A giant planet around a tiny star: A discovery that challenges planet formation theories
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Updates every hour. Last Updated: 27-Jun-2025 15:10 ET (27-Jun-2025 19:10 GMT/UTC)
The host star, TOI-6894, is a red dwarf with only 20% the mass of the Sun, typical of the most common stars in our galaxy. Until now, such low-mass stars were not thought capable of forming or retaining giant planets. But as published in Nature Astronomy, the unmistakable signature of a giant planet — TOI-6894b — has been detected in orbit around this tiny star.
A groundbreaking study by researchers from Chongqing University and the Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, reveals that diatoms can transform lunar soil, boosting its water retention and nutrient levels to support robust plant growth. This breakthrough paves the way for sustainable agriculture in lunar habitats, offering a vital step toward humanity’s long-term survival and interplanetary exploration.
A group of astronomers from across the globe, including a team from the University of Washington and led by Queen’s University Belfast, have revealed new research showing that millions of new solar system objects will be detected by a brand-new facility, which is expected to come online later this year.