Julian Date: 2459095.16
2020-2021: III
THE DAILY ASTRONOMER
Wednesday, September 2, 2020
Remote Planetarium 81: Galactic Survey I
Today and tomorrow we're going to conduct a thorough survey of our Milky Way Galaxy. We can pretend that we've been granted a 100 million year life span and have to figure out ways to spend all that time by composing a galactic travel itinerary. What to see. What to avoid. What to admire from a great distance. In a sense we will be roaming through the Milky Way Galaxy over the next few courses. What will we encounter?
The Supermassive Black Hole in the nucleus:
A very good object to avoid! Tucked away in the galactic nucleus is a supermassive black hole about four million times more massive than our Sun. While not visible optically owing to the intervening gas and dust clouds within the 26,000 light years of space separating it from us, the central black hole is detectable as a powerful radio source dubbed Sagittarius A*. Astronomers have determined its diameter to be about equal to 60 million kilometers. Scientists were able to estimate its mass by measuring the velocities of stars within its vicinity. As we learned yesterday in our dark matter discussion, stellar velocities are determined by the mass of the material surrounding the stars. While life tends to be placid out here on our spur, the region surrounding this black hole is a sight of furious activity. It is likely every elliptical and spiral galaxy contains such a supermassive black hole at their cores. We would be well advised to avoid them, as well.
Major Spiral Arms:
The Milky Way Galaxy is a barred spiral, meaning that its center consists of a bar from which protrudes a series of curling spiral arms. The four major arms are:
- Norma
- Sagittarius
- Scutum-Centaurus
- Perseus
Yes, that is correct. Each arm is named for a different constellation that defines the region these arms seem to occupy. Our Sun is actually located on a minor arm, the Orion-Cygnus. More specifically, the Sun is located within the Orion spur, an offshoot arm of stars approximately 2/3 out from the nucleus. Spiral arms contain the densest collections of stars, gas and dust. Here one will encounter most of the star formation as gaseous nebulae condense to create new stars from the galactic material. Astronomers estimate that 5 - 8 stars are formed each year within the Milky Way.
Galactic Halo:
We recognize three main parts of the galactic halo, the spherical region surrounding the nucleus:
- Stellar Halo the halo containing the "metal poor" stars within the globular clusters. These globe-shaped clusters -hence the name- contain some of the oldest stars that are deficient in heavier elements as they formed from material that wasn't as chemically enriched as the matter from which the Sun was made. Up to one percent of the galaxy's mass is contained within his halo, which extends up to 100 kiloparsecs (100,000 parsecs) from the nucleus. According to the most recent census, the halo contains about 150 - 200 globular clusters
- Galactic corona a region of hot ionized gases within the galactic halo. This rarefied region is likely replenished by cataclysmic events such as supernovae in and around the galactic nucleus. These "bubbles" travel up as though a chimney in this corona before being disseminated through the disc region.
- Dark matter halo a vast region that might encompass the entire galaxy. This DMH is hypothetical as dark matter has not yet been observed. However, as we discussed yesterday, the surprisingly rapid stellar motions within the galaxy's outer regions might be explicable by the presence of such a halo.
We conclude our survey tomorrow...
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