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!
FTA: "That means the planet has...a band of eternal sunrise or sunset where water — and perhaps life — could subsist comfortably."
A Habitable Exoplanet - for real this time
11–20 of 21 posts
Re: A Habitable Exoplanet - for real this time
#12Re: A Habitable Exoplanet - for real this time
#1320 lightyears is a long way, but not that long. What we're 'seeing' via our instruments was taking place around 1990.
So if we had pointed Voyager at it back in the 1970s, we would only have 19.997 lightyears left to travel! 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?"
Re: A Habitable Exoplanet - for real this time
#14Earlier quoted context omitted.
According to http://news.yahoo.com/s/afp/20100929/sc_afp/usastronomyplane... , surface gravity might only be slightly higher than earth's.
How is that possible?
Re: A Habitable Exoplanet - for real this time
#15Earlier quoted context omitted.
How is that possible?
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.
Proof: http://hyperphysics.phy-astr.gsu.edu/hbase/mechanics/sphshel...
Re: A Habitable Exoplanet - for real this time
#1620 lightyears is a long way, but not that long. What we're 'seeing' via our instruments was taking place around 1990.
So if we had pointed Voyager at it back in the 1970s, we would only have 19.997 lightyears left to travel! Space is big. We are slow. Everything cool about scifi is fiction. None of this will change in our lifetimes.
Re: A Habitable Exoplanet - for real this time
#17Earlier quoted context omitted.
How is that possible?
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.
Inverse square law.
Re: A Habitable Exoplanet - for real this time
#1820 lightyears is a long way, but not that long. What we're 'seeing' via our instruments was taking place around 1990.
So if we had pointed Voyager at it back in the 1970s, we would only have 19.997 lightyears left to travel! Space is big. We are slow. Everything cool about scifi is fiction. None of this will change in our lifetimes.
Re: A Habitable Exoplanet - for real this time
#19Earlier quoted context omitted.
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.
Surprisingly not so. 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...
Re: A Habitable Exoplanet - for real this time
#20Earlier quoted context omitted.
Surprisingly not so. 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...
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.
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.