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International Astronomical Union / Office of Astronomy for Development Kevin Govender – [email protected] J.-C. Mauduit – [email protected] OAD www.astro4dev.org IAU: International Astronomical Union NRF: National Research

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Page 1: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

International Astronomical Union / Office of Astronomy for Development

Kevin Govender – [email protected]

J.-C. Mauduit – [email protected]

OAD

www.astro4dev.org

IAU: International Astronomical Union

NRF: National Research Foundation

Page 2: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Dr. Jean-Christophe MauduitIAU Office of Astronomy for Development

From planets to superclusters of galaxies

The different scales of the Universe

National Research Foundation

Page 3: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

From the Solar system to the Milky Way…

Page 4: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 5: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 6: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The blue planet: Earth

Radius ~ 6 378 km Atmosphere < 600 km

Troposphere < 15 km

Page 7: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

From the Earth to the Moon

Earth-Moon distance: 384 401 km

30 Earth planets one after the other

~ 2 months of high speed train

Apollo missions : less than 2 days

(Speed of ~ 8000 km/h to ~ 40 000 km/h)

Page 8: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Space shuttle take-off

Page 9: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 10: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The crescent Earth from the Moon

Page 11: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

You are here !

As imaged from the red planet, Mars

Page 12: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Our star, the Sun

Characteristics:

Radius~ 695,000 km

Mass = 1.9891×1030 kg

Volume = 1.41×1018 km³

Luminosity = 3.827×1026 W

Comparison to Earth:

109 × Earth

332 950 × Earth

1 300 000 × Earth

9.15 × 1016 tons of TNT / s

Page 13: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Distances in the Solar system

The astronomical unit (A.U.) is the Earth-Sun distance :

1 A.U. = 149 597 871 km

Voyager,The furthest probe sent by humans is at 12,5 billion kilometres of the Earth, hence 82 A.U. of us…

Sun 0 109

Mercury 0,39 0,38

Venus 0,72 0,95

Earth 1,0 1,00

Mars 1,5 0,53

Jupiter 5,2 11

Saturn 9,5 9

Uranus 19,2 4

Neptune 30,1 4

Pluto 39,5 0,18

MassDistance

Page 14: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 15: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 16: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 17: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 18: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 19: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 20: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 21: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The Solar system, as seen from the Voyager probe

Credits : Sonde Voyager

Page 22: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The speed of light

The Sun is at~ 8 light-minutes

The Voyager probe is at ~ 12 light-hours

c ~ 300 000 km/s

Light-minutes Astronomical Units

Average planet distances to the Sun

1 Light-year = 63240 Astronomical Units = 9,46 x 1012 km

Page 23: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The stars in the sky are similar to our Sun

But so far away that we see them as points of light

Page 24: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

• Located at 4.22 Light-year from the Sun.

• Its light takes about 4 years to reach us

Proxima Centaurus,The closest star from our Sun

Page 25: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Stars sometimes form clusters

Messier 3 (M3) Star cluster

D (Sun– M3) ~ 34 000 light years

Page 26: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 27: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Before AfterThe Milky Way

The city sky

Page 28: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 29: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

A little geography of our Milky Way

Page 30: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Magellanic cloudsGalactic bulbSpiral arms

The Milky Way, as seen from the inside

Two satellite galaxies of the Milky Way

Page 31: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The extragalactic domain

Page 32: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The extragalactic « nebulae »

M75

Star clusters belong to our

Galaxy

M32 M101

But these other diffuse objects are

galaxies

Page 33: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Voie LactéeVoie Lactée

Petit nuage de Magellan

Grand nuage de Magellan

Voie Lactée

Petit nuage de Magellan

Grand nuage de Magellan

Voie Lactée~ 160 000 l.y.~ 2.5 million l.y..

~ 200 000 l.y.

Page 34: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Our greatest neighbor, the “Andromeda” galaxy

D (Milky Way – M31) ~ 2.5 million l.y.r ~

50000 l.y.

Page 35: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

M31 fait partie du groupe “ Local ” de galaxies …

1 Million Light Years

Our Galaxy

Page 36: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

From Earth…

To the Local Group of galaxies

Page 37: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

M74 : 30 million l.y.

Page 38: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Sombrero : 40 million l.y.

Page 39: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 40: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 41: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

A compact group

500 000 l.y.

Hickson compact group 79

Page 42: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Virgo cluster

At ~ 60 Million Light Years

10 million l.y.

Page 43: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The large-scale structure of the Universe

Page 44: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 45: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Abell cluster 1689

10 million l.y.

Page 46: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Hubble Ultra-Deep Field

How many galaxies on this image?

!

Page 47: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

2D view of galaxies in the sky as observed in infrared

… to the large-scale structure of the Universe

From the Perseus cluster…

Page 48: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

~ 1 B

illion l.y

.

Large galaxy surveys generally focus on small portions of the sky

Page 49: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

3D Diagram

~ 163 million l.y.

Scale:

100 Million l.y.

~ 26

0 M

illion

s l.y

.

The local group of galaxies within the local supercluster

Page 50: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The most distant galaxies ever observed

~ 11 Billion years

Page 51: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The “most distant” picture of the Universe at its “youngest”

Page 52: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

The “beginning” of the Universe

Page 53: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 54: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Thank you!

Page 55: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Vidéos et Images d’astronomie

Page 56: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Loi de Hubble (1929)

v= H0 d

Edwin Hubble

Galaxie proche :

Galaxie distante :

Page 57: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 58: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

From the ground

From space

M51 and its companion

Pairs of galaxies

Page 59: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

In this computer simulation, one can see the formation of the large scale structures of the Universe

Page 60: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 61: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 62: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 63: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD
Page 64: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Groupe de galaxies : des galaxies en intéraction ?

Du visible … à la radio !

Page 65: International Astronomical Union / Office of Astronomy for Development Kevin Govender – kg@astro4dev.org J.-C. Mauduit – jcm@astro4dev.org OAD

Elliptiques

Spirales

Les différents types de galaxies

simples

barrées