Archive for the The Universe and Stuff Category

Planet Wave

Posted in Jazz, Poetry, The Universe and Stuff with tags , , on November 17, 2009 by telescoper

Regular readers of this blog (both of you) will know that from time to time I like to post little bits of poetry. The verses are usually related to astronomy (or science generally)  and they’re usually things I come across pretty much by accident when I’m browsing through the books of poetry I occasionally buy. This evening I was leafing through a collection called A Book of Lives, by the popular and highly respected Scottish national poet Edwin Morgan.  In the middle of this set is a long sequence of poems called Planet Wave, each of which is to do with a specific historical episode or important character, such as Copernicus or Darwin. The first poem in the cycle is about the Big Bang so I thought it would be a good choice.

However, regular readers will also know that I like to post bits of jazz on here too – although the blog statistics suggest that these are much less popular than the poetry!  I read in the Book of Lives that the first half the sequence of poems making up Planet Wave was commissioned by the Cheltenham International Jazz Festival and set to music by the excellent Tommy Smith. The poetry and music combination was first performed in Cheltenham Town Hall on 4 April 1997.

Great, I thought. Here’s a chance to combine jazz and poetry (for what would only be the second time on here, the first being this post). Unfortunately, though, I’ve been unable to locate any recording of a performance of this work. I found an interview with Tommy Smith on the net which suggests a recording was made but never released. I’d certainly love to hear it and I hope that there might be a jazz fan out there somewhere who knows what happened to it.

Anyway, in the absence of the music here’s just the first verse of the first poem of the cycle.  As you will see, Morgan’s style is very inventive, often extremely funny, and always extremely Scottish.

In the Beginning
(20 Billion BC)

Don’t ask me and don’t tell me. I was there.
It was a bang and it was big. I don’t know
what went before, I came out with it.
Think about that if you want my credentials.
Think about that, me, it, imagine it
as I recall it now, swinging in my spacetime hammock,
nibbling a moon or two, watching you.
What am I? You don’t know. It doesn’t matter.
I am the witness, I am not in the dock.
I love matter and I love anti-matter.
Listen to me, listen to my patter.

(Reproduced by kind permission of Carcanet Press.)

If you want to read the rest you’ll have to buy the book! And if anyone out there knows what happened to the recording of Planet Wave please let me know. I’d love to hear it!

The Monkey Complex

Posted in Bad Statistics, The Universe and Stuff with tags , , , , , on November 15, 2009 by telescoper

There’s an old story that if you leave a set of monkeys hammering on typewriters for a sufficiently long time then they will eventually reproduce the entire text of Shakespeare’s play Hamlet. It comes up in a variety of contexts, but the particular generalisation of this parable in cosmology is to argue that if we live in an enormously big universe (or “multiverse“), in which the laws of nature (as specified by the relevant fundamental constants) vary “sort of randomly” from place to place, then there will be a domain in which they have the right properties for life to evolve. This is one way of explaining away the apparent fine-tuning of the laws of physics: they’re not finely tuned, but we just live in a place where they allowed us to evolve. Although it may seem an easy step from monkeys to the multiverse, it always seemed to me a very shaky one.

For a start, let’s go back to the monkeys. The supposition that given an infinite time the monkeys must produce everything that’s possible in a finite sequence, is not necessarily true even if one does allow an infinite time. It depends on how they type. If the monkeys were always to hit two adjoining keys at the same time then they would never produce a script for Hamlet, no matter how long they typed for, as the combinations QW or ZX do not appear anywhere in that play. To guarantee what we need the kind their typing has to be ergodic, a very specific requirement not possessed by all “random” sequences.

A more fundamental problem is what is meant by randomness in the first place. I’ve actually commented on this before, in a post that still seems to be collecting readers so I thought I’d develop one or two of the ideas a little.

 It is surprisingly easy to generate perfectly deterministic mathematical sequences that behave in the way we usually take to characterize indeterministic processes. As a very simple example, consider the following “iteration” scheme:

 X_{j+1}= 2 X_{j} \mod(1)

If you are not familiar with the notation, the term mod(1) just means “drop the integer part”.  To illustrate how this works, let us start with a (positive) number, say 0.37. To calculate the next value I double it (getting 0.74) and drop the integer part. Well, 0.74 does not have an integer part so that’s fine. This value (0.74) becomes my first iterate. The next one is obtained by putting 0.74 in the formula, i.e. doubling it (1.48) and dropping  the integer part: result 0.48. Next one is 0.96, and so on. You can carry on this process as long as you like, using each output number as the input state for the following step of the iteration.

Now to simplify things a little bit, notice that, because we drop the integer part each time, all iterates must lie in the range between 0 and 1. Suppose I divide this range into two bins, labelled “heads” for X less than ½ and “tails” for X greater than or equal to ½. In my example above the first value of X is 0.37 which is “heads”. Next is 0.74 (tails); then 0.48 (heads), 0.96(heads), and so on.

This sequence now mimics quite accurately the tossing of a fair coin. It produces a pattern of heads and tails with roughly 50% frequency in a long run. It is also difficult to predict the next term in the series given only the classification as “heads” or “tails”.

However, given the seed number which starts off the process, and of course the algorithm, one could reproduce the entire sequence. It is not random, but in some respects  looks like it is.

One can think of “heads” or “tails” in more general terms, as indicating the “0” or “1” states in the binary representation of a number. This method can therefore be used to generate the any sequence of digits. In fact algorithms like this one are used in computers for generating what are called pseudorandom numbers. They are not precisely random because computers can only do arithmetic to a finite number of decimal places. This means that only a finite number of possible sequences can be computed, so some repetition is inevitable, but these limitations are not always important in practice.

The ability to generate  random numbers accurately and rapidly in a computer has led to an entirely new way of doing science. Instead of doing real experiments with measuring equipment and the inevitable errors, one can now do numerical experiments with pseudorandom numbers in order to investigate how an experiment might work if we could do it. If we think we know what the result would be, and what kind of noise might arise, we can do a random simulation to discover the likelihood of success with a particular measurement strategy. This is called the “Monte Carlo” approach, and it is extraordinarily powerful. Observational astronomers and particle physicists use it a great deal in order to plan complex observing programmes and convince the powers that be that their proposal is sufficiently feasible to be allocated time on expensive facilities. In the end there is no substitute for real experiments, but in the meantime the Monte Carlo method can help avoid wasting time on flawed projects:

…in real life mistakes are likely to be irrevocable. Computer simulation, however, makes it economically practical to make mistakes on purpose.

(John McLeod and John Osborne, in Natural Automata and Useful Simulations).

So is there a way to tell whether a set of numbers is really random? Consider the following sequence:

1415926535897932384626433832795028841971

Is this a random string of numbers? There doesn’t seem to be a discernible pattern, and each possible digit seems to occur with roughly the same frequency. It doesn’t look like anyone’s phone number or bank account. Is that enough to make you think it is random?

Actually this is not at all random. If I had started it with a three and a decimal place you might have cottoned on straight away. “3.1415926..” is the first few digits in the decimal representation of p. The full representation goes on forever without repeating. This is a sequence that satisfies most naïve definitions of randomness. It does, however, provide something of a hint as to how we might construct an operational definition, i.e. one that we can apply in practice to a finite set of numbers.

The key idea originates from the Russian mathematician Andrei Kolmogorov, who wrote the first truly rigorous mathematical work on probability theory in 1933. Kolmogorov’s approach was considerably ahead of its time, because it used many concepts that belong to the era of computers. In essence, what he did was to provide a definition of the complexity of an N-digit sequence in terms of the smallest amount of computer memory it would take to store a program capable of generating the sequence. Obviously one can always store the sequence itself, which means that there is always a program that occupies about as many bytes of memory as the sequence itself, but some numbers can be generated by codes much shorter than the numbers themselves. For example the sequence

111111111111111111111111111111111111

can be generated by the instruction to “print 1 35 times”, which can be stored in much less memory than the original string of digits. Such a sequence is therefore said to be algorithmically compressible.

There are many ways of calculating the digits of π numerically also, so although it may look superficially like a random string it is most definitely not random. It is algorithmically compressible.

I’m not sure how compressible Hamlet is, but it’s certainly not entirely random. When I studied it at school I certainly wished it were a little shorter…

The complexity of a sequence can be defined to be the length of the shortest program capable of generating it. If no algorithm can be found that compresses the sequence into a program shorter than itself then it is maximally complex and can suitably be defined as random. This is a very elegant description, and has good intuitive appeal.  

I’m not sure how compressible Hamlet is, but it’s certainly not entirely random. At any rate, when I studied it at school, I certainly wished it were a little shorter…

However, this still does not provide us with a way of testing rigorously whether a given finite sequence has been produced “randomly” or not.

If an algorithmic compression can be found then that means we declare the given sequence not to be  random. However we can never be sure if the next term in the sequence would fit with what our algorithm would predict. We have to argue, inferentially, that if we have fit a long sequence with a simple algorithm then it is improbable that the sequence was generated randomly.

On the other hand, if we fail to find a suitable compression that doesn’t mean it is random either. It may just mean we didn’t look hard enough or weren’t clever enough.

Human brains are good at finding patterns. When we can’t see one we usually take the easy way out and declare that none exists. We often model a complicated system as a random process because it is  too difficult to predict its behaviour accurately even if we know the relevant laws and have  powerful computers at our disposal. That’s a very reasonable thing to do when there is no practical alternative. 

It’s quite another matter, however,  to embrace randomness as a first principle to avoid looking for an explanation in the first place. For one thing, it’s lazy, taking the easy way out like that. And for another it’s a bit arrogant. Just because we can’t find an explanation within the framework of our current theories doesn’t mean more intelligent creatures than us won’t do so. We’re only monkeys, after all.

Lev Kofman

Posted in The Universe and Stuff with tags , on November 14, 2009 by telescoper

June 17, 1957 – November 12, 2009

DSC00517 copy___china_head_cut_LRI heard yesterday from Andrew Jaffe of the death a few days ago of Lev Kofman (left), from cancer. Lev was a wonderfully spontaneous  and generous character as well as a very fine physicist. I hadn’t known that he was ill, which made the news of his death all the more shocking and the sense of loss even deeper. My thoughts and those of my colleagues who were lucky enough to know Lev are with his family and friends at what must be difficult time for them.

I first met Lev about twenty years ago and we bumped into each other fairly frequently over the following years. Then I went on sabbatical to Toronto, where Lev was based, and therefore spent a quite a bit of  time with him talking cosmology, drinking and failing to play football.  It’s hard to believe that now, just a few years later, the wonderful light he cast on those around him has actually gone out. He was such a hive of activity all the time I once joked that I thought the Lev should be a unit of energy (like Gev).

I’m sure there will be very many formal tributes paid to Lev by people who knew him far better than me – there is an item on cosmic variance which is worth reading if you didn’t know much about him. For my part, I’ll just say that I liked and admired him enormously and the field of cosmology will be much poorer for his passing.

An email letter was sent out by Lev’s family and friends, which I hope they will not mind me reproducing here, as I think it perfectly conveys the deep affection which Lev inspired in all who had the opportunity to meet and work with him.

We are deeply saddened  to inform you that the fabulous Lev Kofman, husband of Anna, father of Sergei 13 and Maria 15, brother of Svetlana, and our great friend, died in the early morning of November 12 from cancer. Many of you were able to commune with Lev as the situation deteriorated over the past weeks, by visits, phone calls, and emails read to him. We are deeply grateful for that: and it provided some solace for Lev to know the tremendous impact he has had on the lives of so many of you.

He bravely kept the physics going strong throughout his illness, characteristic of Lev. His scientific outpourings and influence  will transcend this passage. As you know, he made fundamental contributions to Lambda cosmology and dark energy, structure in the cosmic web, inflationary theory, its Gaussian and non-Gaussian aspects, and gravitational waves. He initiated and developed the theory of preheating, showing how all matter could arise from a coherent vacuum energy at the end of inflation, his cosmic baby. And much more besides. He was the quintessential leader, for CITA and CIFAR as a whole, and for the vibrant early universe group he established, providing inspirational guidance to a generation of young researchers.

He felt the physics to his very core. Beyond this, it is the indomitable, fun-loving, deeply philosophical spirit, a gourmand of life in all its manifestations, that we will miss so much.

With our best wishes in these sad times,

Anna Chandarina (Kofman)
Svetlana Kofman
Dick Bond
Andrei Linde
Renata Kallosh

And if you never had the chance to see the man in action you can find some videos of lectures he gave at the Perimeter Institute here.

For Your Listening Pleasure…

Posted in The Universe and Stuff with tags , , , on November 12, 2009 by telescoper

Well, this is blogging made easy. I’ve just cut-and-pasted the following item directly from the School’s news page with very few alterations, but it’s all done for a good reason, so please read on:

A leading member of the School of Physics and Astronomy at Cardiff University, whose research helped create one of the most powerful and ambitious astronomical satellites ever made will feature in a two-part Radio 4 programme.

The Herschel Space Telescope is a two-part series to be aired on Radio 4 on Wednesday 18th November, 11:00-11:30am and Wednesday 25th November, 11:00-11:30am. BBC science reporter Jonathan Amos follows the engineers and scientists working on the SPIRE instrument for the European Space Agency’s Herschel satellite. Herschel is one of the most important missions in the history of European spaceflight and was launched successfully on May 14 this year.

The SPIRE instrument was built by an international team led by Professor Matt Griffin, School of Physics and Astronomy. The programme tells the story of the UK SPIRE team, including several members from Cardiff, as they prepared for the launch of Herschel and as the first results came in.

As well as Professor Griffin, other members of staff in the School of Physics and Astronomy who contributed to the project are also featured. They include: Professor Steve Eales, Dr Jon Davies, Dr Kate Isaak, and Dr Pete Hargrave as well as post-doctoral researchers Dr Jason Kirk, Dr Michael Pohlen, and Dr Luca Cortese.

Professor Matt Griffin

Herschel carries the biggest mirror ever sent to space and is already giving astronomers their best view yet of the Universe at far-infrared and sub-millimetre wavelengths. It can peer through obscuring clouds of dust to look at the early stages of star birth and galaxy formation; it can examine the composition and chemistry of comets and planetary atmospheres in the Solar System; and it is able to study the star-dust ejected by dying stars into interstellar space which forms the raw material for planets like the Earth.

Professor Griffin said: “With its big telescope and sophisticated and sensitive instruments, including SPIRE, Herschel is a very powerful observatory for many studies from our own solar system to the most distant galaxies. Already we can see that its results will reveal how stars like the Sun are forming in our own galaxy today, how planetary systems can develop from the dust and gas around young stars, and how the galaxies grew and evolved over cosmic time.

“Astronomers from Cardiff are at the forefront in making these exciting scientific discoveries – we are delighted that the work of Cardiff scientists will be featured in such an important radio programme.”

I should also point out that BBC Radio 4 programmes can be listened to online, and are available to download for a week after the broadcast from the BBC website (even to foreigners).

PS. I should also mention that today’s “Material World” (another Radio 4 programme) was a special edition from Cardiff University and also featured an astronomy item. If you missed it, or if you want to hear it again, you can listen to it here.


Viva Voce

Posted in Biographical, The Universe and Stuff with tags , on November 11, 2009 by telescoper

Just back from a flying visit to the beautiful city of Edinburgh, where I was involved in the examination of a PhD candidate at the Institute for Astronomy, which is housed on the site of the Royal Observatory.

For those of you not familiar with how this works, a PhD involves doing research into a particular topic and then writing up what you’ve done in a thesis. The thesis is a substantial piece of work, often in the region of 100,000 words (200 pages or so), which is then assessed by two examiners (one internal to the university at which the research was done, and one external). They read copies of the thesis and then the candidate has to defend it in an oral examination, which was what happened today, after which they make a recommendation to the university about whether the degree should be awarded.

At most universities the supervisor does not attend the oral examination, but is not normally required to go into hiding for the day, which is what seemed to happen in this case…

There aren’t many rules for how a viva voce examination should be conducted or how long it should last, but the can be as short as, say, 2 hours and can be as long as 5 hours or more. The examiners usually ask a mixture of questions, some about the details of the work presented and some about the general background. The unpredictable content of a viva voce examination makes it very difficult to prepare for, and it can be difficult and stressful for the candidate (as well as just tiring, as it can drag on for a long time). However, call me old-fashioned but I think if you’re going to get to call youself Doctor of Philosophy you should expect to have to work for it. Some might disagree.

As it happens, my own PhD examination 20 years ago was quite long (about 4hrs 30 minutes) and my external examiner was John Peacock, who happened to be the supervisor of today’s candidate Berian James. It wasn’t a deliberate consequence of me wanting to take vicarious revenge as external examiner on John’s student, but this turned out to be a long examination too. We did break twice (once, briefly, for the remembrance day silence and then for a longer period for lunch), but it was still a lengthy affair.

Obviously I can’t give details of what went on in the examination except that it was long primarily because the thesis was very interesting and gave us lots to discuss. In the end internal examiner Philip Best and I agreed to recommend the award of a PhD. Berian then went off to celebrate while we completed the necessary paperwork. At Edinburgh as in most UK universities, the examiners simply make a recommendation to a higher authority (e.g. Board of Graduate Studies) to formally award the degree, but in the overwhelming majority of cases they follow the recommendation.

After doing the paperwork I still had time to join the party for a glass or two of fizzy. At the do and at various points during the day I had the chance to say hello to some old friends, including Andy Taylor, Bob Mann, and Alan Heavens who all work at the ROE and Richard Nelson who was there for a meeting that I hadn’t known about when we arranged the date and time of the viva.

All in all, it was a very pleasant trip. Although I had to dash around to and from airports a bit getting to and from Scotland, all the planes went on time and since it’s less than an hour flying time from Cardiff to Edinburgh, it was all remarkably hassle-free.

Just before I left to get a taxi to the airport I had a quick chat with one of the PhD students, Alina Kiessling, who joked that I must be rushing off to write about the day on my blog. I never had time to read blogs when I was a PhD student (but  they hadn’t been invented then).

Perhaps I should start charging people to put their name in lights on In the Dark

Planck’s Progress

Posted in The Universe and Stuff with tags , , on November 10, 2009 by telescoper

Only time for a very quick post today, so I thought I’d just pass on some news I got via Chris North about how Planck is doing. As it happens, the satellite has recently reached  the point where it has observed about half the sky. It spins on its axis in rather stately fashion (at about one revolution per minute) and, as it moves in its orbit, that sweeps the telescope across the celestial sphere. Each scan is almost a great circle, but  these gradually creep around over about a six month period to cover the whole sky.

The nice picture below, in ecliptic coordinates, shows how far it has got. You can also see the Galactic plane, arching across the sky and showing up clearly at the frequencies Planck is sensitive to.

Planck3NovSkyCoverage

The Planck Consortium had an official meeting last week in Bologna at which they drank lots of wine and ate lots of food, but other than that nobody who was there has told me anything.

It’s all very hush hush don’t you know.

I want it painted … beige?

Posted in The Universe and Stuff with tags , , , , , on November 4, 2009 by telescoper

I was quite pleased when I saw that Pass Notes No 2,677 in Today’s Guardian was about “the universe”. Like the other pieces in this series, it looks at the subject matter from a deliberately bizarre angle, focussing on the fact that it appears to be coloured beige, or at least if you blend the light from all the stars we can see in the right proportions, that’s the colour you would get.

Actually the work discussed in this item was done quite along time ago; it was featured in a New Scientist article in 2002. One of the authors, Karl Glazebrook had previously claimed that the colour produced by all the stars in all the galaxies that could be seen was in fact something like turquoise. For some reason, this trivial bit of science fluff captured the (obviously limited) imagination of journalists around the world. However it turned out to be have been wrong and a grave announcement was made pointing out that the Universe was actually more like beige. This story gave a few people their 15 minutes of fame, but I think the episode made cosmologists as a whole look very silly.

I had hoped this would be forgotten but, the Guardian decided to revive memories of the affair today, with obviously humorous intent. They also called Glazebrook an “astrologist”, although that appears to have been a mistake rather than a joke as it has now been changed to “astrophysicist”.

Anyway, this important observation requires a theoretical explanation and I now want to step into the limelight beigelight to offer a radical insight into the vexed issue of cosmological chromaticity.
My hypothesis has its inspiration in TV shows like House Doctor in which homeowners wishing to impress prospective purchasers are always advised to paint everything beige or magnolia. Since the Divine Creator appears to have decorated the Universe according to the same prescription, the obvious inference is that the cosmos is about to be put on the market. He might have had the courtesy to tell the sitting tenants.

Come to think of it, Glazebrook missed a trick here. We astrophysicists are always being castigated for not doing anything that leads to wealth creation. What he should have done was to produce a paint with the same colour as the Universe. Glazebrook Beige has a nice ring to it.

Highlights

Posted in Biographical, The Universe and Stuff with tags , , on November 2, 2009 by telescoper

Despite popular demand, here is more of the Unravelling the Universe show I posted a little bit from a few days ago. My total screen time on this programme only amounted to a couple of minutes, so I asked if it was possible to do an appropriate edit of the hour-long footage. Unfortunately, Ed got the wrong idea, so removed most of the highlights and left practically only the few minutes with me in them. You just can’t get the help these days.

The film  was shot in a studio in Greenford and I had to hang around there a long time before they even started shooting. I think that was because of the lights. I need a special form of  illumination if I am to present the illusion of having three dimensions. The director had insisted I wear my leather jacket for the sequence and under the very powerful lights I was sweating so much I had to wear make-up to stop me shining.

They reckon that there is a ratio of about 100:1 of film shot to film broadcast on programmes like this, and this is probably even higher when the subject is as inarticulate as me. In my memory it certainly took several hours just for my little bits.

If nothing else this tape gives you the chance to see Rocky Kolb in a splendid jumper that puts that of the new Lucasian professor well and truly in the shade. What was that about chromodynamics?

The Michael Green Experience

Posted in Biographical, The Universe and Stuff with tags , , , on October 30, 2009 by telescoper

It’s been a couple of weeks since the University of Cambridge announced that the successor to Stephen Hawking as Lucasian Professor  of Mathematics would be Michael Green, who is best known for his work on string theory. Heartiest congratulations to him for reaching a position of such eminence.

I was trying to think of a suitable way of marking the occasion of his election to this prestigious post when I suddenly remembered that we were actually on a TV programme together years ago. The show in question was called Unravelling the Universe and was first broadcast in December 1991 as part of a science documentary series called Equinox.

I eventually found my ancient VHS copy of the broadcast master tape of this show and persuaded Ed and Stephen, two of the excellent elves that work in the School of Physics & Astronomy here at Cardiff University, to transfer it to a digital format and put a bit on Youtube for all to see. Many thanks to them for their help.

Other people involved in the programme included Rocky Kolb, Chris Isham and Paul Davies but the short (2-and-a-half minute) clip below features just Michael Green (who basically put the show together) and myself (who was just there to make up the numbers), plus wonderful narration by the late great Peter Jones.

Michael Green hasn’t changed a bit in 18 years. In fact, I saw him last year and am sure he was even wearing the same sweater.

I, on the other hand….Oh dear.

The Edge of Darkness

Posted in The Universe and Stuff with tags , , , on October 29, 2009 by telescoper

I just picked up an item from the BBC Website that refers to news announced in this week’s edition of Nature of the discovery of a gamma-ray burst detected by NASA’s Swift satellite.  The burst itself was detected in April this year and I had a sneak preview that something exciting was going to be announced earlier this month at the Royal Astronomical Society meeting on October 9th. However, today’s press releases still managed to catch me on the hop owing to the fact that a rather different story had distracted my attention…

In fact, detections of gamma-ray bursts are not all that rare. Swift observes one every few days on average. Once such a source is found through its gamma-ray emission, a signal is sent to astronomers around the world who then work like crazy to detect an optical counterpart. If and when they find one, they try to measure the spectrum of light emitted in order to determine the source’s redshift. This is very difficult for the distant ones, and is not  always successful.

However, what happened in this case – called GRB 090423 – was that a spectrum was that not one but two independent teams obtained optical spectra of the  object in which the gamma-ray burst must have happened. What each time found was that their spectrum showed a sharp cut-off at wavelengths shorter than a given limiting value.

Hydrogen is very effective at absorbing radiation with wavelengths shorter than 91.2 nm (the so-called Lyman limit, which is in the ultraviolet part of the spectrum), and all galaxies contain large amounts of hydrogen; hence galaxies are virtually dark at wavelengths shorter than 91.2 nm in their rest-frame. The position of the break in an observed frame will be at a different wavelength owing to the effect of the cosmological redshift.

The Lyman break for the host of  GRB 090423 appears not in the ultraviolet but in the infrared, indicating a very large redshift. In fact, it’s a truly spectacular  8.2.

Together with the direct observations of galaxies at high redshifts I blogged about a month or so ago, this discovery helps push back the frontiers of our knowledge of the Universe not just in space but also in time. A quick calculation reveals that in the standard cosmological model, light from a source at redshift 8.2 has taken about 13.1 billion light years to reach us. The gamma-ray burst therefore exploded about 600 million years after the Big Bang.

Another interesting thing about this source is its duration. The optical afterglow of a gamma-ray burst  decays with time. Gamma-ray bursts are usually classified as either short or long, depending on the decay time with the dividing line between the two classes being around 2 seconds. The optical afterglow of GRB 090423 lasted about ten seconds. But that doesn’t make it a long burst. We actually see the afterglow stretched out in time by the same redshift factor as an individual photon’s wavelength. So in the rest frame of the source the optical glow was only a bit over a second in duration, i.e. it was a short burst.

Long gamma-ray bursts are thought to be associated with core-collapse supernovae which arise from the self-destruction of very massive stars with very short lifetimes. The fact that such things die young means that they are only found where star formation has happened very recently. One might expect the earliest gamma-ray bursts to therefore be of this type.

I don’t think anyone is really sure what the shorter ones really are, but they  seem to happen in regions without active star formation in which the stellar populations are quite old, such as in elliptical galaxies. The fact that the most distant GRB yet discovered happens to be a short burst is very interesting. How can there be an old stellar population at a time when the  Universe itself was so young?

If the Big Bang theory is correct, astronomers  should eventually be able to reach back so far in time that the Universe was so young that no stars had had time to form. There would be no sources of light to detect so we would have reached the edge of darkness. We’re not there yet, but we’re getting closer.