[net.space] Halley/Hartley-Good Comet Hunting

SECRIST%OAK.SAINET.MFENET@LLL-MFE.ARPA (01/30/86)

Date:    Wed, 29-JAN-1986 23:50 EST
To:      Space@Angband.Arpa
Message-ID: <[OAK.SAINET.MFENET].0A836F20.008E9C6C.SECRIST>
Quote: "May your future be limited only by your dreams." -- Christa McAuliffe
Organization: Science Applications Int'l. Corp., Oak Ridge, Tenn.
CompuServe-ID: [71636,52]
X-VMS-Mail-To: ARPA%"Space@Angband.Arpa"

From the East Coast Forth Board  (affiliated with the Potomac Forth Interest 
Group, Jerry Shifrin, SYSOP).  The following text has been edited from the
original sources indicated.

-=<***>=-

Francis R. Scobee
Michael Smith
Ronald E. McNair
Ellison S. Onizuka
Judith Resnik
Gregory Jarvis
Sharon Christa McAuliffe

Let each of us carry on their mission in our hearts and souls 
that humankind may one day share the heavens with them.

Richard Secrist
SECRIST%OAK.SAInet.MFEnet@LLL-MFE.Arpa


-----------------------------------------------------------------------------
                                                                                
                * * *   H A L L E Y   F A C T S   * * *
        by Morrison, & Cole, c/o STAR-NET at (305) 639-0715 by modem

                               INTRODUCTION

Halley's  [rhymes  with "valleys"] Comet is composed  of  a  small,  bright 
nucleus  (probably 1-3 km across),  surrounded by a much larger fuzzy head, 
or "coma" (Latin for "hair"),  10 000 to 1 000 000 km across, and a fainter 
gas (mainly carbon monoxide and nitrogen) and dust tail streaming away from 
the head.   Only the nucleus,  composed of ice, dust, and stones mixed with 
frozen  gases,  is  solid.   The total mass of the comet  is  approximately 
65,000,000 metric tons.

                               WHERE IS IT?

This  month  the comet continues moving west and south,  dipping below  the 
Great  Square  of  Pegasus,  through the  Circlet  of  Pisces,  and  toward 
Aquarius.  It will brighten rapidly, from 6.4 at the beginning of the month 
to  5.9  at the end.   The comet will transit the north-south  meridian  at 
about  18:00  and  be about 50 degrees above the southern  horizon  (at  40 
degrees  north latitude).   Note that this position and time mean that  the 
comet  is  moving  into  the sunset region of  the  sky,  and  will  become 
progressively washed out by the sunlight until its re-appearance in Spring.


                         COMET DATA FOR MID MONTH

        Right Ascension:  03 hours 49.02 minutes                        
        Declination:      23 degress 17.652 minutes (near Gamma Piscium)
        Distance:         122 982 530 km from Earth                     
        Magnitude:        6.2                                           
        Velocity:         32.31 km/s                                    


                            OBSERVING THE COMET

During this month's moon-free "window" (1st to 15th),  the comet should  be 
bright enough to spot easily in binoculars and finderscopes.  It is several 
arc  minutes across,  with a condensed nucleus and a small tail,  which  is 
generally   oriented  away  from  Earth  (hidden  mostly  - until  Spring).  
Binoculars  (7x35,  7x50,  or 10x50) will be perfect for an  overall  view.  
They're portable, light, relatively inexpensive, and offer good light grasp 
and ease in locating faint celestial objects like Halley's Comet.  Although 
telescopes  may reveal subtle details in the head,  they aren't  wide-angle 
instruments.  Binoculars will be required to encompass the comet's tail.


                          PHOTOGRAPHING THE COMET

The  simplest  way to photograph the comet is to use a tripod and a  35  mm 
camera  with  a  cable release.   Aim the camera and  focus  the  lens  for 
infinity.  A 30-second exposure will record bright stars and show the comet 
as a non-stellar ball with a fuzzy tail.  Exposures of more than 60-seconds 
will  record dimmer stars,  but show trailed images of stars and the comet.  
Choose a 28 to 50 mm lens (for adequate sky coverage) with a focal ratio of 
f/4 or faster (for a brighter image).   Tracking by mounting a camera  with 
normal  or 135mm lens "piggyback" atop a motor-driven telescope is the only 
way  to manage longer exposures.   For best results,  use FUJICHROME  color 
slide  film  with marked ISO (ASA) value of 400.    Ektachrome is a  second 
choice,  due to real speed falling off in time exposures like these: marked 
values of speed are NO indicator past 60 second exposures!!


                                NEXT MONTH

During  January  the comet moves into the barren star  field  of  Aquarius, 
which  rapidly  sinks into evening twilight during the  month.   It  should 
enter  dim  naked-eye visibility (5th magnitude) and be visible  relatively 
easily in binoculars or a finder telescope.  The moon-free observing window 
will be the 1st to the 15th.


                EPHEMERIS FOR COMET HALLEY STARTING 11/20/1986
                Courtesy of STAR-NET at (305) 639-0715 by modem

Comparing  this current info to the tables that follow for April shows that 
brightness (low value of "magntude") is part of the rationale for the  best 
expectations for seeing to occur in the Spring.  A difference of 1.0 in mag 
is a brightness ratio of 2.5,  or more than one camera F stop.  Only a more 
detailed  examination  of the coordinate data will show those not  familiar 
with  celestial charts that the comet is getting too close to the  sun  now 
(contrast dies due to sun's glare),  and will be too low on the horizon for 
viewing from points in the USA when it re-appears in Spring.  In April from 
the  Florida  Keys,  the  comet will be within about 30 degrees  above  the 
horizon, which is the region where atmospherics severely limit contrast and 
definition  of  celestial  objects.

    PAGE  1     DAYS FROM    COORDINATES:        DISTANCES (AU):  PREDICTED
       DATE     PERIHELION    RA       DEC        SUN    EARTH    MAGNITUDE
    +----+----+----+----+----+----+----+----+----+----+----+----+----+----+
     1/ 1/86       -40       22:15   -02:35       1.00   1.18        5.3 
     1/ 2/86       -39       22:13   -02:49       0.99   1.20        5.3 
     1/ 3/86       -38       22:11   -03:02       0.97   1.22        5.2 
     1/ 4/86       -37       22:08   -03:15       0.96   1.24        5.2 
     1/ 5/86       -36       22:06   -03:28       0.94   1.26        5.2 
     1/ 6/86       -35       22:04   -03:41       0.93   1.28        5.1 
     1/ 7/86       -34       22:02   -03:53       0.91   1.29        5.1 
     1/ 8/86       -33       22:00   -04:04       0.90   1.31        5 
     1/ 9/86       -32       21:58   -04:16       0.88   1.33        5 
     1/10/86       -31       21:56   -04:27       0.87   1.35        4.9 
     1/11/86       -30       21:54   -04:39       0.85   1.37        4.9 
     1/12/86       -29       21:53   -04:50       0.84   1.39        4.8 
     1/13/86       -28       21:51   -05:01       0.83   1.41        4.8 
     1/14/86       -27       21:49   -05:11       0.81   1.42        4.7 
     1/15/86       -26       21:47   -05:22       0.80   1.44        4.6 
     1/16/86       -25       21:45   -05:33       0.78   1.46        4.6 
     1/17/86       -24       21:44   -05:42       0.77   1.47        4.5 
     1/18/86       -23       21:42   -05:53       0.76   1.49        4.5 
     1/19/86       -22       21:40   -06:04       0.74   1.50        4.4 
     1/20/86       -21       21:38   -06:15       0.73   1.52        4.4 

Note: the coordinates RA & DEC are celestial coordinates that designate the 
position  in the sky relative to the star field,  not your position on  the 
earth.   Use  them  by comparison to the coordinates of something  you  can 
recognize.   The charts in Sky & Telescope magazine are exellent references 
to  aid  in locating things (Sky & Tel's $18 is included in  $20  dues  for 
membership  in  the  Central FL Astronomical Society,  Inc.  - if  you  are 
interested:  contact CFAS or Star-Net by sending a note to Chuck Cole).

Comparing  this info to the tables above for December or January shows that 
brightness (low value of "magntude") is part of the rationale for the  best 
expectations  for seeing to occur in the Spring and further South than  the 
Florida Keys.   A difference of 1.0 in mag is a brightness ratio of 2.5, or 
more  than  one camera F stop.   Only a more detailed  examination  of  the 
coordinate data will show those not familiar with celestial charts that the 
comet  will be too low on the horizon for decent viewing from points in the 
USA  when it re-appears in Spring.   In April from the  Florida  Keys,  the 
comet  will  be  within about 30 degrees above the horizon,  which  is  the 
region  where  atmospherics  severely  limit  contrast  and  definition  of 
celestial  objects.   

    PAGE  1     DAYS FROM    COORDINATES:        DISTANCES (AU):  PREDICTED
       DATE     PERIHELION    RA       DEC        SUN    EARTH    MAGNITUDE
   +----+----+----+----+----+----+----+----+----+----+----+----+----+----+
     3/ 1/86        19       20:27   -16:21       0.73   1.26        3.5 
     3/ 2/86        20       20:25   -16:43       0.74   1.24        3.5 
     3/ 3/86        21       20:23   -17:06       0.75   1.21        3.5 
     3/ 4/86        22       20:22   -17:29       0.77   1.19        3.5 
     3/ 5/86        23       20:20   -17:51       0.78   1.17        3.6 
     3/ 6/86        24       20:18   -18:15       0.79   1.14        3.5 
     3/ 7/86        25       20:16   -18:41       0.81   1.12        3.6 
     3/ 8/86        26       20:14   -19:07       0.82   1.10        3.6 
     3/ 9/86        27       20:12   -19:34       0.83   1.07        3.6 
     3/10/86        28       20:10   -20:02       0.85   1.05        3.6 
     3/11/86        29       20:08   -20:32       0.86   1.02        3.6 
     3/12/86        30       20:06   -21:02       0.88   1.00        3.6 
     3/13/86        31       20:03   -21:34       0.89   0.97        3.6 
     3/14/86        32       20:01   -22:08       0.91   0.95        3.6 
     3/15/86        33       19:58   -22:43       0.92   0.92        3.6 
     3/16/86        34       19:55   -23:20       0.94   0.90        3.6 
     3/17/86        35       19:52   -23:59       0.95   0.87        3.6 
     3/18/86        36       19:49   -24:40       0.97   0.85        3.6 
     3/19/86        37       19:46   -25:23       0.98   0.82        3.6 
     3/20/86        38       19:42   -26:09       1.00   0.79        3.5 
     3/21/86        39       19:38   -26:57       1.01   0.77        3.5 
     3/22/86        40       19:34   -27:48       1.03   0.74        3.5 
     3/23/86        41       19:29   -28:42       1.04   0.72        3.5 
     3/24/86        42       19:24   -29:40       1.06   0.69        3.4 
     3/25/86        43       19:18   -30:41       1.07   0.67        3.4 
     3/26/86        44       19:12   -31:46       1.09   0.64        3.4 
     3/27/86        45       19:05   -32:54       1.11   0.62        3.4 
     3/28/86        46       18:58   -34:06       1.12   0.59        3.3 
     3/29/86        47       18:49   -35:22       1.14   0.57        3.3 
     3/30/86        48       18:39   -36:42       1.15   0.54        3.2 
     3/31/86        49       18:29   -37:00       1.17   0.52        3.1 
     4/ 1/86        50       18:17   -39:24       1.18   0.50        3.1 
     4/ 2/86        51       18:04   -40:49       1.20   0.48        3.1 
     4/ 3/86        52       17:48   -42:13       1.21   0.46        3 
     4/ 4/86        53       17:31   -43:35       1.23   0.44        3 
     4/ 5/86        54       17:12   -44:50       1.24   0.42        2.9 
     4/ 6/86        55       16:50   -45:56       1.26   0.41        2.9 
     4/ 7/86        56       16:27   -46:47       1.28   0.39        2.8 
     4/ 8/86        57       16:02   -47:21       1.29   0.38        2.8 
     4/ 9/86        58       15:36   -47:33       1.31   0.37        2.8 
     4/10/86        59       15:09   -47:22       1.32   0.37        2.8 
     4/11/86        60       14:42   -46:46       1.34   0.36        2.8 
     4/12/86        61       14:16   -45:48       1.35   0.36        2.8 
     4/13/86        62       13:52   -44:29       1.37   0.37        2.9 
     4/14/86        63       13:30   -42:55       1.38   0.37        3 
     4/15/86        64       13:10   -41:10       1.40   0.38        3.1 
     4/16/86        65       12:51   -39:18       1.41   0.40        3.2 
     4/17/86        66       12:35   -37:23       1.43   0.41        3.3 
     4/18/86        67       12:21   -35:28       1.44   0.43        3.5 
     4/19/86        68       12:08   -33:35       1.46   0.45        3.6 
     4/20/86        69       11:57   -31:46       1.47   0.47        3.7 
     4/21/86        70       11:48   -30:03       1.49   0.49        3.8 
     4/22/86        71       11:39   -28:24       1.50   0.51        4 
     4/23/86        72       11:31   -26:52       1.52   0.54        4.1 
     4/24/86        73       11:24   -25:25       1.53   0.56        4.2 
     4/25/86        74       11:18   -24:05       1.55   0.59        4.4 
     4/26/86        75       11:13   -22:49       1.56   0.62        4.5 
     4/27/86        76       11:08   -21:39       1.58   0.65        4.6 
     4/28/86        77       11:03   -20:34       1.59   0.68        4.8 
     4/29/86        78       10:59   -19:33       1.61   0.71        4.9 
     4/30/86        79       10:56   -18:37       1.62   0.74        5 
     5/ 1/86        80       10:53   -17:44       1.64   0.77        5.1 



        Courtesy of Greg Walz-Chojnacki c/o STAR-NET @ (305) 639-0715 by modem
                        Comet HARTLEY-GOOD, from STAR-NET

     Here is the latest information on Comet Hartley Good from the  Central 
Bureau  for Astronomical Telegrams.  Note,  by the way,  that this comet is 
more  spectacular than Halley's through early January,  due to placement in 
the  sky.   The  designation of Comet Hartley-Good  is  1985l.  Any  future 
uploads  to STAR-NET on this comet will be named 1985l.DCx (where x is  the 
version, starting with 3) to reflect a nomenclature correction.

     The comet is moving swiftly west toward the Sun.   While the comet  is 
expected  to  attain  reach  a total maginitude of  6.6,  when  it  reaches 
perihelion  in Ophiuchus it will be too close to the Sun to be  seen  well. 
Nevertheless,  it should be worth viewing with even modest telescopes.   It 
will  also  make a reasonable photographic subject.   Look for  it  through 
early December in the progressively earlier evening sky. 

     Below  are  the improved parabolic orbital elements,  followed by  the 
ephemeris.  I would appreciate observers' reports on this  object.   Please 
include  such circumstances as time,  date,  altitude of comet,  instrument 
(aperture and magnification), etc.  Thanks.

T = 1985 Dec 9.092       w = 87.040 degrees (arg. of peri.)
                         W = 357.702  "     (long. of asc. node)
q= .69435                i = 79.897


               Ephemeris for Comet Hartley-Good (epoch 1950)          
                                                                  
      DATE  |   r.a    |   dec.     |    Delta  |    R   | t. mag.
      mm/dd |(hh mm.mm)| ( dd mm.m )|    (AU)   |   (AU)          
      ______|__________|____________|___________|________|_______ 
      9/22  | 00 14.21 |  -27.54.7  |    0.644  |  1.602 |   9.1  
      9/27  | 23 33.81 |  -26 55.1  |           |        |        
      10/2  | 22 46.43 |  -24 30.5  |    0.529  |  1.457 |   8.3  
      10/7  | 21 56.19 |  -20.29.2  |           |        |        
      10/12 | 21 08.60 |  -15 16.4  |    0.511  |  1.311 |   7.7  
      10/17 | 20 27.53 |  -09 42.9  |           |        |        
      10/22 | 19 54.03 |  -04 31.6  |    0.581  |  1.166 |   7.5  
      10/27 | 19 27.18 |  -00 01.8  |           |        |        
      11/01 | 19 05.47 |   03 44.6  |    0.699  |  1.026 |   7.3  
      11/06 | 18 47.43 |   06 52.6  |           |        |        
      11/11 | 18 31.84 |   09 28.0  |    0.828  |  0.896 |   7.1  
      11/16 | 18 17.79 |   11 35.0  |           |        |        
      11/21 | 18 04.56 |   13 15.8  |    0.948  |  0.787 |   6.8  
      11/26 | 17 51.69 |   14 30.1  |           |        |        
      12/01 | 17 38.95 |   15 16.8  |    1.044  |  0.714 |   6.6  
      12/06 | 17 26.31 |   15 34.2  |           |        |        
      12/11 | 17 13.93 |   15 21.9  |    1.106  |  0.695 |   6.6  
      12/16 | 17 02.01 |   14 41.4  |           |        |        
      12/21 | 16 50.70 |   13 35.7  |    1.127  |  0.736 |   6.9  
      12/26 | 16 40.06 |   12 09.1  |           |        |        
      12/31 | 16 29.98 |   10 25.6  |    1.109  |  0.825 |   7.4  
      01/05 | 16 20.25 |   08 28.7  |           |        |        
      01/10 | 16 10.57 |   06 20.7  |    1.061  |  0.944 |   7.9  
      01/15 | 16 00.56 |   04 03.0  |           |        |        
      01/20 | 15 49.79 |   01 35.8  |    0.991  |  1.078 |   8.3  
      01/25 | 15 37.82 |  -01 01.0  |           |        |        
      01/30 | 15 24.17 |  -03 47.8  |    0.913  |  1.221 |   8.7