Milky Way - Observations
Andrew Conway
Galaxies are faint
Copyright: 20th Century Fox
Clustering
- Quarks and electrons are fundamental (?)
- Quarks make up protons and neutrons
- Protons, neutrons and electrons make up atoms
- Atoms make up molecules
- Molecules make up solids, liquids and gases
- Gases make up stars
- Stars make up galaxies
- Galaxies make up galaxy clusters
- Galaxy clusters make up super-clusters
Our galaxy - the Milky Way
- Several hundred billion stars.
- Mass is about a thousand billion solar masses.
- About 100,000 light years in diameter.
- Oldest known star is 13.6 billion years old.
- Appears as a faint, fuzzy band encircling the Earth.
Observing hydrogen
- Our galaxy contains many gas clouds mainly composed of hydrogen.
- Hydrogen emits radio waves at a wavelength of 21 cm.
- We can use this line to find hydrogen clouds and map out our galaxy.
- And, we can measure the speed at which they move towards or away from us (the Doppler effect, see earlier).
Dark matter
- The graph shows the speed of rotation at different distances from the centre of the galaxy
- 1 kpc = 1000 parsecs = 3260 light years.
- The red curve is the theory based on mass we can see in the galaxy.
- The blue curve are the observations (with error bars).
- The fact that they are different means there is mass we cannot see - dark matter.
Satellite galaxies?
- The LMC and SMC are dwarf galaxies passing the Milky Way.
- It was previously thought they orbited the Milky Way.
- The LMC is 160,000 light years away.
- The SMC is 200,000 light years away.