* Astronomers from the Astronomical Observatory of Palermo, National Institute for Astrophysics (INAF), and the University of St Andrews investigated the 5–10 Jupiter mass free-floating planetary-mass object (FFPMO) Cha 1107-7626 during a powerful and protracted accretion outburst event.
* The X-shooter spectrograph on the European Southern Observatory’s (ESO’s) Very Large Telescope (VLT) detected an enhanced mass accretion rate of 10−7MJupiteryr−1, corresponding to six billion tonnes per second, between June and August 2025.
* According to lead author Víctor Almendros-Abad, this finding provides the strongest evidence yet for a planetary-mass object behaving like an EXor-type variable star, profoundly challenging current planetary formation models.
*( P.S. If you like byte-sized space summaries like this you’ll enjoy* [*therisedaily.com*](http://therisedaily.com/) *)*
jwely on
At this mass and accretion rate, is it any less than certain that this „planet“ will soon be a star?
ForAThought on
The newly studied object, which has a mass five to 10 times the mass of Jupiter… …this rogue planet is still forming and is fed by a surrounding disc of gas and dust. This material constantly falls onto the free-floating planet, a process known as accretion… …at a rate of six billion tonnes a second.
Luke_Cocksucker on
I’ve seen this one before. Someone needs to find the fifth element.
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[Main Article](https://www.eso.org/public/news/eso2516/) | [Image of Cha 110-7-7626](https://www.eso.org/public/images/eso2516b/)
* Astronomers from the Astronomical Observatory of Palermo, National Institute for Astrophysics (INAF), and the University of St Andrews investigated the 5–10 Jupiter mass free-floating planetary-mass object (FFPMO) Cha 1107-7626 during a powerful and protracted accretion outburst event.
* The X-shooter spectrograph on the European Southern Observatory’s (ESO’s) Very Large Telescope (VLT) detected an enhanced mass accretion rate of 10−7MJupiteryr−1, corresponding to six billion tonnes per second, between June and August 2025.
* According to lead author Víctor Almendros-Abad, this finding provides the strongest evidence yet for a planetary-mass object behaving like an EXor-type variable star, profoundly challenging current planetary formation models.
*( P.S. If you like byte-sized space summaries like this you’ll enjoy* [*therisedaily.com*](http://therisedaily.com/) *)*
At this mass and accretion rate, is it any less than certain that this „planet“ will soon be a star?
The newly studied object, which has a mass five to 10 times the mass of Jupiter… …this rogue planet is still forming and is fed by a surrounding disc of gas and dust. This material constantly falls onto the free-floating planet, a process known as accretion… …at a rate of six billion tonnes a second.
I’ve seen this one before. Someone needs to find the fifth element.