3Hubble finds a new Jupiter-like planet forming in an unusual way: NASA
Context
The Hubble Space Telescope has photographed a Jupiter-like protoplanet.
About
About the finding:
NASA's Hubble space telescope has produced a direct photograph of a Jupiter-like protoplanet embedded in a protoplanetary dusty disk around 2 million years old.
It is forming through what researchers describe as an "intense and violent process."
This discovery supports a long-debated theory for how planets like Jupiter form, called "disk instability."
A protoplanetary or circumstellar disk is a disk of gas and dust orbiting a newly formed star that is believed to be forming planets.
According to disk instability theory, matter in this disk slowly moves inward while dust particles grow into centimeter-sized pebbles.
This is seen as the first step in the formation of kilometer-wide planetesimals, which eventually coalesce into planets.
About the newly forming Planet:
The protoplanet, which is encased in the womb of a protoplanetary disc rich in dust and gas, is already nine times more massive than Jupiter.
Scientists established the presence of the cosmic entity as a planet when the massive disc of dust and gas moving around the star AB Aurigae was discovered turned approximately face-on to the Earth's view.
NASA stated that the new world, which is under construction, is embedded in a protoplanetary disk of dust and gas with distinct spiral structure swirling around surrounding a young star.
The star is estimated to be around two million years old, which is the age of our solar system when planet formation was underway.
Important to note that the solar system's age is currently 4.6 billion years.
It orbits its parent star at a distance of 8.6 billion miles, more than twice the distance between our Sun and Pluto.
This has led researchers to conclude that the disc’s instability allowed this planet to form at such a great distance from its parent star.
The observations also stand in stark contrast to the expectation of planet formation by the widely accepted core accretion model.