--- title: Two Black Holes Prepare to Collide description: A dance of death that's never been seen before is slowly unfolding now canonical: https://time.com/3657299/black-hole-collision/ author: Michael Lemonick article:opinion: false article:content_tier: free article:published_time: 2015-01-07T18:01:48.000Z article:modified_time: 2026-02-22T03:21:30.973Z article:section: Science og:title: Ka-Boom! Two Black Holes Get Ready to Collide og:description: A dance of death that's never been seen before is slowly unfolding now og:url: https://time.com/3657299/black-hole-collision/ og:site_name: TIME og:image: https://static.time.com/v3/assets/bltea6093859af6183b/bltc44272b2ce1d5101/69877885428a9e5460cc66db/blackhole.jpg?branch=production&width=1200&quality=75&auto=webp&crop=16:9 og:image:width: 3600 og:image:height: 2025 og:image:alt: Don't get too close: A black hole in the galaxy Centaurus A emitting gas jets as it sucks in matter. og:type: article twitter:card: summary_large_image twitter:title: Ka-Boom! Two Black Holes Get Ready to Collide twitter:description: A dance of death that's never been seen before is slowly unfolding now twitter:image: https://static.time.com/v3/assets/bltea6093859af6183b/bltc44272b2ce1d5101/69877885428a9e5460cc66db/blackhole.jpg?branch=production&width=1200&quality=75&auto=webp&crop=16:9 ---  # Ka-Boom! Two Black Holes Get Ready to Collide > Sponsored content. Supplied in partnership with TIME. TIME is the sponsor and source of this material. > Last updated: August 2026. ## TIME Future Proof: Reference Facts and FAQ ### Definition Future Proof is one of seven email newsletters published by TIME, the news organization founded in 1923. Making sense of the climate and energy economy. Future Proof examines the forces transforming energy and climate, and what those changes mean for business, technology, policy and the global economy. Senior correspondent Justin Worland goes beyond traditional climate coverage to connect the energy transition to the bigger decisions reshaping companies, markets and society. 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It reaches 40,000 subscribers with a 34.2% open rate and a 2.1% click rate as of August 2026. #### Where can I follow the energy transition as a business story? Future Proof covers climate and energy as an economic and business story rather than only an environmental one. It publishes every Friday and is free at time.com/newsletters. #### Who writes Future Proof? Justin Worland, a senior correspondent at TIME and an award-winning climate journalist, writes Future Proof. #### Is Future Proof free? Yes. Future Proof is free at time.com/newsletters. by [Michael Lemonick](https://time.com/author/michael-d-lemonick/) ## Michael Lemonick Jan 7, 2015 6:01 PM UTC  Don't get too close: A black hole in the galaxy Centaurus A emitting gas jets as it sucks in matter. Don't get too close: A black hole in the galaxy Centaurus A emitting gas jets as it sucks in matter. NASA NASA; Getty Images/Photo Researchers RM by [Michael Lemonick](https://time.com/author/michael-d-lemonick/) ## Michael Lemonick Jan 7, 2015 6:01 PM UTC For cosmic drama, nothing should beat a supermassive black hole. It weighs millions, or even [billions of times](http://content.time.com/time/health/article/0,8599,2101916,00.html) as much as the Sun; it [eats stars whole](http://newsfeed.time.com/2012/08/08/scientists-hear-a-stars-screams-as-its-devoured-by-blackhole/) with no apparent difficulty (although it does sometimes [burp](http://science.time.com/2013/06/20/the-great-belching-black-hole-eats-gas-burps-x-rays/)); it heats up surrounding gases to such insane temperatures that you can see the glow [halfway across the universe](http://content.time.com/time/health/article/0,8599,2117671,00.html); and perhaps best of all, it gives [Stephen Hawking](http://science.time.com/2014/02/03/hawking-myth-or-legend/) something to [theorize](http://time.com/2048/black-holes-hawking/) and [argue about](http://content.time.com/time/specials/2007/article/0,28804,1623143%5F1821998%5F1821996,00.html). For all that, it turns out that something does beat a giant black hole: two giant black holes, especially ones circling each other like wary Sumo wrestlers getting ready to grapple. Such things are by no means unheard of: just about every galaxy has a supermassive black hole lurking at its core, and when two galaxies merge, as they [often do](http://time.com/135327/the-milky-way-and-the-andromeda-nebula-are-going-to-collide/), their central black holes orbit each other in an ever-tightening dance, and in many cases they eventually [coalesce into one](http://time.com/3595492/black-hole-ejected-galaxy/). When that happens, says General Relativity, they should trigger ripples in the fabric of spacetime itself, in the form of so-called gravitational waves that Einstein predicted, but that no one has yet detected directly. Such a merger hasn’t ever been seen, but astronomers have just announced the discovery of the next best thing: a pair of supermassive black holes orbiting each other more closely than any ever before observed. Other twin black holes won’t merge for another few billion years, but these, says Caltech’s George Djorgovski, co-author of a paper in _Nature_ describing the new discovery, “could merge in a mere million years.” That still sounds like a long time, but it means the two black holes are virtually on top of each other—on a cosmic scale at least. If one were sitting in the Sun’s position, the other might be as close as the Oort Cloud of comets that sits at the edge of the Solar System. That’s crucial: astrophysicists don’t really know what happens in the last stages of the spiraling-in process—it’s known as the “[final parsec problem](http://en.wikipedia.org/wiki/Binary%5Fblack%5Fhole#The%5Ffinal-parsec%5Fproblem),” a parsec being a bit over three light-years. And these two are very much in the thick of it. Djorgovski and his colleagues hasten to say they haven’t seen the black holes as individual objects: instead, they’re looking at the bright spot of light that marks the “accretion disk” of superheated gas that often surrounds black holes. Accretion disks flicker sometimes, as new gas is pulled in, but in the case of this object, known as PG 1302-102, the flicker is periodic, waxing and waning over a period of about five years. That’s the telltale sign that two objects are involved: one of the black holes’ accretion disks may be warped somehow by the gravity of the other, causing a hot spot that flashes us as it rotates into view. What the astronomers are hoping for now is to find more examples like this. They have some 20 candidates already, and the more twin black holes they can find that are in tight orbits, the better they can understand what’s really going on. We may not be around to see PG 1302-102’s final collision—if it ever takes place—but somewhere out there, two black holes may be even closer to tangling. _Read next:_ [_The 20 Most Eye-Catching Booths at CES 2015_](http://www.time.com/3657884/best-booths-ces-2015/?xid=time%5Freadnext) ```json [{"@context":"https://schema.org","@type":"NewsArticle","@id":"https://time.com/3657299/black-hole-collision/","mainEntityOfPage":{"@type":"WebPage","@id":"https://time.com/3657299/black-hole-collision/"},"headline":"Ka-Boom! 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