Science Blogs Physcial Sciences
"Without a wish, without a will,
I stood upon that silent hill
And stared into the sky until
My eyes were blind with stars and still
I stared into the sky." -Ralph Hodgson The next month -- from May 5th to June 5th -- brings three of the most spectacular astronomy sights possible on Earth back-to-back-to-back for skywatchers of all types, without telescopes, binoculars, or any special equipment. Tonight, May 5th, marks what's come to be known as a Supermoon, or the largest, brightest full Moon of the year.
(Image credit: Chris Kotsiopoulos at Earth Science Picture of the Day.)
Not that you'll notice, mind you, unless you've got both an incredible eye and an incredible memory. The full Moon is, by far, the brightest thing in the night sky, outshining the brightest star in the sky by a factor of around 40,000.
A supermoon, on the other hand, is only about 30% brighter than a normal full Moon.
(Image credit: science @ NASA, retrieved from Tara Hastings at WDTN.)
The Moon, of course, orbits the Earth in an ellipse, rather than in a perfect circle. When the Moon is farther away from Earth in its orbit -- or closer to apogee -- it appears smaller in the sky, while when it's closer to Earth -- near perigee -- it appears larger. The supermoon is the one full Moon out of the year that occurs when the Moon is at its minimum distance from the Earth, and hence appears the brightest.
(Image credit: Essay Web's astronomy site.)
These differences, however, are relatively small. The full Moon at apogee is only 20% smaller than the full Moon at perigee, a difference completely un-noticeable to even a trained observer, unless you put these two images right next to one another.
(Image credit: Marco Langbroek, the Netherlands, retrieved here.)
Having the closest, brightest full Moon of the year is a great excuse to go out and look at it, attempt to photograph it, or if you're far away enough from streetlights, enjoy the shadows cast by the moonlight.
There's nothing you can't do with a supermoon that you couldn't do with any, ordinary full Moon, but it is fun to think about why this happens.
(Image credit: Ryan, footnote #3 on Carrie Fitzgerald's site.)
The Moon makes an ellipse around the Earth, which in turn makes an ellipse around the Sun. Right now, the Moon's perigee is in the opposite direction of the Earth from the Sun, so full Moons appear as large as they're ever going to. New Moons and crescents, on the other hand, will appear somewhat smaller, as they occur closer to apogee.
But six months from now, the Earth (and Moon) will be on the other side of the Sun, so the Moon's apogee will occur close to the full phase, resulting in somewhat smaller full Moons, while new Moons and crescents will be larger. You can see NASA's apogee and perigee calculator for more information, but I think the diagram below illustrates things pretty clearly.
(Image credit: NASA, Fred Espenak and Jean Meeus.)
Right now, we're extremely close to position "C" in the diagram above, where the Moon's apogee (farthest from Earth) occurs close to the Sun, and the Moon's perigee (closest to Earth) occurs away from the Sun. This gives us the supermoon that you can see tonight, but fifteen days from now, it's going to give us something far more rare and special.
The Moon's apogee occurs on May 19th, and the very next day, at nearly its most distant from Earth, the Moon, Earth, and Sun will all line up, producing the spectacular and rare sight of an annular Solar Eclipse!
(Image credit: Kopernik Observatory and Science Center.)
On the evening of May 20th in North America, close to Sunset, the Moon will pass in front of the Sun. But because the Moon is so close to apogee, it will actually appear ever so slightly smaller than the Sun in the sky, and thus will not be sufficiently large to block it completely!
Astute skywatchers who plan their trip right and are blessed with clear skies will get to observe the elusive "Ring of Fire" shown above. I've already written my eclipse guide for those of you preparing to join me in watching this, but there is one cheap piece of equipment I'll recommend that everyone pick up for looking at the Sun: a pair of Welder's Goggles.
For around $10 (tops), you can get a piece of equipment that will allow you to look at the Sun, whenever you want, for short periods of time. Make sure the density of the goggles is 14 or greater, and never use a telescope or binoculars with them, just your naked eye. But this is an inexpensive, easy way to allow yourself to view partial or annular eclipses (or perhaps even sunspots) whenever it strikes your fancy. (I've got my pair already.)
But there's another reason to get welder's goggles that's even more rare and spectacular than the upcoming solar eclipse. Those of you who've had clear skies in the west for the past month or two may have noticed an extremely bright object there just after sunset.
(Image made with stellarium.)
This is what the night sky will look like at 9 PM at 45 degrees latitude (where I live) tonight. That bright object, fifteen times brighter than Sirius, is the planet Venus, which just achieved its greatest apparent brightness in the sky. (And appears as a gorgeous crescent with binoculars if you can focus properly!)
Venus, being an interior planet to Earth, appears brightest not when it is closest to us, nor when it's in its full phase, but rather when it's a crescent, where the combination of proximity to us and the amount it's illuminated is maximized.
(Image credit: Torquay Boy's Grammar School's Observatory.)
Over the coming month, Venus will descend in the sky, with progressively less and less of the planet becoming illuminated to our eyes, percentage-wise. However, Venus' angular size will increase, as the apparent diameter of the planet will increase in the sky due to it physically getting closer and closer to us.
(Image credit: Shamefully retrieved from this website.)
Eight years ago, Venus didn't just pass interior to Earth, missing the Sun by just a degree or two; in 2004, Venus actually transited across the disc of the Sun, blocking a small fraction of the Sun's light. These transits are incredibly rare; you and I will get two in our lifetimes.
The last Venus transit before the 2004 one took place in 1882, and the next one won't be until 2117. Unless, that is, you're ready on June 5th of this year.
(Image credit: Tonk at CloudyNights.)
It is perfectly safe to look directly at the Sun for brief periods of time with a good pair of Welder's goggles, and I've already got mine.
Where should you be to see it? That depends on where you live.
(Image credit: Fred Espenak / NASA, retrieved here.)
Where I am in North America, the Venus transit will start at about 3:00 PM on June 5th and will continue through sunset. The entire transit won't be visible in North America, as it takes many hours to complete, but this is your one chance to witness an event like this with your own eyes.
In Europe, parts of Africa, and most of Asia, of course, you'll be able to see the transit in the morning of June 6th instead. But those of you living in Iceland get the most special treat of all: a transit that spans both sunset and sunrise!
(Video credit: user transitvenus on YouTube.)
Three major astronomical events -- the supermoon, tonight, the annular solar eclipse, on May 20th/21st, and the transit of Venus, on June 5th/6th -- all occurring within a month of one another! There's never been a better time to purchase a pair of welder's goggles, that's for sure!Read the comments on this post...
Enough slagging of beloved popularizers-- how about some hard-core physics. The second of three extremely cool papers published last week is this Nature Physics paper from the Zeilinger group in Vienna, producers of many awesome papers about quantum mechanics. Ordinarily, this would be a hard paper to write up, becase Nature Physics are utter bastards, but happily, it's freely available on the arxiv, and all comments and figures are based on that version.
You're just obsessed with Zeilinger, aren't you? All right, what have they done this time? The title is "Experimental delayed-choice entanglement swapping," and it's pretty much what it sounds like. They've demonstrated the ability to "swap" entanglement so as to create quantum correlations between two photons that have never been close to one another. And they've done this in a "delayed-choice" fashion, where the decision about whether to entangle them or not is made well after the two photons they're entangling have been detected.
Oh, OK, that sounds-- Wait, what? They entangled them after detecting them? Yep. The basic scheme is illustrated by this quasi-spacetime-diagram from the supplementary material:
The vertical axis represents time, moving into the future as you go up. They start with two pairs of entangled photons, which are sent into optical fibers. Two of these (one from each pair) go directly to detectors that record their polarizations roughly 35 ns after they were produced. The other two go into very long fibers, and are sent to a detector that either records the two original polarzations, or makes a joint measurement of the two together. If they measure the individual polarizations, the original pairs remain independent of one another, but if they make a joint measurement of the two, that entangles their states, meaning that the polarizations of the other two photons are now entangled with each other, and should be correlated.
Since these photons went into much longer fibers (104m vs. 7m), though, the entangling measurement is made after the two photons whose states are being entangled have had their polarizations measured-- about 520 ns after they were produced.
In keeping with the silly jargon of the field, the two photons that are detected immediately (Photons 1 and 4) go to detectors that are imagined to be held by people named "Alice" and "Bob." The two that are measured together to determine the entanglement (Photons 2 and 3) go to a third imaginary person named "Victor," and it's Victor's measurement that determines everything.Read the rest of this post... | Read the comments on this post...
I was tremendously disappointed and frustrated by this book.
This is largely my own fault, because I went into it expecting it to be something it's not. Had I read the description more carefully, I might not have had such a strong negative reaction (which was exacerbated by some outside stress when I first started reading it, so I put it aside for a few weeks, until I was less mad in general, and more likely to give it a fair reading). I'm actually somewhat hesitant to write this up at all, for a number of reasons, but after thinking it over a bit, I think I have sensible reasons for being disappointed in the book, and it's probably worth airing them.
As mentioned in yesterday's post about "Big Science", this is a book whose central message is that we ought to be spending more money than we are on space exploration in order to boost science as a whole. And when I saw Tyson promoting this on either the Daily Show or the Colbert Report, I was excited by the idea. As anybody who's been reading the blog for any length of time knows, I'm all in favor of bringing science to a broader audience (which is why I write books where I discuss physics with my dog). While I'm skeptical the space is the most effective tool for getting the job done, I'm prepared to hear a good argument for that, and Tyson seemed like just the guy to do that: to provide a clear and coherent vision of what space exploration ought to be in order to serve as a driver of science in general.
But this is not that book. Instead, it's a collection of... stuff. Some essays, some speeches, some interview transcripts, a whole bunch of Twitter posts. Collectively, they're all about space exploration as a general matter, and many of the individual pieces are as good as you would expect. But it's not a sustained and coherent argument. And that's a missed opportunity.Read the rest of this post... | Read the comments on this post...
- Andrew Johnston has a review of the UK edition, praising it because "it's bang up to date, and goes beyond the basic quantum concepts into more complex areas like decoherence, entanglement and quantum teleportation," which I like to see because that's one of the things I especially wanted to do.
- Natasha Zaleski, a grad student, has a review of How to Teach Relativity to Your Dog, which is good but not great, because it hit the usual failure mode: the talking-to-the-dog thing wore thin for her. Which is, of course, the danger of the whole talking-to-the-dog conceit.
- The Polish edition is out-- I got my author copies, which are very nice. This has led to a review in a pop-culture magazine, between Steig Larsson and Terry Pratchett. Google Translate makes hash of it, in part because it does a literal translation of my surname, leading to sentences like "Even so, Eagle shows the world a lot of physics accessible, than does the bulk of textbooks for physics."
- The vanity search also turned up a mention of the books in the Raised Indoors podcast-- one of the hosts bought both from Amazon in Canada (thanks!), but hasn't yet read them. Hope you like them. The podcast itself is a general-interest pop-culture thing, and the Clive Cussler rant is pretty amusing.
And that's the latest from the vanity search.Read the comments on this post...
"This is the way I wanna die. Torn apart by angry fans who want me to play a different song." -Regina Spektor You're familiar with the classic picture of a black hole: a dark, dense region at the center from which no light can escape, surrounded by an accretion disk of matter that constantly feeds it, shooting off relativistic jets in either direction.
(Image credit: University of Warwick, retrieved from here.)
This is a pretty accurate picture of active black holes. But most black holes aren't active, and of the ones that are, they aren't active most of the time!
Most people think of black holes as marauders, gobbling up whatever poor stars happen to get in their way. You very likely have a picture of a black hole as though it behaves like a great cosmic vacuum cleaner, sucking up anything that dares get too close to it.
I can't fault you for thinking that; this is a genuine NASA video, and the picture that some very smart people have been painting for you for a long time. But that isn't quite how the Universe works.
So, how does it work? When any object falls in close to a black hole, it experiences different forces on different parts of the object. We call these forces tidal forces, because they're the same types of gravitational forces that cause the tides we experience here on Earth!
(Image credit: Barger and Olsson.)
Only, in the vicinity of a black hole, the tidal forces are much stronger than we experience on Earth. They are, in fact, much stronger than Jupiter's innermost moon, Io, experiences, and those forces are powerful enough to constantly tear Io apart, making it the only volcanically active moon in the Solar System!
No, when you get close to a black hole, you get stretched at either end so severely, and compressed in the middle so thinly, we call the process spaghettification, one of the greatest astrophysics words ever invented!
(Image credit: John Norton at Pittsburgh.)
But "falling in" to a black hole, like illustrated above, practically never happens! Space is simply too big, and even for supermassive black holes -- like the multi-million-solar-mass behemoth at the Milky Way's center -- the event horizon is too small. Most stars and objects that pass nearby to a black hole simply do what all other objects in the Universe do.
Gravitate! (Ha ha ha ha haaaaa!)
Remember that space is huge, and that getting within a paltry 0.001 light years of our galaxy's supermassive black hole won't even disrupt the passing star, much less "vacuum it up," as you might have thought.
"But what if the star does get close enough," you ask, "then what happens?"
(Video credit: NASA, S. Gezari (Johns Hopkins), and J. Guillochon (UCSC).)
Note how, first, the star gets completely ripped apart by these intense tidal forces! But rather than acting like a vacuum cleaner and sucking it all up, most of the mass from this star doesn't get devoured at all; quite to the contrary, most of it gets ejected back out into the space around the black hole! It's only a small fraction of the original that gets swallowed, but that's totally sufficient to take a quiet, supermassive black hole, and bring it back to life!
And we know this, because we just observed a super distant galaxy -- more than 2 billion light years distant -- just become ultra bright thanks to its supermassive black hole sneaking a bite out of an unlucky passerby! Let's take a before-and-after look.
(Image credit: NASA, S. Gezari, A. Rest, and R. Chornock, as are the next two.)
The above images, from GALEX (in the Ultraviolet) and Pan-STARRS (in the visible/IR), show this distant galaxy shortly before it started snacking on its newly accreted material. The images are low-resolution because GALEX and Pan-STARRS focus on grabbing very wide fields-of-view; when you're looking for very rare occurrences like this, you need to grab as much of the deep sky as possible!
So, that was 2009. But the next year...
The galaxy has brightened by a factor of around 350 in the Ultraviolet, and the visible/IR image has turned much bluer, an indication of the extraordinarily high energies being belched out by this suddenly noisy galaxy!
Taking a look at the before-and-after images together, you can really see the difference.
But don't be fooled by the vacuum cleaner description; it's not eating the entire thing that ran into it! This is, in fact, something that we may see happening for much smaller black holes that are much closer to us; the nearby galaxy Messier 83 just had a very similar outburst from a much smaller black hole!
Black holes aren't giant leviathans, devouring anything that comes nearby, but nor are they dainty, steady nibblers on objects that orbit. Rather, black holes are wild, violent and inevitable, tearing anything that dares approach too closely into shreds, but coming away with a snack-sized meal whose first bite makes quite an impression!
Now, if you'll excuse me, all this black hole talk has made me hungry! Where did I put the spaghetti...Read the comments on this post...
A week or so ago, lots of people were linking to this New York Review of Books article by Steven Weinberg on "The Crisis of Big Science," looking back over the last few decades of, well, big science. It's somewhat dejected survey of whopping huge experiments, and the increasing difficulty of getting them funded, including a good deal of bitterness over the cancellation of the Superconducting Supercollider almost twenty years ago. This isn't particularly new for Weinberg-- back at the APS's Centennial Meeting in Atlanta in 1999, he gave a big lecture where he spent a bunch of time fulminating about what idiots politicians were for cancelling the project. If anything, the last decade and a bit has mellowed him somewhat.
Sort of in parallel with this, I've also been reading Neil deGrasse Tyson's latest book, Space Chronicles (I say "sort of" because I actually stopped reading it for a couple of weeks, because I found it maddening for reasons that I may go into in another post). This is a collection of things from other sources that collectively sort of advances the argument that we need to spend flipping great wodges of cash on space exploration, for the good of science and society as a whole.
While these aren't directly related to each other-- and, indeed, are somewhat in conflict, as Weinberg has no use for manned space flight-- they're both making a similar argument: that we should be spending money on Big Science projects, because they're important for science as a whole. Which is fine, to a point-- I'm all in favor of increasing the amount of money we spend on scientific research-- but I can't help thinking that it's awfully easy to make this argument when the Big Science projects just happen to fall very close to your area of interest.Read the rest of this post... | Read the comments on this post...
Check out the image below from NASA's Earth Observatory:
Clock Synchronization Done Right: "A 920-Kilometer Optical Fiber Link for Frequency Metrology at the 19th Decimal Place" [Uncertain Principles]
I've been busily working on something new, but I'm beginning to think I've been letting the perfect be the enemy of the good-enough-for-this-stage, so I'm setting it aside for a bit, and trying to get caught up with some of the huge number of things that have been slipping. Which includes getting the oil changed in my car, hence, I'm sitting in B&N killing time, which is a good excuse to do some ResearchBlogging.
Last week was a banner week for my corner of physics, with three really cool experiments published. Two of those are on the arxiv, which means I can use images from the paper (but those take longer to write). The third was in Science and isn't available in preprint form, and since the AAAS are bastards about permissions, and I'm not paying them $30 for the sake of a blog post, we'll do that one first.
The paper in question has the incredibly sexy title "A 920-Kilometer Optical Fiber Link for Frequency Metrology at the 19th Decimal Place", and got a pretty good write-up in Physics World, but there's still room for some Q&A:
Seriously? Optical fibers and frequency metrology? What do those even mean? Seriously. This is a significant advance for people who care about precision measurement of time. The authors took two ultra-precise atomic clocks in labs at opposite ends of Germany, and were able to compare their frequencies at the level of a few parts in 1019. That's 0.0000000000000000004 times the original frequency, or, since they started with an optical frequency, 0.00008Hz out of 194,000,000,000,000.
OK, I admit, that's a lot of zeroes. But why does that matter? Isn't the whole point of ultra-precise atomic clocks that they all work exactly the same way? Why do you need to compare them? All atomic clocks using a given type of atom have the same basic frequency, but not all clocks are equally well made. The only way to determine the performance of a new one is to compare it to one you know works, but they're also not very portable, so you need to be able to do the comparison remotely.
There's also the fact that the local conditions for different clocks will be different, which can lead to some small shifts in the frequency due to things like general relativity, which means you can study some interesting physics using a distributed network of clocks. You can also check to see if the constants of nature are changing by comparing clocks based on different atoms, and again, these are not easy to make or move around, so being able to reliably do the comparison over long distances is a bug deal.Read the rest of this post... | Read the comments on this post...
"A journey is a person in itself; no two are alike. And all plans, safeguards, policing, and coercion are fruitless. We find that after years of struggle that we do not take a trip; a trip takes us." -John Steinbeck Here on Earth, we all get to enjoy the delight of being located in an extremely fortuitous place in our Solar System. Not just today, mind you, but billions of years ago, when the Solar System's planets were first forming!
Located close enough to our Sun, when the Earth first formed, like our neighbors Mercury, Venus and Mars, we were chock full of heavy elements. Not just the carbons, nitrogens and oxygens that abound on all the known worlds, but important ones much higher up on the periodic table, including silicon, sulphur, iron, nickel, tin, lead, and even the radioactive uranium!
This might not sound so special to you, but our world would be a lot more boring if we had formed farther from the Sun. See for yourself:
Jupiter and Saturn aren't simply less dense than Earth is because they retained all that excess hydrogen that our wimpy gravitational field couldn't hold. Although that's true, they're also made out of elements that are intrinsically less dense!
We can identify where an object found anywhere in the Solar System -- including meteorites that fall to Earth -- simply by examining what they're made out of.
(Image credit: NASA, retrieved from National Geographic.)
One of the most spectacular applications of this knowledge came when we first journeyed to the Moon. For the first time, we'd be able to analyze rocks from the Moon and their chemical composition! What we found was simultaneously profound and the most boring thing imaginable.
(Image credit: NASA / Apollo 11, retrieved from here.)
Because the Moon is made out of the same stuff that the Earth is!
Before you start saying, "Duhhhhh," as some of you are wont to do, let's remember that it didn't have to be this way. We need only look at our nearest moon-ed neighbor.
Because Mars' two moons, Phobos and Deimos, are not made out of the same stuff Mars is! They formed significantly farther out in the Solar System, originating in the asteroid belt. Only a chance encounter with another body (probably Jupiter) flung them in to the inner Solar System, where they were gravitationally captured by the red planet!
If it happens for Mars from the asteroid belt, you may be wondering about that other, even bigger belt in our Solar System, and what the possibilities might be from there.
(Image credit: Don Dixon / Cosmographica.)
I refer, of course, to the Kuiper Belt, the band of leftover proto-planetesimals from the formation of our Solar System. These small, icy objects are only about a third the density of Earth, but are more dense than the gas giants that lie interior to them.
If the asteroids could be flung towards the inner, rocky worlds due to the gravitational influence from Jupiter, it stands to reason that these Kuiper Belt objects could similarly be flung inwards thanks to Neptune.
(Image credit: source unknown, retrieved from clowder.net.)
There are some dead giveaways that your object isn't from the same part of the Solar System as its initial planet is. There's the elemental composition / density argument, of course, but simply via random chance, 50% of these objects that get captured will wind up revolving around their planet the wrong way. One obvious guy like this is Neptune's largest moon, Triton.
(Image credit: Voyager Spacecraft, S. Albers / NOAA / GSD.)
Triton is maybe the easiest one; he's so large that if he were still in the Kuiper belt, he'd be the largest object there, dwarfing (burn!) both Pluto and Eris!
But there are others, elsewhere, that don't quite look like they belong. And a Saturnian mystery may, in fact, be on the cusp of being solved thanks to this idea.
(Image credit: Cassini / NASA / JPL-Caltech.)
This is Iapetus, one of Saturn's moons, looking like it always does: like it came out on the wrong side of a trip through the mud. Iapetus does all the moon-like things correctly: it revolves the right way around Saturn, it's got the right density for its spot in the Solar System, its surface is even made of the same elements -- as far as we can tell -- as it ought to be.
Except for that muddy mess that discolors one of its face. What's going on here? It turns out Iapetus isn't alone.
(Illustration credit: AP / NASA, retrieved from here.)
A giant, diffuse outer ring, well beyond the Saturnian rings you're used to, pollutes Iapetus' orbit. As the tidally-locked moon speeds around Saturn, these grains from the ring smack into Iapetus, discoloring it like billions of bugs on a windshield.
The question, of course, is where did this ring come from? Because it isn't Saturn. The answer is much more fun than that!
(Image credit: Cassini / NASA / JPL-Caltech.)
Say hello to Phoebe, Saturn's very suspicious moon, located in the same vicinity as both this outermost ring and Iapetus. Phoebe is full of craters, a different color and elemental composition than the other moons, and -- this is a big and -- it revolves around Saturn the wrong way!
In other words, this outsider came all the way from the Kuiper Belt to become a moon of Saturn! And the journey was no picnic for Phoebe, either.
(Image credit: NASA / Cassini / Caroline Porco / CICLOPS.)
Those craters on its surface are from a lifetime of bombardment! The once-spherical Phoebe has lost a lot of its mass, and that's almost certainly where the material that makes up both the outermost ring and the diffuse discoloring of Iapetus comes from!
Let this be a lesson to all of you: if you want to be adopted by another planet, make sure you orbit the same direction as everything else! In the meantime, know that objects from the asteroid belt or Kuiper Belt could come in at any time, and could even become our planet's next additional moon!Read the comments on this post...
2004-2005 was the last complete year before the move to ScienceBlogs in January of 2006, after which the making of these posts will become more complicated, because my posting rate went way up. For this year, though, I was still sticking to one post a day, and the blog had settled into a pretty decent groove.
The year did feature a brief foray into silly physics-related fiction, which might possibly be called a precursor to the books, and a local tv appearance related to the election of 2004 (which I had otherwise tried to blot from memory. Ye gods, that was depressing to relive). This was back before YouTube became really big, so I didn't include a clip in the post, but I added it a few years later, so you can see me talking about lying with statistics for a few seconds.
Specific posts of interest, by tagline category:Read the rest of this post... | Read the comments on this post...
Thank You from the USA Science and Engineering Festival! [USA Science and Engineering Festival: The Blog]
The 2012 USA Science and Engineering Festival was a huge success this past weekend! More than 150,000 attendees battled the rain, traffic and crowds to celebrate science at the Convention Center!
The Festival would not have been possible without the hard work of our amazing volunteers! Over 750 volunteers dedicated their valuable time and showed incredible patience and enthusiasm during their shifts at the Festival. We are so grateful to ALL of you! We received wonderful feedback about our exhibitors and the amazing hands-on activities. Exhibitors made each person feel welcome and thoroughly explained their activities to attendees of all ages. And finally, we are so thankful for the extraordinary generosity of our sponsors and Festival Host Lockheed Martin.
With over 3,000 exhibits and 150 stage shows, there are so many wonderful Festival moments to highlight. Our Festival Host Lockheed Martin surprised us all with a few last minute additions including presentations by US Olympic Speed Skaters and cast members of NCIS Los Angeles. R2D2 made a special appearance along with our science celebrities including astronauts, Bill Nye, the Mythbusters, Mayim Bialik and NAO the robot! It was quite apparent that kids of all ages explored their "inner scientist" and had an amazing time at the Festival!
Bill Nye the Science Guy delighted crowds all weekend long! Watch this clip courtesy of The Epoch Times:
We received quite a number of comments and suggestions via email, twitter and Facebook. Twitter followers were tweeting and posting pictures all weekend long! We greatly appreciate all of the feedback and will definitely take it all into consideration for the next celebration!
Here are some of our favorite comments:C.N. writes: "I can't say enough good things about this event! It was wonderful to see so many children so engaged with science, and clearly having fun at the same time! This was probably the best children's festival I have ever attended. Please bring it back to DC next year!"
C.J. writes: "What a FABULOUS Festival! You guys outdid yourselves. The exhibits and volunteers were wonderful. Loved all the cool giveaways, especially Lockheed Martin's blue lighty necklace. Wish we could have seen more... I too am home resting my feet! Thank you!"
NAEYC writes: "It was wonderful to see so many families at the Festival, and teachers who came from a distance to get ideas for their program."
Exhibitor SEM Link writes: "Thank you USA Science & Engineering Festival for allowing SEM Link to be a Partner and Exhibitor for the 2nd US Science and Engineering Festival Grand Finale and Expo. We had a blast and look forward to participating in next year's festival."
J.B. writes: "Whoever came up with the idea of the Science Festival should be congratulated. It made science fun for my children to learn about."
And one of the best comments we received in response to the enormous crowds that attended the Festival was from L.Y. "How nice to see people excited about science and engineering! Nice switch from what people usually complain about.....lines, crowds at concerts, sporting events, etc! Maybe we are making progress!"
Once again, we appreciate all of the feedback and please continue to share your favorite Festival moments on our Facebook page! Stay connected with the Festival and thank you all again your support and enthusiasm! We hope that the Festival inspired you to see that with hard work, dedication and of course the desire to dream big the possibilities are endless!
Read the comments on this post...
Real Climate has done two posts recently that I thought would be served well by their juxtaposition. The first one highlights an early projection of global mean temperatures made by Jim Hansen in 1981.Read the rest of this post... | Read the comments on this post...
Sometimes it's spelled "Waco" but we all know that it should be Wacko. Yet Another Zany Thing (YAZT) has happened there which you may find amusing.Read the rest of this post... | Read the comments on this post...
I'm about a week late talking about this, but I've mostly resigned myself to not doing really topical blogging these days. Anyway, there was a lot of excitement last week over the announcement that an all-star team of nerd billionaires is planning to do commercial asteroid mining. (The post title is a reference to the Sean Connery movie, not the post-Bloom County comic.) I find it kind of amusing that this made the news while I'm doing retrospective blog posts (the next of which is coming), which have turned up a bunch of old posts where I say skeptical things about space in general. So I sort of feel like I ought to say something, and give other people the chance to talk about it in comments.
All in all, I'm pretty much on board with Phil Plait's cautious optimism. The three-stage plan they sketch out seems well considered, they have some plausible-sounding technology, and the principals involved are both seriously smart rich people and people who have shown a willingness to spend huge sums of money to achieve goals they find worthwhile. If this sort of project is ever going to work, this is the kind of team you want working on it.
My primary initial reaction to this was not so much excitement at the idea of asteroid mining per se, because there are a huge number of things that have to fall out the right way for that to work. What struck me as interesting about the initial plan is the first stage, where they plan to launch some unspecified number of small space telescopes. The idea is to use these to detect, identify, and try to determine the composition of asteroids passing relatively near the Earth, but this strikes me as the sort of thing that's likely to turn out to have some scientific benefit that isn't part of the original plan. They're not very large (9" diameter is the spec that keeps getting thrown around), so I'm not quite sure what you'd do with them, but I'm pretty sure that if you gave a bunch of astronomers access to a whole bunch of these, they'd find something interesting to do. Actual astronomers are invited to chime in in the comments.
(The "can be turned toward the Earth" aspect of those seems slightly more problematic, though the resolution wouldn't be all that great. If I'm doing the math right, from the low-ish orbit of the ISS, they'd be able to resolve ~1m objects on the Earth's surface, and only around ~100m from geosynchronous orbit, so this isn't a total panopticon scenario.)
Anyway, I wish them luck, and I'm interested to see what comes of this.Read the comments on this post...
"They will see us waving from such great heights
'Come down now,' they'll say.
But everything looks perfect from far away
'Come down now,' but we'll stay." -The Postal Service Whether you're under urban, city skies, where only a few dozen stars are visible on a clear night, or beneath some of the darkest skies on Earth, the Universe is out there, and you can get started discovering it, right now, for yourself. You can have yourself, as Bishop Allen would sing,
or you can take advantage of it. For me, I currently live in Portland, OR, where the twilight looks like this.
(Image credit: FocusX7 / B. Emmerling on flickr.)
When the Moon sets and the neighbors turn off all their lights, I can get skies that are darker than purely urban skies: maybe all the way down to (lower is better) a seven on the Bortle dark-sky scale.
(Image credit: Stellarium.)
But even with only the most major constellations and asterisms visible, there's still plenty to see, even in the city, if you're interested in exploring the night sky. Darker skies will only net you more (and fainter, dimmer, and more diffuse) objects, of course, so you'll want equipment that will be versatile. Normally, people just starting to take an interest in it have a large number of things they want, some of which they don't even realize they want. What are they?
- You want something relatively inexpensive, because no one wants to blow a lot of money on something you're not even sure you'll like.
- You want something that's quick easy to set up and take down, so that you'll use it often, even late at night, when you're tired and/or unmotivated.
- You want something where the optics are high-quality, because you want to see out into the Universe, not a scratchy, blurry haze.
- You want something with a lot of light-gathering power, capable of seeing as much as you can for the skies that you have.
- And, let's face it, you want something that's durable, because you never take as good care of your stuff as you wish you did.
(Image credit: Focus Scientific.)
This is my preferred tool for checking out the night sky, no matter where I am: a pair of Celestron Skymaster, 20x80mm binoculars. These are versatile -- both for people who do and don't wear glasses -- and they meet all of the criteria above.
- They're cheap, costing only about $100 if you shop around.
- You'll also need a (not included) tripod. The crummy $40 one I bought at Circuit City five years ago is just fine for this, but this is really the upper limit (in weight) that a cheap tripod like this can handle.
- Some lying liars will tell you that you can do just fine without them, but they're no longer with us because they've burned to a crisp from the fires that engulfed them, originating in their pants. Why do you think it has a built-in tripod mount?!
(Images credit: a review at Buzzillions.)
- The 80mm number in that title refers to the diameter of each light-gathering lens, which means these binoculars (when you use both eyes) have the equivalent light gathering power to a 4.5" telescope!
- The optics are multi-coated and the telescope is water/weather resistant, which is very good, but not quite the best. If you want to pay a lot more, you can go for fully-coated optics, and/or a waterproof pair, but for this price point you're not going to find better.
- Finally, setup takes only about 10 minutes, including focusing. The lone exception is that for some pairs (mine wasn't one of them), collimation is a problem, which requires you to either fix them yourself (with an eyeglasses screwdriver), send them in to Celestron, or take them into a camera shop. If you do have this problem, it's a one-time-only fix.
I like these binoculars much better than a telescope for quick setup and takedown, and they really shine -- especially for beginning skywatchers -- for a few reasons. First off, they have a much wider field of view, meaning that when you see an object in the sky, it's much easier for a novice to locate it through binoculars than through a telescope. Second, it's much easier to get to know your night sky, to just move around and explore. Poke around your favorite constellations and bright stars and see what's there. You can see roughly 30-100 times as many stars through a pair of binoculars like this than you can with your naked eye, no matter what the viewing conditions are. The deep-sky objects, ideal for viewing under skies with less light pollution, can be found with these binoculars, too. (The free, downloadable software Stellarium is invaluable for finding what is where, and when.)
And finally, the 20x magnification (what that first number means in binocular-speak) is enough to see some amazing things! The last time I took them out was Sunday night, which was unseasonably warm and clear. Yes, I got to see the color of some of my favorite stars, as well as the pink/red disk of Mars. But there were a few highlights that I wanted to share.
(Image credit: gaelicstorm7 (Alan) of Stargazers Lounge.)
Saturn, bright and yellow in the night sky, has rings that are actually distinctly visible through these binoculars! I wasn't entirely sure I'd be able to see them, but when I had it centered in the field of view and truly focused the binoculars properly, the nearly edge-on rings came into crisp view, and it was my first time seeing them with my own, personal equipment!
(Image credit: John Graham at Cloudy Nights.)
As far as stars go, whenever the Big Dipper is prominent, you owe it to yourself to check out the second star from the end of the handle: Mizar. It's not only a binary star system, with the bright star Alcor also present, but there are many other, fainter stars there as well! Even with my lousy, fairly urban skies, I was very clearly able to see the third brightest star in there, which marked only the second time in my life I'd ever seen it, and again, the first time I'd found it on my own.
And last of all, there's the brightest object that isn't named the Moon in our current night sky.
(Image credit: David at the Astronomy Nexus.)
Venus! Currently in its crescent phase, you'll be able to watch Venus' crescent progressively shrink and shrink over the coming 5 weeks, until in early June it actually transits in front of the Sun, for the last time until 2117!
So if you've got an interest in the night sky, but not a lot of time, money, and not even necessarily good skies, there are still some amazing sights just waiting for you. The question is what are you waiting for; the Universe is yours to explore!Read the comments on this post...
"And what I wanted to do was, I wanted to explore problems and areas where we didn't have answers. In fact, where we didn't even know the right questions to ask." -Donald Johanson You can learn an awful lot about the Universe by asking it different questions than you asked about it previously. If all you ever used were your own senses, there would be an awful lot to learn, but you would be severely limited.
(Image credit: Kerri Rankin Thoreson.)
Even from the highest mountaintops, for example, you'd never be able to distinguish whether the Earth was round like a sphere or flat as a pancake, if all you used were your eyes. But by looking at the Earth on a larger scale than you could achieve otherwise, its roundness becomes both apparent and indisputable.
(Image credit: NASA / Johnson Space Center.)
The same thing applies to the Universe, both on large scales and small. If you want to know what the overall structure is of the Universe, you have to look at it on the largest scales. Looking at individual galaxies or even large clusters of galaxies won't get you there at all; if you want to know what your Universe looks like, you need to look at it on the largest and grandest of all scales, spanning billions of light years in all directions.
(Image credit: Sloan Digital Sky Survey - III / Data Release 8.)
In the above image, still showing just a fraction of the Universe scanned and measured by the Sloan Digital Sky Survey, each pixel represents an entire galaxy. By measuring how galaxies cluster and clump together -- how they are distributed throughout the Universe -- we can determine what it takes to create a Universe that looks like ours.
(Image credit: Millennium-XXL / Raul Angulo & Simon White / MPA-Garching.)
What we learn, as you can go through in detail, is that the structure of the Universe requires that there be a type of matter in it that does not collide with either normal matter or with photons, that outnumbers our (normal) matter by a factor of five- or six-to-one, that don't respond to either electric or magnetic fields, and that... frustratingly, can not be any of the known particles in the Universe!
(Image credit: Contemporary Physics Education Project.)
This would be a very, very big problem under one condition:
If the known particles and laws of physics explained all of the observed phenomena in the Universe.
In other words, if there's no new physics out there (beyond the standard model), then there's no need for any new particles out there, and so, why would there be any dark matter? There simply wouldn't be a strong motivation, not from an elementary physics standpoint.
(Image credit: retrieved from io9.)
And yet the opposite of that is also true: if there is physics out there that isn't explained by the standard model, then there must be new types of particles out there! And if there are new particles out there, there are good candidates for this dark matter. You've probably heard of some of the speculations that abound:
(Image credit: retrieved from École Polytechnique Fédérale de Lausanne.)
For example, if there's a symmetry of nature known as Supersymmetry (or SUSY, for short), then there ought to be twice as many fundamental particles as the ones we currently know about. Moreover, the lightest one is a perfect candidate for dark matter! Until we know what this particle's properties are, however, we don't know exactly what predictions to make as far as particle-particle interactions go.
While dark matter may or may not be supersymmetric in nature (many argue that SUSY may not even exist), this last part -- that until we know what dark matter's particle properties are, we don't know what predictions to make for dark matter's interactions -- is generally true. But there are plenty of other ideas. Two more speculative ones, first, and then two definitive ones.
(Image credit: Kamioka Observatory, ICRR, Univ. of Tokyo.)
The electromagnetic, weak, and strong nuclear forces could all unify at some high energy, in what's called a Grand Unified Theory, or GUT. One of the universal consequences of GUTs is that they all predict that protons will decay, and so that's one of the things we look for. In many variants of GUTs, there are candidates for dark matter that emerge naturally.
(Image credit: Brian Greene / Columbia University.)
Same case for extra dimensions; they may or may not exist, but if they do, then there are plenty of new particles and interactions that certainly exist, and one (or some) of them may make excellent dark matter candidates.
But those -- supersymmetry, grand unification, and extra dimensions -- are speculative ideas, and may not describe our Universe. But there are two observations that we have already made in the Standard Model that already cannot be explained by the particles and interactions we know today. This means there are new particles out there, yet undiscovered, that could easily solve the dark matter problem.
(Image credit: Hiroshi Nunokawa.)
They are observed to have non-zero mass. In fact, all three types of neutrinos have non-zero mass, meaning there is new physics and there are new particles out there! Right-handed (or sterile) neutrinos could very easily make up the dark matter; we are searching for them as you read this! But perhaps the new physics that explains neutrinos isn't also what explains dark matter. There's another problem.
(Image credit: Normal Rockwell, retrieved from here.)
There are a couple of fundamental symmetries of nature that, at least in everyday life, seem pretty obvious. One is that the laws of physics in a mirror -- where left and right are reversed -- are the same as our normal laws of physics. (We call that Parity, or P-symmetry.) Another is that matter and anti-matter obey the same laws of physics. (We call that Charge Conjugation, or C-symmetry.) Most laws of physics that you know, like gravity and electromagnetism, always obey these symmetries.
According to the standard model, they have to; it's coded into the physics. But these symmetries don't exist for the nuclear (weak and strong) forces in the standard model. If I took something like a muon, reflected it in the mirror (applying P-symmetry), and replaced that image with an anti-muon (applying C-symmetry), I'd be testing whether the combination of CP-symmetry was a good one or not.
(Image credit: James Schombert at University of Oregon.)
If it were a good symmetry, then if all the muons decayed with one orientation, all the anti-muons would decay with that specific, mirrored orientation. But they don't, and so that CP-symmetry is violated. This is good for the Universe, because CP-violation is one of the necessary things to make more matter than anti-matter. But if it happens for an interaction like this -- the Weak nuclear interaction -- then it stands to reason that it should also happen for the strong nuclear force.
But it doesn't! Why wouldn't it?
The same reason this unicycle toy doesn't tip over: there must be some sort of extra, hidden weight that provides extra balance, or in the particle's case, crushes the amount of strong CP violation. Theoretically, the standard model allows you to violate both C and P together here, but we've looked, and to something like one part in a billion, we don't see any. So something -- and this means there's new physics -- has got to be forbidding it!
This outstanding problem, known as the Strong CP problem, is the second hint of new physics that must go beyond the standard model. And at least one class of solutions to it produces an outstanding dark matter candidate, known as the axion.
There's definitely physics in this world that's beyond the standard model, there's definitely more to neutrinos than we know, and there's definitely something stopping CP violation from occurring in the strong interactions. There may also be extra dimensions, grand unification, supersymmetry, or something even more exotic or surprising. But all of these possibilities require new particles, many of which make good dark matter candidates, and all of which have unknown particle parameters.
When you combine this information with our astrophysical knowledge of dark matter, you can see why I prefer the approach of using the astrophysics to try and reconstruct/determine some of the particle properties of dark matter, and try to guide us as to what we should look for. (No, really, I sometimes research that!)
We've got lots of options and lots of searches going, but there's so much we don't know about it at this point! Cross-sections, masses, reaction rates, lifetimes, etc., they're all mysteries at this point. We may not know what dark matter is, exactly, but we've got lots of strong possibilities for what it could be, and some hints that simply can't be ignored. We're desperately trying to be able to detect it directly, and solve this mystery once and for all. Welcome to the cutting edge!Read the comments on this post...
The excitement is filling the air at Sneak Peek Friday today as we are gearing up for an amazing weekend! The Festival takes place Saturday from 10-6 and Sunday from 10-4 at the Walter E Washington Convention Center in Washington, D.C. Please visit our "Plan Your Day" section on our website for important information regarding attending this FREE event. Those attending the Festival will be in for quite a treat with over 3,000 hands-on science and engineering activities and over 150 stage shows!
We have had some incredible events leading up to this weekend including our AT&T Sponsored Nifty Fifty Program. The 'Nifty Fifty (times 2)' are a group of one hundred noted science and engineering professionals who visited Washington, D.C. area schools to speak about their work and careers. We were absolutely thrilled with the speakers and the students seemed to really enjoy this talented group that presented with such passion and enthusiasm.
Some of the Nifty Fifty Speakers included NIH Director Francis Collins, NASA Deputy Administrator Lori Garver, Evolutionary Biologist Dr. Beth Shapiro, Nerd Girls Founder & Engineer Dr. Karen Panetta and many more! Students learned about the need to preserve coral reefs, sustainable 'Styrofoam' made from mushrooms, how diseases are cured and best of all the importance to follow their dreams and overcome obstacles.
This weekend the Festival will be jam packed with entertainment for the entire family. The Expo exhibits and stage shows are suitable for ALL AGES! We have a huge line up of entertainment for the little ones including PBS Kids, a plethora of exhibits and events for students of all ages and of course some in depth STEM exhibits for those with the advanced scientific palate. We have some big name science celebrities that will be in attendance including Bill Nye the Science Guy, Adam Savage and Jamie Hyneman from the Mythbusters, Big Bang Theory's Mayim Bialik, Sleight-of-hand Artist Apollo Robbins and Discovery Channel's Jeff Lieberman. Our Book Fair features 36 of the TOP science authors such as Homer Hickam, Robin Cook, Carl Zimmer, Lisa Randall and Ken Denmead.
Here are just a few of the stage shows and hands-on exhibits that you can look forward to:
The Many Worlds of Lockheed Martin. Check out more than 25 new exhibits from Lockheed Martin, the official host of the Festival! Immerse yourself in the cockpit simulator of an F-22 fighter jet, tour cities of the future; delve into the wonders of robotics and the Hubble telescope, plus many more exciting adventures!
Meet the Scientists/Engineers. Chat one-on-one at this Career Pavilion location with some of the nation's top scientists, engineers to learn about such fields as medical research, oceanography, national security with the CIA, microbiology, and technology intellectual property law!
Innovative Entrepreneurs. Hear these exciting entrepreneurs who are changing the course of technology: Elon Musk, creator of rocket manufacturer SpaceX, and legendary computer video game innovator Richard Garriott who became the sixth private citizen to journey into Earth's orbit.
Music by Monty Harper. Dance like a dinosaur and spin like a planet. You'll do it all to the music of this science singer-musician who was recently named a winner in the Festival's songwriting competition.
Ready for the Science Olympiads? Learn how to compete in the Science Olympiads from Olympiad student teams in the DC Metro area who will demonstrate vehicles, structures, musical instruments and other devices they've developed for the competition!
Saving the Humpback. Nan Hauser, founder of the Center for Cetacean Research & Conservation, will inspire you with her fascinating expeditions to save the endangered humpback whale and other marine species.
Circus Physics. How do all those clowns fit in one car? What's involved in the physics of the ferris wheel and roller coaster? Come to the circus exhibit of the American Institute of Physics and other partners to find out!
The Science of Bubbles. The fascinating Keith Michael Johnson (as seen on the Discovery Channel's Time Warp), uses soap bubbles to explain liquids, solids and gasses, geometry, tension and pressure.
Enjoy yourself this weekend and take time to explore as much as you can. We hope the Festival ignites the "Inner Scientist or Engineer" in you! Thank you for all of your support and have an amazing time!Read the comments on this post...
I've been falling down on the shameless self-promotion front, lately, but that doesn't mean I'm not tracking How to Teach Relativity to Your Dog obsessively, just that I'm too busy to talk about it. Happily, other people have been nice enough to talk about it for me, in a variety of places:
- The most significant, in terms of probable impact on sales, is this excerpt at BoingBoing, which is the text for the dog dialogue from Chapter 8. This is the same dialogue that became the "Looking for the Bacon Boson" video, and, indeed, they were nice enough to include the video in the post, too. Woo-hoo!
- Over at Backreaction, Bee gave the book a nice review ("a flawless popular science book that gets across a lot of physics in an entertaining way. If you always wanted to know what special and general relativity is all about and why it matters, this is a good starting point."). This is a huge relief not just because she said nice things about it, but because she didn't spot any huge mistakes, which I'm always paranoid about when I see actual physicists writing about my stuff.
Just Two Days Until the Largest Celebration of Science & Engineering! [USA Science and Engineering Festival: The Blog]
The 2nd USA Science & Engineering Festival has finally arrived! The Expo will take place this weekend at the Walter E Washington Convention Center in Washington, DC. The hours are Saturday from 10-6 and Sunday from 10-4. Evening shows are also scheduled for the weekend including the Stargazing Party with Bill Nye and Featured Author Panel Discussion- Science Stories in Society & School: Using Narrative to Bridge the Gap.
The Festival will be packed with entertainment for the whole family with 3,000 amazing hands-on exhibits and over 150 incredible stage shows. This FREE event is perfect for all ages and has something special for just about everyone. We have created "thematic tracks"' including Tiny Animal Lovers, Math is Really Fun, Be a Robotics Engineer, Nuclear to Stellar and much more to make your Festival experience fun, easy and enjoyable. Please visit our Plan Your Day Section on our website for all your Festival questions. And be sure to download our free Festival App to stay connected to the Expo using your mobile device. Iphone users can download the app here and Android users can download the app here.
We thank you for all of your support and look forward to seeing you this weekend! Please enjoy this awesome video created by Festival Founder Larry Bock's talented daughter:
Read the comments on this post...