Themes > Science > Physics > Astrophysics > Introduction to Astrophysics > Properties of Stars > Temperature of the Sun


( and Spectral Classification)

We will first discuss how one goes about determining the temperature of the Sun (and also how one goes about determining the temperatures of stars in general). We will talk about

  • methods which use the continuous emission from the Sun
  • methods which use spectral lines (which will necessitate a discussion of some of the ideas of atomic physics).

But before I go on, let me make some remarks about a few bits of background information (e.g., what is light? (reprise), what do I mean by continuous emission, what do I mean by spectral lines?)

What is Light?

This is actually a fairly profound question and so I will not delve too deeply into the issues but rather I will simply point out some interesting aspects of light and some of the questions that we have about light (today)?

Earlier I noted that light (EM radiation) has wave-like properties. However, there are also experiments where we find that light has particle-like properties. The gist of the issues concern this duality in the nature of light. It is a problem because waves are things are spread out in space, while particles are like BB's. There are some nice experiments which bring these points home.


The interesting is that light will behave like a wave when it shines upon a single slit or a double slit. That is, it doesn't act like a stream of particles (although I note an interesting point later).

Planck was only able to understand the results of the experiments by making the radical assumption that the light came in discrete bundles of energy of size

Energy = h x f = h x c / W

where h is known as Planck's constant, W is the wavelength of the radiation, f is the frequency of the wave, and c is the speed of light. Note that f x W = c. These packets of light (energy) are referred to as

photons.

A wave can have any energy, and so this notion is foreign to a wave. There are other examples of experiments where light behaves as a discrete particle rather than as a smoothly varying, spread-out wave, e.g., in the Photo-electric Effect. where some threshold for the ejection of particles seems to exist.

In this experiment, the low intensity beam of radiation seems to interact with the screen discretely (one at a time), i.e., like a particle. However, if we wait long enough, the pattern which gets built up on the screen is the one predicted by wave mechanics, and so the light also seems to behave like a wave,

Light cannot simultaneously be both a wave and a particle. However, we note that we can make some comments about how light behaves. What apparently is happening is that light seems to travel through space (propogate through the Universe) as if it were a wave, but when it comes time for the light to interact with matter (exchange energy and momentum with matter), it seems to behave as a particle in that it exchamges energy and momentum in discrete chunks. This is apparently true and what it is telling us is that light may be something other than a wave or a particle (something which we don't know about).


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