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THE ROYAL ASTRONOMICAL SOCIETY OF CANADA
STANDING COMMITTEE ON OBSERVATIONAL ACTIVITIES
LUNAR SECTION BULLETIN NO.5
Announcement
Upon the recent retirement of the Lunar Co-ordinator, Mr. R.R. Thompson, President
of the Toronto Centre, the writer was asked by Mr. Vent Ramsay, as Chairman of the
National Committee on Observational Activities, to assume this position.
LUNAR ECLIPSE, JUNE 24th, 1964
The first lunar eclipse since the very dark eclipse of December
30th, 1963, has
aroused considerable interest among lunar observers, particularly
those wishing to
ccnpare these two eclipses with the two very dark total lunar
eclipses of 1913.
Unfortunately for observers in Centres west of Windsor, Ontario, totality will be
over when the moon has risen, a few minutes before sunset.
The following is a list of the nine Centres with contacts in each which are pre-
sently cooperating with the National Committee on Lunar Observing; moonrise and sun-
set times are provided in Universal Time (U.T.) for Wednesday, June 24th, 1964:
Centre Contact Moonrise Sunset
Halifax W. L. Orr 00 00 00 04
Quebec Pierre Houde 00 38 00 44
Montreal George Wedge 00 44 00 49
Ottawa W. M. Cameron 00 49 00 53
Kingston Raymond Burns 00 48 00 52
Niagara Falls Frank Campbell 00 55 00 59
Toronto Archie Ostrander 01 00 01 04
Hamilton J. G. Craig 00 59 01 03
Edmonton William Cable 04 06 04 10
U.T.
h. m.
Moon enters penumbra 21 58
Moon enters umbra (1st con.) 23 09
Totality begins (2nd con.) 0 16
(Diagram here.) Middle of eclipse 1 06
Totality ends (3rd con.) 1 57
Moon leaves umbra (4th con.) 3 03
Moon leaves penumbra 4 14
While Halifax is the only Centre which can observe 2nd contact, valuable contribu-
tions can be made by other Centres should they wish to carry out one or more of the
following programmes.
Crater Timing
One of the maze important aspects of this event will be the timing of the passage
of the moon through the earth's shadow. It is recommended that a small team (2 to 3
persons) be organised to time the immersion and emersion of specific craters into, and
out of, the shadow as it crosses the face of the moon. Timing is best accomplished
by radio time signals (CHU Ottawa, 3.330 K.C.). If these are simultaneously recorded
on tape, along with the observer's verbal estimate, a very accurate time determination
is provided, as well as a permanent record. As the official record of these events
consists of the reports of those specifically responsible for timing, it is best to
station them at considerable distance from the others participating. In deciphering
a tape, much confusion can result when the record contains unwanted contributions from
several, people in addition to the comments of the appointed observers.
date:
640612
object:
Lunar5A
description:
Lunar Section Bulletin No. 5 (pg.1)
folder:
Other Bulletins
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