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The Milky Way Galaxy. Greeks called the hazy band of light around the sky ‘galaxias kuklos’ – milky circle Romans called it ‘via lactia’ – milky road, or milky way But what is it? By the mid-18 th century, astronomers new that it was made up of an enormous number of distant stars. - PowerPoint PPT Presentation
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The Milky Way Galaxy
• Greeks called the hazy band of light around the sky‘galaxias kuklos’ – milky circle• Romans called it ‘via lactia’ – milky road, or milky way• But what is it?• By the mid-18th century, astronomers new that it was made up of an enormous number of distant stars
• 1785: William and Caroline Herschel try to map out the distribution of stars: published the ‘Grindstone model’ – the Sun at the center ofAn irregularly shaped disc of stars
The Sun
•1922: Jacobus Kapteyn’s model The Sun
•Harlow Shapley: noticed that although open clusters were randomly scattered about the sky, globular clusters were concentrated in the direction of Sagittarius
• Therefore center of oursystem of stars must besomewhere towards Sagittarius
• Previously, astronomers had thought that galaxy was much smaller and that we were near the center because they did nottake into account the dimming of light from stars
•The Disk: - Contains most stars and dust - Contains most GMCs, so most star formation takes place in disk - Contains all open clusters, a few million to a billion years old - By proportion, the disk is thinner than a pizza crust (not deep dish!)
•The Halo: - Contains about 200 globular clusters, average age of 11 billion years
• Spiral Arms: - Long spiral patterns of bright stars, HII regions, star clusters, gas and dust - Sun is located on inner edge of one
• Galactic year: - The galaxy is rotating: our solar system takes 225 – 250 million years to orbit the galactic center
Differences between disk stars and halo stars
• Astronomers define metals to be any elements that are not H or He• Population I stars are metal rich (2 to 3% of their mass is metals)• Population II stars are metal poor (0.1% metals)• Population I stars are located in the disk, population II stars in the halo• Population II stars must be very old – the gas clouds they were formed out of were not enriched with metals by supernovae of previous stars
Finding Spiral Arms: 21cm Radiation
Mass of the Milky Way
• From Kepler’s third law, mass of galaxy is about 400,000,000,000 MSun
We seem to be missing about 90% of the mass of the galaxy!- Most of it cannot be emitting or absorbing light- Astronomers name it Dark Matter
Center of the Milky Way
