Tag Archives: Science Week

The Speech/Song Illusion

This post was contributed by Rosy Edey, PhD student and graduate teaching assistant in the Department of Psychological Sciences. Rosy attended a Birkbeck Science Week 2016 event on Thursday 14  April – ‘Talk: The Speech/Song Illusion’ (led by Dr Adam Tierney)

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Sadly all good things must come to an end, and the finale of Birkbeck’s 2016 Science Week was a compelling musical one, by one of Birkbeck’s newest members of the Psychology Department, Dr Adam Tierney. In a humorous and engaging way Adam took the audience through the scientific story of the “evolution of music”. Music seems almost completely purposeless, and let’s face it a little bit strange, so why do we love it so much?

What is music?

Adam placed the first known musical instrument (an intricate bone flute) back 40,000 years, which was way before the first record of written word (5000 years ago), but much later than (a good estimate of) when we first evolved to make vocalisations (400,000 years ago). The absolute origin of music is obviously very difficult to pinpoint – as it is possible (and probable) that way before we built tools – like the bone flute – to make music, we were signing our hearts out in the moonlight.

This questionable timing of the birth of music raises the question: what came first, speech or music? Whichever one came first, if one evolved from the other we would expect music and language to share similar characteristics. Indeed, Adam presented evidence that both the huge varieties of globally spoken languages and music from around the world share common universalities (which at first seemed very unlikely based on the diversity of music that was perfectly demonstrated through a bizarre example of washing machine “music” and also a collection of songs from the playlist from the Voyager I and II spacecraft gold plates).

These shared acoustic qualities included alternating beat patterns, descending melodic contours, and increases in final phrase duration. Using the very complicated sounding “Normalised Pairwise Variability Index” (i.e. jargon for a measure of rhythmic alteration, or a measure of paired stress in phrases) Adam showed there were also commonalities between languages and music within and between specific countries (basically English music sounds English, and French sounds French, but English music/ language does not sound like French music/language). All of these beautiful subtleties hidden in the acoustics of spoken word and music provide vast amounts of data, which signal meaning to the listener. These underlying similarities do hint that music and speech are distant cousins.

Music as Speech with added extras

Playing music with speech can change it into a song; The Jazzy Sarah Palin Interview was a good example of this:

 

And it seems even without music our brains can transform speech into music. Diana Deutsch discovered this phenomenon in 1995, while looping some spoken data.

After several iterations the phrase “sometimes behave so strangely” no longer sounded like speech, and had converted into song (I now cannot even read this phrase without hearing the tune). All the phrases in Adam’s Corpus of Illusion Stimuli turned into singing, but interestingly, the “control” sentences didn’t have the same effect. This illusion appears to be a useful tool to test further the idea of music evolution and ask more detailed questions, such as: “what is required for speech to become song?” and “what mechanisms are going on in our brains when we change speech into song?”

Testing the Science

Dr Adam Tierney

Dr Adam Tierney

Adam has pulled out the acoustic elements that predict what speech phrases are heard as song. He suggests there are two main factors which induce the illusion; increased beat variability and increased pitch intervals. Remarkably, there is large variability between people’s experience, and being a trained musician doesn’t improve your ability to detect the illusion.

So what is going on in the brain? Adam’s hunch was that these ‘musical’ phrases are processed in the same way as when listening to speech, but with a little added extra. And this does in fact seem to be the case, we activate a similar network to when we hear normal speech, but extra activation in regions that are highly pitch sensitive (e.g. Heschl’s Gyrus – a very early part of the auditory system), and also motor regions (e.g. precentral gyrus – which hosts a map of the body, but specifically the mouth region) when we listen to the ‘song’. Interestingly, there were no regions that were more active for just speech over the song phrases. Adam suggested participants were imagining singing and tapping along to the beat, and processing the pitch more deeply in these ‘song’ phrases. This evidence neatly fits the behavioural data, showing that phrases that have a strong rhythm and more of a melody are processed differently by the brain, which results in them being distorted from speech into song.

Although it is virtually impossible to know the true origin of music, Adam managed to make quite a convincing case that song is just speech with some ribbons on, and quite possibly did evolve from speech.

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Investigating the moon and meteorites

This post was contributed by Dr Jennifer Harris, postdoctoral researcher in Birkbeck’s Department of Earth and Planetary Sciences. Dr Harris attended two Birkbeck Science Week 2016 events on Tuesday 12 April: Analysing the Moon (led by Dr Louise Alexander); and Looking Inside (led by Natasha Almeida)

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What small fragments of rocks can tell us about the moon, the formation of the Solar System and even the early Milky Way was the subject of the second half of Birkbeck Science Week 2016’s Planetary Science evening on Tuesday 12th April.

Dr Louise Alexander, a postdoctoral researcher and Birkbeck student alumna based in the UCL/Birkbeck Centre for Planetary Sciences, and Natasha Almeida, a Birkbeck PhD student and Meteorite Curation Assistant at the Natural History Museum spent an entertaining and informative hour detailing just how much could be gleaned from tiny fragments of extra-terrestrial rocks, and how exactly they go about doing this in their own research.

Apollo Moon samples

Dr Louise Alexander

Dr Louise Alexander

The first half of the session was dedicated to the Moon with Louise Alexander giving us an introduction to the lunar samples brought back by the Apollo astronauts that she uses in her research.

As anyone who’s ever spent any time looking at the full moon can tell you, the moon can be divided into two rough units, one bright and one dark. Lunar samples also fall into these two categories representing the dark Mare basalts and the brighter highland rocks together with a third category of pyroclastic samples. Information from these samples can be used to provide evidence to support the Giant Impact Formation theory of the moon, tell us about the moons internal structure and help to validate surface age estimates from crater counting techniques.

The particular samples that Louise’s work has focused on are all Mare Basalts and are fragments only millimetres in size. Key instruments for extracting data from such small samples are Electron Microprobes, like the one housed by Birkbeck Department of Earth and Planetary Sciences, and Gas Mass Spectrometers.

These instruments enable scientists to peer inside tiny fragments of rock and identify the different mineral crystals that comprise it. Despite the size of each sample, by looking at a large number of them Louise and her collaborators are able to build up a picture of the petrological variety that exists within the Apollo 12 site.

It’s now been over 40 years since the last samples were brought back from the moon and so it’s in the interests of those scientists lucky enough to be in possession of any of them to squeeze as much data out of them as possible. Having used them to gain an understanding of the history of the moon Louise and her colleagues are now investigating the possibility that these samples could have recorded evidence of high energy galactic events over the past few billions of years as the moon has moved through the Milky Way.

This research is still in its infancy and Dr Alexander was keen to point out that the best samples for doing this would be ones from several metres beneath the lunar surface. Sadly for this research no such samples have ever been collected, but if we were to send people back to the moon they could be!

Mapping inside meteorites

Natasha Almeida

Natasha Almeida

An important consideration of the analysis that was described in the first half of the session was that many of the techniques resulted in the destruction of the sample. However not all analysis has to be destructive as we would find out from Natasha Almeida. As a curator Natasha has a professional bias towards preserving her unique and precious samples, whilst as a researcher, still wanting to exploit them as much as possible.

The Natural History Museum in London is home to the oldest collection of meteorites in the world and makes crucial loans of their 4870 samples to researchers across the globe. These meteorites are fragments of the surfaces of Mars and the Moon, and surfaces and interiors of numerous asteroids, some of which have been identified and some of which have not. In order to analyse these rare rocks Natasha uses equipment most of us will have some experience of, an X-Ray scanner, more specifically a micro-CT scanner. Just like a medical CT the NHM’s micro-CT makes use of X-rays to scan through the rock and build up a 3D picture of its interior.

There are some clear differences however; primarily the strength of the beam and the duration of the scan. Rock is more impervious to X-Rays than flesh and bone requiring a much stronger beam and a longer scan time. Each scan results in a 3D image with a resolution of down to 5mm/voxel (a voxel is a 3D pixel) and around 20 – 30Gb of data.

With these images Natasha has extracted a variety of information from numerous meteorites including spotting internal structures and features that would otherwise only be found by cutting into the sample, tracing cracks to establish the possibility of internal contamination by the atmosphere of the Earth and mapping out internal fractures and pores. This final result is especially key for meteorites as the historical methods for working out the porosity of a rock sample involve dunking it in a bucket of water. This method is a purely quantitative one that tells you how much space is in the rock but not how it is distributed unlike micro-CT.

In addition submerging your sample in a tank of water definitely counts as a high contamination risk, something meteoriticists and curators try and avoid like the plague! Unlike the electron microprobe analysis discussed in the first half of this session micro-CT for meteorite analysis is a technique that is still in its infancy but it certainly holds a lot of promise, especially if we have to wait another 40 years for people to bring us back more samples from another planetary body.

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Life Story: The Race for the Double Helix

This post was contributed by Professor Nick Keep, Executive Dean of the School of Science. Professor Keep attended the Birkbeck Science Week 2016 film screening of “Life Story: The Race for the Double Helix” on Monday April 11 at the Birkbeck Cinema.

DNA

“Life Story: the race for the Double Helix”is a 1987 BAFTA award winning film length TV dramatisation of the story of the discovery of the structure of DNA. The film screening was co-introduced by Dr Richard Hamblyn from the Dept of English and Humanities, who works at the interface of science and literature, and Dr Tracey Barrett from the Dept Biological Sciences, a female protein crystallographer in a Birkbeck tradition that goes back to Rosalind Franklin.

Richard described the film as having two classic odd couples; Crick and Watson in a glossy tourist Cambridge, and Wilkins and Franklin in a rainy London, contrasting with Franklin’s former sunny life in Paris and the easy going relationship with her previous collaborator Vittorio Luzzati, the inventor of the Luzzati plot.

The search for truth in science

Tracey outlined the importance of the science and the changes for women in Science. There are no longer men-only common rooms, such as Franklin encountered at Kings, but there are still problems. They also discussed the interplay between the search for truth in science and competition to be first and famous. Birkbeck is mentioned in the film as the place of refuge Franklin can relocate to escape the oppressive atmosphere at Kings. Richard quoted Rosalind Franklin as writing that she “will be moving from a palace” (Kings) “to a slum” (Birkbeck)” but I’m sure I will find Birkbeck pleasanter all the same”.

The film itself was excellent with Juliet Stevenson as Franklin, Alan Howard as Wilkins, Tim Piggot-Smith as Crick and Jeff Goldblum as the ambitious Watson. I found Clive Panto very convincing (if a little overweight) as Max Perutz, the only character that I knew in person, albeit later in his life. The widespread smoking was an authentic period touch that stood out for me. Whether a 2017 production would do that I am not sure.

Discussing the injustice

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By Source, Fair use, https://en.wikipedia.org/w/index.php?curid=46189683

After the showing, the audience discussed the injustice of Rosalind Franklin not winning the Nobel Prize. Firstly the prize is never awarded to more than three people so a decision had to be made and by this time Rosalind Franklin had tragically died. Interestingly, checking afterwards, the ban on posthumous prizes was only formalised in 1974, well after the 1962 award for DNA (See section on Posthumous Nobel Prizes), although observed in practice for Science awards until it was discovered that one of the 2011 winners for Physiology and Medicine had died three days before the announcement, but this was not known to the Swedish Academy when they released the names.

The 1961 Peace prize, just a year before the Medicine and Physiology award to Crick, Watson and Wilkins, was knowingly awarded to the UN Secretary General, Dag Hammarskjöld, who had recently died in an air crash, as was the 1931 Literature Prize to a Swedish Poet. Whether Rosalind Franklin is better known now for not having been awarded the Nobel Prize, than she would have been if she had received it is a matter for debate. Birkbeck, where she worked at the end of her life, remembers her via the Rosalind Franklin Laboratory built in 1996 and, from this year, the annual Rosalind Franklin lecture by a leading woman scientist in a field Birkbeck researches in.

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The Search for Life in the Universe

This post was contributed by Phyllis Hughes, editor of U3A magazine Sources. Phyllis attended the Birkbeck Science Week 2016 U3A talk: “The search for life in the universe – The new science of astrobiology” on Monday April 11 at the University of East London.

Science Week - astrobiology event Ian CrawfordThe search for life in the universe ranging from simple organisms to intelligent beings was the subject for Prof Ian Crawford from Birkbeck University.

Prof Crawford is an astrobiologist whose work looks at the possibility of life on other planets. He told his audience of members of the University of the Third Age that Earth was the only place currently where life was known to exist.

Scientists therefore were concentrating their research on planets that were thought to have been similar to Earth when life first developed.

“Life appeared on Earth fairly soon after the planet formed,” he said. “However it took a long time for microbiological life to develop into multi-cell animals.”

He said that Mars was currently of interest because it was known that it had an atmosphere similar to Earth 4bn years ago when simple life forms were first developing. This atmosphere contained water and was comparatively warm.

In 1976 the Viking space probes took samples of the Mars soil to see if there was evidence of life, but these had proved negative. However the samples were very small and research was continuing in this field.

Professor Ian Crawford

Professor Ian Crawford

Other places that were thought to be worth investigating included one of the moons of Jupiter, called Europa which was first discovered by Galileo in 1609.

Two moons of Saturn, Enceladus and Titan were also potentially similar in atmosphere.

As well as examining the geology there was also interest in trying to pick up radio signals from the galaxy that might have been transmitted by intelligent life. The Search for Extra Terrestial Intelligence (SETI) had also proved negative so far.

“Given all the necessary factors I think the possibility of advanced technological life is rare,” Prof Crawford said.

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View the full Science Week 2016 programme of free events

Courses at the School of Science

Prof Ian Crawford

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