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.
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.
Data collected by the team show the astrocomb will make it possible to detect Earth-mass planets that cause colour shifts equivalent to a star wobble of about one metre per second — at least 10 times better than previously achieved in the infrared region of the electromagnetic spectrum.
Infrared light is the main type emitted by M dwarf stars.
While the idea of using frequency combs to aid planet discovery has generated a lot of interest around the world, NIST’s astrocomb is the first in operation at near-infrared wavelengths, researchers said. Other combs currently operating on a telescope, such as the High Accuracy Radial Velocity Planet Searcher (HARPS) in Chile, are dedicated to visible light measurements, they said. (PTI)
