Ch. 8 – Characterizing Stars

part 3:

The Hertzsprung-Russell DiagramLuminosity Classes

Spectral Types

The Hertzsprung-Russell Diagram

• We will plot stars on a chart which has temperature on the horizontal axis and the luminosity on the vertical axis.

• Named after two astronomers who made this type of plot in the 1920’s.

• Use units of solar luminosity and Kelvin

H–R Diagram of Well-Known Stars

Notice the luminosity is a special kind of scale

called a logarithmic scale, in powers of ten.

The temperature is plotted in reverse:

hot on the left, cooler on the right.

H–R Diagram of Nearby Stars

Now this shows the Main Sequence of stars that are in the shaded region.

Stellar size is indicated by the diagonal lines. (These dotted lines are a result of the luminosity-radius-

temperature equation).

H–R Diagram of the 100 Brightest Stars

This is biased in favor of giants, which are

very luminous, so we see all the giants in a large volume of

space, and don’t see the smaller stars in

such a large volume. As a result, very few smaller stars show

up on this plot.

Hipparcos H–R Diagram

This is a more representative set of

stars for a plot like this.

Determination of Stellar Distances by different methods:

Spectroscopic parallax is really a misnomer, it is not a direct measurement, but empirical, based on a statistical estimate, the most likely

distance for a star based on luminosity and color.

Luminosity class is an additional criterion, based on spectral line width and its correlation to gas pressure in the star’s photosphere.

We get several types of stars, listed in the Table on Stellar Luminosity Classes.

Spectra vary according to temperature.

Stellar luminosity and spectral type

can be used to characterize stars

rather than use the luminosity and

temperature.

Visual binary stars

Stellar masses can be determined most easily in Binary Stars.

Kruger 60

Spectroscopic binary stars

Binary Spectra have line shifts due to the Doppler effect.

Orbital periods and the velocities can be plotted vs. time.

Eclipsing binary stars

Binary Light Curves sometimes indicate a transiting companion.

Stellar massesdetermine a star’s position along the main sequence, more than other properties do.

Stellar Mass Distribution

for some nearby stars.

Giants are rare.

Stellar Radii and Luminosities:

Radius is proportional to mass

Luminosity is proportional to (mass)4

Main sequence stars show some trends:

The small mass stars tend to be cooler and so they burn hydrogen more slowly in their core. Hence they have longer lives, in some cases,lives that will be much longer than the present age of the Universe (trillions of years).