Rare glimpse of giant planet still ‘in the womb' yet nine times the mass of Jupiter
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Loading... - Zach Jackson
- 07 Apr 2022
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Scientists have observed an enormous planet about nine times the mass of Jupiter at a remarkably early stage of formation – describing it as still in the womb – in a discovery that challenges the current understanding of planetary formation.
The researchers used the Subaru telescope, near the summit of an inactive Hawaiian volcano, and the orbiting Hubble space telescope to detect and study the planet called AB Aurigae b, a gas giant orbiting unusually far from its young host star. Gas giants are planets, like our solar system’s largest ones Jupiter and Saturn, composed mostly of hydrogen and helium, with swirling gases surrounding a smaller solid core.
“We think it is still very early on in its ‘birthing’ process,” said astrophysicist Thayne Currie of the Subaru Telescope and the Nasa-Ames research center, lead author of the study published on Monday in the journal Nature Astronomy. “Evidence suggests that this is the earliest stage of formation ever observed for a gas giant.”
It is embedded in an expansive disk of gas and dust that bears the material that forms planets and surrounds a star called AB Aurigae. It lies 508 light years from Earth. This star had a fleeting moment of fame when its image appeared in a scene in the 2021 film Don’t Look Up.
About 5,000 planets beyond our solar system, or exoplanets, have been identified. This one is among the largest. It is approaching the maximum size to be classified as a planet rather than a brown dwarf, a body intermediate between planet and star. It is heated by gas and dust falling into it.
Planets in the process of formation – called protoplanets – have been observed around only one other star.
Almost all known exoplanets have orbits around their stars within the distance that separates our sun and its most faraway planet Neptune. But this planet orbits three times as far as Neptune from the sun and 93 times Earth’s distance from the sun.
Its birth appears to be following a different process than the standard planetary formation model.
“The conventional thinking is that most – if not all – planets form by slow accretion of solids onto a rocky core, and that gas giants go through this phase before the solid core is massive enough to start accreting gas,” said astronomer and study co-author Olivier Guyon of the Subaru telescope and the University of Arizona.
In this scenario, protoplanets embedded in the disk surrounding a young star gradually grow out of dust- to boulder-sized solid objects and, if this core reaches several times Earth’s mass, then begin accumulating gas from the disk. Read More…
