The moon : $b a full description and map of its principal physical featuresElger, Thomas Gwyn
Science
The moon : $b a full description and map of its principal physical features
Elger, Thomas Gwyn
Moon
The insertion of meridian lines and parallels of latitude at every ten
degrees, and the substitution of names for reference numbers, will add to
the usefulness of the map.
With respect to the text, a large proportion of the objects in the
Catalogue and in the Appendix have been observed and drawn by the author
many times during the last thirty years, and described in _The
Observatory_ and other publications. He has had, besides, the advantage
of consulting excellent sketches by Mr W.H. MAW, F.R.A.S., Dr. SHELDON,
F.R.A.S., Mr. A. MEE, F.R.A.S., Mr. G.P. HALLOWES, F.R.A.S., Dr. SMART,
F.R.A.S., Mr. T. GORDON, F.R.A.S., Mr. G.T. DAVIS, Herr BRENNER, Herr
KRIEGER, Mr. H. CORDER, and other members of the British Astronomical
Association. Through the courtesy of Professor HOLDEN, Director of the
Lick Observatory, and M. PRINZ, of the Royal Observatory of Brussels,
many beautiful photographs and direct photographic enlargements have been
available, as have also the exquisite heliogravures received by the
author from Dr. L. WEINEK, Director of the Imperial Observatory of
Prague, and the admirable examples of the photographic work of MM. PAUL
and PROSPER HENRY of the Paris Observatory, which are occasionally
published in _Knowledge_. The numerous representations of lunar objects
which have appeared from time to time in that storehouse of astronomical
information, _The English Mechanic_, and the invaluable notes in
"Celestial Objects for Common Telescopes," and in various periodicals, by
the late REV. PREBENDARY WEBB, to whom Selenography and Astronomy
generally owe so much, have also been consulted.
As a rule, all the more prominent and important features are described,
though very frequently interesting details are referred to which, from
their minuteness, could not be shown in the map. The measurements (given
in round numbers) are derived in most instances from NEISON'S (Nevill)
"Moon," though occasionally those in the introduction to Schmidt's chart
are adopted.
THOMAS GYWN ELGER.
BEDFORD, 1895.
CONTENTS
INTRODUCTION
MARIA, OR PLAINS, TERMED "SEAS"
RIDGES
RING-MOUNTAINS, CRATERS, &C.
Walled Plains
Mountain Rings
Ring-Plains
Craters
Crater Cones
Craterlets, Crater Pits
MOUNTAIN RANGES, ISOLATED MOUNTAINS, &c.
CLEFTS, OR RILLS
FAULTS
VALLEYS
BRIGHT RAY-SYSTEMS
THE MOON'S ALBEDO, SURFACE BRIGHTNESS, &c.
TEMPERATURE OF THE MOON'S SURFACE
LUNAR OBSERVATION
PROGRESS OF SELENOGRAPHY, LUNAR PHOTOGRAPHY
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