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Bad Astronomy

A case study of the tactics of climate change denial, in which I am the target

Over the years I have pointed out the fallacious arguments of climate change deniers when they attack legitimate climatologists like James Hansen and Michael Mann. This is, of course, like kicking at a bee hive, and whenever I do the comments section of my posts fill with lots of angry buzzing.

But now, for what I think is the first time, I find myself the target of an attack. And I have to admit, I welcome it: it’s a textbook case of denialist sleight of hand, of distraction, distortion, error, and misdirection.

Stick around for all of this. It’ll be… interesting.


Our story so far

OK, first, here’s the scoop: a few days ago, I wrote a blog post taking apart two intellectually bankrupt climate change denial articles, one in the Wall Street Journal, and the other in the UK’s Daily Mail. Both were claiming that global warming appears to have stopped in the past few years, a claim which is trivially easy to show wrong. In fact, I linked to two articles doing just that: one at Skeptical Science, and another I myself wrote. Finding actual scientists destroying that claim is not hard at all; those two links have many more links therein.

In my post about the WSJ and DM, I included a graph. It pretty clearly shows temperatures rising from 1973 to the present. And this is where the fun begins.

That’s the plot. It’s from a recent, independent study done at Berkeley, and represents actual, measured, data. Just to be clear, those points are from weather stations across the globe, and the method used to collect and analyze those measurements is described by the Berkeley team themselves (PDF). With me so far?

Apparently, William Briggs is not with me. He takes very vigorous exception to the graph in an article he wrote which he titled "Bad Astronomer Does Bad Statistics: That Wall Street Journal Editorial." I encourage you to read it, so that you can assure yourself I am not misrepresenting his arguments in any way.

I found out about this article when I saw a tweet by Dr. Briggs himself. My first thought was: Uh oh. I sure hope I didn’t make a math mistake somewhere in my WSJ post! I better read Briggs’ article and see… So I read it.

My next thought after reading his arguments was then: Ho-hum. So?


The mismeasure of an argument

Basically, Briggs accuses me of not understanding statistics, of not including error bars, of misrepresenting that points in that plot, of not displaying the plot correctly, and so on ad nauseum. His biggest claim: that those points aren’t measurements at all, but estimates.

Here’s the thing: he’s wrong. Those point are in fact measurements, though they are not raw measurements right off the thermometers. They have been processed, averaged, in a scientifically rigorous way to make sure that the statistics derived from them are in fact solid. The Berkeley team describes in detail how that was done (PDF), and does actually call them estimates, but not because they are just guessing, or using some arcane computer model. They are technically estimates, in the sense that any measurement is an estimate, but they are really, really good ones. Greg Laden tears this use of words apart, as well as pretty much everything else Briggs wrote.

Oddly, Briggs then goes on to call them "predictions" for some reason, and that they came from "models", which is just weird. It’s as if he’s trying to use a word choice that raises doubt about the measurements. But again he’s wrong. They really are measurements, not model predictions. At Open Mind, Brigg’s word choice once again is ripped apart. [Note: Briggs has left a comment there, further verifying the fact that his use of words is incorrect.]


This reminds me of one of my favorite skeptic jokes. Question: How many legs does a dog have if you call its tail a leg?

Answer: Four. It doesn’t matter what you call a tail, it’s not a leg.


There are many other places where Briggs makes mistakes that render his arguments null; for example, the error bars (what statisticians usually call "uncertainty") are in fact made available by the Berkeley team, and are small compared to the long-term rise in temperature. For another, Briggs says I should’ve shown the plot going farther into the past, because 1973 was actually a low point. However, that’s completely wrong: it’s actually a high point! As Deep Climate points out here, this actually makes the warming trend lower. So in true contrarian fashion, Briggs is contrary even to himself. It’s bizarre.

So really, there goes Briggs’ argument. His main point is wrong, so we’re done, right?

Well, no. There’s more fun to be had here.


Beside the point

If you read Briggs’ article, you certainly get the impression that because the graph I use is statistically meaningless (so he incorrectly claims), then my whole argument about global warming is wrong.

And this is where I found myself greatly amused, though in a schadenfreude sort of way.

Think of it this way: if my argument hinged on that graph, and I removed it, my argument would have no foundation, correct? It would change the tenor of the entire blog post.

Go look at my article. If you remove that graph from it, what changes? Nothing. My main point — that the WSJ and DM articles are wrong, that we have lots of evidence the Earth is warming up, that 9 of the 10 hottest years on record occurred since the year 2000, that the DM article specifically uses scientific studies and presents them as if they say the exact opposite of what they actually say — still stands.

So even if that graph is wrong and misrepresents what I’m saying — which it does not — it doesn’t matter. In fact, I used that graph as an illustration, to show how we’re warming up. I never intended it to be the basis for the argument I was making, just a way of further showing it. If you read the actual words I wrote, including the links to many, many articles backing up my position, you’ll see that Briggs has not refuted a single actual point I made.

So even if he’s right about that graph, it doesn’t matter. And he’s not right.

But notice what he’s done. He’s taken what is clearly a minor point and blown it up as if it’s my main point. He’s used shady words (predictions, models) to cast aspersions, and to make someone (me!) look bad. Then, by "refuting" this minor issue he can then poison the well, strongly implying that all my arguments are wrong. That’s kind of a big no-no when trying to argue a point.

But it packages well. Watts Up With That, another denialist blog, has run with Briggs’ claims about me as well. He also makes the false claim that warming has stalled, and so on. Note WUWT also says the signers of the WSJ OpEd are "16 scientists", which isn’t true: not all are scientists, and only four have actually published climate science research. And don’t forget about the article the WSJ refused to print talking about the reality of global warming, signed by 255 actual scientists.

Oops.


Denialism’s dark mirror

I will admit the irony of this attack amuses me greatly; Briggs accuses me of many things he himself is doing. That is standard fare from antiscience group: creationists, global warming deniers, and alt-medders, for example, all seem to project their own tactics on the scientists with whom they disagree. Don’t like real medicine? Accuse scientists of being in the pocket of Big Pharma (and forget about the millions being made by quacks on useless "remedies"). Don’t believe in evolution? Accuse scientists of being too dogmatic. Don’t think global warming is real? Accuse scientists of misrepresenting the data.

My favorite irony is that a lot of these global warming denialists take money from fossil fuel interests, but then routinely say to "follow the money", as if it’s the climatologists who are raking in the big bucks from shady think tanks with undisclosed bankrollers. While Briggs points out he gets no money from them, he asks where my money comes from. Think on this, Dr. Briggs; how much money would I make if I suddenly turned coat and said global warming wasn’t real? I’ll guarantee you it would be a lot more than I make now, probably with a couple of zeroes added to the end. So that argument falls a wee bit flat here.

Like all the others.

Of course, given the comments I’ve seen on my blog, on Briggs’ blog, on Watts Up With That, or in any other blog discussing global warming, I know how this will go. You can bring up the major pieces of evidence supporting reality again and again, but the denialists will ignore them and go after phantoms instead. Because if they do acknowledge the actual evidence, they lose.

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February 2nd, 2012 7:00 AM Tags: climate change, denialism, global warming, William Briggs
by Phil Plait in About this blog, Alt-Med, Antiscience, Debunking, Piece of mind, Politics, Religion, Science, Skepticism, Top Post | 266 Comments »

Give Pluto your stamp of approval

In 2015, NASA’s New Horizons spacecraft will zip past Pluto, giving us our first close-up view of this tiny world.

The team behind the space probe have a nice idea to help raise awareness of it: make a new US Post Office stamp commemorating it. My friend Dan Durda, both an accomplished astronomer and artist, created this lovely design of the stamp:

[Click to enhadesenate. Note: the word "Forever" means the stamp is always good for first class postage, and is crossed out here to prevent forgery.]

It shows the spacecraft going by Pluto and its (relatively) freakishly large moon Charon. I like how he didn’t go for photorealism, but instead used an oil paint-like feel for it. The stamp is meant as a followup — I might even say send-up — of a US stamp issued in 1990 about Pluto that has the label "Not Yet Explored".

I like this stamp! I’d love to see it made official, too. Alan Stern, the head guy for the mission, created a petition to help that along. It takes more than just a nice stamp design to get the PO’s notice; it has to have public support as well. I signed the petition, and if you want to, please do.

I’ll note that I expect this to raise the specter of whether Pluto is a planet or not. I have some thoughts on that, and I’ll be posting again soon on that topic.


Related posts:

- Pluto has another moon!
- Find cold, distant worlds with Ice Hunters
- Pluto still may be the biggest dwarf planet
- Percy, Percy, me

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February 1st, 2012 11:00 AM Tags: Alan Stern, Dan Durda, New Horizons, Pluto, stamp, US Post Office
by Phil Plait in Astronomy, Cool stuff | 43 Comments »

What caused the Little Ice Age?

Over the course of several hundred years – most notably in the 17th and 18th centuries — winter temperatures in western Europe were much lower than normal. Glaciers came much farther south than they had before, and a famous painting shows people ice skating on the Thames river — which hasn’t been frozen since. The period is known as the Little Ice Age, and its cause has always been something of a mystery.

However, new research by scientists at the University of Colorado-Boulder (yay team!) may have pegged it: the LIA appears to have started abruptly in the late 13th century, between the years 1275 and 1300. Radiocarbon dating of plants from Baffin Island (north of the Hudson Bay in Canada) and sediment samples from a lake in Iceland indicate that there was a rapid onset of severe cooling at that time. It’s been thought that the cooling started around then, but it’s been hard to pin down until now.

More importantly, this narrows down the cause of the LIA: four tropical volcanoes erupted violently in that period. The ash would have darkened the atmosphere, letting slightly less sunlight down. Some of the gases emitted by volcanoes also cool the air. It seems clear these volcanoes are what triggered the Little Ice Age. But why did it last so long?

That may be due to what happened after the volcanoes erupted. Most likely, the warmer temperatures would have melted the north polar sea ice. This fresh water is less dense than salty water, so it would flow on top of the oceans, and wouldn’t have mixed well with the deeper water. This would have slowed the transport of heat from the equatorial waters back up north, cooling them further. That system is what maintained colder temperatures for so long. There were variations — the Ice Age was more of as series of pulses of temperature drops than one long period — but for centuries the heating of the Earth was disrupted in that region.

For a long time it’s been suspected that the Sun played a role here, too. During the period of 1645 to 1715 there were few or no sunspots, a time called the Maunder Minimum. Sunspots are dark, but they’re surrounded by a region, a rim, that emits strongly in the UV. These faculae, as they’re called, actually more than make up for the darker regions of the spots, so in reality sunspots add to the amount of light and heat the Earth receives, by a fraction of a percent. So an active Sun, it’s thought, may warm the Earth a teeny bit more.

Read the rest of this entry »

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February 1st, 2012 7:00 AM Tags: climate change, global warming, Little Ice Age, volcanoes
by Phil Plait in Antiscience, Debunking, NASA, Piece of mind, Science | 98 Comments »

Amazing moonset video taken from space!

Thanks to astronaut Ron Garan on Google+, I was alerted to some amazing footage of the Moon setting as seen by astronauts on board the International Space Station. I uploaded it to YouTube and added some comments to show you something really cool…

[Set it to high-def and make it full screen!]

Astonishing, isn’t it? As the Moon sets, you’re seeing it through thicker and thicker air. The air acts like a lens, bending the light upward. The part of the Moon nearer the Earth’s limb gets bent up more, so the Moon looks like it’s getting flattened. Watch it again; the top of the Moon doesn’t appear to be affected much. It looks more like the bottom slows down and the top pushes into it. You can read about this effect in more detail in an earlier blog post.

Weirdly, as I watched the video, it looked very much like the whole Moon was shrinking as it set, as if it were receding rapidly. When I saw that I knew intuitively that couldn’t be real; the ISS is only moving a few thousand kilometers over the time this whole video was taken (about ten minutes), not nearly enough to see that big a change in the size of the Moon. It’s 400,000 kilometers away, after all! So I measured the size of the Moon on the screen, and incredibly the width doesn’t change. Do you see it appear to shrink too? It’s an illusion!

Funny how our brain interprets such things. As if seeing a gigantic rock moving through the sky while perched on board a football-field sized satellite moving at 30,000 km/hr isn’t weird enough!

Credit: Image Science and Analysis Laboratory, NASA-Johnson Space Center. "The Gateway to Astronaut Photography of Earth".


Related posts:

- The Moon is flat!
- The twice reflected Moon light
- Incredible time lapse: Milky Way over Africa

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January 31st, 2012 6:32 PM Tags: Earth, International Space Station, ISS, Moon, moonset
by Phil Plait in Astronomy, Pretty pictures | 9 Comments »

Q&BA: What happens if you are exposed to the vacuum of space?

[Note: Every week I hold a live video chat on Google+ where I answer questions from readers. I call it Q&BA, and when I get a question that stands alone, I'll make it its own video. ]

A lot of people, it seems, have morbid thoughts about space. Why else would I get asked this so much: "What would happen to the human body exposed to the vacuum and cold of space?"

Of course, this sort of thing is depicted in scifi movies a lot, and people are curious about it. And even though the movies always get it wrong — you don’t explode, or freeze instantly — it does make folks wonder about it. And while the reality isn’t maybe as gooey as in the movies, it’s still pretty nasty.

I wrote about this in my review of the movie "Mission to Mars", as well as answering a question many years ago from a reader. And even though it’s an icky thing to think about, it does give me a chance to talk about heat transfer, which is pretty, um, cool.

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January 31st, 2012 12:21 PM Tags: exposure to space, human body, Q&BA, vacuum
by Phil Plait in Cool stuff, Debunking, Q & BA, Science, TV/Movies | 73 Comments »

Does the planet Fomalhaut b exist?

Well, this is depressing: Fomalhaut b may not exist.

Fomalhaut is one of the brightest stars in the sky, and is only about 25 light years away — that’s close, on a cosmic scale. It’s young, not more than a few hundred million years old, and surrounded by a vast ring of dust, leftover from the formation of the star itself. The ring is about 20 billion km (12 billion miles) in radius, and has a sharp inner edge.

That last bit is important: the easiest way we know to make the inside edge that well-defined is if a planet is orbiting the star just inside the ring. Its gravity would draw in particles, sculpting what would otherwise be a fuzzy boundary into a clean-cut ring. Not only that, but the ring is off-center; again, that’s likely due to the gravitational influence of a planet.

In 2008, astronomers announced they had found that planet: it appeared in two different Hubble Space Telescope images (shown above; click to embiggen) separated by two years. During that time, it had moved a little bit, by just what you’d expect for a planet at that distance from the star. The news came out the same day as other planets were seen around a different star, and I, along with lots of other folks, made it a headline (see the gallery at the bottom of this post showing all the planets we’ve been able to detect directly in images). This was, after all the first direct detection of a planet orbiting a Sun-like star!

Except, maybe not so much. A new paper has come out (PDF) trying to see Fomalhaut b using the Spitzer Space Telescope. Spitzer is sensitive to infrared, where the planet is far brighter.

And what did they see? Nothing.

Dang.

This image is pretty damning for the existence of Fomalhaut b. It’s the Spitzer infrared observations of the star, with the star’s light carefully removed. On the left is the actual image, and on the right they artificially added a point of light calculated to be equal to what the planet would emit, in the same position the planet should be — that’s what Arrow 1 is pointing at. It should be one of the brightest things in the image (Arrow 2 points to an unrelated bright spot). And while it’s obvious on the right, nothing can be seen on the left, in the real image. In other words, the planet isn’t seen.

Dang again.

Looking over the paper, it’s clear the astronomers were very careful, and did a number of tests. There’s no known way to make a planet as bright as what was seen in the Hubble images yet invisible in the Spitzer images. If the planet were there, they should’ve seen it. Also, a recent study has shown that if the two images show the planet moving, it would be on an orbit that crosses the ring! That seems extremely unlikely, if not outright impossible. A planet that big and massive — more massive than Jupiter — would disrupt the ring in short order if it physically crossed it. That really does make it very, very likely this is not a planet*.

So what is it? It’s probably a clump of dust orbiting the star, reflecting light from the star enough to show up in the Hubble images but not warm enough to show up in the infrared observations.

That’s too bad. If this is true — and it probably is — then that takes away one of the very few planets directly seen in telescopic observations. However, there are still plenty more, and those have been confirmed (again, see the gallery below). And that number will tend to increase as time goes on, even if every now and again it drops by one or two.

Hmph. I once wrote that destroying a planet is hard. Sometimes, all you need to do is try to observe it a different way, and poof! It’s gone.

And now I have to update that gallery, and all my previous pages about it too. Dang science. Always learning more stuff and changing what we thought we knew.

Image credit: Paul Kalas, U C Berkeley; NASA/Spitzer/Markus Janson et al.


* I chatted with an astronomer friend of mine about this, and he agreed with the authors of this new study. "Overall," he wrote me, "it smells like fish.". I couldn’t help myself. I wrote him back: "Of course it does. Fomalhaut is the brightest star in Pisces!"


[Below is a gallery of exoplanets that have been directly imaged using telescopes on ground and in space. Click the thumbnail picture to get a bigger picture and more information, and scroll through the gallery using the left and right arrows.]

In 1994, finding planets orbiting other sun-like stars was still something of a dream. Then, just a year later, the first one was found, opening a floodgate of discoveries.<br /><br />We know of nearly 500 other planets orbiting other stars. However, the methods of finding these <em>exoplanets</em> are indirect. We measure their effect on their parent stars, but we didn't directly see the planets themselves... until 2005, when the first image of an actual world orbiting another star was announced. <br /><br />As of October 2010, only 7 such planets have been imaged, but we'll soon have more. This gallery shows the best of these images, including the first alien solar system to have its picture taken. <br /><br />The picture above is an artist's drawing of <a href="http://blogs.discovermagazine.com/badastronomy/2010/09/29/possible-earthlike-planet-found-in-the-goldilocks-zone-of-a-nearby-star/" target="_blank">the planet Gliese 581c</a>. Until recently, the only tool we had to see alien planets was our imagination. But that's changed... it'll be a <em>long</em> time before we get pictures as detailed as this, but in the meantime, we're still getting amazing images and learning a lot about these exotic worlds.<br /><br /><strong>Click the image to go to the next one in the gallery, or use the nifty index slider at the top of the post.</strong><br /><br /><em>Original Gliese 581 c blog post:</em> <em><a title="Permanent Link: Possible earthlike planet found in the Goldilocks zone of a nearby star!" href="http://blogs.discovermagazine.com/badastronomy/2010/09/29/possible-earthlike-planet-found-in-the-goldilocks-zone-of-a-nearby-star/" target="_blank">Possible earthlike planet found in the Goldilocks zone of a nearby star!</a></em><br /><em><br />Artwork credit: ESO</em>The planet LkCa 15b is probably only about 2 million years old, and is still forming from a disk of material surrounding its star. On the left is a far-infrared image of the disk, and on the right is a near-infrared picture showing the planet (blue) and material swirling around it (red). <br /><br />The planet is roughly six times the mass of Jupiter, and is glowing in the IR with the heat of its formation, still brewing at 500 - 1000 Kelvins. It orbits its star at distance of about 2.5 billion kilometers, inside the central gap in the larger disk, which is probably due to the planet having swept up material.<br /><br /><span style="color: #555555; font-family: 'normal Arial', Helvetica, sans-serif;"><span style="line-height: 18px;"><span style="color: #000000; font-family: Verdana, Arial, Helvetica, sans-serif; line-height: normal;"><em>Original blog post: <a href="http://blogs.discovermagazine.com/badastronomy/2011/10/20/the-first-direct-image-of-a-baby-planet-being-born-maybebut-probably/" target="_blank">The first direct image of a baby planet being born! (maybe!)(but probably!)</a><br /></em></span></span></span><em><br />Artwork credit: Kraus and Ireland </em>There's no other way to put it: this is the historic first picture of a planet orbiting another star. <br /><br />The star in question is a <a href="http://www.badastronomy.com/bitesize/bd.html" target="_blank">brown dwarf</a> (what some people unfairly call a failed star) called 2MASSWJ1207334-3932 - or 2M1207 for short - located about 230 light years from Earth. This false-colored infrared image shows the star as blue, and the planet red.<br /><br />The planet, called 2M1207 b, has about 5 times the mass of Jupiter, and orbits the star over 8 billion km (5 billion miles) out, about twice the distance of Neptune from the Sun. <br /><br />The planet was first seen in 2004, but astronomers had to wait a year to confirm it really was a planet and not a background star or galaxy. Over time, as the star moved slightly in our sky, <a href="http://blogs.discovermagazine.com/badastronomy/2005/04/29/first-exoplanet-imaged/" target="_blank">the planet moved with it</a>, confirming they were a pair. <br /><br />This picture is indeed historic, but left many people unsatisfied. Brown dwarfs are bigger than planets, but not really stars, either. And while 2M1207 b was definitely a planet, everybody was hoping to find a planet around a bona-fide star like the Sun. <br /><br />They didn't have to wait long...<br /><br /><em>Original blog post: <a href="http://blogs.discovermagazine.com/badastronomy/2005/04/29/first-exoplanet-imaged/" target="_blank">First exoplanet imaged!</a></em><br /><br /><em>Credit: ESO</em><br />When this picture of the nearby bright star Fomalhaut was released by Hubble, I had to laugh. We got a picture of Sauron's eye!<br /><br />The star is actually not seen in this image; it's so bright the light from it was masked and subtracted away so that fainter objects could be seen. Amazingly, this bright ring of material popped right out of the picture; it's a vast circle of dust 36 billion km (21 billion miles) across. <br /><br />Hidden in that picture is the exoplanet Fomalhaut b. It looked like just another pixel of noise in the first 2004 image, but was seen to move a little bit in an image taken in 2006. It took two more years to confirm it, but then the announcement was made in 2008: the second extrasolar planet had been directly seen!<br /><br />It orbits Fomalhaut at a distance of 18 billion km (10.7 billion miles), but its mass is unknown, though estimated from to be about three times that of Jupiter (if it were any more massive, it would noticeably distort the ring). Amazingly, the star is about <strong>one billion</strong> times brighter than the planet, giving you an idea of how freaking hard these observations are. <br /><em><br />Original blog post:<a title="Permanent Link: HUGE EXOPLANET NEWS ITEMS: PICTURES!!!" href="http://blogs.discovermagazine.com/badastronomy/2008/11/13/huge-exoplanet-news-items-pictures/" target="_blank"> HUGE EXOPLANET NEWS ITEMS: PICTURES!!!</a></em><br /><br /><em>Credit: <a href="http://www.nasa.gov/">NASA</a>, <a href="http://www.spacetelescope.org/">ESA</a>, P. Kalas, J. Graham, E. Chiang, E. Kite (University of California,  Berkeley), M. Clampin (<a href="http://www.nasa.gov/">NASA</a> Goddard Space Flight Center), M. Fitzgerald (Lawrence  Livermore National Laboratory), and K. Stapelfeldt and J. Krist (<a href="http://www.nasa.gov/">NASA</a> Jet Propulsion  Laboratory)</em>The previous image shows the discovery of the planet Fomalhaut b, about 25 light years from Earth. <a href="http://astro.berkeley.edu/~kalas/images/Fomb_3panel.jpg" target="_blank">This image</a> shows better how they confirmed it was a planet: over the course of two years, the planet moved a tiny bit as it orbited its parent star. It takes over 870 years to circle the star once!<br /><br /><br /><em>Credit: <a href="http://astro.berkeley.edu/~kalas/images/Fomb_3panel.jpg" target="_blank">Paul Kalas</a>, U C Berkeley</em><br /><br /><br />The same day astronomers announced the discovery of Fomalhaut b seen in the previous two pictures, they had another surprise: <em>the first picture of an actual exoplanet solar system!</em><br /><br />They found not one but <strong>three</strong> planets orbiting the star HR 8799, a slightly hotter and more massive star than the Sun, located about 130 light years away. The star is about 60 million years old. The brilliant light from the star has been masked out to show the much fainter planets.<br /><br />The planets, labeled b, c, and d, are about 7, 10, and 10 times the mass of Jupiter, respectively, and orbit their star at 68, 38, and 24 times the distance of the Earth from the Sun. <br /><br />HR 8799 b is clearly a planet, but the other two have masses uncertain enough that they might barely qualify as brown dwarfs. However, models of the system show that if the planets really <em>are</em> more massive, their mutual gravity would destabilize the system. It's likely then they are closer to the lighter end, making them planets as well.<br /><br />This picture qualifies as another first as well: the first one taken <em>from the ground</em> of planets around a sun-like star. The first exoplanet was seen orbiting a brown dwarf, and the Fomalhaut pictures were taken from space, using Hubble. What this picture meant is that it was possible to take high-contrast, high-resolution images using ground-based observatories, which are far easier to manage and are far easier and cheaper to build than space observatories. It promised to usher in a new age of planetary detection.<br /><br /><em>Original blog post:<a title="Permanent Link: HUGE EXOPLANET NEWS ITEMS: PICTURES!!!" href="http://blogs.discovermagazine.com/badastronomy/2008/11/13/huge-exoplanet-news-items-pictures/" target="_blank"> HUGE EXOPLANET NEWS ITEMS: PICTURES!!!</a></em><br /><br /><em>Credit: Gemini Observatory</em>The first exoplanetary family system gets a new addition! In 2010, astronomers announced that they had discovered a fourth planet orbiting the star HR 8799. Called HR 8799 e, it's closer in than the previously-known three planets, orbiting the star at a distance of about 2.2 billion km (1.3 billion miles) - roughly the same distant of Uranus from the Sun.<br /><br />The planet has a mass of about 7 times that of Jupiter, though that's an estimate; it depends on the age! The planet is still glowing with the leftover heat of its formation, and the brightness depends on both its mass and its age. Since the age isn't exactly known, the mass can only be estimated. <br /><br />Interestingly, the authors of <a href="http://arxiv.org/pdf/1011.4918" target="_blank">the discovery paper</a> note that current planet formation computer models can't make planets like this at the distance of HR 8799 e from its parent star. Either the models are wrong, or the planet formed farther out from the star and moved inwards; the latter is something that is fairly certain to happen when planets are young.<br /><br />Either way, this new discovery adds excitement to the new field of exoplanet hunting, as well as those who are scratching their heads trying to figure out how these planets form.<p>Four planets were found orbiting the star HR 8799 in 2008. However, observations of the star taken in <em>1998</em> were found to have three of those planets in them, hidden by the glare of the star! Improved techniques in software and analysis revealed the planets, buried in the star's glare.<br /><br /><a href="http://blogs.discovermagazine.com/badastronomy/2011/10/06/exoplanets-seen-by-hubble-in-1998-finally-revealed/"><br /></a><span style="color: #000000;"><em>Original blo</em></span><span style="color: #000000;"><span style="color: #000000;"><em>g post: <a href="http://blogs.discovermagazine.com/badastronomy/2011/10/06/exoplanets-seen-by-hubble-in-1998-finally-revealed/" target="_blank">Exoplanets seen by Hubble in 1998 finally revealed</a><br /><br /></em></span></span>Image credit: <span style="font-family: Georgia, serif; font-size: 13px; line-height: 18px;">NASA, ESA, and R. Soummer (STScI)</span></p>Detecting exoplanets is hard enough. Getting a spectrum from one is, quite literally, adding a new dimension of difficulty.<br /><br />A spectrum is simply the mapping out of the colors of light, spreading out the light from an object into its component colors. Right away, you can see why doing this with faint objects is hard. You're taking the light that would normally be concentrated into a small circle a few pixels across and then spreading it out over a line that might be hundreds or thousands of pixels long! That takes a faint object and makes it hundreds of times fainter.<br /><br />Worse, when you're taking an exoplanet's spectrum, it's also sitting very close to a star that might be millions of times brighter, which totally swamps the exoplanet signal. I spent quite a bit of time years ago doing this exact thing, and it nearly drove me nuts. Nearly.<br /><br />But some other astronomers were more successful than me: <a href="http://www.eso.org/public/news/eso1002/" target="_blank">they were able</a> to tease out the spectrum of HR 8799 c in the infrared, obtaining a direct spectrum of an exoplanet for the first time. In fact, their data were good enough <a href="http://arxiv.org/pdf/1001.2017" target="_blank">to show</a> that models of how exoplanetary atmospheres absorb and reflect their star's light must be modified!<br /><br />In this picture, the star HR 8799 is shown on the left, with the position of the planet circled. The picture on the right shows the blaring spectrum of the star, some reflections called "ghosts", and the extremely faint spectrum of the planet. It really shows you just how tough this observation was.<br /><br />
<p><em>Credit: ESO/M. Janson</em></p>
<br /><br /><br />In September 2008, <a href="http://www.gemini.edu/sunstarplanet" target="_blank">astronomers announced</a> the confirmation of yet another exoplanet, this one orbiting the star 1RXS J160929.1-210524, an orange dwarf about 500 light years from Earth. <br /><br />It was touted as the first direct image of an exoplanet orbiting a sun-like star, but that's not really the case. The system of planets around HR 8799 shown in the previous image was first observed in October 2007, and the confirmation came in July 2008. This planet, called 1RXS 1609 b, was seen in images taken in April 2008 but not announced until September.<br /><br />In the exoplanet hunting game, weeks count! And the order of observations may not match the confirmation and announcements. Now imagine if planets are eventually detected in images taken earlier than any of these. How confusing would that be?<br /><br />Either way, record or not, this is an interesting case. The large distance of the planet from its star - <strong>50 billion km</strong> (30 billion miles) - is far more than any other planet discovered. It's a struggle to understand how such a planet could have formed that far out. Perhaps it formed closer in and got tossed out by another massive planet orbiting nearby. Perhaps it formed more like a brown dwarf, collapsing from the material from which the star itself formed (planets usually form from disks of material closer in, slowly gaining mass through collisions). That seems unlikely though; that process should make objects more massive than this planet (which has about 8 times the mass of Jupiter).<br /><br />We're still new at this, and observations are scarse. As we get better, we'll learn more... and solve some of the pervasive mysteries about how planets form and how they age.<br /><br /><em>Original blog post:</em><em></em><a title="Permanent Link: Another direct picture of a planet orbiting an alien star confirmed!" href="http://blogs.discovermagazine.com/badastronomy/2010/06/30/another-direct-picture-of-a-planet-orbiting-an-alien-star-confirmed/" target="_blank"><em> Another direct picture of a planet orbiting an alien star confirmed!</em></a><em><br /><br />Credit: Gemini Observatory</em><br /><br />When astronomers released this image in November 2008, it wasn't clear if the labeled object was a planet or not. A year later, observations were taken that confirmed it... but that's for the next gallery picture.<br /><br />In this infrared image - taken in 2003, by the way, making it the oldest image known to have an exoplanet in it - the star Beta Pictoris has its light masked out, revealing the planet Beta Pic b, as well as a ring of dust seen edge on (a bit like Saturn's rings). The disk was first discovered in the 1980s, and as imaging got better, the disk was seen to have several features making it look like something closer in to the star was disrupting it.<br /><br />That "something" turned out to be the planet. Of all the directly imaged exoplanets, it's the closest to its star; it's about the same distance from Beta Pic as Saturn is from the Sun. The planet probably has a mass about 9 times that of Jupiter, and orbits the star once every 15 years or so. <br /><br />Two more interesting points: Beta Pic is only about 12 million years old. This means planets form extremely quickly after their star does! Also, back in November 1981 the light from the star mysteriously dipped for about a day. It's been suggested that the planet passed directly between us and the star, blocking a bit of its light! If that's the case, then  astronomers can use all kinds of techniques to nail down the size of the planet and its distance from the star. <br /><br />Beta Pic will probably be the most heavily observed of all the planet-bearing stars we know. We have an excellent chance here to learn a whole lot about exoplanets, and all we have to do is catch it at the right time!<br /><br /><em>Original blog post</em>: <em><a href="http://blogs.discovermagazine.com/badastronomy/2008/11/21/another-exoplanet-imaged/" target="_blank">Another exoplanet imaged!</a></em><br /><br /><em>Credit: ESO</em>The planet Beta Pictoris b was discovered in November 2008, but as mentioned in the last picture, it wasn't confirmed until the next year. Then, in 2010, <a href="http://www.eso.org/public/archives/images/screen/eso1024c.jpg" target="_blank">this extraordinary image</a> was released. Composed of two separate pictures taken in 2003 and 2009, it shows the planet first on one side of the star (left), then on the other (right)! For the first time, an exoplanet was seen to move to the other side of its parent star.<br /><br />That may not seem terribly important, but it is. For one thing, it helps nail down the orbital size and period of the planet. Also, in 2008 the planet wasn't seen at all; it was most likely behind or too close to the star to be seen. Again, that helps determine the orbit of the planet.<br /><br />As mentioned in the previous entry, it's possible that the planet will transit the star. If it does, then we'll know the orbit even better, allowing things like the mass of the star to be better determined, as well as other orbital characteristics of the planet.<br /><br /><em>Original blog post</em>: <em><a title="Permanent Link: Astronomers see exoplanet orbiting its parent star!" href="http://blogs.discovermagazine.com/badastronomy/2010/06/10/astronomers-see-exoplanet-orbiting-its-parent-star/" target="_blank">Astronomers see exoplanet orbiting its parent star!</a></em><br /><br /><em>Credit: <a href="http://www.eso.org/public/news/eso1024/" target="_blank">ESO</a></em><br />Here is another picture of Beta Pic b, this time taken using a new technique that better blocks the light from the parent star. When stars are observed with telescopes, the wave nature of light spreads the image out a little bit into a bright core and a more diffuse halo. This new sophisticated method takes some of the light from the core and uses it to cancel out the light from the halo, allowing fainter nearby objects - like, say, planets - to be seen.<br /><br />This technique, once set up correctly, is actually not terribly hard to adapt to other telescopes. This means that new planets may be found far more rapidly than before. Direct imaging, once the most difficult of planet-finding methods, may become the most prolific!<br /><br /><em>Original blog post</em>: <em><a title="Permanent Link to Get ready to see lots more exoplanet images soon" href="http://blogs.discovermagazine.com/badastronomy/2010/10/17/get-ready-to-see-lots-more-exoplanet-images-soon/" target="_blank">Get ready to see lots more exoplanet images soon</a></em><br /><br /><em>Credit: ESO</em>New observations of Beta Pic b taken in 2010 show it has moved even more in its path around its star. The top two images show its position in 2003 and 2009, and the bottom the new position in 2010. <br /><br />This new infrared observation, taken with the Very Large Telescope, also indicate the planet has a mass of 7 - 11 times that of Jupiter, and is in the temperature range of 1100 - 1700 degrees Celsius.<br /><br />Original blog post: <a href="http://blogs.discovermagazine.com/badastronomy/2011/03/03/more-images-of-exoplanet-show-it-orbiting-its-star/" target="_blank">More images of exoplanet show it orbiting its star</a><br /><br /><a title="Permanent Link to More images of exoplanet show it orbiting its star" href="../badastronomy/2011/03/03/more-images-of-exoplanet-show-it-orbiting-its-star/"></a> <em>Artwork credit: M. Bonnefoy et al., published in Astronomy &amp;amp; Astrophysics, 2011, vol. 528, L15</em>Where do we go from here?<em><br /><br /></em>Direct imaging of exoplanets is perhaps the newest field in all of astronomy. Ten years ago it didn't exist, and was something of a dream. Now we have images of seven tiny dots, seven blips of light indicating the presence of mighty planets. <em><br /><br /></em>And with the advent of spectroscopy, we'll learn even more: how hot they are, and what they have in their atmospheres. Eventually, with new technology, new telescopes on space, we'll be able to split their light ever finer, and who knows? Maybe, one day not too long from now, we'll see the tell-tale sign of molecular oxygen... the only way we know of to have molecular oxygen in an atmosphere over long periods of time is through biological activity. If we ever see it... that, my friends, will be quite a day indeed. <br /><br />I think that is ultimately our goal. We're looking for planets now, but what we're really looking for is life, or at least planets capable of supporting it. That day may be a long way off, but in my opinion it's a day that will, eventually, come.<br /><em><br /><br />Artwork of HR 8799 b credit: NASA, ESA, and G. Bacon (STScI). Larger versions available on <a href="http://www.nasa.gov/multimedia/imagegallery/image_feature_1320.html" target="_blank">the NASA Images website</a>.</em>

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January 31st, 2012 7:00 AM Tags: exoplanet, Fomalhaut b, Hubble Space Telescope, Spitzer Space Telescope
by Phil Plait in Astronomy, Science | 50 Comments »

Q&BA: Getting kids into science

A few years ago, I started doing a weekly video question-and-answer session I called "Q & BA". It was a series of short videos that were a lot of fun to make. Unfortunately, the overhead got to be too high — it took all day to edit them! — and I had to stop.

But now, Google+ has changed that: Hangouts On Air is a feature that allows me to go on camera and broadcast a live video chat session to an unlimited audience. I take questions via Twitter and G+, and it’s a lot of fun. It lasts about an hour, and I put the whole session on YouTube. But some of the answers stand alone, and it’s easy to extract them out, package ‘em up, and post ‘em by themselves.

So I’m very pleased to announce I’m starting the series again! The first Q&BA is a great question: "What’s the best way to get kids into science and skepticism?" — what better way to get the series going again? Enjoy.

I’ll be posting more of these, maybe even one per day as time allows. If you like them, please give them a thumbs-up on YouTube, and drop by the Q&BA Hangout when I do them live! I announce them on Twitter and G+, so follow me there and stay up-to-date. Also, I have an archive with links to all the videos. Thanks!

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January 30th, 2012 2:24 PM Tags: Q&BA
by Phil Plait in Piece of mind, Q & BA, Science, Skepticism | 15 Comments »

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