From the December 2011 issue

How do astronomers determine what causes starlight to shift toward the red end of the electromagnetic spectrum?

Ron Barnes, St. Louis, Missouri
By | Published: December 27, 2011
Galaxies in HUDF
Astronomers know the galaxies in the Hubble Ultra Deep Field are redshifted because of the expansion of the fabric of the universe itself. HUDF WFC3/IR
Reddened starlight can come from a few different sources. (1) When a star moves away from us through pre-existing space, its spectral lines (which show characteristic patterns) are shifted to longer wavelengths, or “redshifted.” This is the common Doppler effect; a familiar version on Earth occurs when we hear a siren (or train) moving away from us, which lengthens the wavelengths and makes a lower sound.

(2) When the spectra of distant galaxies are redshifted, it’s due to the expansion of the fabric of the universe itself. As space expands, electromagnetic waves from celestial sources become longer (or redder). We can tell this effect is at play because galaxies’ surface brightnesses (their brightness per unit area) decrease with increasing redshift in a way that’s consistent with the expansion of space, but not with the Doppler effect. The more distant a galaxy, the farther back in time we see it. The redshifts of galaxies are proportional to their distance, which is caused by the expansion of the universe itself, not because the light becomes “tired” and loses energy with time.

(3) When light from a star passes through gas and dust on its way to an observer, the intervening material can scatter the light out of the line of sight, causing the star to look dimmer. Because blue wavelengths are scattered much more efficiently than red ones (that’s why our sky looks blue during daylight), a star looks redder than it should. Dust also absorbs blue light more than red, making the star appear even redder. The overall effect is called “interstellar reddening,” and it is similar to the reason the setting Sun looks progressively more yellow, orange, or even red as it gets closer to the horizon. In the interstellar reddening effect, there is no redshift.

If we look at a star’s (or galaxy’s) spectrum, we can tell which method is responsible for making that object appear redder. — Alex Filippenko, University of California, Berkeley