It’s Possible to Hack a Phone With Sound Waves, Researchers Show

Photo
Kevin Fu and other researchers have found a way to take control of or influence devices using a standard component in cellphones and other gadgets. Credit Joseph Xu/University of Michigan
SAN FRANCISCO — A security loophole that would allow someone to add extra steps to the counter on your Fitbit monitor might seem harmless. But researchers say it points to the broader risks that come with technology’s embedding into the nooks of our lives.
On Tuesday, a group of computer security researchers at the University of Michigan and the University of South Carolina will demonstrate that they have found a vulnerability that allows them to take control of or surreptitiously influence devices through the tiny accelerometers that are standard components in consumer products like smartphones, fitness monitors and even automobiles.
In their paper, the researchers describe how they added fake steps to a Fitbit fitness monitor and played a “malicious” music file from the speaker of a smartphone to control the phone’s accelerometer. That allowed them to interfere with software that relies on the smartphone, like an app used to pilot a radio-controlled toy car.
“It’s like the opera singer who hits the note to break a wine glass, only in our case, we can spell out words” and enter commands rather than just shut down the phone, said Kevin Fu, an author of the paper, who is also an associate professor of electrical engineering and computer science at the University of Michigan and the chief executive of Virta Labs, a company that focuses on cybersecurity in health care. “You can think of it as a musical virus.”
The flaw, which the researchers found in more than half of the 20 commercial brands from five chip makers they tested, illustrates the security challenges that have emerged as robots and other kinds of digital appliances have begun to move around in the world.
With dozens of start-ups and large transportation companies pushing to develop self-driving cars and trucks, undetected vulnerabilities that might allow an attacker to remotely control vehicles are an unnerving possibility.
Still, computer security researchers said the discovery was not a sky-is-falling bug but rather a revealing window into the cybersecurity challenges inherent in complex systems in which analog and digital components can interact in unexpected ways.
“The whole world of security is about unintended interactions,” said Paul Kocher, a cryptographer and a former executive at the chip company Rambus.
Photo
A speaker can make tones that fool a sensor and cause a microprocessor to accept the sensor readings. Credit Joseph Xu/University of Michigan
Accelerometers are instruments that measure acceleration and are frequently manufactured as silicon chip-based devices known as microelectromechanical systems, or MEMS. Accelerometers are used for navigating, for determining the orientation of a tablet computer and for measuring distance traveled in fitness monitors such as Fitbits.
In the case of the toy car, the researchers did not actually compromise the car’s microprocessor, but they controlled the car by forcing the accelerometer to produce false readings. They exploited the fact that a smartphone application relies on the accelerometer to control the car.
While toy cars might seem like trivial examples, there are other, darker possibilities. If an accelerometer was designed to control the automation of insulin dosage in a diabetic patient, for example, that might make it possible to tamper with the system that controlled the correct dosage.
Dr. Fu has researched the cybersecurity risks of medical devices, including a demonstration of the potential to wirelessly introduce fatal heart rhythms into a pacemaker.
He said the current research was inspired by a discussion in his group about a previous study in which drones were disabled with music. He added that earlier research demonstrated denial-of-service attacks that used sound to disable accelerometers.
In 2014, security researchers at Stanford University demonstrated how an accelerometer could be used surreptitiously as a rudimentary microphone, for example. And in 2011, a group from the Massachusetts Institute of Technology and the Georgia Institute of Technology demonstrated the use of an accelerometer in a smartphone to decode roughly 80 percent of the words being typed on a nearby computer keyboard by capturing vibrations from the keyboard.
In the case of the research by the University of Michigan and the University of South Carolina, scientists stopped the accelerometer from functioning and changed its behavior.
In testing 20 accelerometer models from five manufacturers, they affected the information or output from 75 percent of the devices tested and controlled the output in 65 percent of the devices.
The Department of Homeland Security was expected to issue a security advisory alert Tuesday for chips produced by the semiconductor companies documented in the paper, Dr. Fu said. The five chip makers were Analog Devices, Bosch, InvenSense, Murata Manufacturing and STMicroelectronics.
The paper, which will be presented at the IEEE European Symposium on Security and Privacy in Paris next month, also documents hardware and software changes manufacturers could make to protect against the flaws the researchers discovered.

The warmth within: Cassini discovers heat beneath the icy surface of Saturn's moon Enceladus!

By Zee Media Bureau | Last Updated: Tuesday, March 14, 2017 - 09:44
The warmth within: Cassini discovers heat beneath the icy surface of Saturn's moon Enceladus!
Image courtesy: NASA/JPL-Caltech/Space Science Institute
New Delhi: NASA's Cassini mission is currently on its last leg and is inching toward its graceful finish in 2017. At present, the spacecraft is performing flybys of the planet Saturn, making its closest approaches to the rings.
The mission, which is about to end some time this year, has definitely been a fruitful one, owing to all the wonderfully insightful information scientists have managed to glean from it.
Every new image beamed back by Cassini carries some evolutionary secret or shows an unpredictable side of the planet or a feature that would have otherwise been impossible to find out.
Now, with another magnificent image delivered by the spacecraft, Saturn's icy moon Enceladus has been revealed to have a warmer south polar region than expected.
A new study in the journal Nature Astronomy suggests that Enceladus' ocean of liquid water might be only a couple of miles beneath this region – closer to the surface than previously thought.
The excess heat is especially pronounced over three fractures that are not unlike the "tiger stripes" – prominent, actively venting fractures that slice across the pole – except that they don't appear to be active at the moment. Seemingly dormant fractures lying above the moon's warm, underground sea point to the dynamic character of Enceladus' geology, suggesting the moon might have experienced several episodes of activity, in different places on its surface.
The finding agrees with the results of a 2016 study by a team independent of the Cassini mission that estimated the thickness of Enceladus' icy crust. The studies indicate an average depth for the ice shell of 11 to 14 miles (18 to 22 kilometers), with a thickness of less than 3 miles (5 kilometers) at the south pole, said NASA.
"Finding temperatures near these three inactive fractures that are unexpectedly higher than those outside them adds to the intrigue of Enceladus," said Cassini Project Scientist Linda Spilker at NASA's Jet Propulsion Laboratory, Pasadena, California. "What is the warm underground ocean really like and could life have evolved there? These questions remain to be answered by future missions to this ocean world," NASA reported.
First Published: Tuesday, March 14, 2017 - 09:44

Astronomers Just Found a Star Orbiting a Black Hole at 1 Percent the Speed of Light

ScienceAlert - ‎5 hours ago

Astronomers Just Found a Star Orbiting a Black Hole at 1 Percent the Speed of Light

The closest we've seen a star get to a black hole.
MIKE MCRAE
15 MAR 2017
Astronomers have just spotted a star whizzing around a vast black hole at about 2.5 times the distance between Earth and the Moon, and it takes only half an hour to complete one orbit.
To put that into perspective, it takes roughly 28 days for our Moon to do a single lap around our relatively tiny planet at speeds of 3,683 kilometres (2,288 miles) per hour, meaning this star is moving at some mind-boggling, break-neck speeds.
Using data from an array of deep space telescopes, a team of astronomers have measured the X-rays pouring from a binary star system called 47 Tuc X9, which sits in a cluster of stars about 14,800 light-years away.
The pair of stars aren't new to astronomers - they were identified as a binary system way back in 1989 - but it's now finally becoming clear what's actually going on here.
"For a long time, it was thought that X9 is made up of a white dwarf pulling matter from a low mass Sun-like star," said researcher Arash Bahramian.
When a white dwarf pulls material from another star, the system is described as a cataclysmic variable star. But back in 2015, one of the objects was found to be a black hole, throwing that hypothesis into serious doubt.
Data from Chandra has confirmed large amounts of oxygen in the pair's neighbourhood, which is commonly associated with white dwarf stars. But instead of a white dwarf ripping apart another star, it now seems to be a black hole stripping the gases from a white dwarf.
White dwarfs are super dense objects that are usually the remnants of a star - think of something with the mass of our Sun but only as big as our planet - so pulling material from its surface would require some impressive gravity.
"We think the star may have been losing gas to the black hole for tens of millions of years and by now has now lost the majority of its mass," said researcher James Miller-Jones from Curtin University and the International Centre for Radio Astronomy Research.
The real exciting news, however, is regular changes in the X-rays' intensity suggest this white dwarf takes just 28 minutes to complete an orbit, making it the current champion of cataclysmic dirty dancers.
"Prior to this discovery, the closest star around any likely black hole was a system known as MAXI J1659-152, which is in an orbit with a 2.4-hour period," said Miller-Jones.
"If the likely black holes in both systems have similar masses, this would imply an orbit three times larger in physical size than the one we found in X9."
To put it in perspective, the distance between the two objects in X9 is about 1 million kilometres (about 600,000 miles), or about 2.5 times the distance from here to the Moon.
Crunching the numbers, that's a journey of roughly 6.3 million kilometres (about 4 million miles) in half an hour, giving us a speed of 12,600,000 km/hr (8,000,000 miles/hr) - about 1 percent of the speed of light.
As exciting as those figures are, the research has yet to be peer-reviewed, with the paper awaiting feedback from the physics community on the pre-publish website arXiv.org. But it's already gaining interest in the field.
"Finding these rare black holes is important, as they are not only the end points of massive stars, produced in supernova explosions, they also continue to play a role in the evolution of other stars after their deaths," Geraint Lewis from the University of Sydney told Marcus Strom at The Sydney Morning Herald.
Our two star-crossed lovers aren't fated to collapse into each other's arms any time soon, at least, with the dance looking like it will continue without the white dwarf falling into the black hole or being ripped apart.
In fact, if anything, it seems the two objects were even closer together in the past and orbiting even faster.
For the black hole to overcome the white dwarf's own intense gravity, the bodies need to be fairly close together. Over time, as material is stripped away, the now-lighter white dwarf would slip a little further back.
"Eventually so much matter may be pulled away from the white dwarf that it ends up only having the mass of a planet," said researcher Craig Heinke. "If it keeps losing mass, the white dwarf may completely evaporate."
That's good news for future scientists keen to study gravitational waves; while the current technology used by the Laser Interferometer Gravitational-Wave Observatory isn't able to spot the slow pulses emitted by X9, it's not out of the question that progress in that field will one day allow us to detect lower frequency waves.
Of course, by then we might have found a new king and queen of cataclysmic variable stars, spinning the night away at even faster speeds.
This research was published in arXiv.org.
.