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(meteorobs) News on the lunar Leonids



     A summary of the six confirmed lunar impacts is given in the 
table below.  This is an ASCII plain text table that must be viewed 
with a fixed-space font such as Courier for the columns to line up 
properly.  We are naming these with letters in the order of 
discovery.  The UT date is 1999 November 18.  In each case, the 
events were confirmed on my videotapes made at George Varros' 
backyard in Mount Airy, Maryland, and the timings are from my tapes. 
The previously-reported estimates of the locations of D and E were 
rather far off in longitude, according to measurements of the video 
images made by Ben Wun and me earlier today.

           Accuracy, Approx. Discovered  Selenographic
Name  UTC     sec. Mag1 Mag2    by       Long. Lat. Description
   h  m   s
F  3:05:44.2   0.6   5   9? David Palmer  69W  44N  50km e of Harding
D  3:49:40.40  0.03  3   7  David Palmer  69W   2N   w. wall of Hevelius
E  4:08:04.1   0.6   5   8  David Palmer  77W  15S 120km SW of Rocca
A  4:46:15.2   0.1   3   8  Brian Cudnik  71W  14N  50km ENE of Cardanus
B  5:14:12.93  0.05  7   8  Pedro Sada    58W  15N 200km WNW of Marius
C  5:15:20.23  0.05  4   7  Pedro Sada    59W  21N  75km S Schiaparelli 

Mag1 is the approximate magnitude of the flash estimated from my tape on 
the half-frame on which it first appears.  Mag2 is the estimated 
magnitude a half-frame, or 1/60th second, later.  In all cases 
I can't see any evidence of the flash in the half-frame 1/30th second 
after the first one, except for D, where it seems to appear there at 
about 9th mag.  The selenographic locations should be accurate to within 
about 2 deg. or 50 km, but the locations of F and E could be in error 
more due to foreshortening near the limb and lack of nearby features in the 
Moon images generated with the Occult program used for the location 
determination.  Their locations can be improved by using a grid overlay 
that we plan to generate.  All of these are in the western part of Oceanus 
Procellarum (Ocean of Storms) except D and E, which are in highlands area 
a short distance west of the western shore of Oceanus Procellarum. The 
times of B and C have been determined by Don Stockbauer, Victoria, Texas, 
after creating an accurately time-inserted copy using an IOTA-Manly video 
time inserter.  He also determined the time of A, but for technical 
reasons to less accuracy; it will be possible to refine it later.  D, E, 
and F have been timed from the tape just using a stopwatch. 

     D seems to be the brightest impact.  Besides Palmer's and my 
videotapes, it is also in videotapes by Pedro Sada and by Rick 
Frankenberger in San Antonio, Texas.  My image for the event also shows 
three stars, from north to south (right to left in the image) being 7.6-
mag. SAO 146577, 8.2-mag. SAO 146578, and 8.9-mag. SAO 146574, all of 
whose occultations were recorded a few minutes later.  The first two stars 
are also visible in David Palmer's frame of the D impact.

     Sada reports two more events estimated at about 5th magnitude at 
4:32:50.8 and 4:34:49.7 UTC, but they have not been found in other tapes 
(the field of view of my 5-inch telescope used for the 6 known events was 
aimed at a more southern part of the Moon than usual, so they would have 
been missed if they occurred a little north of the equator).  The 2nd 
event was fairly close to the terminator.  Other possible unconfirmed 
events (some chance of their being videotape defects) were recorded by me 
at 4:50:15.9 UTC and by David Palmer at 2:42:02.

     The images for all six events are at http://iota.jhuapldot edu
That site also has a link to the article about the impacts that was 
published on page 2B of the December 1st Baltimore Sun, 
and the NASA news Web site that has an animation of impact A.
Some of Palmer's images are on the IOTA Web site at 
http://www.lunar-occultations.com/iota

     The mass of the impacting meteoroids, and the resulting craters, has 
still not been resolved.  Mass estimates range from 50 grams to 20 kg, and 
crater sizes from several meters to almost 100 meters, in any case 
probably too small to be visible from earth-based observations.

David Dunham, IOTA, 1999 December 3

Joan and David Dunham
7006 Megan Lane
Greenbelt, MD 20770
(301) 474-4722
dunham@erols.com
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