# What does a hot, optically thin gas *look* like?

In another question I tried to answer what a sample of the Sun's photosphere or core would look like, if it could be brought into the lab.

Here is a broader question - if I have a small inert container of gas in local thermodynamic equilibrium, that has the solar photospheric composition and photospheric density ($\sim 10^{-9}$ g/cm$^3$ -i.e. it will be optically thin for a small lab sample), what would it look like (to the human eye) and how would it change as I cranked up the temperature from say 1000K through the solar photospheric temperature to say as high as 100,000K?

EDIT: Just as a steer - I know it will look nothing like a blackbody - that is why I am interested in it and why I emphasize the optically thin nature of the problem.

• Wikipedia says photospheric density is approximately 2E-4 kg/m^3. I think 100g/cc of stuff at 4500-6000K would be relatively opaque due to the dynamic range of the eye alone. Dec 15 '14 at 2:16
• We define the sun's surface as the point where it becomes optically thick. However, we know the entire thing is a giant ball of ionized gas and has no solid surface. We only see the corona due to Thomsen scattering of photons off the electrons. So if the gas is optically thin, how would you "see" it? Have I missed something? Jan 1 '15 at 15:51
• @honeste_vivere Optically thin simply means that the optical depth is much less than 1 so that emitted photons leave the gas without further interaction. e.g. The corona is not only seen by Thomson scattering (and very few escaping white light photons interact in this way) it is seen via optically thin (X-ray) emission from a $>10^6$K plasma. Jan 1 '15 at 15:59
• @RobJeffries - Ah, I understand now. I was inappropriately assuming by "look like" you meant what one could see with the naked eye. If you meant what is measurable then that is different, as you correctly state. Haven't astronomers gone through all sorts of emissivity calculations for optically thin gases? Jan 1 '15 at 17:05
• @honeste_vivere I do mean what you could see with the naked eye. What is the optical appearance of an optically thin gas at a range of temperatures. For example I know there are some highly excited iron ion optical transitions that could be seen in 1 million degree gas, but I am interested in more modest temperatures. Jan 1 '15 at 17:39