New planet discovered 35 light years away
The team utilised NASA's TESS (Transiting Exoplanet Survey Satellite) space telescope to identify the planet, named L 98-59 f. It is one of five planets orbiting a red dwarf star in the L 98-59 system.
Located in the habitable zone
L 98-59 f lies within the star's habitable zone, the region where liquid water could potentially exist. It receives a similar amount of stellar energy as Earth does from the Sun, making it a candidate for possible habitability.
A compact and diverse planetary system
The L 98-59 system was previously believed to host only four planets. However, after extensive analysis of data from both space- and ground-based telescopes, the fifth planet was identified.
Detected through stellar motion
Unlike the other planets in the system, L 98-59 f does not transit between its star and Earth, making it invisible to standard transit detection methods. Instead, scientists detected it by observing subtle shifts in the motion of its host star — a method known as the radial velocity technique.
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New planet discovered 35 light years away
Discovery made using NASA's TESS Telescope The team utilised NASA's TESS (Transiting Exoplanet Survey Satellite) space telescope to identify the planet, named L 98-59 f. It is one of five planets orbiting a red dwarf star in the L 98-59 system. Located in the habitable zone L 98-59 f lies within the star's habitable zone, the region where liquid water could potentially exist. It receives a similar amount of stellar energy as Earth does from the Sun, making it a candidate for possible habitability. A compact and diverse planetary system The L 98-59 system was previously believed to host only four planets. However, after extensive analysis of data from both space- and ground-based telescopes, the fifth planet was identified. Detected through stellar motion Unlike the other planets in the system, L 98-59 f does not transit between its star and Earth, making it invisible to standard transit detection methods. Instead, scientists detected it by observing subtle shifts in the motion of its host star — a method known as the radial velocity technique.
