The mountains to the northeast were silhouetted against the almost
equally dark sky; the forest at their feet was indistinguishable. No
glow or spark of light suggested the presence, anywhere in the scene,
of the men who had escaped nine hours before, though Little and Dennis
strained their eyes looking. Not even a reflection from the river the
doctor believed must be present broke the dark expanse.
The sky offered more material for comment. The Galaxy was lower in
the west and the moon higher. Dennis, looking at the latter, did some
rapid mental arithmetic. It had risen about an hour and a half ago,
and would probably reach the zenith in a little more than another hour.
Its siderial period, then, must be about eight hours, and its distance,
if this world had the same size and mass as Earth, a little over eight
thousand miles from the surface. It was now nearly at "first quarter,"
but its dark side was faintly visible, presumably illuminated by the
reflected light of the planet. Somewhat less than four hours after
sunset, the satellite should enter the planet's shadow and be eclipsed
for about forty minutes, unless its orbit were more highly inclined to
that of the planet than appeared to be the case.
Little was looking at the stars, spread over the sky in unfamiliar
constellations. "Which of these is the local navigation beacon, and how
do you identify it?" he asked. "And why do you pick out one star to
call a beacon?"
"It would be possible to obtain our position from any three stars whose
location is on the charts," answered Dennis, "but it is much easier, as
a rule, to use certain individuals, because tables have been computed
for use with them, and they are easier to identify. I don't have the
tables with me, of course, but the beacon for this neighborhood and
the Galaxy, together, would give me a fairly good idea. We use the
brightest available stars for beacons, naturally--Rigel and Deneb in
the Solar sector, for example. For navigation in the Larger Cloud
we use a slightly different system, which employs two super-giant
stars back in the Galaxy and the one local beacon which covers the
whole Cloud--S Doradus. It shouldn't be hard to find, even without
instruments, since it's a first-magnitude star at a thousand parsecs;
but we always like to check the spectrum, if possible. Most beacon
stars, of course, are O, B, or M supergiants, but there are usually
detectable individual differences which can be picked out by a good
instrument. We haven't a good instrument but fortunately S Doradus has
a very distinctive spectrum."
Little nodded. "I can see that much. Don't tell me how you reduce the
observations to get your position; it would certainly go beyond my
mathematical limit, and I don't like to be shown up."
Public-domain text, read in full here on John Shaqi.
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