We can estimate the mass of the central black hole in the Milky Way by measuring the orbital speeds of stars near it.
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Q1: A dwarf galaxy is currently being ripped
Q2: The Milky Way has lived out its
Q3: Stars in the halo are most easily
Q4: The Milky Way has two major spiral
Q6: Halo stars formed before the Milky Way
Q7: Our galaxy is classified as an Sd
Q8: Globular clusters have much higher stellar densities
Q9: The Milky Way is like most other
Q10: The locations of globular clusters on the
Q11: Our galaxy is a typical barred spiral
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