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Melbourne Guy
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So, I think it's possible to place an object in an orbit such that it remains perpetually in the planet's shadow, like in my awesome graphical representation. But is it?
Yes, this is possible if you place the object in the L2 Lagrange point. However, depending on the masses and sizes of the involved bodies, L2 may lie in the umbra or antumbra. If it is the latter, then it will not be perfectly shadowed as, seen from the Lagrange point, the star will cover a larger part of the sky than the planet. For the Sun-Earth system, it is a borderline case if I recall correctly.Melbourne Guy said:So, I think it's possible to place an object in an orbit such that it remains perpetually in the planet's shadow, like in my awesome graphical representation. But is it?
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Not all the colonies in my novel are planet-based, @Algr, and especially the early ones, which were just inflated habitats to lay claim to the star system. For instance, in late 2204, Proxima Development Corp. inflated a hab around Proxima Centauri and shuttle staff back and forth to substantiate their claim to the system. Minter and Hogan did the same around Gliese 1061 d, with 200 staff rotated on a six-monthly basis.Algr said:Well the planet of such a small star would be tidally locked. So why not put the colony on the planet's night side surface? (Of course you have drawn a jovian there, so that might answer my question.)
Thanks @Orodruin, that could lead to some spectacular mishaps, esp. in the early years of colonisation, I'll have some fun with that.Orodruin said:Also note that the L2 Lagrange point is unstable. In order to maintain the orbit you will need to regularly correct it.
It sounded like Melbourne Guy was describing something different then a Lagrange point. This idea can only work for planets that orbit very close to their stars. If a planet orbits its star in five days, and the station orbits the planet in five days, then the orbit could be timed such that the planet was always between the sun and the station. (Or indeed at any other angle desired.)Orodruin said:Yes, this is possible if you place the object in the L2 Lagrange point.
No, by definition of the description in the OP, what is required is a point that is stationary in the corotating frame of the star-planet system and that by definition is a Lagrange point.Algr said:It sounded like Melbourne Guy was describing something different then a Lagrange point. This idea can only work for planets that orbit very close to their stars. If a planet orbits its star in five days, and the station orbits the planet in five days, then the orbit could be timed such that the planet was always between the sun and the station. (Or indeed at any other angle desired.)
Any civilization advanced enough to know how to construct an orbital colony will likely be aware that L2 is unstable. The plot twist could likely only be some sort of technical failure of the propulsion system intended to keep the station at L2.Melbourne Guy said:Thanks @Orodruin, that could lead to some spectacular mishaps, esp. in the early years of colonisation, I'll have some fun with that.
That's exactly the type of thing that sprung to mindOrodruin said:The plot twist could likely only be some sort of technical failure of the propulsion system intended to keep the station at L2.
Algr said:It sounded like @Melbourne Guy was describing something different then a Lagrange point.
I'm going to have to work out a Lagrange point and see if it fits, because my initial understanding is not enough to confirm (or deny) @Algr's observation. Certainly, I want the station hidden from the star at all times, but as an orbit, not having to continually fire the thrusters.Orodruin said:No, by definition of the description in the OP, what is required is a point that is stationary in the corotating frame of the star-planet system and that by definition is a .
There is nothing to confirm. For any two body system in circular orbit, there are exactly five stationary points for a test particle in the corotating frame, which your setup would require it to be. These stationary points are the Lagrange points L1-L5 and out of those only L2 satisfies your requirement of having the lighter of the two bodies in between the larger and the Lagrange point. There simply are no other such solutions.Melbourne Guy said:I'm going to have to work out a Lagrange point and see if it fits, because my initial understanding is not enough to confirm (or deny) @Algr's observation.
Why do PF forum people do this? We just described a solution and you just ignore it and declare that there isn't one. If it's wrong, at least make some effort to say why.Orodruin said:There simply are no other such solutions.
I did say why:Algr said:Why do PF forum people do this? We just described a solution and you just ignore it and declare that there isn't one. If it's wrong, at least make some effort to say why.
What we are describing is a special case that would not work on Earth, do you understand that part?
Orodruin said:For any two body system in circular orbit, there are exactly five stationary points for a test particle in the corotating frame, which your setup would require it to be. These stationary points are the Lagrange points L1-L5 and out of those only L2 satisfies your requirement of having the lighter of the two bodies in between the larger and the Lagrange point.
That's definitely one option,@hmmm27, but not necessarily the easiest for the first interstellar colonies. Inflating a habitat in orbit is simpler than having to land - even on an airless planet - and the first FTL craft are rudimentary, so it takes a while before 'on the ground' (or in the ground, I guess) bases are built.hmmm27 said:Find a tide-locked moon and dig a pit.
Phobos has a neat divot that always almost-directly faces Mars.
It is possible to hide an orbital colony behind a planet from a flare star by strategically positioning the planet between the colony and the star. This will block the direct radiation and heat from the flare star, providing some protection for the colony.
No, not all planets are suitable for hiding an orbital colony from a flare star. The planet must have a suitable atmosphere and magnetic field to deflect the harmful radiation and heat from the flare star.
The length of time an orbital colony can remain hidden behind a planet from a flare star depends on the intensity and frequency of the flares. However, with proper shielding and precautions, it is possible for an orbital colony to remain hidden for extended periods of time.
While hiding an orbital colony behind a planet from a flare star can provide some protection, there are still potential risks. The planet may not provide enough shielding, and the colony may still be exposed to some radiation and heat. Additionally, the orbital colony may face other challenges such as limited resources and communication during the hiding period.
Yes, there are alternative methods for protecting an orbital colony from a flare star. These include building the colony underground or using advanced shielding materials. However, these methods may be more costly and may not be suitable for all situations.