<<

Spiral like the and Andromeda Edge on and face on

L of Milky Way ~ few x 10 10 Lsun SDSS image by D. Hogg The Sombrero 12 kpc 40,000 light years

Cartoon of the edge‐on Milky Way galaxy Palomar 5 M5

M13 M15

Images of globular clusters (GCs) (Sloan Digital Sky Survey) Dwarf Galaxy A galaxy that has 1/10 or fewer the number of in a Milky Way sized galaxy Dwarf galaxies

Halo of dark maer 250 kpc 800,000 LY

Large Magellanic cloud Wei‐Hao Wan, UH image credit (Giant) ellipcal galaxies

This type of galaxy is oen found at the centers of galaxy clusters

Ellipcal galaxies have relavely less gas, dust, and formaon than spiral galaxies.

They look redder because the ages of their stars are on average older than the stars in a It is believed that a 2 billion solar mass black hole lives at the center of M87. Electrons accelerang along the strong magnec field near the black hole produce this jet of light and charged parcles. Irregular galaxies forming lots of stars and/or interacng with other galaxies

Large Magellanic Cloud – luminosity ~ 1/10 luminosity of the Milky Way The Mice Galaxies Many galaxies live in clusters or groups

Hickson Group 87 Image taken at Gemini South Abell Cluster S0740 Image was obtained with the Map of the Of Galaxies A dozens of dwarf galaxies and 2 giant spirals (the Milky Way and Andromeda) NGC 205 image credit: www.noao.edu ~ 1/40 Milky Way luminosity Image credit: David W. Hogg, Michael R. Blanton, and the Sloan ~ 1/300 Milky Way Digital Sky Survey Collaboraon luminosity Image credit: David W. Hogg, Michael R. Blanton, and the Sloan ~ 1/2700 Milky Way Digital Sky Survey Collaboraon luminosity