Astronomers See the Glow of a Boiling Planet
The Bad Astronomer writes "For the first time, astronomers have detected the light from a 'super-Earth' exoplanet. The planet 55 Cancri e (with twice the radius and 8 times the mass of Earth) circles its host star every 18 hours, and is so hot it glows in the infrared. By observing in that wavelength, the astronomers measured the dip in light as the planet's glow was blocked by the star itself. This is the reverse of the usual method of detecting a planet as it blocks the light of its host star."
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Before it doesn't emit infrared radiation?
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What exactly justified it to be called super-Earth? The size is close to Earth (half order of magnitude), but it is close to Venus as well, and Venus is hotter.
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Will Elon Musk super-retire on this planet?
I suggest we send Finnish astronauts. They actually like this sort of place.
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(long delay)
"Shhh... I'm relaxing"
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A watched planet never boils...
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Why did God design so many planets inhospitable to life? The universe seems a little more empty when you think there are so many planets that can't support life.
One small dip is when the planet is covering the sun.A larger dip is when the sun is covering the planet.
S+P vs S vs S +P - coveredfractionofsun*S.
When the planet is colder the first dip is larger and the second dip is less. With a hot planet I think both dips may well be measurable.
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Something isn't right here.
Even if the planet were so close to the star that it was in the corona, If it were a star the size of our sun, the speed of the planet would be, really really big.
Anybody have any numbers on this?
Wait. If it orbits the star every 18 hours then at least one of the following must be true.
1. It orbits at a high fraction of the speed of light.
2. It is a very very small star.
3. It can't really be considered a "Super Earth" due to proximity to the star.
Hot enough to boil lead more like.
The orbital image leaves a lot to be desired... Come on, 1/3 of the phase is shown! Thanks to Nasa's usual attempts to hoard its images, here has a little more information on that orbital phase.
Although they try to explain what is theorised to happen, HTF does the infrared dip when the planet passes behind the star? Is the star not the total possible output of IR available in that system? i.e. The effects of IR don't stack when the planet is in front of the star; you don't get more output from the system than is available from the source! The planet AFAICT is dark sided, relative to us, when passing the forward facing part of the star, relative to us, which means it should be much cooler on that side than the star facing side blasting towards earth when as the planet egresses the occultation, from the opposite in which they ascribe above...
Without any mention or reference to the stars wobble regarding the planet to disprove my theory, I suspect the orbital times are more likely half that TFA suggests which means it is seriously nipping around. Maybe it is too difficult to get a wobble indication due to the fast speed of the planet and the distance from the star? I doubt it though. I speculate that the dip in question is the time it takes to pass the front of the star, relative to us.
Would someone care to make a speed calculation based on the possible variables such that: the star is similar in size to ours, the planetary orbit is 18hrs (imo 9hrs).
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