Borderline habitable, anyway. Rocky planet, two Earth masses, looks promising, but so close to its (small, dim) star that it's probably tidally locked, meaning the same side will always point towards its sun. This means that the vast majority of its surface will either be too hot or too cold for life.
But a certain ring will have constant perfect weather!
I would argue that this falls into the "cool" part of what, until now, has been entirely scifi - and that I'm absolutely ridiculously excited about seeing more and more of these discoveries in the years to come.
No, there's no hope of ever visiting this place in our respective lifetimes (sans cryogenics), but I'd put money on the prediction that we will certainly see real imagery of exoplanets within 50 years. And that's cool. Really cool. So cool that we'll look back and laugh at the original question of "are all exoplanets bigger than Jupiter and closer to their suns than Mercury?"
I was thinking more of spectroscopic interferometry. We probably can't make laser strong enough now, but a 40 year round trip for a light probe to start feeding data is enough for one person to consider making it a lifetime endeavour.
Density of a planet's interior is not uniform, and gravity tapers exponentially with distance. So, a planet with a dense core and a less-dense middle area could easily have less gravitational force than you might expect since the surface is so far away from the dense core.
If you have a body with a spherically symmetric mass distribution, from the outside it always has exactly the same gravitational field as a point mass at the centre.
Wait, but didn't I specifically say I was referring to a body without a spherically symmetric mass distribution? Maybe I'm incorrect in my understanding of symmetric, but I was definitely referring to a non-symmetric case in my text.
Spherically symmetric means that it looks the same no matter which way you rotate it. You talked about a dense core, less dense middle-region planet, which is spherically symmetric.
If the planet had an ultra-dense region off to one side then it wouldn't be spherically symmetric and it would have gravity slightly stronger on one side than on the other... it's hard to imagine such a planet existing though.
It's more massive, but the radius is bigger as well. It could be as low as 1.5 Gs. Modifying the gravitational formula (http://en.wikipedia.org/wiki/Earths_gravity), it's m/r^2, so 3/(1.4^2) = 1.53 Gs. That's neglecting any local variations.
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[ 3.4 ms ] story [ 58.5 ms ] threadBut a certain ring will have constant perfect weather!
"That means the planet has...a band of eternal sunrise or sunset where water — and perhaps life — could subsist comfortably."
Space is big. We are slow. Everything cool about scifi is fiction. None of this will change in our lifetimes.
No, there's no hope of ever visiting this place in our respective lifetimes (sans cryogenics), but I'd put money on the prediction that we will certainly see real imagery of exoplanets within 50 years. And that's cool. Really cool. So cool that we'll look back and laugh at the original question of "are all exoplanets bigger than Jupiter and closer to their suns than Mercury?"
If you have a body with a spherically symmetric mass distribution, from the outside it always has exactly the same gravitational field as a point mass at the centre.
Proof: http://hyperphysics.phy-astr.gsu.edu/hbase/mechanics/sphshel...
If the planet had an ultra-dense region off to one side then it wouldn't be spherically symmetric and it would have gravity slightly stronger on one side than on the other... it's hard to imagine such a planet existing though.
Inverse square law.