Researchers have developed a new technology that can shape the spectrum of light emitted from a laser frequency comb across the visible and near-infrared wavelengths with more precision than previously possible. This advance could provide an important new tool in the hunt for Earth-like planets outside our solar system.
When searching for exoplanets, astronomers use high-precision spectroscopy to detect tiny shifts in starlight that reveal a star’s subtle “wobble” due to an orbiting planet. But for Earth-sized planets, these wavelength changes are smaller than the spectrograph’s natural instabilities, so laser frequency combs—lasers that emit thousands of evenly spaced spectral lines —are needed to provide a reference, acting like precise wavelength rulers.
“For astronomers, the big prize would be to find a planet with a mass similar to Earth and orbiting a star similar to our sun,” said research team leader Derryck T. Reid, from Heriot-Watt University in the U.K. “Our spectral shaper can make the lines on a laser frequency comb more uniform, which allows the spectrograph to detect smaller stellar motions, such as those from Earth-like planets, that would otherwise be hidden in the noise.”








