Archive for March, 2010

Astronomy with Knobs on

Posted in The Universe and Stuff with tags , , , on March 12, 2010 by telescoper

I just saw a splendidly smutty blog post which contains graphic examples of astronomical objects in the form of male genital organs. Since this appears to be an entirely suitable topic for a Friday afternoon blog post, here is my suggestion of  a contribution to her gallery. It’s the X-rated X-ray satellite XMM Newton which, as you can see, has a disturbingly phallic appearance.

I wonder if astropixie might be able to make room for this one?

Astronomy Look-alikes, No. 18

Posted in Astronomy Lookalikes with tags , on March 11, 2010 by telescoper

I wonder if anyone else has noticed the similarity between Ray Sharples of Durham University and erstwhile Geordie Messiah Kevin Keegan? They sound similar too!

Taken for Granted

Posted in Science Politics with tags , , , , on March 10, 2010 by telescoper

It’s been a couple of weeks since the Astronomy group in the School of Physics & Astronomy at Cardiff University was informed of the result of its recent application to the Science and Technology Facilities Council (STFC) for a continuation of its rolling grant. I haven’t been able to post anything about it because it has led to some difficult personal situations and we didn’t want anyone to hear about it other than face to face from relevant members of the department.

In case you weren’t aware, a rolling grant covers a 5-year but a group holding one has to apply for renewal every three years at which point the programme of research is reviewed by a panel of experts. If this review is positive a new 5-year grant is awarded and the two years remaining on the old grant or cancelled. In the case of a negative review, however, there is two years’ grace until the funding is terminated, giving the applicants the chance to try again next time.

At least that’s what used to happen.

The previous Cardiff Astronomy roller supported 6 postdoctoral research assistants (PDRAs) as well as providing other funds for travel, equipment, infrastructure and other staff time. This time we requested an increase, primarily in order to enable us to exploit the wonderful data coming from the Herschel observatory. I joined Cardiff after the last review so I wasn’t included in the existing  funding package. However, I did succeed in getting a standard grant in last year’s grant round which provides support for a 3-year period. This time, I applied to have this grant subsumed into the rolling programme when it completes in 2012. I requested an extension to the 3-years to tide this over until the next rolling grant and bring me into phase with the rest of the group.

That was the idea, anyway. STFC is extremely short of money, so despite what we felt was a strong case for supporting our Herschel work we weren’t particularly optimistic of a good outcome, especially since  additional cuts to research grants were announced last December.  In fact the rolling grant application went in last year, but the process is extremely lengthy. Three of us had to go to Swindon last October to present the case to the grants panel. The panel had apparently completed its work by December, but when new cuts were announced they had to revisit their decisions. That’s why we were only informed at the end of February of the level of support that we would get from April 1st this year.

In fact we received two announcements, one detailing what we would have got had the panel’s original recommendations been followed, then another showing the result of the additional 15% cut decided in December. In the first we were cut from 6 PDRAs to 5, but in the second an additional position was cut leaving us with 4 surviving from the previous grant. Moreover, STFC has basically abandoned the rolling grant concept entirely, and refused us permission to let the previous grant roll out. We had no choice but to accept the new grant, which means that we have insufficient funds from 1st April 2010 to honour contracts already issued to two scientists. Not a pleasant situation to be presented with. We’ve managed to find a way of coping to the extent that nobody will be made redundant in the short-term, but it’s still a time of great uncertainty for those involved.

For my own part, the circumstances are a bit better. The panel did award me an extension of my grant to enable me to merge my research with the rest of the programme by the next review date. They also – unexpectedly, I must admit – gave me a small uplift in my existing funding. I’ll be OK, at least for another 3 years.

Overall, we’re disappointed. The outcome wasn’t as good as we’d hoped but, then again, it wasn’t as bad as we’d feared. Taking into account the standard grant I hold, we’ve gone down from 7 PDRAs to 5. I’ve heard rumours of much more drastic cuts elsewhere, and I’m sure other departments are feeling the pain much more than we are right now. I don’t have a clear picture of what has happened nationally, so I’d be grateful for any information people might be prepared to divulge through the comments box as long as you don’t betray any confidences!

The whole business of securing grant funding can be deeply frustrating, and sometimes the  decisions seem bewildering. However, I’ve been on these panels before and I know how hard it is, so I’m never tempted to whinge. In fact, I’m going to be joining the panel again for this round. Not that I’m looking forward to it very much!

However, I can’t resist ending with a comment about the current management of STFC. It really seems quite absurd to be cutting grant funding at precisely the time that Herschel and Planck are starting to deliver huge quantities of exquisite data.  I say that as a scientist of course, not a civil servant. However, the prevailing mentality at STFC – instigated by the Treasury – seems to be that science part of their remit is much less important than the technology and the facilities. Although the Science Minister Lord Drayson recently announced a proposal that purports to fix some of STFC’s difficulties, this seems more than likely to keep grant funding at a miserably low level for the indefinite future. The STFC management’s readiness to rewrite the rules governing rolling grants, cut funding at absurdly short notice, and raid the grant budget in order to solve problems elsewhere has convinced me that there will be no improvement until there are people at the top that recognize that it’s science that matters, that science is done by people, and that the way to manage those people is not to treat them the way they are doing now.

Especially if they want people to provide free advice to their panels…

To look at a star by glances..

Posted in Literature, The Universe and Stuff with tags , , , , , on March 9, 2010 by telescoper

I’ve blogged before about my love of classic detective stories and about the intriguing historical connections between astronomy and forensic science. However, I recently finished reading a book that gave me a few more items to hang on that line of thought so I thought I’d do a quick post about them today.

I picked up a copy of The Suspicions of Mr Whicher by Kate Summerscale when I saw it in a stack of discounted books in Tesco a few monthsa go. I thought it might be mildly diverting, so I bought it. It turned out to be a fascinating read. I won’t spoil it by telling too much about the story, but it is basically an investigation into the circumstances surrounding a real-life murder that happened on 30th June 1860. The case involved a truly shocking crime, the brutal slaying of a young boy, but it also offers great insights into the history of the Criminal Investigation Division (CID) of the Metropolitan Police, which was based at Scotland Yard from about 1842 onwards. Mr Jack Whicher was the Yard’s most celebrated detective at the time, but this crime went unsolved until, about five years later, the perpetrator walked into a police station and confessed to the murder.

In telling the story, Kate Summerscale touches on a lot of fascinating social history. For example, I had never realised that in the early days of the CID people were strongly opposed to the idea that plain clothes policemen might be snooping about so all detectives were required to wear their uniforms even when off duty! It’s also fascinating to note that the rise of the true-life detective coincided with the rise of the detective story in popular fiction.

Edgar Allan Poe’s short story The Murders in the Rue Morgue, generally accepted to have been the first real detective story, was first published in 1841. Even in this first example of the genre, we find a clear parallel being drawn with astronomy by the detective Dupin:

Thus there is such a thing as being too profound. Truth is not always in a well. In fact, as regards the more important knowledge, I do believe that she is invariably superficial. The depth lies in the valleys where we seek her, and not upon the mountain-tops where she is found. The modes and sources of this kind of error are well typified in the contemplation of the heavenly bodies. To look at a star by glances–to view it in a side-long way, by turning toward it the exterior portions of the retina (more susceptible of feeble impressions of light than the interior), is to behold the star distinctly–is to have the best appreciation of its lustre–a lustre which grows dim just in proportion as we turn our vision fully upon it. A greater number of rays actually fall upon the eye in the latter case, but in the former, there is the more refined capacity for comprehension. By undue profundity we perplex and enfeeble thought; and it is possible to make even Venus herself vanish from the firmament by a scrutiny too sustained, too concentrated, or too direct.

No less a figure than Charles Dickens also had thoughts along these lines. In 1850 in a short article called A Detective House Party, he compared detectives with the astronomers Urbain Leverrier and John Couch Adams who in 1846 had simultaneously discovered the planet Neptune. Dickens died in 1870 leaving his own detective story The Mystery of Edwin Drood still unfinished but his good friend Wilkie Collins did a great deal to establish the literary genre of detective fiction with The Moonstone and The Woman in White. Indeed, in the mid-19th Century the idea of detection seems to have imprinted itself on fields as diverse as natural history and journalism as well as astronomy.

The point that strikes me is that astronomy and criminal investigations are primarily observational rather than experimental. One has one Universe and one scene of the crime. In both disciplines the task is to reconstruct what happened from what is seen and what is not.

The detective instinct, brightened by genius, marked unerringly the place of that missing planet which no eye had seen, and whose only register was found in the calculations of astronomy.

I use metaphors like this quite often in popular lectures, and they seem to go down quite well. On the other hand, I’ve often had my leg pulled for admitting to watching TV programmes like CSI: Crime Scene Investigation. Admittedly, the characterisation is very weak and the plots often ridiculously far-fetched. However, these stories do at least attempt to portray something of what the scientific method is about. And that’s something that not many so-called science programmes bother to do these days.

Two Poems for March

Posted in Poetry with tags , , on March 8, 2010 by telescoper

Just time to post a couple of poems today, both of them to do with the month of March. I posted my absolute favourite poem about March around this time last year.

This is one by A.E. Housman, and is taken from his collection A Shropshire Lad.

The sun at noon to higher air,
Unharnessing the silver Pair
That late before his chariot swam,
Rides on the gold wool of the Ram.

So braver notes the storm-cock sings
To start the rusted wheel of things,
And brutes in field and brutes in pen
Leap that the world goes round again.

The boys are up the woods with day
To fetch the daffodils away,
And home at noonday from the hills
They bring no dearth of daffodils.

Afield for palms the girls repair,
And sure enough the palms are there,
And each will find by hedge or pond
Her waving silver-tufted wand.

In farm and field through all the shire
The eye beholds the heart’s desire;
Ah, let not only mine be vain,
For lovers should be loved again.

And the second is by Emily Dickinson

Dear March, come in!
How glad I am!
I looked for you before.
Put down your hat–
You must have walked–
How out of breath you are!
Dear March, how are you?
And the rest?
Did you leave Nature well?
Oh, March, come right upstairs with me,
I have so much to tell!

I got your letter, and the birds’;
The maples never knew
That you were coming,–I declare,
How red their faces grew!
But, March, forgive me–
And all those hills
You left for me to hue;
There was no purple suitable,
You took it all with you.

Who knocks? That April!
Lock the door!
I will not be pursued!
He stayed away a year, to call
When I am occupied.
But trifles look so trivial
As soon as you have come,
That blame is just as dear as praise
And praise as mere as blame.

Pix Mix

Posted in Columbo, The Universe and Stuff with tags , , on March 7, 2010 by telescoper

I just remembered that while I was at CERN last week I took a few crummy pics with my phone, so I thought I’d stick them on here.

This first one is actually of the control room of the ATLAS experiment, but it looked to me rather like the inside of a betting shop.

These two were taken in the facility where they test the magnets for the Large Hadron Collider. Each section of superconducting thingummyjig is about 10 metres long; the whole thing is 27km long so that’s a lot of sections! Although the magnets carry a huge current – 10,000 Amps – since they’re superconducting they have no resistance and therefore dissipate no power. However, they have to be kept at liquid helium temperatures, which does require quite a lot of power.

I like the sign on the second one: RISK OF LIQUID AIR.

Finally, here’s the most important one. While I am away Columbo is looked after by a lady called Helen who sends me daily updates. Here is Columbo in a characteristic pose.

Feed me. Feed me NOW!

Tosca

Posted in Opera with tags , , , on March 6, 2010 by telescoper

I’ve been so busy over the last couple of weeks that I almost forgot that the current run of Tosca at Welsh National Opera was about to come to an end without me having seen it. Nightmare. I suddenly remembered on Thursday that yesterday’s performance was the last one in Cardiff, but I managed to get tickets just in the nick of time. Unsurprisingly, there was a packed house in the Wales Millennium Centre last night; we were treated to an evening of jealousy and murder set to gorgeous music by Giacomo Puccini.

Tosca is an opera in three acts (which means two intervals, glug glug..). It’s basically a melodrama, and is set in Rome in 1800. Each act takes place in a very specific location within the eternal city. Act I is in the Church of  Sant’Andrea della Valle, Act II in the Palazzo Farnese, and the final denouement of Act III takes place among the battlements at the top of the Castel Sant’ Angelo overlooking the Tiber. The setting is so specific to time and place that it resists being monkeyed about with, done in modern dress, staged in a chip shop or whatever. Thankfully, Michael Blakemore’s production (of which this is a revival) is very firmly of the period and location required. As a longstanding opera bore, I have to admit that I have been on a Tosca pilgrimage and have visited all three locations in Rome. The scenery used in last night’s performance isn’t exactly as the real locations but it definitely evokes them very well.

(Incidentally, there was a famous reconstruction of Tosca made in 1992 in which all the action was staged at the true location. You can find an example from Act III here.)

Floria Tosca (Elisabete Matos) is a celebrated opera singer who is in love with an artist (and political radical) by the name of Mario Cavaradossi (Geraint Dodd), who helps to hide an escaped political prisoner while working on a painting in Act I. The odious Baron Scarpia (Robert Hayward), chief of police, comes looking for the convict and decides to catch Tosca and Cavaradossi too. He lusts after Tosca and hates Cavaradossi. In Act II, we find Scarpia at home eating dinner for one while Cavaradossi is being tortured in order to find out the location of the escapee. Tosca turns up to plead for his life, but she hasn’t bargained with the true depths of Scarpia’s depravity. He wants to have his way with her, and to put pressure on he lets her listen to the sound of her lover being tortured. She finally consents, in return for Scarpia’s promise to let Cavaradossi go and grant free passage to the two of them. This he seems to do, but while she is waiting for him to write the letter of conduct she sees a knife. Instead of letting Scarpia defile her, she grabs it and stabs him to death. Act III begins with Cavaradossi facing execution, sure he is about to die. Tosca is convinced that this is just a charade and that Scarpia ordered them to pretend to shoot Cavaradossi so he wouldn’t look like he was being merciful, which would be out of character. The firing squad fire and Cavaradossi falls. But it was no fake. He is dead. Tosca is distraught and bewildered. Shouts offstage reveal that the police have found Scarpia’s body and that Tosca must have murdered him. To avoid capture she hurls herself from the battlements. Her last words are “O Scarpia, avanti a Dio!” – I’ll meet you before God, Scarpia.

The opera wasn’t particularly well received when it was first performed in 1900, being famously described by one critic as “a shabby little shocker”. I think the secret of its success is twofold. First and foremost the music is wonderful throughout. Of course there are the great arias: Vissi d’arte, Vissi d’amore sung by Tosca in Act II and E Lucevan le Stelle from Act III, sung by Cavaradossi; but even apart from those tremendous set-pieces, Puccini uses the music to draw out the psychology of the characters. And that leads to the second point. Each of the three principals could have been very two-dimensional. Cavaradossi the good guy. Scarpia the bad guy. Tosca the love interest. But all the characters have real credibility and depth. Cavaradossi is brave and generous, but he succumbs to despair before his death. No superhero this, just a man. Scarpia is a nasty piece of work all right, but at times he is pathetic and vulnerable. He is monstrous, but one is left with the impression that something made him monstrous. And then there’s Tosca, proud and jealous, loving but at the same time capable of violence and spite. They’re all so real. I guess that’s why this type of opera is called Verismo!

The orchestra and cast were excellent. Elisabete Matos has a fine voice for the role, and also managed to spit venom at Scarpia in authentic fashion. Geraint Dodd sang wonderfully, I thought. E Lucevan le Stelle is done so often that it’s difficult to make it fresh but his rendition was overwhelmingly emotional. Best of all, Robert Hayward has a dark baritone voice that gave Scarpia a tremendous sense of power and danger.

The only problem with the performance was right at the end. Elisabete Matos didn’t appear on cue for her curtain call. I was baffled. Eventually she appeared on stage, helped by a member of the backstage team. She looked very unwell and was clutching her ribs. I think she must have landed badly after her fall from the battlements. I hope she’s not badly hurt.

Whoever was responsible for health and safety might be for the firing squad themselves.

The Joy of Natural Units

Posted in The Universe and Stuff with tags , , , on March 5, 2010 by telescoper

I’m glad it’s the end of the week. It’s been ridiculously busy. It didn’t help that I was already exhausted before it started, after a hectic three days in Geneva. Part of the reason for being so heavily occupied is that my teaching duties have just doubled. I teach the second half of a module called Nuclear and Particle Physics, and I’ve just taken over  for the second half of the semester to cover the part about particle physics. I started my set of 11 lectures with one about natural units, which is a lot of fun because it usually divides the class into two opposing camps.

About half the students think natural units are crazy, and the other half think they’re great. I’m in the second camp. The motivation is straightforward: particle physics combines quantum theory, which involves Planck’s constant

\hbar \simeq 1.05 \times 10^{-34}\,\,\,{\rm Js}

with special relativity, which involves the speed of light

c\simeq 3 \times 10^{8}\,\,\,{\rm m s}^{-1} .

Using everyday SI units (metres, seconds and kilograms) to deal with quantities that are either ridiculously small or ridiculously large doesn’t make any sense but, more importantly, the SI units don’t really reflect the physics very clearly.

In natural units we take these two constants to be equal to unity, so they don’t appear in any formulae:

\hbar = c =1

For example, the energy invariant in special relativity is usually written

E^2=p^2c^2 + m^2c^4

This is where the most famous equation in physics

E=mc^2

comes from. However, the equivalence between mass and energy (and also momentum) is much more clearly expressed in the natural units system:

E^2=p^2 + m^2

None of those tiresome factors of c^2 to remember! Mass, energy and momentum are all expressed in terms of the same natural unit of energy (usually, in particle physics, the GeV).  You can keep track of which is which by the simple expedient of using different names.

Velocities are, of course, always expressed as a fraction of c in this system so have no units.

In quantum theory we find energy E=\hbar \omega becomes E=\omega so energy is expressed in the same units as frequency. Energy is thus a measure of inverse time.  Momentum p =\hbar k becomes just p= k so momentum is an inverse length.  This is in accord with the various forms of Heisenberg’s Uncertainty Principle too:  \Delta p \Delta x \sim \hbar is \Delta p \Delta x \sim 1 and \Delta E \Delta t \sim \hbar becomes \Delta E \Delta t \sim 1. A particle with a finite lifetime thus has a finite energy width which is inversely proportional to the lifetime. It makes sense to use energy units for both of these things.

As an extra bonus we can dispense with the clumsy way that electromagnetism is handled in the SI system by noting that

\frac{e^2}{4\pi \epsilon_0 \hbar c} \equiv \alpha\simeq \frac{1}{137}

is dimensionless. In the SI system the coulomb force between two electrons is \frac{e^2}{4\pi \epsilon_0 r^2} whereas in natural units it is just \frac{\alpha}{r^2}, which is much nicer. Incidentally, the strange quantity \epsilon_0 that appears in the SI version is called the permittivity of free space. Nice name, but I wonder what it means?

The dimensionless quantity \alpha on the other hand, has a very clear  physical meaning: it is the fine structure constant,  a coupling constant that measures the strength of the electromagnetic interaction.

Some people – including emeritus professors of observational astronomy – object to natural units because they hide the units that things are expressed in. They don’t actually. What they do is express things in units that are better geared to the physics. In any case, if you want to convert back to SI units you can always do so straightforwardly with a little bit of dimensional analysis. This is necessary if you have to talk to engineers and the like, perhaps so they can build you a particle accelerator, but in the more elevated company of particle physicists you should definitely follow proper etiquette and keep your units natural.

Two Cheers for Lord Drayson

Posted in Science Politics with tags , , on March 4, 2010 by telescoper

The long awaited announcement of Lord Drayson‘s review of the structure of the Science & Technology Facilities Council (STFC)  has finally appeared together with parallel announcements by STFC and RCUK. There’s already been a lot of reaction on Twitter about this, and it has also reached the  BBC News.

There’s actually not much in the announcement that’s particularly surprising.  The plan is to insulate STFC from the effects of currency fluctuations on its subscription commitments to international organizations, and also to share the cost of large domestic facilities across the whole science programme rather than just STFC on its own. In the shorter term (i.e. 2010-11) STFC will continue to receive some help to deal with the uncontrollable external pressures on its budget.

In the longer term it is anticipated that the subscription to the European Space Agency will move to a new UK Space Agency anyway.

These moves are all good news, and will probably help STFC to reach some level of stability. I am certainly grateful to Lord Drayson for getting involved in this process. It will be a while before we find out how it will work out in practice, but at least it’s a start.

The big problem I see is that STFC may well reach “stability”, but the position of equilibrium looks likely to be one with a very low level of grant funding for astronomy and particle physics. Perhaps I’m being excessively cynical, but it still looks to me like this financial crisis was deliberately engineered in order to squeeze fundamental research by 25%. That has now been achieved, so the grey men of the Treasury can now remove the straitjacket. I don’t see any signal that our grants will return to a sustainable level, however, so the astronomy community will probably continue to wither away. The Drayson review may staunched the flow of blood, but the patient will remain  dangerously  ill unless additional measures are taken. (Too many metaphors, Ed.)

Which brings me to a final point. Having a sensible management structure for STFC isn’t the same as having a sensible STFC management. I know I’m not the only astronomer in the UK to have lost all confidence in the current Chief Executive, Keith Mason. As long as he remains in charge I’m suspicious that any structural modifications will amount to no more than window-dressing and astronomy and particle physics will continue to be neglected in favour of technology-driven projects.

We might – just might –  have stopped going backwards, but in order to start going forwards we need a new leader.

PS. For  the best compilation of sources on the STFC crisis, see Paul Crowther’s pages here.

Astronomy Look-alikes, No. 17

Posted in Astronomy Lookalikes with tags , on March 3, 2010 by telescoper

It’s been a while so I thought I’d try this one. It’s not at all unusual for my former colleague and cosmologist extraordinaire Professor Bernard Carr to be mistaken for the popular television celebrity Mr Noel Edmonds. I wonder if by any chance they might be related?

Mr Noel Edmonds

Professor Bernard Carr