(meteorobs) Observation May 24/25 2009
Pierre Martin
dob14.5 at sympatico.ca
Tue Jun 23 00:08:42 EDT 2009
On the Sunday May 24, I returned to Bootland Farm to observe meteors
for two hours, centered on midnight. Sky transparency was very good,
with a limiting mag of 6.6 at the zenith. No mosquitoes, and
comfortably cool temperature.
Meteor rates were a bit better than I expected... In 2.13 hours teff,
I recorded 11 sporadics (six on the first hour, and five in the second).
The highlight came at the very beginning, only seconds into my
watch... a very slow moving yellow sporadic was spotted descending in
the north-east, swelling up to a bright mag 0 with a deep orange
color. Then it dramatically fragmented into two distinct pieces
travelling side-by-side until they both slowly faded away. Wow!
Another memorable meteor came just 9 minutes later, which looked
completely different than the first one. This time it was a very
swift-moving mag 0 streak shot a good 30 degrees across southern
Hercules, leaving behind a 2 seconds train.
Pierre Martin
Ottawa, Ontario
DATE: May 24/25 2009
BEGIN: 02:50 UT (22:50 EDT) END: 05:00 UT (01:00 EDT)
OBSERVER: Pierre Martin (MARPI)
LOCATION: Long: -76 29' West; Lat: 45 23' North Elevation: 400 ft
Observing site: Bootland Farm, Ontario, CANADA
RECORDING METHOD: talking clock/tape recorder, plotting
----------------------------------------------------------
OBSERVED SHOWERS:_______________________________radiant position
ANT (Antihelion)_________________________________17:00 -23
SPO (sporadics)
----------------------------------------------------------
OBSERVING PERIODS: 0 = none seen; / = shower not observed
PERIOD(UT)____FIELD_______Teff____F______LM____SPO_ANT
02:50-03:51___15:42 +12___1.00___1.00___6.55____6___0
03:51-05:00___16:41 +12___1.13___1.00___6.55____5___0
TOTALS:___________________2.13_________________11___0
Note: 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 not spent
looking at the sky). The 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
_____0__+1__+2__+3__+4__+5______AVE
SPO__2___0___1___1___5___2_____+3.18
Note: 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
(IMO definition). The above table contains the magnitudes from all
observed meteors, and the average (last column) for showers.
------------------------
SKY OBSCURED (FOV) (UT): None
------------------------
Dead time: 2.5 min (for plotting)
Breaks (UT): none
More information about the Meteorobs
mailing list