Astronomers studied the new images of a young star taken by the Karl G. Jansky Very Large Array (VLA) and said it reveals very early stages of planet formation. The scientists used the VLA to see unprecedented detail of the inner portion of a dusty disk surrounding the star, nearly 450 light years from Earth. The star and its disk were studied in 2014 with Atacama Large Millimeter/submillimeter Array (ALMA), which produced what astronomers then called the best image ever of planet formation in progress, National Radio Astronomy Observatory posted online on Thursday. Also Read - First-ever image of 'monster' black hole capturedAlso Read - Super Blood Wolf Moon, partial solar eclipse: Date, timings, where and how to watch in India
The ALMA image showed gaps in the disk, presumably caused by planet-like bodies sweeping out the dust along their orbits. This image showed in real life what theorists had proposed for years. However, scientists were surprised to see this phenomenon because the star, called HL Tau, is only about a million years old — very young by stellar standards. The ALMA image showed details of the system in the outer portions of the disk, but in the inner portions of the disk, nearest to the young star, the thicker dust is opaque to the short radio wavelengths received by ALMA.
The new VLA images revealed a distinct clump of dust in the inner region of the disk that contains roughly three to eight times the mass of Earth.
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“We believe this clump of dust represents the earliest stage in the formation of protoplanets, and this is the first time we have seen that stage,” said Thomas Henning from Max Planck Institute for Astronomy (MPIA). “This is an important discovery, because we have not yet been able to observe most stages in the process of planet formation,” said Carlos Carrasco-Gonzalez from the Institute of Radio Astronomy and Astrophysics (IRyA) in Mexico.
This region, the scientists said, is presumably where Earth-like planets would form, as clumps of dust grow by pulling in material from their surroundings. Eventually, the clumps would gather enough mass to form solid bodies that would continue to grow into planets.