It's lucky there's no water on that rocky planet.
Can you imagine what the tides would be like?
Astro-boffins have located an alien planet pair that are orbiting so close to each other, any inhabitants would see a planet-rise as well as sunrise. Gas giant sits on the Seattle skyline Gas giant sits on the Seattle skyline. Pic credit: NASA, Frank Melchior, Eric Agol Both of the planets are a little too toasty to play host …
Can you imagine what the tides would be like?
Lava is liquid-ish too.
And there's no Rocky on that planet either!
(The one with the boxing gloves, please)
I'm still waiting for a cool planet arrangement that is also habitable. Come on, let's find that Niven-style surface-friendly planet!
Ah, but we're looking at whole planets. A fair few of Niven's worlds would get missed since he was fond of worlds with small habitable zones on otherwise inhospitable planets.
Can somebody please explain to me how they can work out that one of the planets is a gas giant and the other is a rock? Presumably you can't tell that just by looking at the 'wobble' they impart on their host star?
I'm no scientist but I believe they look at how the radiation spectrum differs when the planet is in front of the star.
It's pretty much the only way to tell that a planet even exists - we don't know much if anything about planets that don't happen to orbit between their star and us.
No spectroscopy here (most likely, anyway) - stars have an annoying habit of being so bright that they drown out any light from the planet itself. Instead, you look at how the light from the star dims as the planet passes in front. You can guesstimate the mass of the star quite well, and from that and the orbital period, you can get the star-planet distance. You then know a bigger planet will block more light at a given distance than a tiny one, so you can work out the radius of the planet by the amount of starlight blocked, the radius of the star itself, and how far apart they are. You then use fairly handwavey arguments and say that if it's Earth radius, it's like Earth, and that if it's Neptune radius, it's like Neptune!
That is, of course, much simpler than how it actually is!
And a few notes now I've posted and re-read that:
The Mass/Radius of the star comes from its colour - bluer stars are more massive, larger, and hotter; red stars are smaller and cooler. We've spent a lot of time modelling these! Look up the "Main Sequence" if you want to know a bit about that.
We're not entirely sure on planet compositions for things that aren't represented in the solar system - this is why we're not too sure what a Super-Earth is actually like. When do you stop being a ball of rock and become an ice/gas giant? The theoretical chappies have been having great fun with all that.
Spectroscopy isn't so good for getting actual planet sizes - you can get the mass ratio of the star:planet easily, and if you guess the star's mass, you can get the planet's one too. But as mentioned above, if something is 3 times the mass of the earth, do we model it as a ball of rock or a ball of gassy ice? Ideally you want to combine information from both spectroscopy and transits ("photometry").
I'll have to see it to believe it.
If those planets have moons, you would get some truly astounding views as both planets rise/set... and you wouldn't melt from the heat either.
Given the proximity and possibility for genetic material making it from one planet to the other, you'd expect similar DNA on both planets. Just slightly bigger tits on 36c.
The star isn't obscured by the clouds over Seattle.
Why is it so dark in the city there? Do blue ones put out that much less visible light?
*Looks out the window*
Hmm, good point...and here I was looking forward to some blue planet-viewing tonight. ;)
As for the dimness in the city, we Seattleites aren't accustomed to bright light so we have to filter it out to protect our sensitive eyes.
And the Welsh complain about *their* weather. I was in Cardiff in March and it felt like summer!
We turn off the rain and clouds when you leave.
Meh, call me when they find 36DD
Hey, neat! Not only did we get a new planet over here, Mt. Rainier has been removed! I wonder if it's from the new planet's tidal actions... Hmmm...
Mount Rainier isn't missing, it is just to the right of where the photo ends
"The bigger planet is pushing the smaller planet around more, so the smaller planet was harder to find."
C'mon professor, it's pulling it around surely?
Errr, do they share an atmosphere?
A blue planet? That's where ye unobtainium is, chaps! Let's get there fast!
(Well, at least the people there had that same blue hue)
Probably the smaller planet was knocked out of stable orbit, and was captured by the gas giant. That, or it formed out of a condensate disc around the giant. (Think about Saturn's rings, but a lot lumpier.)
Either way, I'd suggest it's in effect a moon, just vastly larger than we're used to thinking of them.
Yeah, a moon except for the part where it's not orbiting the gas giant either, which is one of the bigger prerequisites for being a moon in the first place.
That's no moon!
Kepler 36 ???
Surely planets should be named after their order of orbit from the parent Star ? As in we are living on Sol 3 ...
I can't imagine calling everything Kepler followed by a number is going to stick or even be very easy to understand.
Are the parent stars not even hardly getting a mention now?
The star itself is Kepler 36 (well, Kepler 36a). You then label planets as b, c, d, and so forth. So we would technically be Sol d, by that naming system!
Quote: The star itself is Kepler 36 (well, Kepler 36a). You then label planets as b, c, d, and so forth. So we would technically be Sol d, by that naming system!
We are Sol3, you don't give the star the A designation. That goes to first orbiting planet. This particular star is Kepler 36a because there is a different nearby star (maybe locally grouped or optically near to it). So to distinguish between the 2 Kepler 36's, a letter is designated to each. Kepler 36b is therefore a star not a planet.
The system described in the article consists of a star (Kepler 36a) and two planets (Kepler 36a 1 and Kepler 36a 2). If a planet has moons, they are given a letter designation starting with a for the closest moon. Our Moon is therefore Sol 3 a. Spaces are optional, but generally dropped except for a numbered star (Kepler 36a)
No idea where you got that information from! The generally accepted system is:
Kepler 36 is the system. In a binary (or more) star system, the stars would generally be A and B - in a single-star system, it is acceptable to drop the A (so Kepler 36 = Kepler 36A). Objects orbitting around Kepler 36A are labelled with lowercase letters, with the central object (the star) being designated Kepler 36Aa = Kepler 36a. The planets are then Kepler 36Ab and Kepler 36Ac, but again the A can be dropped as there is no ambiguity.
An alternative example would be the 16 Cygni system, consisting of 3 stars (16 Cyg A, B and C), with the 16 Cyg B system containing two components - 16 Cyg Ba, the star, abd 16 Cyg Bb, a planet.
Hessman et al's paper is a good reference for this: http://arxiv.org/pdf/1012.0707v1.pdf
Quote: Hessman et al's paper is a good reference for this: http://arxiv.org/pdf/1012.0707v1.pdf
Specifically the section called "Proposal" you mean? As in not yet implemented!
The artist(s) who produced those pictures just didn't grasp the size of gas giants. To say that the gas giant, when seen from the rocky world, would be much larger in the sky than those images suggest would be a gross understatement; the gas giant would fill most of the sky.
Is this where we get out the plastic cow?
Neptune is 10x wider than the moon, but this planet is 5x further away - so it would only be double the width of the moon in the sky, which actually seems to be what that image shows!
Oops! - you're quite right; I initially read it as being much closer
You mean 1/20 (one twentieth) the distance?
Paris, because you don't yet have a Brian Cocks...
The Nubiri nuts will have a field day with this one, mark my words.
Two planets that close. When they discover life on each others planet, it will be a race to build big rockets. Not to visit, but to start a war.