Comet Tails 

 
Comet tails come in two flavors: the ion tail and the dust tail.

The ion tail is thin, blue and linear - points directly away from the Sun.

The dust tail is white, broad and points generally (but not precisely) away from the Sun

What is happening?
 
 

Physics of the Ion Tail

The ion tail is made up of ions (surprise!) - mostly CO+, N2+, CO2+.  As the comet comes into the inner solar system, the Sun's radiation heats up the nucleus, "boiling off" and ionizing these gases.

These ions are electrically charged particles, and interact with the sun's solar wind (charged particles coming from the sun). The interaction between the comet and the solar wind distorts magnetic field lines, causing a cometary magnetotail which points away from the Sun. The charged ions stream along the magnetic field lines in the magnetotail, so the ion tail always points away from the Sun.

CO+ absorbs sunlight and flouresces, emitting energy at a wavelength of 4200 Angstroms, which is blue light.


Physics of the Dust Tail

The dust is not necessarily charged -- why should the dust tail point away from the Sun?

I. Radiation Pressure

II. Solar wind collisions


Both radiation pressure and solar wind collisions are less effective at pushing on dust particles than magnetic fields are at containing ions, so the dust tail is broader than the ion tail, and it is not as precisely aligned away from the Sun as the ion tail is.

Finally, the dust tail reflects sunlight, so it appears yellow/whitish in color.