MADRID, 10 Sep. (EUROPA PRESS) -
A new study carried out using the telescopes at the European Southern Observatory (ESO) has allowed astronomers to reconstruct for the first time a detailed picture of the inside of disk of material around a young star. Stéphanie Renard the Laboratoire d'Astrophysique de Grenoble and his colleagues used the ESO VLT Interferometer for probing the secrets of the star HD 163296.
Young stars are surrounded by disks of dust and gas and scientists believe it is on these disks where planets are born. The disk dust grains stick to each other to make larger clumps which in turn also recently added. It is believed that this growth process is kept up that form rocky bodies the size of Earth.
So far the information I share only in part, because although I consider it almost necessary to the formation of a disc when the star is formed from a nebula where the dust is enough, why not born planets of the dust, before I consider it impossible, only if there is a sufficient body mass may accumulate some dust, ie a planet of former existence, would finished and a star when the planet is unbalanced in its forces will begin to break off adding more dust to dust.
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