(meteorobs) Observation September 3/4 2005
Pierre Martin
dob14.5 at sympatico.ca
Thu Sep 29 00:51:32 EDT 2005
This morning session was spent under the *very* dark skies of Algonquin
Provincial Park. By the time the skies cleared, it was very late.
Still, it was a very enjoyable experience to observe meteors under such
a clear, pristine night! The limiting magnitude exceeded 7th
magnitude, M33 was an easy naked eye object and the faint Zodiacal Band
was visible along the ecliptic going north of Mars and between the
Pleiades and Hyades. Low over the north, a faint aurora pulsated ever
so slightly. It was the kind of night one wished it would not end!
In the one hour teff of observing before morning twilight, I recorded
19 meteors. Sporadics were the main activity, but a few Alpha Aurigids
and Antihelions were also seen.
The highlight was at 4:26 EDT with a very nice slow moving mag -2
sporadic. It had a very distinct blue changing to white color and had
a short wake following.
Pierre Martin
Ottawa, Ontario
DATE: September 3/4 2005
BEGIN: 0810 UT (0410 EDT) END: 0920 UT (0520 EDT)
OBSERVER: Pierre Martin (MARPI)
LOCATION: Long: -78 29' West; Lat: 46 01' North Elevation: 1035 ft
City & Province: Brent, Algonquin Park, Ontario, CANADA
RECORDING METHOD: talking clock/tape recorder, plotting & cord align
-----------------------------------------------------------------------
OBSERVED SHOWERS:_____________________________________radiant position
DAU (Delta Aurigids)_____________________________03:36 +46
ANT (anthelions)_________________________________23:44 -02 AUR
(Alpha Aurigids)_____________________________05:48 +42
SPO (random sporadics)
-----------------------------------------------------------------------
OBSERVING PERIODS: 0 = none seen; / = shower not observed
PERIOD(UT)_FIELD____Teff__LM_____SPO_DAU_ANT_AUR
0810-0920__0159+12__1.16__7.12___14___0___2___3 = 19
*Note: SIA/ANT activity combined together
The first column (Period UT) refers to observing periods broken down as
close as possible to one hour of true observing, in Universal Time. The
second column (Field) is the area in in the sky where I centered my
field of view. The third column (TEFF) represents effective observing
time (corrected for breaks or any time I did not spent looking at the
sky). The next column (LM) is the average naked eye limiting
magnitude, determined by triangle star counts. All following columns
indicate the number of meteors for each shower observed.
------------------------
MAGNITUDE DISTRIBUTIONS:
SHOWER
_______-2__-1___0__+1__+2__+3__+4__+5__+6_____AVE
SPO_____1___0___0___0___0___3___5___3___2_____+3.86
AUR_____0___0___0___1___0___1___1___0___0_____+2.66
ANT_____0___0___0___0___0___0___0___1___1_____+5.50
Note: Magnitude scale is to determine the brightness of sky objects.
Magnitude -8 is comparable to a quarter moon, magnitude -4 with the
planet Venus, magnitude -1 with the brightest star Sirius, magnitude +2
to +3 with most average naked eye stars and magnitude +6 to +7 are the
faintest stars the naked eye can see under typical dark conditions. A
meteor of at least magnitude -3 is considered a fireball. The above
table contains the magnitudes from all observed meteors, and the
average (last column) for showers.
------------------------
SKY OBSCURED (FOV): None
F = 1.00
------------------------
Dead time: None
Breaks (UT): None
-------------------------
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