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I just came across this really fun page. What would happen to our solar system if another star came hurtling through it? Well, this page will show you. Give it a try. [img]/phpBB/images/smiles/icon_biggrin.gif[/img]
http://janus.astro.umd.edu/orbits/rstar.html Try these inputs to see something really funny: Start date: Jan. 01, 1990 Show outer planets Star's mass: .5 Closest distance: 5 AU Speed: Average Have fun. And hope it never happens in real life.
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...And that, my liege, is how we know the Earth to be banana-shaped. --Sir Bedevere |
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Great Site, David.
Has anyone been able to get the Earth to become a satellite of the Rogue Star? I've been able to pawn off Venus, but not the Earth. [img]/phpBB/images/smiles/icon_smile.gif[/img] |
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I ran it twice, using David's suggested starting conditions, once at Average and once at Below Average speed, and got different results. That doesn't bother me, of course, I would more or less expect that--except that in the first run, we had Uranus literally bouncing off the Sun! Ran right up to it and bounced as clearly as you could ask.
I somehow suspect that that wouldn't actually happen that way! [img]/phpBB/images/smiles/icon_razz.gif[/img] Anyway, certainly a great site! The (I wonder if it's available as a screen-saver) Curtmudgeon |
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Get rid of all those pesky outer planets; show Jupiter whose its daddy! 2/01/01 Start Outer Planets .4 Solar Masses 2.3 AU closest Above Average Speed
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But I, remembering, pitied well And loved them, who, with lonely light, In empty infinite spaces dwell, Disconsolate. For, all the night, I heard the thin gnat-voices cry, Star to faint star, across the sky. —— Rupert Brooke, |
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Great!
But years ago I had a share-ware program for my Mac that did things like this, only better. I can't run it on this PC and I'd love to find a Windows version. I appeal to anybody; do you know of any simple (free or cheap! ) celestial mechanics programs out there that can let you set up your own system with whatever masses and orbital parameters you choose? I need one as a teaching tool, soon! Any leads appreciated! |
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I tried it with average speed, .5 solar masses and a distance of 1 AU. Earth was history. I then tried it with 5 AU. Earth faired OK but Mars was quite perturbed.
I ran it again with the same parameters to see what happened to the outer planets. All of them except Saturn got kicked out of the system. Saturn ended up in a highly eliptical orbit. Very cool site. |
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I did [img]/phpBB/images/smiles/icon_smile.gif[/img] Really close orbit though... 02-01-2001, 9 masses(!) closest approach 1 AU, Very slow speed... Actually it was an accident I meant to put in .9 masses... [img]/phpBB/images/smiles/icon_razz.gif[/img]
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"Ignorance has caused more calamity than malignity" H.G. Wells "Getting lost is part of exploring." Uniqua in "Backyardigans-Heart of the Jungle" "Trying to wrap my head around creationist astronomy is like trying to ride a unicycle around a Moebius strip: it’s off-balance, physically impossible, full of one-sided arguments, and in the end you don’t go anywhere." Phil Plait |
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Kizarvexis |
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02/01/2001 Inner .1 Solar Masses .1 AU Above Avg Speed Kizarvexis P.S. Then change the speed to average to get a close up view of Mars and Mercury. [img]/phpBB/images/smiles/icon_smile.gif[/img] PPS. Just try all the speeds with .1 mass and .1 AU. You get some really weird and dangerous orbits. <font size=-1>[ This Message was edited by: Kizarvexis on 2002-07-20 07:04 ]</font> <font size=-1>[ This Message was edited by: Kizarvexis on 2002-07-20 07:06 ]</font> |
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I've been playing. [img]/phpBB/images/smiles/icon_smile.gif[/img]
I'm tired of orbiting clockwise around the sun and getting a tan takes too long. Try this. 02/01/2001 Inner .1 mass .2 AU Above Avg Speed Kizarvexis |
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Well I'm glad everybody liked my find. It sure is fun to see what kind of havoc you can inflict upon our system isn't it.
Now, I'm sure the simulation uses real physics, but it's also true that it doesn't take every possible influence into account. For one thing, it's only 2-dimensional and the rogue star must come in along the ecliptical plane. Also, I noticed that if you have a simulation that sends an outer planet into the inner solar system, and then run the same simulation on the inner system, that outer planet doesn't appear, which would probably alter things quite a bit. Now as for the "bouncing Uranus" example I gave above, I was shocked to see it too, which is why I gave that example. My guess is that it's not really bouncing, but just circling the Sun at such a tight perihelion that the scale can't show it, so it looks like a bounce. The same could be said of any simulation where two planets seem to collide. There also seems to be a bug in the system. I can't get any simulation to appear where the star is exactly 1 solar mass. The server is also appallingly slow to connect sometimes. Maybe it sometimes takes a lot of time to process the inputs. So, while it can't be said to be a completely accurate simulation, it sure shows you what kind of effects there would be in such an encounter. And judging from all the possible times I've put in, it looks like most of them would be unpleasant (to understate it terribly). Finally, thanks to roidspop for the system simulator program. I'm going to give it a try.
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...And that, my liege, is how we know the Earth to be banana-shaped. --Sir Bedevere |
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Seems to be a general problem with most simulations in that you like to use the sun as a reference point and therefore have it's position stated as a constant. Hopefully someone will be brave and program the sun to move around as well. Might try it myself at some point, then I can play around with binary system sims....
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I don't think that's a problem. The simulation is given with the Sun as the reference frame, so naturally it stands still. It's not that it isn't affected, just that the "camera" is always centered on it.
In a different frame of reference you'd be seeing the Sun orbiting the rogue star.
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...And that, my liege, is how we know the Earth to be banana-shaped. --Sir Bedevere |
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I think it is a problem. In the case I described, the star performed a perfectly elliptical orbit around the Sun, when they should revolve around a common CG. Then, even if the Sun was a fixed reference, the orbital pattern of the rogue star wouldn´t be that fashion. An astronomy newby would be confused.
Predictably they couldn´t cope with the 3 bodies problem. But i´m not willing to disrepute the simulation, which is very nice indeed. |
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With the following parameters:
Date: 4/28/03 Inner Planets .5 Solar Masses .9 Au Average Speed Mercury gets carried off and orbits the rogue star! ![]()
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"Is that a laser pointer? Well...that's fantastic! I mean...wow..that's just...GREAT!" -Donald Rumsfeld before a Nov. 2001 speech (His enthusiasm was muted, however, when he learned he could not guide a bomb with it.) |
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A question:
The site does not seem to have any parameters to account for the position of the rogue star when it enters the solar system. Just the shortest distance to the Sun. Surely, the effect on the orbits also depends on the direction from which the rogue star approaches the planets! Still a cool simulation, anyway. |
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Jupiter as a ping pong ball?
2/01/2001 Outer Planets 6 Solar Masses 6 AU Average Speed All of the outer planets scatter except Jupiter, which keeps pinging off the Sun!
__________________
"Is that a laser pointer? Well...that's fantastic! I mean...wow..that's just...GREAT!" -Donald Rumsfeld before a Nov. 2001 speech (His enthusiasm was muted, however, when he learned he could not guide a bomb with it.) |
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PANDEMONIUM!!!!!!!
4/28/4003 Outer Planets 100 Solar Masses 20 AU Average Speed WHOA!!!!!!!!!!
__________________
"Is that a laser pointer? Well...that's fantastic! I mean...wow..that's just...GREAT!" -Donald Rumsfeld before a Nov. 2001 speech (His enthusiasm was muted, however, when he learned he could not guide a bomb with it.) |
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