The Structure of the Milky Way - PowerPoint PPT Presentation

1 / 15
About This Presentation
Title:

The Structure of the Milky Way

Description:

Begin with properties of globular star clusters (crucial for mapping out the galaxy) ... They are too far away (think of the theodolite lab). You need another method. ... – PowerPoint PPT presentation

Number of Views:61
Avg rating:3.0/5.0
Slides: 16
Provided by: StevenS49
Category:

less

Transcript and Presenter's Notes

Title: The Structure of the Milky Way


1
The Structure of the Milky Way
What is the size and shape Of the system of stars
in which We live?
2
Outline of lecture
  • Lecture taken from Chapter 22
  • Skip material on interstellar gas
  • Skip historical stuff
  • Begin with properties of globular star clusters
    (crucial for mapping out the galaxy).

3
Globular clusters and why they are important in
this context
  • Big balls of about 100,000 stars
  • You can see them at great distances
  • About 150 cataloged
  • They are unevenly distributed in the sky (great
    summertime objects, few in the winter). (Figure
    22.25)

1/5 of globular clusters In 2 of the sky
4
Distribution of globular clusters on the sky
implies a distribution in space like Figure 22.26
5
Where (on the sky) is the galactic center?
  • In Sagittarius
  • RA 17h45m
  • DEC-28.3 degrees
  • Position on SC1 Chart

6
You cant determine the distances to globular
clusters by parallax. They are too far away
(think of the theodolite lab). You need
another method. If you know the absolute
magnitude M of an object and can measure the
apparent magnitude m, you know the distance.The
distance modulus (m-M) is a direct measure of the
distance.
7
Object of choice Cepheid Variables (after Delta
Cephei)
  • Cepheid variables vary in brightness periodically
  • Periods range from a couple of days to 100 days.
  • Absolute magnitude dependent on period

8
Distances to globular clusters and the galactic
center
  • 1 parsec 3.26 light years
  • Need bigger yardsticks for these objects
  • 1000 parsecs1 kiloparsec3260 light years
  • Distance to galactic center 8.5 /- 0.50
    kiloparsecs

9
How far is 8.5 kiloparsecs?
  • Let 1 au 1cm
  • Nearest star (1.3 parsecs) 2.68 km 1.66 miles
  • 8.5 kiloparsecs 17,532 km 10,870 miles (2.74
    Earth radii)
  • Light signal transmitted from the GC would take
    27,700 years to reach us

10
A view of the galactic center (visible only at
radio wavelengths)
11
New Coordinates galactic coordinates
  • imaginary lines on the sky
  • A line through the middle of the Milky Way
    galactic equator
  • 0 degrees galactic longitude in direction of the
    galactic center
  • Coordinates are galactic latitude and longitude

12
Galactic coordinates
13
Observations indicate the shape and size of the
Milky Way Galaxy
14
Structure of the Milky Way
  • Disk
  • Bulge
  • Galactic center
  • Galactic halo

Question what simple observation Is consistent
with a part of this picture
15
A view of the Milky Way with an artists touch
Write a Comment
User Comments (0)
About PowerShow.com