- 35,014
- 21,725
Just for fun, I calculated what Proxima Centauri would look like from a planet orbiting Alpha Centauri A. It would be somewhere between 3rd and 4th magnitude. Maybe noticed by the natives (if any), maybe not.
Vanadium 50 said:I still have doubts that a planet will not tide-lock.
Vanadium 50 said:Just for fun, I calculated what Proxima Centauri would look like from a planet orbiting Alpha Centauri A. It would be somewhere between 3rd and 4th magnitude. Maybe noticed by the natives (if any), maybe not.
No. The torque depends on how aspherical the planet is.Vanadium 50 said:The degree of torque on the planet depends on how aspherical the body they are orbiting. The sun is spherical (mostly). Two suns are not.
Stars are pretty fluid objects so I'd imagine that they would form a fast rotating spheroid. Would the presence of a nearby mass disturb this, bearing in mind that the orbit period would have to be many times greater than the rotation period (years vs hours)? That implies no locking(?).Vanadium 50 said:I still have doubts that a planet will not tide-lock.
Wrong, And I'm out of here - I have decided not to participate in the arns race of correcting misinformation.snorkack said:No.
Most planets in solar neighbourhood are planets of red dwarfs.Algr said:Interesting. Not many planets anywhere will have Red Dwarfs naked-eye-visible at all.
The known circumbinary planets:Algr said:So I'm looking this up on Wikipedia and the skies from any planet in that system could never look like Tatooine. My drawing up top might be possible at some times of the year, if a planet was in the habitable zone of A or B. But then the distant star would appear far from the large one most of the year, and could be on the opposite side of the sky.
I meant seeing them as stars at night, not orbiting them as a sun. A developing civilization might face a smallsnorkack said:Most planets in solar neighbourhood are planets of red dwarfs.
Now this is interesting. It occurs to me we have no idea what a tidally locked gas giant would be like. Would it be round? Shaped like a pear or comet? The same forces that cause tidal locking would also make moons unstable and short lived, right?snorkack said:Kepler-34. A binary of two Sun-like stars, orbiting at semiaxis 0,22 AU. The first that could look like Tatooine.
What do you classify as "seeing them as stars at night"?Algr said:I meant seeing them as stars at night, not orbiting them as a sun.
They also would not see night sky.Algr said:A developing civilization might face a small
hurdle with this, as the stars they see in their night sky would all be fundamentally different than their sun.
Moon is tidally locked but not so conspicuously out of round.Algr said:Now this is interesting. It occurs to me we have no idea what a tidally locked gas giant would be like. Would it be round? Shaped like a pear or comet?
Agreed.Algr said:The same forces that cause tidal locking would also make moons unstable and short lived, right?
How stringent is the last condition?Algr said:"Look like Tatooine" actually turns out to have some rather stringent requirements:
- Stable Habitable planet. (This may or may not preclude tidal locking.)
- Two stars of near equal size.
- Distance from one star to the other is no more that 6x the radius of the stars.
https://en.wikipedia.org/wiki/Nightsnorkack said:What do you classify as "seeing them as stars at night"?
Unless they have feet and can walk to where the night is.snorkack said:They also would not see night sky.
Moon is not a jovian. It does not have a density significantly higher on one side than the other. It's mass isn't mobile via air currents.snorkack said:Moon is tidally locked but not so conspicuously out of round.
I'm thinking that the planet's orbit would destabilize if the two stars were too far apart. So the second star has to be either very close to the first, or so far as to have no effect on the planet. (not circumbinary).snorkack said:How stringent is the last condition?
Note that even when the stars have a maximum distance rather more than that, they will nevertheless have conjunctions. There are good stability reasons why planet´s orbital plane is likely to be close to the stars´ orbital plane.
Yes, travel thousands of kilometres into a hostile environment.Algr said:Unless they have feet and can walk to where the night is.
Well, we have Kepler-34. The second star is close enough. What it means: B semimajor axis 0,228 AU, eccentricity 0,52, gives maximum distance 0,346 AU. About 52 million km, which is about 65 radii of A.Algr said:I'm thinking that the planet's orbit would destabilize if the two stars were too far apart. So the second star has to be either very close to the first, or so far as to have no effect on the planet. (not circumbinary).