formation and Structure
 
The Stars And The Galaxies In The Universe 2 L
The Stars And The Galaxies In The Universe 2 LThe Stars And The Galaxies In The Universe 2 L
The Stars And The Galaxies In The Universe 2 L
 
Origin of the universe
Origin of the universeOrigin of the universe
Origin of the universe
 
Big bang cosmology
Big bang cosmologyBig bang cosmology
Big bang cosmology
 
Galaxy
Galaxy Galaxy
Galaxy
 
What Is Red Shift
What Is Red ShiftWhat Is Red Shift
What Is Red Shift
 
Igcse 16-astronomy
Igcse 16-astronomyIgcse 16-astronomy
Igcse 16-astronomy
 
Stars & The Solar System
Stars & The Solar SystemStars & The Solar System
Stars & The Solar System
 
Gravitation, free fall, variation in 'g' and keplers law lecture wise
Gravitation, free fall, variation in 'g' and keplers law lecture wiseGravitation, free fall, variation in 'g' and keplers law lecture wise
Gravitation, free fall, variation in 'g' and keplers law lecture wise
 
Astronomy
AstronomyAstronomy
Astronomy
 
Lunar eclipses
Lunar eclipsesLunar eclipses
Lunar eclipses
 

Ähnlich wie IB Astrophysics - intro to the universe - Flippingphysics by nothingnerdy

Unit 1 - Our Planetary Neighborhood
Unit 1 - Our Planetary NeighborhoodUnit 1 - Our Planetary Neighborhood
Unit 1 - Our Planetary Neighborhood
KCTCS
 
Solar system & constellation(g 4)
Solar system & constellation(g 4)Solar system & constellation(g 4)
Solar system & constellation(g 4)
queeyee
 
Solar system & constellation(g 4)
Solar system & constellation(g 4)Solar system & constellation(g 4)
Solar system & constellation(g 4)
queeyee
 
Thesolarsystem
Thesolarsystem Thesolarsystem
Thesolarsystem
Foo Ling
 
Our Solar System
Our Solar SystemOur Solar System
Our Solar System
Prahlad Pai
 
Science planets ppt
Science planets pptScience planets ppt
Science planets ppt
sesilia_m
 
Space Test Review
Space Test ReviewSpace Test Review
Space Test Review
theMrNeale
 

Ähnlich wie IB Astrophysics - intro to the universe - Flippingphysics by nothingnerdy (20)

E1 - Introduction to the Universe
E1 - Introduction to the UniverseE1 - Introduction to the Universe
E1 - Introduction to the Universe
 
Stellar quantities 2018
Stellar quantities 2018Stellar quantities 2018
Stellar quantities 2018
 
Unit 1 - Our Planetary Neighborhood
Unit 1 - Our Planetary NeighborhoodUnit 1 - Our Planetary Neighborhood
Unit 1 - Our Planetary Neighborhood
 
Solar system & constellation(g 4)
Solar system & constellation(g 4)Solar system & constellation(g 4)
Solar system & constellation(g 4)
 
Solar system & constellation(g 4)
Solar system & constellation(g 4)Solar system & constellation(g 4)
Solar system & constellation(g 4)
 
Thesolarsystem
Thesolarsystem Thesolarsystem
Thesolarsystem
 
Our Solar System
Our Solar SystemOur Solar System
Our Solar System
 
Astronomy.ppt
Astronomy.pptAstronomy.ppt
Astronomy.ppt
 
8. universe and earth ana
8. universe and earth ana8. universe and earth ana
8. universe and earth ana
 
Science and astronomy club (types of celestrial objects)
Science and astronomy club (types of celestrial objects)Science and astronomy club (types of celestrial objects)
Science and astronomy club (types of celestrial objects)
 
Jupiter
JupiterJupiter
Jupiter
 
Solar system
Solar systemSolar system
Solar system
 
Igcse 16-astronomy
Igcse 16-astronomyIgcse 16-astronomy
Igcse 16-astronomy
 
Physices
PhysicesPhysices
Physices
 
Solar system - a powerpoint presentation by Tanisha Pahwa - 5th
Solar system - a powerpoint presentation by Tanisha Pahwa - 5thSolar system - a powerpoint presentation by Tanisha Pahwa - 5th
Solar system - a powerpoint presentation by Tanisha Pahwa - 5th
 
Science planets ppt
Science planets pptScience planets ppt
Science planets ppt
 
Our universe as a whole
Our universe as a wholeOur universe as a whole
Our universe as a whole
 
Day 1 Journet to the light ves 4.pptx
Day 1 Journet to the light ves 4.pptxDay 1 Journet to the light ves 4.pptx
Day 1 Journet to the light ves 4.pptx
 
Dtu10e lecture ppt_ch09 2
Dtu10e lecture ppt_ch09 2Dtu10e lecture ppt_ch09 2
Dtu10e lecture ppt_ch09 2
 
Space Test Review
Space Test ReviewSpace Test Review
Space Test Review
 

Mehr von Nothingnerdy

Mehr von Nothingnerdy (20)

Human sciences introduction no build
Human sciences introduction no buildHuman sciences introduction no build
Human sciences introduction no build
 
What does an it facilitator do?
What does an it facilitator do?What does an it facilitator do?
What does an it facilitator do?
 
IB Sl Physics Sight and Waves Flippingphysics by Nothingnerdy
IB Sl Physics Sight and Waves Flippingphysics by NothingnerdyIB Sl Physics Sight and Waves Flippingphysics by Nothingnerdy
IB Sl Physics Sight and Waves Flippingphysics by Nothingnerdy
 
IB Physics Polarisation flippingphysics by Nothingnerdy
IB Physics Polarisation flippingphysics by NothingnerdyIB Physics Polarisation flippingphysics by Nothingnerdy
IB Physics Polarisation flippingphysics by Nothingnerdy
 
IB Physics Resolution flippingphysics by Nothingnerdy
IB Physics Resolution flippingphysics by NothingnerdyIB Physics Resolution flippingphysics by Nothingnerdy
IB Physics Resolution flippingphysics by Nothingnerdy
 
IB Physics Diffraction flippingphysics by Nothingnerdy
IB Physics Diffraction flippingphysics by NothingnerdyIB Physics Diffraction flippingphysics by Nothingnerdy
IB Physics Diffraction flippingphysics by Nothingnerdy
 
Purely particles - nothingnerdy IGCSE Physics
Purely particles - nothingnerdy IGCSE PhysicsPurely particles - nothingnerdy IGCSE Physics
Purely particles - nothingnerdy IGCSE Physics
 
IB Physics Doppler effect flippingphysics by Nothingnerdy
IB Physics Doppler effect flippingphysics by NothingnerdyIB Physics Doppler effect flippingphysics by Nothingnerdy
IB Physics Doppler effect flippingphysics by Nothingnerdy
 
IB Physics Standing Waves Flippingphysics by Nothingnerdy
IB Physics Standing Waves Flippingphysics by NothingnerdyIB Physics Standing Waves Flippingphysics by Nothingnerdy
IB Physics Standing Waves Flippingphysics by Nothingnerdy
 
Tok science nothingnerdy
Tok science nothingnerdyTok science nothingnerdy
Tok science nothingnerdy
 
Mainly Mains - nothingnerdy igcse physics
Mainly Mains - nothingnerdy igcse physicsMainly Mains - nothingnerdy igcse physics
Mainly Mains - nothingnerdy igcse physics
 
Really radioactive - igcse physics
Really radioactive - igcse physicsReally radioactive - igcse physics
Really radioactive - igcse physics
 
IB Astrophysics - cosmology - Flippingphysics by nothingnerdy
IB Astrophysics - cosmology - Flippingphysics by nothingnerdyIB Astrophysics - cosmology - Flippingphysics by nothingnerdy
IB Astrophysics - cosmology - Flippingphysics by nothingnerdy
 
IB Astrophysics - stellar distances - Flippingphysics by nothingnerdy
IB Astrophysics - stellar distances - Flippingphysics by nothingnerdyIB Astrophysics - stellar distances - Flippingphysics by nothingnerdy
IB Astrophysics - stellar distances - Flippingphysics by nothingnerdy
 
IB Astrophysics - stellar radiation and types - Flippingphysics by nothingnerdy
IB Astrophysics - stellar radiation and types - Flippingphysics by nothingnerdyIB Astrophysics - stellar radiation and types - Flippingphysics by nothingnerdy
IB Astrophysics - stellar radiation and types - Flippingphysics by nothingnerdy
 
Vaguely voltage - nothingnerdy igcse physics
Vaguely voltage - nothingnerdy igcse physicsVaguely voltage - nothingnerdy igcse physics
Vaguely voltage - nothingnerdy igcse physics
 
Chiefly charge - igcse physics
Chiefly charge - igcse physicsChiefly charge - igcse physics
Chiefly charge - igcse physics
 
Deductive logic
Deductive logicDeductive logic
Deductive logic
 
Simple electric circuits
Simple electric circuitsSimple electric circuits
Simple electric circuits
 
Energy, power and climate change
Energy, power and climate changeEnergy, power and climate change
Energy, power and climate change
 

Kürzlich hochgeladen

Gardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch LetterGardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch Letter
MateoGardella
 
Making and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdfMaking and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdf
Chris Hunter
 
Activity 01 - Artificial Culture (1).pdf
Activity 01 - Artificial Culture (1).pdfActivity 01 - Artificial Culture (1).pdf
Activity 01 - Artificial Culture (1).pdf
ciinovamais
 

Kürzlich hochgeladen (20)

Key note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdfKey note speaker Neum_Admir Softic_ENG.pdf
Key note speaker Neum_Admir Softic_ENG.pdf
 
Measures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SDMeasures of Dispersion and Variability: Range, QD, AD and SD
Measures of Dispersion and Variability: Range, QD, AD and SD
 
Ecological Succession. ( ECOSYSTEM, B. Pharmacy, 1st Year, Sem-II, Environmen...
Ecological Succession. ( ECOSYSTEM, B. Pharmacy, 1st Year, Sem-II, Environmen...Ecological Succession. ( ECOSYSTEM, B. Pharmacy, 1st Year, Sem-II, Environmen...
Ecological Succession. ( ECOSYSTEM, B. Pharmacy, 1st Year, Sem-II, Environmen...
 
Nutritional Needs Presentation - HLTH 104
Nutritional Needs Presentation - HLTH 104Nutritional Needs Presentation - HLTH 104
Nutritional Needs Presentation - HLTH 104
 
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 ...
 
PROCESS RECORDING FORMAT.docx
PROCESS      RECORDING        FORMAT.docxPROCESS      RECORDING        FORMAT.docx
PROCESS RECORDING FORMAT.docx
 
Web & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdfWeb & Social Media Analytics Previous Year Question Paper.pdf
Web & Social Media Analytics Previous Year Question Paper.pdf
 
Mehran University Newsletter Vol-X, Issue-I, 2024
Mehran University Newsletter Vol-X, Issue-I, 2024Mehran University Newsletter Vol-X, Issue-I, 2024
Mehran University Newsletter Vol-X, Issue-I, 2024
 
Class 11th Physics NEET formula sheet pdf
Class 11th Physics NEET formula sheet pdfClass 11th Physics NEET formula sheet pdf
Class 11th Physics NEET formula sheet pdf
 
Gardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch LetterGardella_PRCampaignConclusion Pitch Letter
Gardella_PRCampaignConclusion Pitch Letter
 
Accessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impactAccessible design: Minimum effort, maximum impact
Accessible design: Minimum effort, maximum impact
 
Application orientated numerical on hev.ppt
Application orientated numerical on hev.pptApplication orientated numerical on hev.ppt
Application orientated numerical on hev.ppt
 
Mattingly "AI & Prompt Design: The Basics of Prompt Design"
Mattingly "AI & Prompt Design: The Basics of Prompt Design"Mattingly "AI & Prompt Design: The Basics of Prompt Design"
Mattingly "AI & Prompt Design: The Basics of Prompt Design"
 
Making and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdfMaking and Justifying Mathematical Decisions.pdf
Making and Justifying Mathematical Decisions.pdf
 
Introduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The BasicsIntroduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The Basics
 
Basic Civil Engineering first year Notes- Chapter 4 Building.pptx
Basic Civil Engineering first year Notes- Chapter 4 Building.pptxBasic Civil Engineering first year Notes- Chapter 4 Building.pptx
Basic Civil Engineering first year Notes- Chapter 4 Building.pptx
 
Unit-IV- Pharma. Marketing Channels.pptx
Unit-IV- Pharma. Marketing Channels.pptxUnit-IV- Pharma. Marketing Channels.pptx
Unit-IV- Pharma. Marketing Channels.pptx
 
Activity 01 - Artificial Culture (1).pdf
Activity 01 - Artificial Culture (1).pdfActivity 01 - Artificial Culture (1).pdf
Activity 01 - Artificial Culture (1).pdf
 
Sports & Fitness Value Added Course FY..
Sports & Fitness Value Added Course FY..Sports & Fitness Value Added Course FY..
Sports & Fitness Value Added Course FY..
 
Advance Mobile Application Development class 07
Advance Mobile Application Development class 07Advance Mobile Application Development class 07
Advance Mobile Application Development class 07
 

IB Astrophysics - intro to the universe - Flippingphysics by nothingnerdy

  • 1. presents a production INTRODUCTION TO THE UNIVERSE based on the IB Astrophysics option 1
  • 2. INTRODUCTION TO THE UNIVERSE What is there in the Universe? Asteroids and comets Moons Planets Stars Nebulae Stellar clusters Galaxies Galactic clusters
  • 3. The Solar System RELATIVE SIZES: if Sun = 100, Earth =1 ... ... and the distance between them is 10 000 They all orbit the Sun on elliptical paths
  • 4. The Sun Mass: 1.99 x 1030 kg Radius:6.96 x 108 m Surface temperature: 5800 K
  • 5. Planets Data (and Pluto) Planet Picture Distance to the Radius (km) Orbital Orbital Surface Density/ Satellite Sun (km) period period day temp g/cm3 s around its (ºC) water=1 Mercury 58 million 4 878 km axis 59 days 88 days 167 5,43 0 Venus 108 million 12 104 km -243 days 225 days 464 5,24 0 Earth 149,6 million 12 756 km 23, 93 h 365,2 15 5,52 1 days Mars 228 million 6 794 km 24h 37min 687 days -65 3,04 2 Jupiter 778 million 142 800 km 9h 50min 12 years -110 1,32 +63 30s Saturn 1 427 million 120 000 km 10h 14min 29,5 years -140 0,69 +56 Uranus 2 870 million 51 800 km 16h 18min 84 years -195 1,27 27 Neptune 4 497 million 49 500 km 15h 48min 164 years -200 1,77 13 Pluto 5 900 million 2 400 km 6 days 248 years -225 2 1
  • 6. Mercury and Venus The rocky planets closest to the Sun
  • 7. Earth and Moon Mariner 10 Many planets have moons which orbit the planet (which orbits the Sun)
  • 8. Mars The fourth of the inner planets Spirit Rover: Mars’ West Valley
  • 9. Asteroid Belt Ceres (480km): it was the first asteroid to be seen. Now it’s a dwarf planet. Mathilde (52km) Eros (13x13x33km)
  • 10. Jupiter The largest gas giant, 5 times more distant from the Sun than the Earth Jupiter and its moons: Io, Approximate size comparison Europa, Ganymede and Callisto of Earth and Jupiter
  • 11. Saturn Nearly twice as far from the Sun as Jupiter A rough comparison of the sizes of Saturn and Earth
  • 12. Uranus Twice as far from the Sun as Saturn Size comparison of Earth and Uranus
  • 13. Neptune Nearly twice as far from the Sun as Uranus (30 times further than Earth) Size comparison of Neptune and Earth.
  • 14. Astronomical units of distance The Astronomical Unit (AU) – this is the average distance between the Earth and the Sun. 1 AU = 150 000 000 km = 1.5x1011m
  • 15. Astronomical distances The light year (ly) – this is the distance travelled by light in one year. c = 3x108 m/s t = 1 year = 365.25 x 24 x 60 x 60= 3.16 x 107 s Speed =Distance / Time Distance = Speed x Time = 3x108 x 3.16 x 107 = 9.46 x 1015 m 1 ly = 9.46x1015 m
  • 16. Relative distances The Moon is 1.3 light seconds from the Earth The Earth is 500 light seconds from the Sun The nearest star to the Sun is about 4 light years away The diameter of a galaxy is about 100 000 light years The distance between galaxies is about 1 000 000 light years
  • 17. Galaxies A galaxy is a collection of a very large number of stars (around 100 thousand million) mutually attracting each other through the gravitational force and staying together. The number of stars varies between a few million and hundreds of billions. There are approximately 100 thousand million galaxies in the observable universe. There are three types of galaxies: - Spiral (Milky Way) - Elliptical (M49) - Irregular (Magellanic Clouds)
  • 18. Spiral Galaxies Spiral galaxies consist of a rotating disk of stars along with a central bulge of generally older stars. Extending outward from the bulge are relatively bright arms. There is a supermassive black hole at the centre. The dark patches in the picture is interstellar dust. Milky Way
  • 19. Spiral Galaxies Andromeda galaxy is the closest large galaxy to Earth. It covers about the same area of the night sky as the Moon but is much dimmer.
  • 20. Spiral Galaxies Sombrero Galaxy
  • 21. Elliptical Galaxies M49 ESO 325-G004 Elliptical cross-section and no spiral arms. They range in shape from nearly spherical to highly flattened ellipsoids and in size from hundreds of millions to over one trillion stars. In the outer regions, many stars are grouped into globular clusters.
  • 22. Irregular Galaxies Irregular galaxies have no specific structure. The Large and Small Magellanic Clouds, the nearest galaxies, are an example of irregular galaxies. Small Magellanic Cloud Hoag's Object, a ring galaxy.
  • 23. Stellar cluster A group of stars within a galaxy which are close to each other, probably held together by gravitational attraction. They are all in the same direction from Earth and the same distance away. A stellar cluster can contain from hundreds to millions of stars. Messier 69 a globular cluster, part of the Milky Way is 30 000 ly distant and 42 ly across.
  • 24. Constellations A group of stars in a recognizable pattern that appear to be near each other in space. They are in the same direction from Earth but are not necessarily the same distance away. Orion includes Bellatrix (250 ly); Betelgeuse (640 ly); Rigel (860 ly)
  • 26. How the stars seem to move The night sky seems to rotate around a point above the Earth’s axis of rotation. In 24 hours, it completes a full circle. Over the course of a year, the stars are in a slightly different position each night due to the Earth’s tilt. Stars which are closer to the Earth also move relative to the background of more distant stars due to the Earth’s orbit around the Sun.
  • 27. Nebulae Nebulous means ‘cloud-like’ Originally, ‘nebula’ was a general name for any extended astronomical object (the Andromeda Galaxy was referred to as the Andromeda Nebula before galaxies were discovered by Edwin Hubble). Nowadays, several different astronomical objects are known as ‘nebulae’. A nebula can be an interstellar cloud of dust, hydrogen gas and plasma. These nebulae are often star-forming regions, such as the Eagle nebula. A nebula can also refer to the remains of a dying star, a planetary nebula (eg Cat’s Eye nebula). Or it can be a supernova remnant (eg Crab nebula).
  • 28. Nebulae Eagle Nebula and the Cone nebula: star-forming regions
  • 29. Supernova remnants Crab Nebula - supernova remnant Eta Carinae - supernova remnant
  • 30. Cat’s Eye Nebula Planetary nebulae are nebulae that form from the gaseous shells that are ejected from low-mass giant stars when they transform into white dwarfs.
  • 31. Eskimo nebula Planetary nebula 3000 ly from Earth, discovered by William Herschel in 1787
  • 32. a production MUCH MORE AT http://nothingnerdy.wikispaces.com http://nothingnerdy.wikispaces.com/E1+INTRODUCTION+TO+THE+UNIVERSE 32

Hinweis der Redaktion

  1. \n
  2. \n
  3. \n
  4. \n
  5. \n
  6. \n
  7. \n
  8. \n
  9. \n
  10. \n
  11. \n
  12. \n
  13. \n
  14. \n
  15. \n
  16. \n
  17. \n
  18. \n
  19. \n
  20. \n
  21. \n
  22. \n
  23. \n
  24. \n
  25. \n
  26. \n
  27. \n
  28. \n
  29. \n
  30. \n
  31. \n
  32. \n