What you want, before you even realise you want it (Image: Jonathan Hordle/Rex Features)
Google attempts to return relevant search results in the blink of an eye. But in future it could go one better, delivering search results to its users even before they know that they want the information.
, one of Google’s veteran search algorithm engineers, wants to develop a search engine that second-guesses users’ needs well ahead of time.
“I call it searching without searching,” he said at a briefing at Google’s London headquarters yesterday.
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In future, your Google account may be allowed, under some as-yet-unidentified privacy policy, to know a whole lot about your life and the lives of those close to you. It will know birthdays and anniversaries, consumer gadget preferences, preferred hobbies and pastimes, even favourite foods. It will also know where you are, and be able to get in touch with your local stores via their websites.
No more present panic
Singhal says that could make life a lot easier. For instance, he imagines his wife’s birthday is coming up. If he has signed up to the searching-without-searching algorithm (I’ll call it “SWS” for now), it sees the event on the horizon and alerts him – as a calendar function can now. But the software then reads his wife’s consumer preferences file and checks the real-time Twitter and Facebook feeds that Google now indexes for the latest buzz products that are likely to appeal to her.
“It might suggest I buy her an iPad and point me to some relevant product reviews,” he says. But SWS might also discover, again from fishing in recent social media, that the local gadget store has a three-week waiting list for iPads. “So it would bring forward its alert to give me time to order it.”
At other times, SWS could give its users a personalised and frequently updated news service by gathering information from social media sites. Singhal points out that Twitter can beat newscasters to warn you of events that might affect you: an earthquake that hit San Francisco in January sent ripples through Twitter 10 minutes before a news alert from the US Geological Survey alerted the professional news media.
More mundanely, real-time updates could highlight a major traffic jam on the way to a meeting that’s marked in your calendar and warn you to delay your trip, or suggest the best alternative route.
Getting to know you
Singhal’s idea taps into a growing research trend that is exploring ways to personalise search. For instance, Yahoo Research in Barcelona, Spain, has demonstrated that basic demographic information can help to reduce the ambiguity of some search terms by weighting search results towards what a particular user is likely to want to know.
But while the technology exists, it won’t be brought to market until ways are be found to address the privacy concerns that highly personalised services will inevitably raise. Google knows this only too well: privacy-sensitive internet users are still feeling stung by Google’s sniffing of private Wi-Fi addresses from its Street View cars.
“If searching-without-searching happens, it needs to be done in an incredibly privacy-preserving way, with full control by the users over what it knows,” Singhal says. “That’s going to take an awful lot of innovation.”
While Google reckons such a system could save a user up to 15Â minutes of conventional searching every day, Singhal stresses that SWS is not a product in development, but a “dream” he has.
However, it’s worth noting that the other dreams he has had in his 10 years at the helm of Google’s algorithmic development include ever-smarter context-sensitive text search, translation engines and location-sensitive search – all of which have come true.
Read previous Innovation columns: Shrewd search engines know what you want, The tech refresher Russia’s spies needed, Smarter books aim to win back the kids, Microsoft’s Kinect isn’t just for games, 19th-century tech makes a smarter iPhone, Invisibility cloaks and how to use them, Methane capture gives more bang for the buck, Slipping into the wireless white space, Teaching robots some manners, Why labs love gaming hardware.
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


