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Certificate programme in Science: Astronomy Core Module 4 Cosmology

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Title: Certificate programme in Science: Astronomy Core Module 4 Cosmology


1
Certificate programme in Science Astronomy (Core
Module 4)Cosmology
  • Dr Lisa Jardine-Wright,
  • Institute of Astronomy, Cambridge University

2
Lecture Overview
  • Jones Lambourne
  • Chapters 6.6 8.5
  • Cosmology A Very Short Introduction
  • Peter Coles
  • Structure Formation
  • Cosmic structures
  • Galaxy clusters
  • Filaments superstructures
  • Voids
  • Cosmic web
  • Gravity!

3
Cosmic Structures
  • Patterns in space
  • APM survey - contains positions, magnitudes,
    sizes and shapes for about 3 million galaxies

4
Cosmic Structures
  • Patterns in space
  • CfA galaxy survey

5
AAO
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Cosmic Structures
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11
Cosmic Structures
  • Galaxy Clusters
  • Vary in size and richness
  • Milky Way is part of the local group - only other
    large galaxy M31

12
http//www.astro.uu.se/ns/local_group.html
13
Cosmic Structures
  • Galaxy Clusters
  • Vary in size and richness
  • Milky Way is part of the local group - only other
    large galaxy M31
  • Rich Clusters / Abell Clusters
  • 100s to 1000s of galaxies per Million Light Years
  • E.g. Virgo Coma

14
Virgo Cluster
http//www.star.ucl.ac.uk/apod/apod/
15
Coma Cluster
http//antwrp.gsfc.nasa.gov/apod/
16
Cosmic Structures
  • Galaxy Clusters
  • Vary in size and richness
  • Milky Way is part of the local group - only other
    large galaxy M31
  • Rich Clusters / Abell Clusters
  • 100s to 1000s of galaxies per Million Light Years
  • E.g. Virgo Coma
  • Greyscale of sizes between these two extremes.
  • Density defines bound and unbound structures
  • Unbound are purely statistic\al

17
Cosmic Structures
  • Galaxy Clusters
  • Vary in size and richness
  • Milky Way is part of the local group - only other
    large galaxy M31
  • Rich Clusters / Abell Clusters
  • 100s to 1000s of galaxies per Million Light Years
  • E.g. Virgo Coma
  • Greyscale of sizes between these two extremes.
  • Density (through gravity) defines bound and
    unbound structures
  • Unbound are purely statistical

18
Cosmic Structures
  • Filaments Superstructures
  • 300 M Lt yrs

19
http//www.astro.princeton.edu/rhl/PrettyPictures
/
20
http//www.astro.princeton.edu/mjuric/universe/
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Voids
http//lepus.physics.ualr.edu/tahall/FINAL/Week1.
htm
30
Voids
http//www.astro.uni-bonn.de/mhetter/index.php?in
dex1
31
Cosmic Web
32
Cosmic Structures
  • Gravitational Instabilities

33
Analysing the Fluctuations
34
Dark Matter and Fluctuations
Galaxy Halo Scales
35
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