My Cameo in the “ClimateGate” Emails | The Intersection

It has been brought to my attention that I am mentioned, once, in the “ClimateGate” email stash. If you go here and search for my name, you find this, an email from Tom Wigley of NCAR, who I have interviewed for various stories:

From: Tom Wigley <wigley@xxxxxxxxx.xxx>
To: santer1@xxxxxxxxx.xxx
Subject: Re: [Fwd: [Fwd: FW: Press Release from The Science & Environmental Policy Project]]
Date: Mon, 10 Dec 2007 17:17:14 -0700
Cc: carl mears <mears@xxxxxxxxx.xxx>, Frank Wentz <frank.wentz@xxxxxxxxx.xxx>, Tom Wigley <wigley@xxxxxxxxx.xxx>, Steven Sherwood <Steven.Sherwood@xxxxxxxxx.xxx>, John Lanzante <John.Lanzante@xxxxxxxxx.xxx>, “‘Dian J. Seidel’” <dian.seidel@xxxxxxxxx.xxx>, Melissa Free <Melissa.Free@xxxxxxxxx.xxx>, Karl Taylor <taylor13@xxxxxxxxx.xxx>, Steve Klein <klein21@xxxxxxxxx.xxx>, Leopold Haimberger <leopold.haimberger@xxxxxxxxx.xxx>, “Thorne, Peter” <peter.thorne@xxxxxxxxx.xxx>, “‘Philip D. Jones’” <p.jones@xxxxxxxxx.xxx>

Dear all,

I think the scientific fraud committed by Douglass needs to
be exposed. His co-authors may be innocent bystanders, but
I doubt it.

In normal circumstances, what Douglass has done would cause
him to lose his job — a parallel is the South Korean cloning
fraud case.

I have suggested that someone like Chris Mooney should be
told about this.

Tom.

In searching my emails, I was never told about this, and certainly never wrote anything about the situation, which I am not familiar with. As a journalist, though, I certainly do want to receive tips of things to write about, and I frequently do from a wide variety of folks. With only the most rare of exceptions, I never get around to writing anything; but in this case, I wasn’t even tipped.

Still, I can see why scientists concerned about global warming, and accepting of the scientific consensus, would want me to cover the topic, including its political side. By 2007 I already had a track record for exposing the misinformation campaign to mislead the public about climate change, something I continue to do today. And given that there is such a misinformation campaign–with “ClimateGate” being the latest and perhaps the most severe example–we need scientists and journalists alike striving to set the record straight.

I guess that that’s my way of saying that, as with virtually all of the “ClimateGate” emails that I have seen, the single one mentioning my name is not very surprising–especially as it regards me, who never even heard of this until now.


A sun pillar gooses the sky | Bad Astronomy

Regular readers know I’m fascinated with sky phenomena. On December 26, 2009, around 4:30 p.m. local time, I happened to look out my office window and saw a gorgeous beam of orange light shooting straight up into the sky out of the sunset. I rushed outside with my camera and got this shot of it:

[Click to embiggen.]

Isn’t that pretty? I think it’s a sun pillar, a vertical column of light caused by the setting sun’s light being reflected off of the flat surfaces of hexagonal ice crystals in the air. Given that it was several degrees below freezing when I shot this, ice crystals in the air isn’t a totally crazy idea.

However, I can’t be sure this isn’t just a run-of-the-mill crepuscular ray, just those normal beams of light you see coming from the setting Sun as it’s broken up by clouds near the horizon. But it’s rare to see a single ray like that, and much rarer to see it beaming straight up like that.

As I was taking this shot, I heard honking coming from the north that I instantly knew was coming from geese. I waited a moment, and then hundreds of geese in formation flew right into the shot! Awesome, and very scenic. I was able to get some pictures, but had to stop down the camera to get the geese, and that introduced noise (the speckly grainy look in digital images) into the sky. I fiddled with the contrast a bit to show the geese, and the picture still looks a little "grainy" but cool:

There were several V-formations of geese this size going by over the course of a minute or two, and during that time the pillar faded, as you can see in this shot. Still, what a sight!

This is the kind of thing you see when you open your eyes and look up. If we could take every human on the planet one at a time, hold their hand, and simply show them this, then I just bet this world would be a better place.

Life is beautiful. You just have to notice it.


Get your mass handed to you | Bad Astronomy

If you want to lose weight, then you should avoid this Ebay auction, where someone has a Higgs boson up for bids.

ebayhiggs

The Higgs boson, for those not up on their Standard Model of Particle Physics, is the subatomic particle that is theoretically responsible for giving all the other little particles their mass, and its detection is one of the main goals of the Large Hadron Collider. Come to think of it, the folks at CERN could’ve saved a lot of cash had they simply bid here instead of building a bazillion dollar machine to look for the Higgs. But then how would Brian Cox find work?

And I love that graphic. 10? That’s a big number. You’d think magnifying the Higgs by that amount would make it look bigger.

Anyway, read the whole thing, because it’s pretty funny. Of course, this is a joke, and Ebay will no doubt take it down soon, so look before it’s gone and you’re doomed to travel the Universe forever with your mass kicked.

Tip o’ the spin 1/2 lepton to BABloggee Martin Kielty.


The Science of Avatar (Part I) | The Intersection

So I finally saw Avatar–the 3D IMAX version–and it exceeded my expectations; not as a result of the much-hyped new technology, but because this story resonates. Though it takes place on an imagined world called Pandora, many themes speak directly to 21st century planet Earth. I’m certainly not about to spoil the plot for those yet to see the film, but would like to emphasize I’m particularly appreciative that James Cameron and his crew got so much of the science in this film right.

Picture 4

Several details struck me as well-researched and extremely innovative and I will do a post in the coming week on some of the most interesting examples. First, I’m curious to learn what aspects of this sci-fi movie appealed most to our readers in the science community. (There are likely posts around the internet about this already, but as I’ve been spending much time offline, have not yet checked). So leave your impressions in comments and we’ll return to the Science of Avatar next week….


Anniversary of a cosmic blast | Bad Astronomy

sgr1806_artFive years ago today — on December 27, 2004 — the Earth was attacked by a cosmic blast.

The scale of this onslaught is nearly impossible to exaggerate. The flood of gamma and X-rays that washed over the Earth was detected by several satellites designed to observe the high-energy skies. RHESSI, which observes the Sun, saw this blast. INTEGRAL, used to look for gamma rays from monster black holes, saw this blast. The newly-launched Swift satellite, built to detect gamma-ray bursts from across the Universe, not only saw this blast, but its detectors were completely saturated by the assault of energy… even though Swift wasn’t pointed anywhere near the direction of the burst! In other words, this flood of photons saturated Swift even though they had to pass through the walls of the satellite itself first!

It gets worse. This enormous wave of fierce energy was so powerful it actually partially ionized the Earth’s upper atmosphere, and it made the Earth’s magnetic field ring like a bell. Several satellites were actually blinded by the event.

So what was this thing? What could do this kind of damage?

Astronomers discovered quickly just what this was, though when they figured it out they could scarcely believe it. On that day, half a decade ago, the wrath of the magnetar SGR 1806-20 was visited upon the Earth.

Magnetars are neutron stars, the incredibly dense remnants of a supernovae explosions. They can have masses up to twice that of the Sun, but are so compact they may be less than 20 kilometers (12 miles) across. A single cubic centimeter of neutron star material would have a mass of 1014 grams: 100 million tons. That’s very roughly the combined mass of every single car on the United States, squeezed down into the size of a sugar cube. The surface gravity of a neutron star is therefore unimaginably strong, tens or even hundreds of billion times that of the Earth.

sgr1806_magfieldartWhat makes a neutron star a magnetar is its magnetic field: it may be a quadrillion (1015) times stronger than that of the Earth! That makes the magnetic field of a magnetar as big a player as the gravity. In a magnetar, the magnetic field and the crust of the star are coupled together so strongly that a change in one affects the other drastically. What happened that fateful day on SGR 1806-20 was most likely a star quake, a crack in the crust. This shook the magnetic field of the star violently, and caused an eruption of energy.

The sheer amount energy generated is difficult to comprehend. Although the crust probably shifted by only a centimeter, the incredible density and gravity made that a violent event well beyond anything we mere humans have experienced. The quake itself would have registered as 32 on the Richter scale — mind you, the largest earthquake ever recorded was about 9 on that scale, and it’s a logarithmic scale. The blast of energy surged away from the magnetar, out into the galaxy. In just 200 milliseconds — a fifth of a second — the eruption gave off as much energy as the Sun does in a quarter of a million years.

sgr1806_mwmapA fireball of matter erupted out of the star at nearly a third the speed of light, and the energy from the explosion moved — of course — at the speed of light itself. This hellish wave of energy expanded, eventually sweeping over the Earth and causing all the events described above.

Oh, and did I mention this magnetar is 50,000 light years away? No? That’s 500 quadrillion kilometers (300 quadrillion miles) away, about halfway across the freaking Milky Way galaxy itself!

And yet, even at that mind-crushing distance, it fried satellites and physically affected the Earth. It was so bright some satellites actually saw it reflected off the surface of the Moon! I’ll note that a supernova, the explosion of an entire star, has a hard time producing any physical effect on the Earth if it’s farther away than, say, 100 light years. Even a gamma-ray burst — an event so horrific it makes the hair on the back of my neck stand up just thinking about it — can only do any damage if it’s closer than 8000 light years or so. GRBs may not even be possible in our galaxy (they were common when the Universe was young, but not so much any more), which means that, for my money, magnetars may be the most dangerous beasties in the galaxy (though still unlikely to really put the hurt on us; see below).

Here’s what Swift detected at the moment of the burst:

swift_sgr1806

As Swift scientist David Palmer describes:

This is the light curve that [Swift's Burst Alert Telescope] saw, showing how many gamma rays it counted in each sixteenth of a second during six minutes of observation. I didn’t draw the main spike because it was 10,000 times as bright as the tail emission, and you would need a monitor a thousand feet tall to look at it.

The blast was so strong Swift saturated, counting 2.5 million photons per second slamming into it, well off the top of that graph (and the actual blast was far brighter yet, as other satellites were able to determine).

See the pulsations in the plot? After the initial burst, which lasted only a fraction of a second, pulses of energy were seen from the magnetar for minutes afterward. The pulses occurred every 7.56 seconds, and that’s understood to be the rotation period of the neutron star. The crack in the crust got infernally hot, and we saw a pulse of light from it every time it spun into view. This same pulsing was seen by other satellites as well.

The damage from the explosion was actually rather minimal here on Earth. But that’s because SGR 1806-20 is 50,000 light years away. Had it been one-tenth that distance, the effects would have been 100 times stronger. We’d have lost satellites at least, and it would have caused billions of dollars in damage in NASA hardware alone. Of the dozen or so known magnetars, none is that close (though a couple are about 7000 light years away). Magnetars aren’t easy to hide, but it’s possible there are some within 5000 light years. It’s unlikely, though, and I’m not personally all that concerned.

I do have one thing to add: when this event occurred, I got an email from someone convinced that the magnetar was responsible for the earthquake in Indonesia that created the devastating tsunami that killed more than 250,000 people. However, there is one small problem with that idea. Well, two problems, really, the first being there’s no physical way it could have triggered an earthquake! But a worse problem is that the earthquake occurred on December 26th at 00:58 UT, and the burst from the magnetar was at December 27 at 21:30:26 UT, about 1.5 days later. Oops.

But why let facts get in the way of a good pseudoscientific theory?

The tantrum from SGR 1806-20 is one of the best studied events of its kind, and is certainly the most powerful ever detected in the modern era. Astronomers will be studying the magnetar, and others like it, very carefully to see what can be learned from them. If you want to read more, then I suggest the NASA page about the event, as well as the Sky and Telescope magazine page on it, too.

And if another blast like that one comes from SGR 1806, or any other magnetar, don’t worry: I’ll report it right here. Unless it fries my computer. Or just my brain, reading about it.

Image credits: NASA


Seasons E-rings! | Bad Astronomy

[It was either that title or "E-ring in the New Year".]

Here’s an unusual shot from the Cassini spacecraft: Saturn’s faint, diffuse E ring, seen almost edge-on:

cassini_ering

I like this picture! First, we’re used to seeing Saturn’s rings looking sharp and well-defined, but this ring is fuzzy. It’s huge; it doesn’t even start until well outside the main rings, about 130,000 km (78,000 miles) above Saturn’s cloud tops, and is 300,000 km (180,000 miles) across! It’s thought that the ice particles in the ring are supplied by geysers from the moon Enceladus.

Second, we’re also used to seeing pictures of Saturn sitting in inky darkness. Saturn, its rings, and most of its moons are very bright, far brighter than the background stars. Exposing the images correctly for Saturn means the stars don’t show up, so the background is black (though not always, as this nice shot of the Pleaides from Cassini attests). But the E-ring is so faint that a longer exposure was needed, and then the fainter stars show up in multitudes.

This image was taken when Cassini was 2.5 million km (1.5 million miles) from Saturn, which was far enough to fit in a good amount of the edge of the ring. I really love all the images Cassini takes, but it’s the more unusual ones I really enjoy. Here’s hoping we see lots more in 2010!

Related Post: Cassini Dances with Enceladus Once Again.

Image credit: NASA/JPL/Space Science Institute


/tæ?tu/ | The Loom

phonetics“My name is Steve Kleinedler, supervising editor for the American Heritage Dictionary, where I have worked since 1997. One of my many responsibilities is pronunciation. The tattoo is a stylized version of a phonetic vowel chart — it shows the relative position of the tongue in the mouth when those vowel sounds are articulated. I had a smaller, simpler version done on my upper back in 1993, and I’ve been wanting to get the full version for quite some time.

“The design is by Kyle Nelson of Stoltze Design and the tattoo artrist was Mike Helz of Stingray Body Art.”

Click here to go to the full Science Tattoo Emporium.


NPR Science Friday interview today | Bad Astronomy

me_nprI’ll be on today’s episode of NPR’s Science Friday! Ira Flatow hosted a round-table panel discussion with Paul Raeburn, Mariette DiChristina (the new editor-in-chief of Scientific American magazine), Wired senior editor Nick Thompson, and me. We chatted about the year in science news including social networking (like Twitter), privacy, Hubble, the Moon, and lots of other things, too. I had a fun time recording it, and I expect it’ll be fun to listen to as well.

It airs on NPR from 2:00 – 4:00 Eastern time, and should be available online too.


A Grand Tour

I’d be going to this if I could!!
THE KNOWN UNIVERSE: A GRAND TOUR
WHAT: The American Museum of Natural History presents Known Universe: A Grand Tour, The longest and most exhilarating trip a New Yorker can take without leaving the city.
..
Join astrophysicist Brian Abbott as he leads guests on an adventure from Earth to the edges of the known universe. Step inside the world’s largest cosmic atlas and prepare for space travel through our solar system and beyond.
..
On the first Tuesday of each month, these interactive cosmic tours display data based on the best scientific research to-date, and are guided by live presenters. The Museum invites all to take the journey of a lifetime.
..
WHEN: Tuesday, January 5, 6:30 pm
..
WHERE: Hayden Planetarium, Space Theater
American Museum of Natural History
Enter at 81st/Rose Center
..
ADMISSION: $15 adults $13.50 Members, students, and seniors

Drying Climate Turned Possum-Like Critter Into the Strange Koala | 80beats

koalaMillions of years ago, a koala looked more like a possum. By studying rare skulls of the famous marsupial that date between 5 and 24 million years old, a team of Australian researchers propose how it got to looking like it does today, with findings published in the Journal of Vertebrate Paleontology.

Food was one driver, they say—millions of years ago koalas ate a variety of foods. The dietary switch to an exclusive eucalypt diet seems to have occurred during the late Miocene period, some 12 to five million years ago, when a drying climate made eucalyptus the dominant forest species [Canberra Times]. As a result, they lost their snouts and developed powerful jaw muscles.

But while koalas need to adapt to the changing food supply, they also needed to stay in communication, and began to develop the low-frequency calls that today can travel half a mile. The researchers hypothesize that the ancient koalas evolved their communication system at a time when the Australian continent was drying out and the koala habitat becoming less dense. By lowering the frequency of their calls, they were able to maintain communication in the sparser forests [Wired.com]. And to hear those low-frequency calls, koalas developed a middle ear with high volume compared to other marsupials.

“The unique cranial configuration of the modern koala is therefore the result of accommodating their masticatory adaptations without compromising their auditory system,” write the researchers [Wired.com]. In other words: you put those two things together and you get today’s adorable but strange marsupial.

Related Content:
80beats: Worsening Drought Threatens Australia’s “Food Bowl”
Discoblog: Rat Risotto And Emu Chips: Thing Not To Eat in Australia
DISCOVER: One Marsupial Too Many

Image: flickr / tinyfroglet