Essays: Scientific, Political, & Speculative; Vol. 1 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.Spencer, Herbert
Philosophy
Essays: Scientific, Political, & Speculative; Vol. 1 of 3: Library Edition (1891), Containing Seven Essays not before Republished, and Various other Additions.
Spencer, Herbert
Philosophy; Political science; Science
In this confused sentence there is implied a belief, that the distances
of the nebulæ from our galaxy of stars as much transcend the distances
of our stars from one another, as these interstellar distances transcend
the dimensions of our planetary system. Just as the diameter of the
Earth's orbit, is a mere point when compared with the distance of our
Sun from Sirius; so is the distance of our Sun from Sirius, a mere point
when compared with the distance of our galaxy from those far-removed
galaxies constituting nebulæ. Observe the consequences of this
assumption.
If one of these supposed galaxies is so remote that its distance dwarfs
our interstellar spaces into points, and therefore makes the dimensions
of our whole sidereal system relatively insignificant; does it not
inevitably follow that the telescopic power required to resolve this
remote galaxy into stars, must be incomparably greater than the
telescopic power required to resolve the whole of our own galaxy into
stars? Is it not certain that an instrument which can just exhibit with
clearness the most distant stars of our own cluster, must be utterly
unable to separate one of these remote clusters into stars? What, then,
are we to think when we find that the same instrument which decomposes
hosts of nebulæ into stars, _fails_ to resolve completely our own Milky
Way? Take a homely comparison. Suppose a man who was surrounded by a
swarm of bees, extending, as they sometimes do, so high in the air as to
render some of the individual bees almost invisible, were to declare
that a certain spot on the horizon was a swarm of bees; and that he knew
it because he could see the bees as separate specks. Incredible as the
assertion would be, it would not exceed in incredibility this which we
are criticising. Reduce the dimensions to figures, and the absurdity
becomes still more palpable. In round numbers, the distance of Sirius
from the Earth is half a million times the distance of the Earth from
the Sun; and, according to the hypothesis, the distance of a nebula is
something like half a million times the distance of Sirius. Now, our own
"starry island, or nebula," as Humboldt calls it, "forms a lens-shaped,
flattened, and everywhere detached stratum, whose major axis is
estimated at seven or eight hundred, and its minor axis at a hundred and
fifty times the distance of Sirius from the Earth."[11] And since it is
concluded that the Solar System is near the centre of this aggregation,
it follows that our distance from the remotest parts of it is some four
hundred distances of Sirius. But the stars forming these remotest parts
are not individually visible, even through telescopes of the highest
power. How, then, can such telescopes make individually visible the
stars of a nebula which is half a million times the distance of Sirius?
The implication is, that a star rendered invisible by distance becomes
visible if taken twelve hundred times further off! Shall we accept this
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account