Bad Astronomy
The entire universe in blog form

Oct. 7 2015 9:30 AM

A Lesson in Crewed Language

In many ways, NASA is slow to change. That’s not surprising; it’s a government agency, for one thing, and for another being a tad conservative isn’t such a bad feature when you’re trying to put people into space safely.

But even NASA is ahead of a lot of the curve when it comes to language used when talking about spaceflight. The terms “manned” and “unmanned” have fallen out of favor with the space agency: The NASA History Program Office Style Guide now specifically states that “All references referring to the space program should be non-gender specific.” The only exceptions are for names of buildings and programs; these are—pardon the expression—grandfathered in.*


I think this is great! Words matter. Using more inclusive words is a tacit invitation to people of all flavors, and diversity = strength.

My friend Emily Lakdawalla wrote about this on her blog for the Planetary Society (the comments there are interesting, too, so be sure to check them out as well). The topic came up again when a few science communicators were trying to come up with a good substitute for “manned” and “unmanned.” A lot of us use “crewed,” but as Emily points out (and as I have said many times) it sounds like “crude” when spoken aloud, which can cause momentary confusion for an audience. I’m still not sure what might be best there. “Crewless” works well for “unmanned,” though.

I did a quick search and found that I used the word “crewed” in a post way back in 2007, though it’s unclear if I did that to be more inclusive or just to switch my word usage up a bit. I stopped using the word “manned” a few years ago, though (except when quoting someone, or referring to something like the Manned Maneuvering Unit). I did that when I got into a conversation on this very topic on Twitter with some science communicator friends a while back. I’m a balding, bearded, middle-aged white guy, the very picture of stereotypical science dork. If I figured this out, others can too.

I know a few folks will froth and fume over this change; some people get very hot and bothered when others want to be more inclusive. But things like this cost us very little, and the payoff is large. Even if the cost were higher it wouldn’t matter, because it’s the right thing to do.

Everyone deserves to feel welcome when it comes to math, science, and tech … really everywhere. There’s no way to know from someone’s sex, skin color, or superficial characteristics what they might contribute. We all have brains. What we all need is a chance—and the environment—to participate.

*Space advocate Ariel Waldman points out that this has been in the style guide since 2006!

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Oct. 6 2015 12:00 PM

Stephen Ramsden’s Traveling Sun Show

I was puttering around online and happened across something that made me quite happy: CNN put out a short video about my pal Stephen Ramsden. He’s a former air traffic controller who travels around with a very, very impressive array of solar telescopes, teaching kids about the Sun.


I met Steve many years ago and was taken right away with his dedication and enthusiasm for teaching. He’s a natural. That video came out last year, but he’s still out there, going from school to school and showing children sunspots, solar flares, prominences, and more. He’s an inspiration.

Stephen Ramsden
Ramsden setting up for a public Sun viewing in Georgia, his home base state.

Photo by Stephen Ramsden

And not to put too fine a point on it, he takes donations, too (there’s a “donate” button on his Web page). He’s doing a fundraiser right now, and if you donate $100 or more, you’ll get entered to win a Lunt LS80 B1200 solar telescope, and I’ll be honest: I have serious lust for this ‘scope. Happily, I have my own smaller version, so I’m OK. But geez, that’s a sweet machine. And not only that, Ramsden is also raffling off a pair of 8 x 32 Lunt SUNoculars every Friday until Oct. 30 to a donor of any amount.

If you prefer to buy stuff, one of his sponsors, Rainbow Symophony, sells safe solar observing glasses; I have several pair myself and I use them all the time. Stephen doesn't make money from those sales (in fact he gives away glasses for free to anyone who asks if they use them for outreach), but it helps his sponsor so that's agood thing. Come to think of it, I bet such things will be in short supply soon as the Great 2017 Solar Eclipse approaches. You might want to pick up some now. He has other swag, too (again, he doesn't make money for those sales; he does that at cost so others doing outreach can have the same shirts he wears). But donations are best!

He’s doing good work, and I hope he continues to do so for a long, long time.

Correction, Oct. 6, 2015: I originally wrote that the sales of glasses and swag support Stephen, but he sent me a note reflecting the text above.

Oct. 6 2015 9:00 AM

The 20th Anniversary of Exploring Strange, New Worlds

Twenty years ago, on this very date, the field of astronomy underwent a magnificent revolution.

On Oct. 6, 1995, Swiss astronomers Didier Queloz and Michel Mayor announced they had discovered a Jupiter-like planet orbiting a Sun-like star.


This was the very first time a planet was seen orbiting a “normal” star. Planets had previously been discovered around pulsars—the compact and furiously energetic cores of stars that had exploded. But it’s thought that the planets may have formed after the supernova event that created the pulsar, and besides, pulsars are nothing at all like the Sun.

Still, this new planet, called 51 Pegasi b, was a surprise. A big one! While it had about the same mass as Jupiter, it orbited its host star (51 Peg) in just four days, meaning it was on an orbit a mere 8million kilometers from the star. Compare that with Mercury, our solar system’s innermost planet, which never gets closer than about 46 million km from the Sun.

This meant 51 Peg b was hot, cooking away at a temperature of about 1,300° C. No one thought a planet that size could be that close to a star. Did I say the discovery was a surprise? I meant it was a shock, one so profound that it was met with deep skepticism.

As well it should! But its existence was quickly confirmed by team of American astronomers, rivals in the hunt for the first extrasolar planets, as they were once called (we now call them exoplanets).

The planet was found using what’s called the “radial velocity” or reflexive “motion method.” A planet orbits a star due to the star’s gravity. But the planet has gravity, too, so as the planet makes a big circle around the star, the star makes a little circle. In reality both orbit the center of mass of the system, called the barycenter. I describe how this works in my episode of Crash Course Astronomy about the discovery of exoplanets:

As far as we knew at the time, planets like Jupiter had to form far out from their stars, half a billion kilometers or more. Because of this, astronomers who were hunting for exoplanets assumed they would take months or years to make an orbit. They completely missed the presence of 51 Peg b in their data.

Once it became clear these “hot Jupiters” existed, more were found in existing data. Within a few years many more were discovered. It’s now thought they do form far out, but then migrate closer to their star over millions of years. Although they make up only a minority of all exoplanets, these are the easiest to find using reflexive motion; their high mass and close orbit make their signal in the data easiest to see.

Once 51 Peg b was found, the floodgate was opened. HD 209458 b was another hot Jupiter found in 1999, and had an orbit so close to being edge-on that astronomers thought it might actually pass in front of its star, transiting it, dimming its light once per orbit. Careful observations later that same year detected a dip in the star’s brightness (only 1.7 percent!), which gave them the first independent observation of an exoplanet. Any lingering doubts about the existence of these alien worlds evaporated.

The field matured so quickly that NASA launched the Kepler spacecraft in 2009, designed specifically to stare at 150,000 stars to look for transiting exoplanets around Sun-like stars. As of today, Kepler has more than 1,000 confirmed exoplanets under its belt, and well over 3,000 more waiting confirmation.

We’ve seen planets big and small, hot and cold, orbiting small cool stars, huge hot stars, multiple stars, and even in systems with multiple planets.

When I was a kid—heck, when I was in grad school—the only planets we knew of were the ones in our solar system. Using simple statistics, we now think that planets outnumber stars in the galaxy and that most stars may have planets. There may be tens of billions of Earth-size planets in our galaxy alone!

But we had to start somewhere. Exactly two decades ago, 51 Peg b gave us that start.

51 Peg star chart
The star 51 Peg is just off the Great Square of Pegasus, which is in the east after sunset for northern hemisphere observers. EarthSky has a finding chart for Pegasus, then you can use this image to find the star.

Map by Sky Safari

The host star, 51 Peg, is close by, just 50 or so light-years from us. It’s actually very much like our Sun, just a hair more massive, hotter, and bigger. It’s visible to the naked eye, barely, from a dark site. The constellation of Pegasus is high in the night sky for Northern Hemisphere observers right now, in fact. If it’s clear where you are, and you have a pair of binoculars, why not take a look at it tonight?

I will. The exoplanet is completely invisible to even the largest of telescopes, drowned by the light of its oh-so-close star. But who knows: Maybe a photon or two from the planet itself will pass into your eye as you look at the star, absorbed into your retina.

The sky may be brimming with planets. We stand on one among billions. And if you look, a small spark, literally the tiniest reflection of one, could become a part of you.

Oct. 5 2015 11:00 AM

How to Make a Rubber Ducky Comet: Smash Two Comets Together! Carefully.

Why is the comet 67P Churyumov-Gerasimenko shaped like a rubber ducky?*

It was a bit of a surprise when the Rosetta probe, after a decade of travel around the Sun, approached the comet and sent the first decently resolved pictures of it back to Earth. We knew going in that most asteroids and comets just a few kilometers across are oddly shaped; they lack the gravity needed to make themselves spheres, and after 4 billion years of impacts their shape can be decidedly odd.


We even know of a few bowling pin shaped comets, like Hartley 2 and Wild 2. But 67P just reinforced the weirdness of this all with its two lobes mismatched in size and shape.

So, why? What’s going on? Comets are rock, gravel, and dust all mixed together with various ices holding them together, frozen stuff like water, carbon dioxide, and carbon monoxide. Did these weird, dumbbell-shaped comets start off more round and, for some reason, lost more ice in their midsections, leaving behind the two big lobes? Or were they the result of two interplanetary snowballs that collided and stuck together?

New results from the Rosetta team have finally answered this question. 67P used to be two different comets, but they merged to become the bizarre bit of solar system fluff we now know and love.

How? Well, when two comets love each other very much …

Oh wait, no, that’s not it. Well, actually, kinda. Back in May 2015 astronomers came up with a pretty good scenario on how to form a rubber ducky comet. Two smaller comets collide in a slow-speed, grazing impact. Some material is lost, and the two major pieces separate a bit, but the impact was slow enough that they become gravitationally bound. They fall back together, stick, and voilà!

As for the “how do we know?,” that’s more subtle, and quite clever. Rosetta has been orbiting 67P since August of 2014. Over that time it’s taken a vast number of high-resolution images, revealing details of the surface. Both lobes have flat regions all over them arranged like terraces, and the steps in between the terraces show layering; these probably built up layer by layer over time when the comet(s) first formed billions of years ago.

terraces and layers
A close-up of 67P shows flat terraces (colored green here) and layers (red).

Photo by ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA; M. Massironi et al. (2015)

If the comet formed as a single object that has since eroded, you’d expect the terraces and layers on both lobes to align so that their flat sides were perpendicular to the center of the comet, somewhere in the neck, plated around it (something like the individual panels on a soccer ball, which all are perpendicular to the ball’s center, or, of you prefer, more-or-less parallel to the ball’s surface).

If, instead, the two lobes formed individually and later merged, then the terraces on each lobe would be perpendicular to the center of their respective lobe.

Using 3-D modeling, the scientists mapped the orientation of the terraces. And what they found is the latter: The terraces align to each lobe individually, not to the center of the comet as a whole. This strongly indicates the lobes formed separately, later merging.

comet map
A 3-D model of the terraces in the comet indicate their orientations, showing the two lobes of 67P formed separately, then later merged.

Photo by ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA; M. Massironi et al. (2015)

That is very, very cool. I’ve been curious about this ever since we literally got the first good pictures of the comet. I allowed myself a bit of speculation back then and felt that a low-speed collision between two small comets was unlikely. I guess I was wrong! While space is big, I neglected to consider that time is also long, and over an eon or four collisions may be likely. After all, 67P isn’t the only object like this; we know of quite a few binary and dogbone-shaped asteroids, too.

How about that? The beauty of this, too, is that the answer gives us insight into more than just why the comet is funny-looking. It also tells us about how comets behave, what their formation processes are like, what happens after they form, and, perhaps most interestingly, how often objects in space collide. That in turn helps us understand the history of our solar system in general, as well as how often the Earth itself gets hit by such cosmic debris.

Over time, we do get hit. The rate of such impacts is a good thing to know, so that we can better understand how to prevent them.

After all, we don’t just want to be a … sitting duck.

*Hint: It’s not because it makes bath time so much fun.

Oct. 5 2015 9:00 AM

Ben Carson vs. Ben Carson

Scientist Ben Carson, talking about his own fetal tissue research: "To willfully ignore evidence that you have for some ideological reason is wrong."

Creationist Ben Carson, talking about scientists who understand the Big Bang, evolution, and global warming are real: "I just don't have that much faith," he said. "But they are welcome to believe whatever they want to believe. I'm welcome to believe what I want to believe."


Do politicians ever actually listen to what they say?

Oct. 4 2015 9:30 AM

Marketing Space

I have to admit, I laughed, especially at the “Pluto” part.

Still, I do sometimes worry about the future of NASA marketing. Promoting movies like The Martian is great, but I wonder if this will backfire in the long run. I agree with my friend Joel Achenbach; Congressional squabbling over NASA’s budget and the lack of a clear vision or plan to get to Mars only serves to contrast what NASA promotes versus what it can actually do.


This is not NASA’s fault, mind you. I lay the blame squarely on Congress. They have a clear path ahead of them—fully funding Commercial Crew—but instead keep throwing money at the Space Launch System (which, if built, will cost so much NASA won’t be able to do anything with it) and the Orion capsule, which now may not be able to take humans in it until 2023, a full eight years after Commercial Crew would’ve been able to send humans into space, had Congress funded it.

What a mess. The majority of Americans love NASA, and it’s incredible that NASA can do such amazing feats like send probes to Pluto and Saturn and protoplanets like Vesta and Ceres at all, let alone given the Keystone Kops feel of the Congress members pulling the purse strings. My only hope now is that these folks in Congress get replaced in the 2016 elections.

It’s hard to look to the stars when the people funding you have their heads jammed into pork barrels.

Tip o’ the spacesuit visor to ruimteaart via astronaut André Kuipers.

Oct. 3 2015 9:30 AM

Crash Course Astronomy: Multiple Star Systems

The stars are not as they seem.

The nearest one is tens of trillions of kilometers away, a distance so terrible that the might and power of Alpha Centauri is reduced to a faint spark that can be washed away by the lights of a nearby city.


Distance shrinks details, too. Alpha Centauri is not one star, but two: one very much like the Sun, though slightly larger, orbiting and orbited by another that is somewhat fainter, cooler, and more orange. There’s also a third star, Proxima Centauri, which orbits the pair but is so faint it can’t be seen by the naked eye even though it is in fact the closest known single star to the solar system.

A large fraction of all the stars in the sky are actually multiple stars—binary, trinaries, or even more complex systems. That alone is enough to want to know more about such multiples; but once you look closer you find that such systems become critically important to our understanding of everything in the Universe.

And, contrary to my usual nature, that’s not an overstatement. Find out why in this week’s episode of Crash Course Astronomy: Binary and Multiple Stars.

I’m excited that this phase of Crash Course is airing: We’re traveling farther out into the Universe, even though we haven’t even left our cosmic backyard yet. But there are larger structures to explore, and grander things yet to see. Just you wait.

Oct. 2 2015 9:15 AM

Behold, the Mess That Is Charon

Charon is so, so weird.

It’s also astonishingly beautiful. Look at it! The image above is a newly released high-resolution color photo of Pluto’s largest moon, taken by the New Horizons spacecraft when it zipped past the Pluto system in July 2015. It’s been enhanced to bring out the color variations more, but this also gives us an idea about the surface features, and how they vary across this strange little world.


There’s so much to see! The most obvious bit is the red splotch at the north pole, informally named Mordor Macula (macula means spot and is commonly used in planetary nomenclature to refer to a big dark region; Mordor is a place you simply don’t walk into).* Pluto is covered in red spots, and it’s thought these are tholins, carbon-based molecules created when ultraviolet sunlight breaks apart molecules, which then reorganize themselves into more complex structures.

Very little of the rest of Charon is red, prompting some scientists to conjecture that Mordor Macula is from some sort of transfer of material from Pluto onto Charon’s surface, possibly from Pluto’s extremely tenuous (but observable) atmosphere. Craters in Mordor are bright, indicating the red material is a veneer; thin enough that small impacts excavate brighter material (likely ices) underneath.

The next most obvious feature is that huge canyon separating the north and south hemispheres. The canyon is staggeringly huge, at least 1,600 kilometers long, making it four times longer than the Grand Canyon and in places far deeper. To scale with Charon, it’s similar to Valles Marineris, the vast canyon scarring the face of Mars.

By the way, the stretch of the canyon just to the right of center, to the right of that centered crater? That’s called Serenity Chasma, and it’s named that way for exactly the reason you think. Shiny.

There’s a big dichotomy between the hemispheres, too. The southern half of Charon has a smoother look—this area is dubbed Vulcan Planum, the Plains of Vulcan—dotted with craters and what looks like cracks or graben (downward thrusted rocks, usually due to faulting as the crust expands). The northern half looks more rugged, less smooth. Perhaps some ancient event caused cryovolcanism—ice volcanoes!—in the southern hemisphere, flooding the plains with ice.

We only have good images of this side of Charon, unfortunately, because the New Horizons mission was a very fast flyby. I’d love to know what the other side looks like in this sort of detail!

A high-res mosaic of part of Charon was also released. It’s well worth your time to peruse the whole thing, but there’s one spot I want to point out:

crater chain
A crater chain dots the surface of Charon.


See that linear feature just above center? That’s a crater chain, usually caused when debris from a big impact is ejected, and then falls back to the ground. But this one is a bit weird; the craters are very close together, almost overlapping, and they don’t seem to point to any other obvious big crater. I’m wondering if this is due to a small body breaking up before it hit, forming a long chain of objects that then hit one after the other along a line. This happened when the comet Shoemaker-Levy 9 hit Jupiter in 1994; Jupiter’s immense gravity ripped the comet into pieces, which hit one after another over several days. Neither Pluto nor Charon has strong gravity, so I’ll admit this seems unlikely. It’s an intriguing formation either way.

As I mentioned, the picture of Charon is enhanced in color to show surface variations. Here’s one more picture, showing what it actually looks like in comparison with Pluto, with both bodies scaled the same way.

Pluto and Charon
The darkness and the light.


Charon is a lot darker than Pluto! That in itself is interesting. Charon most likely formed when an impact on Pluto blew some or most of its crust into space, which went into orbit and coalesced to form Charon (and perhaps the smaller moons, too). It seems to me that they may have started off looking similar, but subsequent events changed them, either brightening Pluto or darkening Charon, or both. Both show evidence of cryovolcanism or more recent resurfacing (the left side of Pluto’s “heart” is likely to be nitrogen ice that’s glacially flowed into lower elevations).

As more images and data trickle back from New Horizons, traveling the long, long emptiness stretching for five billion kilometers, we’ll learn more about the surfaces of these worlds. But every new picture shows something weird and wonderful, and while we get traction on some mysteries, others deepen.

Oh, how I love that! Science is fun.

*Features on Charon are informally named at the moment, but the agreed-upon nomenclature is that they are named after fictional destinations, ships, or voyagers.

Oct. 1 2015 9:30 AM

GOP Presidential Candidates, Science, and Reality

It’s time to not only face facts, but to call them out, too: This cohort of Republican presidential candidates isn’t exactly a brain trust.

Every time I see an article about something one of the GOP contenders has said, I’m stunned at just how much lower they can sink. It’s as if they’re scrambling on purpose to brag about the dumbest possible thing they can come up with.


Think I’m exaggerating? Here are some choice examples of ideas that have come out of the mouth holes of the remaining viable candidates:

None of this stuff is exactly rocket science … but when it comes to climate science, not a single one of these people is even close to planet Earth. They’re in their own alternate reality where up is down and, I suppose literally, hot is cold.

Let’s do a quick rundown of where they all stand:

I’ve been railing against the GOP’s party plank on climate change for years now, so none of this is surprising. But it’s upsetting. I disagree with almost all of the stances of the Republican Party these days, but in the past they at least used to embrace science. Now, though, if one of their candidates says the Sun will rise in the East, I’d lay better odds on the Earth’s rotation having reversed.

This stunning intellectual deficit, whether real or pandering, is wholly the fault of the party itself (and, to an extent, the American public for letting it slide this far). The abject dismissal of reality has become more and more mainstream in the party politicians, and its power soared upward like a hockey stick graph when the Tea Party gained congressional seats in the in 2010 election.

The fallout from this is as fascinating as it is maddening. For example, the Heartland Institute—or as I think of it, the Mos Eisley of think tanks—attacked the pope on his climate change stance, and even a Catholic congress person boycotted the pope’s speech. The internal paradoxes in the minds of these folks must be incredibly turbulent.

More examples can be easily found from other conservative groups. But there’s a glimmer of hope, a glimpse of the path back to reality for the GOP. As the pope showed, religious belief doesn’t necessarily lead to rejecting science; one need only look to outspoken climatologist and Christian evangelist Katharine Hayhoe for that as well. This reveals an underlying aspect of all this that seems to be forgotten: Belief in conservative principles doesn’t lead inevitably to the denial of science.

Conservative political parties in other countries don’t necessarily deny global warming either. It’s only endemic to the GOP. And while funding from the über-far-right Koch brothers clearly affects the way politicians vote in the U.S., not all wealthy donors are the same; Republican businessman Jay Faison has put the incredible sum of $175 million on the table to invest in climate-change–accepting Republican politicians.

The response to that was as predictable as rising temperatures: James “Snow disproves global warming” Inhofe, R-Oklahoma, denounced it. Of course he did; Inhofe is so far removed from reality he actually thinks the pope wasn’t discussing climate change in front of Congress.

I can make a laundry list of problematic GOP planks, but global warming is perhaps the single biggest threat facing humanity today. Faison’s move is a step forward, even if it makes some deniers froth and fume. Their staunch denial may yet lead to political extinction: A majority of Republican voters acknowledge the reality of global warming, and humanity’s role in it. That’s hopeful indeed.

And to those who still deny it, I’ll note that it’s better to take the carrot than the stick: Some people are proposing siccing the RICO Act on corporations actively suppressing global warming and climate change information. This isn’t fringe stuff; an investigation into Exxon revealed they allegedly knew about the threat of global warming for 40 years, yet still funded misinformation campaigns about it. Fossil fuel interests use the same tactics employed by the tobacco industry to downplay harm, and it was the RICO Act that brought those same tobacco companies low.

I’d rather not see things go this far, of course, but that’s the world we now live in: a planet that needs saving from those who would actively burn it down. And that, in sum, accurately describes the current crop of GOP presidential candidates.

Perhaps most sad is that it needn’t be this way. Republicans are supposed to be conservatives. Isn’t it about time they started conserving?

Sept. 30 2015 9:30 AM

Bloom With a View. Two of Them, in Fact.

Oh, I do so love a coincidence. And when it’s about imaging Earth from space, that’s even better.

I subscribe to NASA’s Earth Observatory Image of the Day (and you should, too!), which, oddly enough, posts an image of Earth every day. They’re almost always satellite shots, featuring various amazing portraits of our planet. As a satellite photo nerd I love it, and I learn a lot about Earth every time I see a new one. The cloud images alone are worth it.


One of the most spectacular and lovely kinds of photos they post are of phytoplankton blooms—huge bursts of growth (usually of cyanobacteria) in the ocean. Warmer waters can create conditions where nutrients and sunlight become abundant to the little plants, and they go forth and multiply. Blooms can be huge, hundreds of kilometers across.

The image above shows (a small part of) a bloom in the Baltic Sea, just north of Poland. It was taken by Landsat 8 on Aug. 11, and it’s not “true color,” that is, what your eye would see. The detectors used are sensitive to colors across a range of the spectrum, so the colors displayed are close to red, green, and blue, but there’s quite a bit of overlap (for example, the detector that sees in the green is also sensitive to yellow, and the blue one sees green as well). Still, the bloom is eerily beautiful. You can see airplane contrails and the wakes of ships in the original full-res image, too.

The spiral pattern is lovely, caused by eddies in the sea currents. Cyanobacteria are plants (more or less) so they flow along with the water.

The coincidence? The European Space Agency released a similar picture taken just a few days before, on Aug. 7, using the Sentinel-2 Earth-observing satellite:

Sentinel bloom
If you told me this was a radio map of a spiral galaxy, I might believe you.

Photo by Copernicus Sentinel data (2015)/ESA

Whoa. I’m not positive that’s the same swirl, but it’s from the same general area of the Baltic Sea (the Sentinel image is also part of a much larger image). Interestingly, both images from Landsat and Sentinel-2 show ships crossing their respective swirl; in each you can see the ship as a dot followed by a black trail.

Cyanobacterial blooms are important to study. They can rob water of oxygen and nutrients, and some phytoplanktons produce toxins that can be dangerous. And here we have two space agencies studying the same bloom at two different times with two different satellites! It’s really gratifying to see nations taking this sort of work seriously … especially when one faction of my own nation doesn’t.

We need to understand our planet as best we can. Not just because doing so produces such wonderful natural art, but because we are part of Nature ourselves, and we influence it just as it influences us. Understanding it is critical.

After all, Nature can live without us, but we can’t live without Nature.