Wrapping our head around proportions August 24, 2009
Posted by Jorge Candeias in Planets.Tags: Ceres, Earth, Eris, Haumea, IAU, Jupiter, Makemake, Mars, Mercury, Neptune, Pluto, Saturn, size comparisons, Uranus, Venus
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After writing the previous post, I was left with this uneasy feeling of not having been entirely fair towards not only placemats, but Solar System skematics in general. The truth is, it’s impossible to draw the Solar System to scale. The distances between the various bodies are so mind-boggingly vast, that something just has to be distorted, usually planet sizes. The only way to actually have everything to scale and to convey a real sense of sizes and distances is to scatter planet models over vast areas, and travel around the Solar System model thus created. Never in a skematic to be found online, in publications or in placemats.
We can also, of course, use numbers that are closer to our day-to-day experience. Inches, feet and miles for the americans; centimeters, meters and kilometers for the rest of the world. Shrink everything to fit into something a bit more palpable than thousands of kilometers and astronomical units. We all know what a meter is, more or less; we can stand up, put a hand somewhere along our torso and say “it’s about this high”, and we shouldn’t be wrong by much. So, if we divide all the true Solar System numbers by the same constant, we can provide a much more palpable notion of the real proportions out there. For instance…
Say the Sun’s diameter is not more than a million km (1 392 000 km, to be exact), but 100 meters. That’s still a pretty big ball: higher than the first level of the Eiffel Tower, in Paris, and wider than the tower, too. Still, if the Sun is that big, the first of the planets is another ball… with a diameter of 35 centimeters. That’s not even twice the size of a football ball (americans: I’m referring to soccer here). And to find that 35-centimeter ball called Mercury, you’d have to walk more than 8 kilometers!
Next is Venus. To find it, you’d have to travel another 7 km, and when you finally do, you’d see a largeish 87 cm wide ball. You are now 15.5 km from your starting point already and your trek is just beginning. Next, the Earth, another largeish 92 cm-wide ball, is found 6 km further along the road, 21.5 km from your starting point. See a pattern here? Centimeter-wide balls separated by kilometers? Yeah, that’s how things will be till the end. Only more so.
Next: Mars. Mars is, of course, smaller, only 49 centimeters in diameter, and to reach it from the Earth you have to travel 11 km more, away from your 100 m Sun ball. You are now 32 km from it, and unless you have been climbing a mountain of some sort, you probably won’t be able to see it anymore. And you’re still in the inner Solar System.
The next planet, Ceres, is also the smallest. At only 7 centimeters in diameter, you can pick it up with ease, but you’ll probably have a real hard time finding it, after travelling almost 27 km from your last stop. The Sun, almost 60 km away, is nowhere to be spotted already.
Now you have a long travel to make: 52 km. That’s about half an hour if you have a car and a highway handy, but a neverending hike if you try to go on foot. At the end, you’ll find the second largest ball of all, a 10 meter wide cliff of a thing, which dwarfs you for the first time since you left the sun behind. That was, remember, almost 112 km ago.
Hop on the car, go back to the highway: you’ll be driving for almost an hour to cover the 93 km that separates you from your next destination: a more than 8 meter wide ball called Saturn. 8 meters would seem a lot, if you weren’t 205 km from your starting point already. That far from the Sun, it strikes you as a positively lonely chunk of planetary real estate. But hey, it’s a beautiful one, with all those rings and stuff, and with many other centimeter-wide balls hundreds of meters distant, in all directions. So it’s fine, kinda. But you have to keep going, so you return to the car, stop at the next gas station and fill your tank, because your next travel is long.
208 km long to be exact. There are capitals in Europe separated by less than that. And yet, it’s simply the distance between Saturn and Uranus in our model. The Sun is 413 km away. And when this long voyage finally ends, what you find is a blue ball with a diameter of three meters and 64 centimeters. You’re tired. But you’re stubborn and you want to reach the end of this, so you go find Neptune. To do it, you’ll have to travel 233 km more, and when you finally reach your destination, you find another blue, 3-meter wide ball. For a moment you may think you went in a circle and returned to Uranus, but when you measure the ball you discover that it’s 10 cm smaller than the previous, so you’re really where you should be. Phew! But where is that? That’s 646 km away from your starting point. In Europe, you’d probably be in another country already. In the Americas, in another state or province.
Now, you know that whoever made the model you’re travelling through didn’t bother with orbits and actual positions in space, only with the average distance to the Sun. Had he taken orbits into the model, you’d be now in big trouble, because the next planet, Pluto, actually gets closer to Uranus than to Neptune due to its orbital resonance with the latter planet. You’d have to make a really long travel to find it. But since the model creator didn’t bother with that, you can go on in a somewhat straight line, and after travelling another 202 km, you’ll find a 17-cm wide ball waiting for you with a slightly smaller one right next to it. You try to get your bearings from the Sun, but it’s no use. It’s now almost 850 km away.
Next stop: Haumea. To reach it, you have to travel another 78 kilometers, and once you do you find a weird ellipsoid some 8-10 cm in diameter. You’ve travelled for so long and so far, that your vision has become blurry, and you begin to have a real hard time seing the planets you’re trying to find. But you push on, travel for another 57 kilometers, and find another ball around 11 centimeters in diameter: Makemake. You think this has to stop somewhere, but you know you’re still to find Eris, so you get back to the car, and start driving.
This time it’s the largest travel of all: 470 km, no less, and when you finally stop, after almost falling asleep during the long hours of driving, you’re a whooping 1455 km from your startng point. You pick up the Eris ball. 19 centimeters in diameter. A foot ball is 22. And it’s cold, oh, so, so cold. You know there’s more. Orcus, Ixion, Varuna, Sedna, Quaoar. But you’re so tired you thank the IAU for its slowness in making officially new dwarf planets. Only one more stop and that’s a wrap. You’ve heard so much about the Oort cloud that you’d like to pay a visit. But when you ckeck your map, you have a surprise: it ain’t there. In fact, you find out you’d have to leave the Earth and almost Earth’s orbit to reach it, for its outer edge is supposedly more than a million km away, almost three times the distance to the Moon. You swear profusely, and all we can hear is a succession of beeps, but you finally give up and go find a hotel. You’ll have a very long way to go back tomorrow. A very long way indeed.
And remember: the Earth is not even one meter wide at this scale.
That’s how huge the Solar System is.
On placemats and other mostly cultural stuff August 24, 2009
Posted by Jorge Candeias in Definition of planet.Tags: Definition of planet, education, Mike Brown, size comparisons
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Today, Mike Brown (I keep talking about this guy, for some reason) decided to post about placemats. I agree, they’re evil, and promote a very erroneous picture of the planetary fauna that exists out there and of the distances between the large and small chunks of rock, ice, gas and a few liquids that circle the sun. They are far from being unique in that, though. More often than not, even scientific illustrations fall prey to the same kind of reality-bending depictions most solar system skematics show. That’s actually part of the reason why I posted those two size comparisons below, and why I may follow with some more. Thanks to all those non-accurate renditions of planets’ sizes and distances, people are very often left with distorted notions about space. They think they know stuff, but they really don’t.
So he’s right. Mostly. Where he really gets it wrong is in thinking his version of placemat could really make a difference in the public perception of the solar system. People want simplicity: that’s why so many of the people complaining about the notion that evertything in hydrostatic equilibrium should be called a planet did it while brandishing the probable number of planets that would ensue. 200 planets? What an absurd, they said. Eight is much better: kids can learn their names by heart, they said. And, of course, have placemats with eight very incorrectly rendered planets instead of nine, much less 200.
That’s one of the cultural consequences of reducing the number of planets to 8. Instead of learning about the real solar system out there, about the various classes of planets that circle the sun, about how they interact with eachother, people will satisfy themselves with parroting some kind of mnemonic and end up knowing less about the solar system than they did when they thought the planets were 9, and much, much less than they could know with the term planet defined as a vast umbrella where every gravitational ball has its place.
And there’s another, recurrent, error 8-planet advocates fall into: to speak of these things as if the Solar System was the only planetary system of the universe. It most definitely is not.
Here’s a great reason to make dwarfs planets too August 20, 2009
Posted by Jorge Candeias in Definition of planet, Dwarf planets.Tags: astrology, Definition of planet, Mike Brown, Mimas
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You know, Mike “Plutokiller” Brown estimates that there may be about 200 objects larger than 400 km in diameter in the Kuiper Belt, and guesstimates the number of similar objects beyond the Kuiper Belt to be around two thousand. He thinks all of these should be in hydrostatic equilibrium, and therefore should be considered dwarf planets. I’m not convinced (the smallest body actually known to be in hydrostatic equilibrium is Saturn’s moon Mimas, which is indeed about 400 km in diameter, but I think satellites will probably be found to have lower limits because tidal stresses should help gravity in the process of rounding them up; in the absense of these stresses, they won’t round up that easily), but I ain’t complaining. And I actually think that this should be a great reason to make all of them planets too. Or at least all of those that actually are in hydrostatic equilibrium.
You see, I’m sick and tired of astrological BS. And you just try to imagine the chaos astrologers would find themselves into if they had to deal with more than two thousand planets in order to make their so-called “predictions”. Ha! Wouldn’t that be a blast?
It would be worth it, just to make these guys’ lives considerably harder, methinks.
Disclaimer for the humour-impaired: this is a tongue-in-cheek post, not a scientific one.
Disclaimer PS: The part about Mimas is serious, though.
Odd balls August 15, 2009
Posted by Jorge Candeias in Extrasolar planets.Tags: Eris, Extrasolar planets, HAT-P-7b, Triton, WASP-17b
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Here’s something you don’t see every day: last week brought news of not one, but two extrasolar planets that are far more oddballish than anything we have in our Solar System. It started with the announcement that the newly discovered WASP-17b had two very bizarre characteristics. For starters, a planet with its mass, about half that of Jupiter, should be smaller than Jupiter… but that one is much larger. In fact, at twice Jupiter’s diameter (i. e., about 140 000 km), it is the largest planet known so far.
BANG! Strike one.
But what I find really juicy is another fact: WASP-17, the planet’s star, rotates in one direction, and the planet goes round it in the opposite direction.
WHAM! Whoa!
Why is this vastly interesting? Because planets form out of the same rotating clouds of matter that creates stars, which means that the direction of planetary movement around the star, at the time of its formation, has to be the same as the direction the star itself rotates. That’s what happens in the Solar System: not only all the planets go rond the sun in the same direction the sun itself rotates, but the same is true for the vast majority of planet’s moons and smaller objects… all the way down to comets. The only significant exception is Triton, the largest moon of Neptune, whose retrograde orbital motion (it’s the name this phenomenon has) led scientists to believe that at some point it was captured by Neptune from an orbit around the sun. That is: Triton is thought to have been a dwarf planet at some point. Fun fact: it’s about the same size as Eris.
OK, this may be true for almost all Solar System objects but isn’t for WASP-17b.
What this means is that something major happened to it after it was formed. Astronomers don’t seem to be giving much credit to a capture scenario, probably because the planet is so close to its star: it’s a “hot jupiter”. Instead they are speculating that at some point, probably after it was fully formed, it must have had a close encounter (a very close encounter!) with another giant planet that sent it spinning into the traffic, so to speak. The other, unknown, planet, was either sent into a very highly elliptical orbit, or ejected alltogether from the system. This last sentence is me, speculating, so don’t go thinking it’s the truth, OK?
Fascinating stuff!
And it gets better: the very next day, two teams announced the discovery of another retrograde planet, HAT-P-7b. This one wasn’t a new find; the planet was already known. The novelty here lies in the disalignment between the plane of the planet’s orbit and the rotation of its star. In this case, numbers are somewhat conflicting and unclear, so the only thing that is an absolute certainty is that HAT-P-7b does not orbit along the equator of HAT-P-7, as happens with all the major Solar System planets (i. e., all planets excluding most dwarfs): it may be highly inclined, orbiting along the poles or close to them, or, which seems more likely, it’s another retrograde, orbiting along the equator but in the opposite direction, like WASP-17b.
Double Whoa!
Planets, special, orderly, well-behaved objects? Yeah, right…
Addendum: Take a look at Exoplanetology blog, where the method used to make the discovery is very well explained. The only thing I don’t think is correct is where he talks about a violent collision: no collision with an object moving in the same direction could make a planet move in the opposite direction… but a very strong transfer of orbital momentum could.
Size comparisons, take two August 14, 2009
Posted by Jorge Candeias in Ceres, Mercury, Neptune.Tags: Celestia, Ceres, Mercury, Neptune, size comparisons
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I’ve already shown you a comparison between the largest Solar System planets in each category, and then I thought, heck, for the sake of completeness let’s do the same with the smallest ones, also with the help of Celestia. So here you go:

Size comparison between Neptune and Mercury

Size comparison between Mercury and Ceres
Isn’t this cute? The proportions look very much like those of the largest planets in each group, and if you prefer some numbers here they are: Neptune is 10 times larger than Mercury, wereas Mercury is nearly 5 times larger than Ceres. If you go check the masses, you’ll find that Neptune is almost 290 times heavier that Mercury, and Mercury 375 times heavier than Ceres. Everything very similar to the proportions between the biggest planets in each class. It should be noted, though, that Neptune may be the smallest of the giants but is not the lightest; that is Uranus’ claim to fame. Or one of them, anyway.
And, again, there isn’t much of a point in this. It’s just a visual reminder that if you look at the objects without taking into consideration their positions relative to eachother, the differences between giant and terrestrial planets tend to be larger than the difference between the terrestrials and the dwarfs.
Why are 8 planets bad science August 12, 2009
Posted by Jorge Candeias in Definition of planet, Plutophiles.Tags: asteroids, Definition of planet, history of astronomy, IAU, Mark Sykes, Pluto, Plutophiles, Titus-Bode Law, twitter
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Yesterday, there was a small rebellion of “plutophiles” on twitter. A hashtag, #bringbackpluto, made it to number one in the trending topics list, and the messages that came along with it were, in general, as silly as you might expect. People just don’t get it.
The people who took part in that particular hashparty vastly misunderstand the reasons why the whole business of Pluto’s “demotion” came about. And their revolt does nothing to further their case and actually “bring back Pluto” (as if Pluto went anywhere; as if it isn’t right where it has always been, going round the Sun beyond Neptune). Quite the contrary. By showing so eloquently that they don’t get it, they simply won’t sway any of the people who actually have some knowledge about this stuff. The only way to sway them is to play their game, which means learning the science and discuss it scientifically. And learning some history of astronomy as well. And remember my mantra: “this ain’t about Pluto!”
Hop aboard. I’m taking you in a small historical trip. A trip you may get from plenty of other sources, but in this there’s no such thing as too many sources of information. And besides, nobody tells it quite like I do. In the end of this necessarily long text, I’ll tell you the main reason why I think that to speak about 8 planets is bad science. You can jump immediately to that point, if you think you already know all the historical stuff, but you’ll be missing my emphasis, on which I base my conclusions. It’s up to you.
Ready? Allright then. Fasten your seatbelts and let’s go visit the ancient Greeks.
Not that those were the guys who discovered the first planets. Ever since the first records of celestial movements were made, probably by the very first astrologers, people knew that there were some lights in the sky that stayed put, wereas other lights walked about. The Greeks were simply the guys who came up with the word “planet”. It means, aptly enough for the level of their understanding, wanderer.
Back then there were two different kinds of wandering celestial objects: those with an obvious disc, and those that looked like point sources of light, like moving stars. The first kind encompassed the Sun and the Moon, and there were all kinds of legends about them; the second kind was composed by 5 objects: Mercury, Venus, Mars, Jupiter and Saturn. These five were always thought of as planets, the Moon and the Sun kept coming and going from that category. The Earth, of course, at first was not thought of as a planet like the others, being as it was the center of it all (and flat). But whatever the actual numbers and groupings were, one thing remained constant: planets were special. Worthy of being used as characters for all sorts of myths and stories. How could they not be special? They were a handful of wandering lights in an otherwise static sky! They had to be pretty important and unique indeed! Right?
Then happened the first revolution in our understanding of these things, when the geocentric models of the Universe gave way to Copernicus’ vision of a universe centered in the Sun, a heliocentric vision. Planets, once rotating around the Earth, were now circling the Sun.
And the Earth with them.
This meant that planets were not point sources of light after all, but (probably) solid, round worlds like our own, maybe even with their own inhabitants. It also meant that the Moon was not a planet, but a satellite, for it circles not the Sun, but the Earth. The Sun? Ah, not a planet either. The Sun now became the center of everything. Not a star, as yet, but so unique it had no category to belong to. It was just the Sun.
This was a complete turnaround in our understanding of what a planet is. But, despite that, the now 6 planets remained very special places indeed. Think about it: thousands and thousands of stars, and only six worlds like our own? They’re special, no question about it!
And more: there was an order to them, an order that was often used as an evidence of divinity, for only an allmighty God could create such perfectly harmonious structures. When Galileo peeked through his telescope and saw for the first time that the other planets were, indeed, discs, that seemed to confirm this notion, although shortly after two discoveries shook things a bit: the discovery of the four galilean moons of Jupiter (which were also called “planets” for a while, as were, later, the first moons of Saturn to be discovered), and a pair of strange “ears” protruding from the sides of Saturn, which even changed shape over time. It was only in mid XVII century that these ears were recognized as rings, and that the first moons of Saturn (starting with Titan, of course) became known. There was something else that also tainted these notions of divine astronomical perfection: the discovery, by Kepler, that the planets did not follow perfectly circular paths, as previously thought, but moved along ellipses.
In the next century two relevant things happened. First, some astronomers noticed that the planetary distances to the sun followed closely a mathematical relation which came to be known as Titus-Bode Law. There was a gap between Mars and Jupiter, though. And the law said nothing about ending the fun at Saturn. So everyone began looking for new planets in the gap and beyond Saturn, and Uranus was found right where the law said something should be. You can imagine by yourselves how that bolstered up its credibility and the notion that, despite some annoying facts, God really did have a finger in making an orderly and predictable universe, in which the planets had their very special parts to play.
When Ceres was found in 1801, again right where Titus-Bode predicted it, it all seemed to be proved beyond a doubt. And Ceres quietly became the 8th planet of the Solar System. But then, shortly after, 3 more planets were discovered in the same general area, and heads began to be scratched.
And then stranger things began to happen. Uranus wasn’t behaving: instead of peacefully following its path, it wobbled back and forth, as if something unseen was pulling it. So the astronomers crunched the numbers, determined the position where the perturbing object should be, pointed their telescopes to that position, and there was Neptune, yet another planet, just waiting to be discovered. This happened in 1846. Great news, right? Wrong. Neptune’s position deviated significantly from what was predicted by the old Titus-Bode Law.
Oops! Could it be that such a venerable law of nature was wrong?
To make things worse, the year before a 5th body had been found between Mars and Jupiter, and from 1847 on new discoveries around the same zone happened at a steady pace. By 1900 they were already 450. Things were a lot more chaotic than they had seemed to be. The neatly ordered plan of God was taking a beating from reality.
These were the signs of a revolution to come.
That’s when astronomers noticed two things: firstly all the chaos was restricted to the zone between Mars and Jupiter, where Titus-Bode predicted there should be a planet. Maybe it exploded, and what was being discovered were mere fragments? All the other planets seemed to behave, kinda. The divergence between Neptune’s position and Titus-Bode could perhaps be a fluke? A statistical outlyer? Astronomers also noticed that all of the well-behaved planets showed typical planetary discs. But the annoying rebels beyond Mars didn’t. Like the planets in the old days, they looked just like moving stars.
And so they were christened “asteroids”, a word that means “similar to stars”, and the number of planets was reduced to 8. And the order was preserved. And the planets continued to be special objects in the sky.
Ah! What a relief! Sometimes you need a revolution to keep things as they were.
Pluto came about in 1930 (although it had been detected much earlier), and deviated so much from Titus-Bode that effectively killed it for good. At first its size was greatly overestimated, but there was little question that it had to be called a planet, even though no disc could be seen and even though its orbit was weird. It was alone out there, very far from the area where asteroids dwell, and much bigger than asteroids were. But that weird orbit… many people found it really hard to swallow. It seemed too odd, too distant from the orderly display the other 8 showed. But, hey, 9 planets in such a large Universe are still pretty special, aren’t they? So they went with it anyway.
But then came the 1990′s. Astronomers began an amazing series of discoveries in the outer Solar System. Small and not so small icy bodies in orbits similar to Pluto’s became commonplace, a chaos of intersecting, eccentric, inclined orbits that seemed to mirror closely what happens in the Main Asteroid Belt. Those that were uncomfortable with Pluto’s oddity became increasingly more uncomfortable. And when finally an object larger than Pluto, Eris, was found, something just had to change again. It was inevitable. We just had to fundamentally rethink what makes a planet for the third time in our history.
It could be simple. Just make with Pluto the same that was made with Ceres, Pallas, Juno and Vesta in the XIX century, reduce once more the number of planets to 8, and get on with it. Keep the order. Keep the specialness of planetary status. That’s what the IAU astronomers did, and that’s the source of the current definition of planet.
But it really is everything but simple. At the same time trans-neptunian objects were being found everywhere, exoplanets were also being found by the hundreds. Around “normal”, sun-like stars, around stars smaller and larger, around red dwarfs, around pulsars, even free-floating, roaming alone the empty spaces between the stars. Other planetary systems were found that didn’t look anything like our own. Systems with planets larger than Jupiter in orbits much more eccentric than those of any Solar System dwarf planet. Systems with 2, 3 or more giant planets packed inside what in the Solar System would be the orbit of Mercury. Systems with resonant giant planets. A wide variety of outcomes of a process that is apparently universal: planetary formation.
And all of a sudden there’s no order, only different outcomes of a process that is inherently chaotic. And all of a sudden planets are no longer special: we already know where are hundreds of them, and it’s now clear that we’ll end up finding many billions in our galaxy alone. Planets are literally everywhere.
And this is why 8 planets are bad science.
By insisting on a small number of planets, the astronomers are trying to perpetuate a notion that science itself has already defeated: that planets are rare and special bodies, that they are well-behaved and orderly, that it’s still possible to find in them the music of the spheres. When none of this is true.
This time, no revolution can leave things as they were. This time, we simply cannot avoid a true, paradigm-shifting revolution.
As Mark Sykes puts it, “we are in the midst of a conceptual revolution [...], shaking off the last vestiges of the mythological view of planets as special objects in the sky – and the idea that there has to be a small number of them because they’re special.” That’s exactly it. And that’s why the most amazing part of all this is, to me, that the IAU definition was already obsolete when it was created and approved.
Which is to say, bad science.
This is also why I’m absolutely certain that it will end up being defeated. This definition will not stand. Not because thousands of “plutophiles” go do some agitprop to twitter, but because it just doesn’t fit reality. Not because people are annoyed by the “demotion” of Pluto, but due to the wide diversity of planets that exist out there. In the end, the only possible outcome of all this is a broad definition of what planets are, as broad and inclusive as planets are varied in this vast universe we live in, and a classification scheme that sets up categories within that definition. They are already emerging, even. The literature is crawling with “jupiters”, “neptunes”, “super-earths”, “hot neptunes”, “gas giants”, “ice giants”, “terrestrial planets”.
And, yes, “dwarf planets”, why not?
Stop it already August 7, 2009
Posted by Jorge Candeias in Plutophiles.Tags: Mike Brown, Pluto, Plutophiles
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Enough is more than enough.
Just saw, on twitter, someone calling Mike Brown a “twit” because he is, says the guy, “against Pluto” and “names a planet after a teevy (sic) show”. Really? A twit?
Yes, Mike Brown is a provocateur, otherwise he wouldn’t have chosen the alias “plutokiller” for his twitter account. But just how dumb and hysterical do you think calling him names makes you look like?
Can this nonsense stop? Can we please talk about planets and what distinguishes them from other objects in the vast Universe without this kind of childishness? And can we please put Pluto aside while we do that?
You too, Mike.
Some size comparisons August 7, 2009
Posted by Jorge Candeias in Earth, Eris, Jupiter.Tags: Celestia, Earth, Eris, HD 139357 b, Jupiter, size comparisons
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Well, I think it’s about time this blog includes a few pictures. And, since posts with pictures tend to require less words, it’s also a great way to give it content without spending in it too much time. So here are two quick renditions I made with Celestia, showing side by side the largest of the Solar System’s giant, terrestrial and dwarf planets:

Size comparison of Jupiter and the Earth

Size comparison of the Earth and Eris
The Earth in the bottom image is slightly larger than Jupiter in the top image (it isn’t easy to get this just right in Celestia without doing some math, which I didn’t), but I think the comparisons are effective even so. Eris (which doesn’t look like that, by the way; since we’ve never seen its surface, Celestia uses by default a generic texture, the same for all bodies in the same situation) is closer to the size of the Earth than the Earth is to the size of Jupiter. If you need numbers, then they are approximately as follows: the diameter of Jupiter is 11 times that of Earth. The diamater of the Earth is 5 times that of Eris (and no, the rather large uncertainties in Eris data don’t change this by much; at most they may drop that number to 4). More interestingly, if you compare not sizes but masses, which are actually more relevant, you get a couple of very similar numbers: Jupiter is about 320 times more massive than the Earth; the Earth is approximately 360 times more massive than Eris.
And the point is?
There isn’t much of a point, really. This just goes to show you that when it comes to compare sizes we’re not all that gifted. The big boys in the block are really big. And if you look at them from this perspective, the dwarfs don’t seem all that insignificant anymore.
And remember: if you look beyond the Solar System you’ll find other big boys that are even bigger than the big boy from our own neighbourhood, making our planet seem even more puny and helpless. HD 139357 b, for instance, is a behemoth 9.76 times more massive than Jupiter, which is to say 3100 times more massive than the Earth. Yes, that’s three thousand Earths needed to make only one gas giant.
Good thing that it strolls around almost 400 light years away, huh?
OK, I’m in August 5, 2009
Posted by Jorge Candeias in Blog stuff.add a comment
In the previous post, I promised I’d tell you what I decided regarding the future of this blog. Thanks to Astroengine‘s (and Discovery Space‘s) Ian O’Neill, who tweeted overjoyously my coming back from the dead as a space-oriented english-language blogger and hastily linked this tiny little blog from his heavyweight one, and to the guy behind Exoplanetology, who retweeted Ian’s tweet, leading to more hits and comments in one day than in the previous three years, I was left with only one option: give a new breath of life to this little Frankenstein of mine.
So OK, fellas, I’m in.
Now, don’t expect this blog to be anywhere near as active as those blogs linked above. I don’t have that much to say, in truth, nor do I have the first hand access to sources major league space bloggers have. Plus I spend a lot of time writing each post in an English that wouldn’t embarrass me too much. Not my mother tongue and all that, you know? I’m likely to go through weeks without posting anything (particularly whenever the deadlines in my day job start to tower over me, which is something that does happen relatively often), although in some occasions I may put out two or three posts in a row. The word is erratic. Expect this blog to be just that.
To stay in the loop without having to come back regularly just to see that nothing has changed, you have, of course, my RSS feed. I toyed with the idea of creating a new twitter account just for this baby, but the two email addresses I check regularly were already taken, and it may not be worth the effort of creating a new one or paying closer attention to the ones I basically ignore. You can, if you will, follow my main twitter account, where I’ll post update notices under the hashtag #1000plans, but be advised that I tweet mostly in Portuguese and on other, non-space, issues, so you may find my twitter feed quite uninteresting.
But do follow @astroengine and @exoplanetology. Those two are most certainly worth it.
One last thing on commenting policy: to avoid spam and the hassle of captchas and logins, everyone’s first comment is moderated. That means that it may take a while to show up, especially if you’re commenting while I’m sleeping or otherwise away. Rest assured, though, that it will show up (unless it’s some sort of spam or particularly trollish), and once you have one comment cleared, you’re free of moderation and your comments will show up as fast as wordpress allows. Just so you know.
See you soon.
Yaya! I’m here! August 5, 2009
Posted by Jorge Candeias in Blog stuff.1 comment so far
Hello, everyone.
As the very few who have visited may have noticed, this blog has been pretty much abandoned for the last three years. The reason is simple, even if somewhat embarrassing: I had misplaced the password for my wordpress account and had a few email issues as well which didn’t make it easy to recover it. Silly, huh? That’s life, the universe and everything for you.
But now, hurray, I found it. Just popped up suddenly, like an old friend who decided to renew an old friendship all of a sudden. Go figure.
So. What to do? I still have to say all those things I promised three years ago, but quite a few were said already by other, more knowledgeable people, people with much better reps than I when it comes to these issues. And even so, I myself kinda spread bits and pieces of them here and there, in the comment boxes of places such as Astroengine or Universe Today. I could go fish out those comments and use them as source for a whole series of posts, but is it worth it? Weren’t those things already said? Could a blog that has been abandoned for so long find any new readers for my thoughts, readers that don’t know all about them already?
Decisions, decisions… Life is made of decisions.
Stay tuned; I’ll let you know what I decide to do. In the meanwhile, if you wish you may tell me your opinion: the comment boxes are open, as they have been all along.
Cheers.