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November 11th, 2008

The First Stars

One of the absolute best spiffs in the world, working for Space Telescope, is the monthly "popular lecture" series.  They’ve had them pretty much ever since I started working there.  Once a month one of the scientists at the Institute, or someone affiliated in some way with the work we do, gives a lecture targeted to a general audience, on the work they’re doing.  The lectures are open to the public and all are welcome to sit in and listen, and ask questions afterward.

It’s really great getting a chance to hear the people doing this work speak for themselves, and hear firsthand the latest thinking about what makes our universe tick.  Tonight’s lecture was about the very first stars to appear after the big bang and it really made me realize just how very…different…the early universe was.

It’s counter-intuitive that generating stars is hard when all you have are the vast tendrils of gaseous hydrogen in the early universe to work with.  But that was the problem facing the theorists.  As it turns out, getting nearly pure hydrogen gas to collapse enough to form a star isn’t easy.  It doesn’t really want to.   It will collapse, but then as it does it heats up slightly and wants to expand again.  So it achieves a stability well below the threshold for generating a star.  To go the rest of the way, the gas needs to cool by radiating off some of its heat, and that’s something it turns out hydrogen isn’t good at.

But molecular hydrogen is…and there’s the key ingredient.  The random motion in a hydrogen gas structure will eventually form molecules and those will radiate heat much more easily.  That will cool the structure down enough that it can collapse some more.  Then it becomes a question of how big it got…and here is where the early universe shows its strangeness. 

Remember…these are the first stars.  They can’t be formed from the shock waves of other stars dying or coming to life, because there are no other stars yet.  And all they have to work with is hydrogen gas.  There are no metals yet, no elements heavier then helium, because those are formed in stars and there aren’t any stars yet.  The presence of metals in the interstellar medium actually makes it easier to form stars.  The way star formation works now, just doesn’t work back then.  The hydrogen structure (gas cloud…whatever…) has to collapse on its own, due to its own random motion and gravity, with no assistance from any other nearby objects, because there are no other nearby objects yet.   And it has to be massive…really massive…for its collapse to break through the threshold where the heat from its own collapse simply pushes it back apart again and it never forms a star.  I mean…Really Massive.  About one-hundred times the mass of our sun massive.  Far more massive then the most massive stars that form in the cosmos as it is now.  Otherwise, it simply achieves stability as a dense cloud of hydrogen gas.

But if the structure got that big when it started collapsing, and was able to keep on collapsing over time as it shrank and heated up, radiated some heat off a bit and collapsed some more, heated up again, cooled down some more, and so on…at some point it hits a threshold where the collapse suddenly runs away and then the only thing that stops it is when the gas gets so dense and hot nuclear fusion starts happening and the gravitational collapse is pushed back by that.  Then what you end up with is…a star about a hundred times the mass of our sun.

Those stars are Strange.  They are fantastically brilliant, live very very short lives, and are massive enough to produce carbon, and then use their own carbon to produce other metals up to iron.  Some of them, in death, may have formed the massive black holes that lit the earliest quasars.

But they didn’t form galaxies.  The galaxies, by the time they began to form, already existed in a cosmic medium that had been seeded by metals from the first stars.  In that medium star formation was easier, resulting in much smaller, more longer lived stars.

No first stars have been observed yet.  They would be too faint, and too red shifted for the instruments we currently have.  The next generation space telescope (the James Webb Space Telescope) may be able to observe the first galaxies.  But observing a first generation star would be possible only in its death supernova, and then only by lucky chance.  But now I know better why the next generation space telescope is so focused on infrared astronomy and not visible light astronomy.  They need that to see the early universe…the first galaxies…and, maybe, the first stars.  All of that stuff is red shifted away from the visible light now, because of the expansion of the universe since then.

I love this job.  Other jobs I’ve had the upper management has been something out of Dilbert.  It’s scary how true to life Dilbert is sometimes.  This one I get to hear the top floors talk about how they’re gathering light from near the beginning of time and trying to figure out what it’s telling us about the universe we live in.  And I get to hear about it before it goes into the textbooks.

by Bruce | Link | React! (1)

August 11th, 2008

And Now…A Wee Moment Of Species Pride…

I’m copying the following from Brad DeLong’s blog comments in their entirety.  Some days you read the news and you just want to write off the human race altogether.  When those moments hit you, it’s good to be able to keep things in perspective…

Hoisted from Comments: The Dawn of Humanity

Grasping Reality with Both Hands: Brad DeLong’s Semi-Daily Journal: The Dawn of Humanity: What astonishes me is the speed. They’ve got the origin date at -56,000, and the oldest modern human remains in Australia are -40,000. The route from East Africa across Asia to Northern Australia is 10K+ miles, which means humans were expanding at close to a mile a year. That’s just unbelievably fast.

We have all sorts of branches of homo surviving stably for a million plus years all over africa, asia, and europe, and this new branch comes out of Africa and by the end of the Great Migration, only a little over ten thousand years later, they are building boats to sail to Australia. And wiping out or out-competing every one of our homo sibling species on the way.

The Singularity is truly in our past.

Posted by: tavella | January 23, 2007 at 05:15 PM

Here’s a link, in case you’re wondering about that reference to "The Singularity".  It was coined mostly to refer to advances in machine intelligence, but others have co-opted the term to refer to where the acceleration of change reaches a point where humanity itself simply becomes unrecognizable from anything we once were.  Those ancient branches of the humanoid family tree, long gone now, would certainly never comprehend us now, but they probably didn’t back when we first emerged, and they first laid eyes on us.

We can do this…we can survive.  We can endure.  We can find our way to the stars.  Maybe it’ll take another ten thousand years.  But we’ll do it.  And in another 56 thousand years they’ll be looking back in amazement at how quickly we did it…

by Bruce | Link | React!

August 23rd, 2007

Oh…Look At The Stars…!

I guess I can blab about this now…since it’s been made public…  Perhaps you’ve heard of Google Earth.  Have you ever wondered what Google Sky might look like?

Wonder no more…

Google puts universe online

Sky at Google Earth, which made its debut in cyberspace early yesterday, turns Googlers around and aims their eyes toward the heavens, with user-friendly tools for navigating and zooming deep into the skies of both the Northern and Southern hemispheres.

In the background there are 100 million individual stars and 200 million galaxies. They’re not randomly generated dots, but real, digitized photos — a million of them — stitched seamlessly together from some of the world’s most complete sky surveys.

Astronomers at the Space Telescope Science Institute in Baltimore have added 127 high-resolution digital photographs from the Hubble Space Telescope. They’ve spent months patching them all into Google’s sky at their proper zoomable distances and precisely in position.

"It’s a very interesting tool to allow people, as never before, to browse the sky," said Alberto Conti, an institute astronomer and development manager for the institute’s Community Missions Office, which works to make Hubble’s discoveries accessible to the public.

Because of light pollution, he said, lots of people, especially in East Coast cities like Baltimore and New York, "have never really seen the sky." With Google Sky’s software, they can "explore things they could never see with their own eyes, or things they probably would not see in a planetarium."

More overlays, or "mashups," available to Sky users can reveal the constellations, and identify stars and planets visible from their backyards. Sky can also forecast the positions of the moon and planets two months in advance.

"I’m looking forward to people adding asteroids, and things that are moving — a lot of comets, you name it," Conti said. Just like Google Earth itself, Sky will allow users to form communities of common interest, and add their own images and lists of interesting sights.

This has been in the works for a while and it’s wonderful, the potential even more vast then with Google Earth.  Imagine being able to view any part of the sky above, as only the most powerful telescopes humankind ever possessed can.  Imagine zooming into a section of sky and viewing it in different wavelengths of light, or watching stellar events unfold over a time selectable period.  Watch the light echo from V838 Monocerotis expand into the distant shells of its own cast-off matter.  View the galaxies in various wavelengths, to pinpoint the regions of active star birth.  Wander among distant galaxies near the dawn of time.

Now you can. 

Some part of our being knows this is where we came from. We long to return.
And we can, because the Cosmos is also within us. We’re made of star stuff.
-Carl Sagan

by Bruce | Link | React!

June 14th, 2007

Nature’s Logic

There’s a kind of primitive variable that probably everyone who writes computer code knows and understands these days…the Boolean.  Unlike other variables which can hold a range of values, be they numbers, or strings of ascii characters, the Boolean is a relentlessly either-or variable.  And for that reason, it maps pretty well to the fundamental logic by which all digital computers operate, and to their smallest unit of data, the bit.  But humans have been considering their world in Boolean logic ever since our minds first emerged from out of the biological background noise.

Yes-No.  True-False.  Right-Wrong.  Good-Bad.  Even as we admit to ourselves that there are often only shades of gray, we persist in reducing our experiences to these terms.  It’s as basic an evaluation as can be.  The second postulate of Aristotelian logic is that of ‘either-or’.  A thing cannot both be, and at the same time not be.  Either yes, or no.  Either true, or false.  Either right, or wrong.  Either it is, or it is not.  It must be one or the other.

Well…tell it to Schrodinger’s cat.  It’s probably no coincidence that our machines are made in our image, that they resemble the way our minds like to think.  The canvas always speaks of the artist.  But as it turns out, that’s not actually the way our brains operate.  It may not even be the way nature, at its most elemental level, works.  There’s this intriguing tri-position logic in the natural world that I keep seeing raise its hand and wave at us from time to time.  But it seems to go unexamined most of the time, and I think that’s because like the extra space-time dimensions physicists keep telling us are there, it’s hard for our minds to wrap themselves around it.   And that’s really interesting, because one place you really see this tri-position logic is in how our brains actually physically work.

Consider the humble synapse.  It is the gap between brain cells, across which two different kinds of chemical "messages" can cross.  One kind of chemical causes the cell on the other side of the gap to fire.  The other chemical inhibits the cell on the other side of the gap from firing.  So far, so good.  We’re still comfortably in the basic Boolean logic of things.  Fire-Don’t fire.  Yes-No.  Off-On.  Either-Or.  But there’s a third thing that synapse can do: Nothing.

So synapse logic has three states, not two.  Fire, don’t fire, and…what?  Here’s where it gets interesting for me.  What is the word here.  We don’t really have one.  And that I think, is because the concept is difficult for us.  The state itself seems foreign enough to the way our minds naturally work, that as far as I know, humans don’t really have a good enough word for that third position.  Neutral doesn’t quite do it.  It isn’t that it isn’t engaged, like a gear shift you put into neutral, say.  It’s connected, to the rest of the brain.  ‘Off’ isn’t quite it either.  Each half of the synaptic gap has a current state that influences the state of the cells on either side of the synaptic gap depending on the direction of the message, or the absence of one.  So there are really three states possible here:  Fire, don’t fire, and a third, that is neither fire or don’t fire.  Depending on the state of the synapses it’s connected to, a brain cell may or may not fire.  So the cell itself may have just two states.  But the synapses have three.

Our minds just don’t seem to grasp that third logical state very well, and we fumble to describe it.  It’s a between state.  No…it’s a middle state.  Wait…a transitional state…  Uhm…  No…it’s…it’s…   (shrug)  I dunno…

Maybe ‘zero’ is the right way to think about it.  But I can only say that because I write software code and I understand how zero is actually something distinct from a positive value, is distinct from a negative value.  But that seems to be a non-intuitive concept for us humans.  Consider that the Arabic invention of the zero as a form of notation actually came well after a lot of other very basic mathematical concepts.  Well of course everyone knew that you can have a zero quantity.  But expressing it abstractly seemed to be a difficulty.  And in many programming languages, 0 evaluates to false anyway, and any other value is true (except in Basic, where  –1 is (was) true, which I think is right from a bitwise NOT sense…but don’t get me started…).  And…this third position isn’t really a ‘nothing’.  It’s more of a ‘neither’.  

Another place you see this tri-position logic is natural selection.  In the grand scheme of things, the winners are those organisms that are best adapted to their environment.  Variation then, that gives an organism an advantage tends to be passed on, and variation that puts an organism at a disadvantage tends not to be passed on.  Over time the advantages accumulate, and the disadvantages get culled out.  Either-Or.  But there is a third thing that can happen.  Nothing.  A variation can simply be neither an advantage nor a disadvantage.  Those variations it seems, get placed in the genetic portfolio right along with the advantages too…

Landmark study prompts rethink of genetic code

The most detailed probe yet into the workings of the human genome has led scientists to conclude that a cornerstone concept about the chemical code for life is badly flawed.

The ground-breaking study, published in more than two dozen papers in journals on both sides of the Atlantic, takes a small percentage of the genome to pieces to draw up a "parts list," identifying the biological role of every component.

For the international team of investigators, the four-year project was the computer-equivalent of passing a fine-toothed comb through a mountain of raw data.

Reporting in the British journal Nature and the US journal Genome Research on Thursday, they suggest that an established theory about the genome should be consigned to history.

Under this view, the genome is rather like a ribbon studded with some 22,000 "nuggets" in the form of genes, which make proteins, the essential stuff of life.

Genes — deemed so valuable that some discoverers of them have been prompted to file patents over them for commercial gain — amount to only around a twentieth, or even less, of the genetic code.

In between the genes and the sequences known to regulate their activity are long, tedious stretches that appear to do nothing. The term for them is "junk" DNA, reflecting the presumption that they are merely driftwood from our evolutionary past and have no biological function.

But the work by the ENCODE (ENCyclopaedia of DNA Elements) consortium implies that this nuggets-and-dross concept of DNA should be, well, junked.

The genome turns out to a highly complex, interwoven machine with very few inactive stretches, the researchers report.

Genes, it transpires, are just one of many types of DNA sequences that have a functional role.

And "junk" DNA turns out to have an essential role in regulating the protein-making business.

Previously written off as silent, it emerges as a singer with its own discreet voice, part of a vast, interacting molecular choir.

"The majority of the genome is copied, or transcribed, into RNA, which is the active molecule in our cells, relaying information from the archival DNA to the cellular machinery," said Tim Hubbard of the Wellcome Trust Sanger Institute, a British research group that was part of the team.

"This is a remarkable finding, since most prior research suggested only a fraction of the genome was transcribed."

Francis Collins, director of the US National Human Genome Research Institute (NHGRI), which coralled 35 scientific groups from around the world into the ENCODE project, said the scientific community "will need to rethink some long-held views about what genes are and what they do."

"This could have significant implications for efforts to identify the DNA sequences involved in many human diseases," he said.

Another rethink is in offing about how the genome has evolved, said Collins.

Until now, researchers had thought that the pressure to survive would relentlessly sculpt the human genome, leaving it with a slim, efficient core of genes that are essential for biological function.

But the ENCODE consortium were surprised to find that the genome appears to be stuffed with functional elements that offer no identifiable benefits in terms of survival or reproduction.

The researchers speculate that there is a point behind this survival of the evolutionary cull. Humans could share with other animals a large pool of functional elements — a "warehouse" stuffed with a variety of tools on which each species can draw, enabling it to adapt according to its environmental niche.

IMO, there’s that third logical position at work again.  The variation is neither good, nor bad, it’s just there.  At some future point, say a rapid change in the organism’s environment, and that gene might be a handy thing to have all of a sudden.  Or, conversely, it might turn into a complete disaster for the organism.  But for the moment, it’s just there, evaluated to position three.  Zero, let’s say.  Neither positive nor negative.  It has the potential to be either one, given a chance to express itself.

From somewhere deep in the physical fabric of the universe, Schrodinger’s cat licks its chops and smiles.  Or doesn’t.  Or both.  Just don’t open the box.

The science fiction writer Larry Niven once averred that giving gay people what we want would be the quickest way of breeding us out of the population.  But then, he didn’t get the fact that his Ringworld needed attitude jets until some real engineers pointed that fact out to him.  I happen to think that having a gay minority does in fact provide a survival advantage to the human line.  But as it turns out, homosexuality can fit comfortably into our gene pool just fine, along with a bazillion other random variations on a theme that simply are, and do no harm. 

I don’t need to pass on my gay genes.  My heterosexual brethren probably have them too…they just aren’t expressing them.  For some reason, I expressed mine.  But I’m fine with that, and so is nature.  I happen to think it’s a plus.  But the point is that a variation only gets culled out if it’s a minus.  A really big minus.  And this one isn’t.

[Edited a tad…] 

by Bruce | Link | React!

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