Travels to Discover the Source of the Nile, Volume 4 (of 5): In the years 1768, 1769, 1770, 1771, 1772 and 1773Bruce, James
History
Travels to Discover the Source of the Nile, Volume 4 (of 5): In the years 1768, 1769, 1770, 1771, 1772 and 1773
Bruce, James
Egypt -- Description and travel; Ethiopia -- Description and travel; Ethiopia -- History; Natural history -- Ethiopia; Nile River
No horse, mule, ass, or any beast of burden, will breed, or even live
at Sennaar, or many miles about it. Poultry does not live there.
Neither dog nor cat, sheep nor bullock, can be preserved a season
there. They must go all, every half year, to the sands. Though all
possible care be taken of them, they die in every place where the fat
earth is about the town during the first season of the rains. Two
greyhounds which I brought from Atbara, and the mules which I brought
from Abyssinia, lived only a few weeks after I arrived. They seemed to
have some inward complaint, for nothing appeared outwardly. The dogs
had abundance of water, but I killed one of them from apprehension of
madness. Several kings have tried to keep lions, but no care could
prolong their lives beyond the first rains. Shekh Adelan had two,
which were in great health, being kept with his horses at grass in the
sands but three miles from Sennaar: neither rose, nor any species of
jessamin, grow here; no tree but the lemon flowers near the city, that
ever I saw; the rose has been often tried, but in vain.
Sennaar is in lat. 13° 34´ 36´´ north, and in long. 33° 30´ 30´´
east from the meridian of Greenwich. It is on the west side of the
Nile, and close upon the banks of it. The ground whereon it stands
rises just enough to prevent the river from entering the town, even
in the height of the inundation, when it comes to be even with the
street. Poncet says, that when he was at this city, his companion,
father Brevedent, a Jesuit, an able mathematician, on the 21st of
March 1699, determined the latitude of Sennaar to be 13° 4´ N. the
difference therefore will be about half a degree. The reader however
may implicitly rely upon the situation I have given it, being the
mean result of above fifty observations, made both night and day, on
the most favourable occasions, by a quadrant of three feet radius,
and telescopes of two, and sometimes of three feet focal length, both
reflectors and refractors made by the best masters.
Public-domain text, read in full here on John Shaqi.
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