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(meteorobs) Comet Comments, March 1998



Greetings!

I had forwarded the following to Lew and some others.... he suggested that,
although slightly off the meteor topic.... that I forward it to the
list..... enjoy!

.........

Below are the Comet Comments from Don Machholz for March.... Don't miss all
the notes after the elements... they are interesting reading!

As an aside here, when he talks about only 4 in recent times found by
accident... Comet Kobayashi-Berger-Milon was also found independently by a
friend of mine in town here, Art Fraser... and several of us helped him
confirm it.... but he was number #4.. and they only take the first 3 names
:(  There are several other Canadian comet discoverers who live in Ottawa...
Rolf Meier, whose place I observe from, who has 4 to his name, and Doug
George, who has his name on Skorichenko-George.

Just some ramblings over morning coffee...

- Cathy
  Great White North
  (Ottawa, Canada)


From: DonM353259@aol.com
Date: Sun, 8 Feb 1998 02:17:28 EST
To: kronkg@medicine.wustldot edu, bbs.ssolar@astro.gea.cesca.es,
        mbh@el94.sawbdot gov.za, 37STAR@newton.phys.sci.chula.ac.th,
        JMaloney7@aol.com, chuckh@starlink.com, JRSanf@aol.com,
        jbryant@extro.ucc.su.oz.au, denis@kisa.iki.rssi.ru,
        Trobert@earthlinkdot net, JBortle@aol.com, ratcliffem@clpgh.org,
        andromed@atm.daldot ca, dave@bas.powernet.codot uk, chall@cyberusdot ca,
        comet.ace@zianet.com, drpaul@humboldt1.com, gc4959@idot bekkoame.or.jp,
        harincar@camworks.com, Musante@ecs.umassdot edu, NTZT04A@prodigy.com,
        DonM353259@aol.com
Subject: CC for March


COMET COMMENTS FOR MARCH 1998 By Don Machholz

   Only a couple of comets remain in our sky this month. Comet Hale-Bopp
   fades in our southern sky. Comet Meunier-Dupouy travels through our
   morning northern sky. The only new finds this past month was by the SOHO
   satellite, which monitors the solar vicinity. It discovered four more
   comets, it has now found forty in less than two years. Like most of the
   others, these four comets disappeared after going behind the sun.
   COMET HUNTING NOTES: Forty-eight of the last 100 visual comet
   discoveries were made by amateurs using reflectors. They range in size
   from 4" to 19.5". The most popular size (16" aperture) was used in 16
   finds. They were also efficient, averaging 231 hours per find compared
   with 391 hours for all visual comet discoveries. All five accidental
   comet discoveries (Berger, Milon, Hale, Bopp and Tillbrook) were made
   with reflector telescopes.
   
                                 EPHEMERIDES
                                       
                        C/1997 J2 (Meunier-Dupouy)
  
   Date(00UT)    R.A. (2000)    Dec     El   Sky   Mag
   02-11        20h43.9m      +34o38'   50o   M    11.6
   02-16        20h52.3m      +34o08'   49o   M    11.6
   02-21        21h00.3m      +33o41'   48o   M    11.6
   02-26        21h08.1m      +33o17'   47o   M    11.7
   03-03        21h15.5m      +32o56'   46o   M    11.7
   03-08        21h22.7m      +32o37'   46o   M    11.7
   03-13        21h29.5m      +32o21'   46o   M    11.7
   03-18        21h36.0m      +32o07'   46o   M    11.7
   03-23        21h42.2m      +31o54'   46o   M    11.7
   03-28        21h48.0m      +31o44'   47o   M    11.7
   04-02        21h53.6m      +31o35'   48o   M    11.7
   04-07        21h58.8m      +31o27'   50o   M    11.7
  
                       C/1995 O1 (Hale-Bopp) 
   
   Date(00UT)    R.A. (2000)    Dec     El   Sky   Mag
   02-11        05h03.3m      -60o33'   88o   E    8.5
   02-16        04h59.8m      -59o45'   87o   E    8.6
   02-21        04h57.3m      -58o57'   86o   E    8.7
   02-26        04h55.6m      -58o08'   85o   E    8.8
   03-03        04h54.7m      -57o20'   84o   E    8.9
   03-08        04h54.6m      -56o33'   83o   E    9.0
   03-13        04h55.1m      -55o48'   82o   E    9.0
   03-18        04h56.2m      -55o04'   82o   E    9.1
   03-23        04h57.8m      -54o22'   81o   E    9.2
   03-28        04h59.9m      -53o43'   80o   E    9.3
   04-02        05h02.4m      -53o06'   79o   E    9.3
   04-07        05h05.3m      -52o32'   78o   E    9.4
   
  
                        55P/Tempel-Tuttle
  
   Date(00UT)    R.A. (2000)    Dec    El    Sky   Mag
   03-03        01h13.2m      +08o27'  38o    E    10.7
   03-08        01h12.7m      +07o01'  32o    E    11.0
   03-13        01h12.3m      +05o46'  27o    E    11.3
  

                                   ELEMENTS
                                       
   Object:            Hale-Bopp            Meunier-Dupouy     Tempel-Tuttle
   Peri. Date:        1997 04 01.1347      1998 03 10.4365    1998 02 28.1034
   Peri. Dist (AU):   0.914008 AU          3.051015 AU        0.976639 AU
   Arg/Peri (2000):   130.5787 deg.        122.6755 deg.      172.4930 deg.
   Asc. Node (2000):  282.4653 deg.        148.8429 deg.      235.256  deg.
   Incl (2000):       089.4268 deg.        091.2731 deg.      162.4861 deg.
   Eccen:             0.995085             1.000760           0.905507
   Orbital Period:    ~2500 years          Long Period        33.23 years
   Ref:               MPC 30738            MPC 30738          MPC 30244
   Epoch:             1997 12018           1998 03 08         1997 12 18
   Absol. Mag/"n":    -1.0/4.0             4.0/4.0            10.0/10.0
   
  
   Don's Comet Hunting Hours
   Comet Hunting Hours 1975-1997: 6277.25
   Hours through Jan. 1998: 7.25
   Total hours at last discovery (10-8-94): 5589.00
   Least hours in any month since I began comet hunting on 1/1/75: 4.50
(01/86), 
   5.50 (02/80)
   Most hours in any month since I began comet hunting: 69.25 (05/76), 63.00 
   (05/78)
  
   COMET HUNTING NOTES FROM JULY 1997: Of the 97 visual comet discovery
   events since 1/1/75-during which 73 comets were found and named- only
   four times was the comet found by accident. In early July 1975 Doug
   Berger and the late Dennis Milon found a comet while observing M 2. It
   had been found the previous day by a comet hunter (Toru Kobayashi of
   Japan). Then, twenty years later Alan Hale and Thomas Bopp chanced upon
   a new comet near M 70.
  
   COMET HUNTING NOTES FROM AUGUST 1977: With Tabur's find, six of the last
   seven visually-discovered comets have been found south of the celestial
   equator; and 14 of the last 17 visually-discovered comets have been
   found in the morning sky.
   
   COMET HUNTING NOTES FROM SEPT. 1997: Many people quote the 1700 hours it
   took me to find my first comet or the 1742 hours to find my second.This
   has been surpassed twice in recent years. In 1987 Noboru Nishikawa took
   3024 hours in 2389 sessions to find his first comet (1987a). In 1990
   Yuji Nakamura discovered his first comet after searching 2236.5 hours in
   1558 sessions.
   
   COMET HUNTING NOTES FROM OCT. 1997: With so many comets from the Kreutz
   Sungrazing Group being discovered by the SOHO satellite, amateurs have
   taken a renewed interest in sweeping along the path by which these
   comets are arriving. That path is now in the morning sky, having been
   behind the sun this past summer. The comets are very faint in the weeks
   before perihelion and it may take CCD imaging to capture them. The
   brightest members, although rare, can still be discovered visually.
  
   COMET HUNTING NOTES FROM NOV. 1997: Since the first day of 1975, 76
   comets have been visually discovered. Some have been discovered by more
   than one person: ten by two visual discoverers and seven by three. This
   amounts to 100 visual discovery events.
   Thirty-two of those 76 comets were found in the evening sky with 44
   found in the morning sky.
   Additionally, 42 were found in the north of the celestial equator with
   34 found south. All of the 23 comets found by observers living south of
   the equator were found in the southern celestial sky. Northern
   Hemisphere observers found comets both north and south of the equator.
  
   COMET HUNTING NOTES FROM DEC. 1997: Since January 1975, 48 different
   individuals have visually discovered comets that now carry their names.
   What countries do they live in? Twenty-three are in Japan, nine reside
   in the USA, with four in Australia.
   Other countries represented are the old USSR, Canada, England, South
   Africa, Philippines, Italy, New Zealand and Norway. The most discovery
   events occurred in Japan (33) followed by the USA (30) and Australia
   (19).
   
   COMET HUNTING NOTES FROM JAN. 1998: Of the last 100 visual comet
   discoveries, 28 were made by amateurs using binoculars. The smallest
   pair of binoculars used was 7x35's by William Bradfield in 1980 to find
   a magnitude-six comet. Three were the 80mm size while six finds were
   made using binoculars with objectives of 110-120 mm. Four finds were
   made with my homemade binoculars (130mm). And half (14) of all binocular
   comet discoveries were made with 150mm (6-inch) binoculars.
  
   COMET HUNTING NOTES FROM FEB. 1998: Of the last 100 visual comet
   discoveries, 23 were made by amateurs using refractor telescopes. The
   smallest was Genichi Araki's 3" scope to find Comet IRAS-Araki-Alcock.
   Toshio Haneda used a 3.3" refractor to find his comet and three other
   instruments were from 4.8 to 5.2 inches in diameter. The remaining 18
   refractors were 6" in size, with William Bradfield finding 12 comets
   since 1975 (and two before) with his 6" telescope.  
   
   
             Notes To Help You Make Better Use Of Comet Comments
                               by Don Machholz
                                       
   
   Each issue of Comet Comments is written three weeks before the "due"
   date, giving time for it to be distributed to the editors and placed
   into the newsletters. Comet Comments contains information about new
   comet discoveries. This is followed by comet news and observing tips for
   the comets currently visible. Next I provide ephemerides (predicted
   positions) for bright comets (usually all those brighter than magnitude
   11) so that amateurs can find them. This is how to read these tables:
   Date: This is the Universal Time for the comet's position. The positions
   are for 00 hr UT. The United States is a few hours earlier than this, so
   for a comet viewable in the evening, look for it on the night preceding
   the indicated date. For morning viewing the comet has already passed the
   position indicated for 00hr UT position, so the comet has passed that
   point and moved on.
   RA. and Dec: Right Ascension and Declination in 2000 equinox
   coordinates. These can be plotted on a star chart and found by
   star-hopping, or by using setting circles.
   El: The elongation of the comet- the number of degrees it is from the
   sun as seen from the earth.
   Sky: Morning (M) or evening (E) sky.
   Mag: The predicted magnitude or brightness of the comet. The brightness
   of a comet is difficult to predict so this is only a guess based upon
   past performance and comet theory.
   The last item I include is the elements of the orbits. This information
   can be entered into most comet orbit computer programs to further
   project the comet's positions.
   Peri. Date: The date the comet is closest to the sun. Year is followed
   by month and day.
   Peri. Dist: The distance from the comet to the sun at perihelion in
   Astronomical Units.
   Arg/Peri, Asc. Node, Incl: These define the angle of the comet's orbit.
   The Arg/Peri is the Argument of the Perihelion; if this figure is under
   180 the comet reaches perihelion north of the ecliptic. The Asc. Node is
   the Ascending Node. The Incl is the inclination of the comet's orbit.If
   it is under 90 degrees indicates the comet is in a direct orbit, while
   over 90 degrees means it is in a retrograde orbit.
   Eccen: This is the shape of the orbit. A "1.00" is a parabola, while
   "0.00" is a circle. An eccentricity of greater than 1 is a hyperbola
   orbit-the comet will never return.
   Orbital Period: The length of time it takes for the comet to orbit the
   sun.
   Ref: The source giving the elements. MPC indicates Minor Planet
   Circulars by the Smithsonian.
   Epoch: The time for which the orbit is most accurate. The orbit is
   generally accurate enough for visual location of the comet for several
   months on either side of this date.
   Absol. Mag/"n": This is the absolute magnitude- the brightness of the
   comet if it were 1 AU from both the earth and the sun. The average comet
   is about 7.0.
   The "n" value is the rate of brightening as the comet nears the sun, or
   dimming as it leaves the sun. The average is 4.0. The "n" value
   presented here may have to be multiplied by 2.5 to enter into some
   computers.