New image reveals clumps of dust that could form giant planets around young star

European Southern Observatory released a new image of a star named V960 Mon that shows material orbiting it in intricate spirals.
Astronomers analyzed the spiral arms and concluded they contain clumps of dust with masses similar to planets, potentially precursors of giant planets.
This observation provides the first detection of clumps around a young star that could form giant planets, supporting the theory of gravitational instability.
Astronomers captured the image after V960 Mon brightened 20 times its normal levels in 2014, allowing the use of advanced telescopes.
Further observations of systems like V960 Mon will enhance understanding of planet formation, and new telescopes will enable more research.