Washington: Scientists have developed an astrocomb, a tool that precisely measures frequencies or colours of light, which can help widen the search for Earth-like planets, and perhaps extraterrestrial life.
The custom-made frequency comb, developed by researchers from National Institute of Standards and Technology’s (NIST) in the US, provides the precision needed for discovering and characterising planets orbiting M dwarf stars, which comprise 70 per cent of the stars in the galaxy and are plentiful near Earth. “These improved tools should allow us to find habitable planets around the most ubiquitous stars in our galaxy,” said Scott Diddams, from NIST.
A star’s nuclear furnace emits white light, which is modified by elements in the atmosphere that absorb certain narrow bands of colour. To search for planets orbiting distant stars, astronomers look for periodic changes in this characteristic ‘fingerprint’, that is, very small variations in the apparent colours of starlight over time.
These oscillations in colour are caused by the star being tugged to and fro by the gravitational pull of an unseen orbiting planet. This apparent wobble is subtle, and measurements are limited by the frequency standards used to calibrate spectrographs.
Hundreds of exoplanets have been discovered using star wobble analysis, but a planet with a mass similar to that of Earth and orbiting at just the right distance from a star — in the so-called ‘Goldilocks zone’ — is hard to detect with conventional technology.