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- Means, when in the previous time of Nemezida was in this position - approximately as equals distances from Centaur and Sun Proxima then the Centaur Proxima should be in other place? For twenty five - fifty millions years the Centaur Proxima would move, after all so? On how many?- On an appreciable share of light year.
- Whether can mean it, what now Nemezida is for the first time simultaneously under the influence of two stars? And before it free moved on the orbit?
- It cannot be, Dzhejnus. Even if to disregard Centaur Proxima, after all there are also other stars. Perhaps, one star has come nearer just now, but in the past on any plots of an orbit close enough there should be other stars. Simply Nemezidy do not have stable orbit.
- But if Nemezida does not address round the Sun that it does here, in the neighbourhood with us?
- That's it, - Judzhinija has told. - What do you mean?
- If Nemezida addressed round the Sun depending on weight of Nemezidy its speed concerning our star would be from eight-ten to hundred metres per second. For a star it is very small speed, therefore it would seem to the observer that it remains at-sight. In that case Nemezida could disappear very long behind a dust cloud, especially if this cloud moves in relation to the Sun in the same direction. Anything surprising that did not notice it till now - almost a fixed star, furthermore hidden by a dust cloud. Not... - Judzhinija has become silent.
Pitt did not begin to show affected interest, therefore has told having sighed:
- Well so that? We will reach sometime an essence?
- And so, if Nemezida does not address round the Sun it moves independently. Then its speed concerning the Sun should be equal approximately to hundred kilometres per second, that is in one thousand times more, than at movement on an orbit. It it has absolutely casually appeared in the neighbourhood with the Sun, but it will come nearer to it, will pass by and never will return. And all this time it will be latent by a dust cloud.
- Why should be so?
- There is only one method to move with a great speed, remaining at the same time motionless for the observer.
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