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A immense cosmic entity could unit astronomers to rethink what a satellite is
The almost Jupiter-sized entity is orbiting a brownish dwarf, which, successful turn, is circling astir a mini star
By Adam Kovac edited by Lee Billings

Artist’s belief of CD-35 2722, a strategy pinch a moon-like object
ESO/M. Kornmesser
When is simply a satellite not a moon? That’s nan riddle raised by a caller study, and nan reply appears to be, erstwhile it’s a planet. Or possibly it’s vice versa.
Such are nan unusual semantic questions raised by studies of CD-35 2722 b, a brown dwarf pinch astir 30 times nan wide of Jupiter that’s orbiting a mini prima immoderate 73 light-years from Earth. The brownish dwarf appears to person its ain satellite, overmuch for illustration Earth has nan moon, albeit 1 almost arsenic large arsenic nan largest satellite successful our star system. While astronomers person discovered thousands of exoplanets, CD-35 2722 whitethorn beryllium nan first prima strategy recovered that exhibits this three-tiered “star-brown dwarf-satellite” hierarchy.
Earlier observations of CD-35 2722 b, taken astatine nan W.M. Keck Observatory successful Hawaii, had shown hints of an exomoon - a type of entity that’s yet to beryllium definitively found - but nan information wasn’t conclusive. To settee nan matter, Kevin Hoy, a PhD student astatine nan Institute of Astrophysics Studies successful Santiago, Chile, turned to nan European Southern Observatory’s much powerful Very Large Telescope (VLT) and its CRIRES+ instrumentality connected a mountaintop successful nan precocious Chilean desert.
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CRIRES+ is simply a spectrograph, an instrumentality that parses a star’s ray into a rainbowlike spectrum of colors; fluctuations successful that spectrum way a star’s mobility successful nan sky, pinch nan spectrum increasing bluer if a prima is approaching Earth and redder if a prima is receding. Astronomers hunt for hidden orbiting companions by nan measurement their gravity tin propulsion a prima to and fro, creating subtle stellar wobbles that registry arsenic a telltale bid of “blueshifts” and “redshifts” successful a star’s spectrum.
Across almost two-and-a-half years, ending successful February, Hoy and his colleagues utilized nan VLT and CRIRES+ to periodically measurement nan brownish dwarf’s spectrum successful hunt of specified wobbles, a method known arsenic radial velocity analysis. As they described successful a caller paper published successful Nature on Thursday, CD-35 2722 b is wobbling indeed, from immoderate benignant of otherwise-unseen outer circling it erstwhile each 170 days.
Exactly what to telephone this companion is simply a matter of debate. While it acts for illustration a moon, it’s large – really, really big, pinch a minimum wide 90 percent that of Jupiter’s. “The wide could beryllium moreover higher,” Hoy notes, adding that nan object’s sheer size apt intends it’s mostly made of gas, alternatively than rock, crystal aliases metal. Were it orbiting a full-fledged prima alternatively than a distinctly substellar brownish dwarf, astronomers would simply telephone nan entity an exoplanet—and a comparatively unremarkable one, astatine that.
Brown dwarfs inhabit a peculiar spot successful nan cosmic pecking order. They’re gassy orbs galore times larger than Jupiter, yet excessively mini to person deed nan captious wide for sustaining nan thermonuclear fusion reactions that make stars shine. (This is why brownish dwarfs are often referred to arsenic grounded stars). Given really weird they are, it makes consciousness that immoderate orbits them would beryllium oddities arsenic well.
The closest analog to Hoy’s uncovering whitethorn beryllium HD 206893 b, a conspicuously wobbling 28-Jupiter-mass exoplanet 129 ray years distant from Earth, says David Kipping, an exomoon-hunting astronomer astatine Columbia University, who did not activity connected nan caller study. But while HD 206893 b’s wobble is accordant pinch nan persistent tug from an accompanying outer of astir half Jupiter’s mass, he says, a insubstantial published successful January showed this awesome could conscionable arsenic good have different explanations, making nan wobble grounds for a “candidate” exomoon, astatine best. CD-35 2722 b’s putative exomoon is technically conscionable a candidate, too, but its associated wobble is overmuch clearer and harder to explicate away.
“It’s a campaigner object, but it astir apt is real,” Kipping says. “In this lawsuit they consciousness for illustration it’s much secure, and I would astir apt bargain that. It does look a really cleanable detection.”
As astronomical instruments proceed to improve, it’s apt much small, unusual campaigner companions will beryllium recovered for brownish dwarfs and exoplanets alike, says Hoy. That intends astronomers will person to commencement coming up pinch amended definitions for what constitutes an exomoon versus an exoplanet successful nan first place. For now, he suggests, we could instrumentality pinch a much neutral word for each these objects: exosatellites.
An already-borderline entity for illustration nan brownish dwarf CD-35 2722 b is “the cleanable spot to kickstart this benignant of conversation, because nan strategy is for illustration nan cleanable trial furniture for arguing astir things,” Hoy says. “The prima is intelligibly a star. The brownish dwarf is besides intelligibly a brownish dwarf. Now we person this caller entity that is excessively large to evidently beryllium a moon. How we tie nan statement betwixt what’s a satellite and what’s a binary satellite is each very fuzzy astatine nan edges.”
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