The discovery of a new planet at a distance has been one of the greatest achievements in modern astronomy. Thanks to advances in telescope technology and observation methods, scientists are now able to detect exoplanets outside our solar system. This discovery process relies on several methods, including transit and radial velocity methods, each of which has its own advantages. One of the greatest achievements was the Kepler mission launched by NASA in 2009. This telescope was specifically designed to search for planets in the habitable zone, places where life can exist. Kepler has identified thousands of exoplanets, with some of them similar to Earth in size and distance to their host stars. The transit method, used by Kepler, observes the dip in light from a star when a planet passes in front of the star. By analyzing this data, scientists can determine the size and orbit of the planet. Meanwhile, the radial velocity method measures the shift in the star’s spectrum as a result of the gravity of the planet orbiting around it. Both methods provide important insights into the composition of the atmosphere and the possible presence of water, which is a vital indication for life. Recently, telescopes such as TESS (Transiting Exoplanet Survey Satellite) and JWST (James Webb Space Telescope) have further expanded the boundaries of discovery. TESS focuses on searching for planets at close range, while JWST is able to analyze exoplanet atmospheres in more depth. The discovery of planets such as LHS 3844 b and TOI 700 d adds to the list of exoplanets that show the potential for conditions that support life. Not only that, increasing international collaboration in astronomy projects also speeds up the research process. By utilizing data collected from various observatories and telescopes around the world, scientists can formulate new theories about planet formation and stellar evolution. The discovery of new distant planets is not only exciting for scientists, but also sparks public interest. Many people are fascinated by the possibility of life beyond Earth. IPP (International Planetary Society) and local astronomy communities often hold seminars and discussions to share this knowledge with the public. Further research on these planets could reveal more information about how planets form and interact with their stars. Additionally, the potential discovery of biosignatures or signs of life in exoplanet atmospheres is one of the most exciting focus areas in astrobiology today. As part of ongoing space exploration, the discovery of new distant planets is an important step towards better understanding our place in the universe. With increasingly sophisticated observation tools, more secrets of the universe will be revealed in the coming decades. This search promises more surprising discoveries and inspires a desire to explore further.
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