THE POSITIONS OF COMET HALE-BOPP
THROUGH 1997

Below is a table giving information about Comet Hale-Bopp through 1997. If you can connect to World Wide Web, double check this data with the most up-to-date Hale-Bopp ephemeris data at the Harvard Center for Astrophysics

In the Ephemeris Table given below, each column has an abbreviation at the top. The abbreviations stand for:

EPHEMERIS TABLE
1994 01 Hale Bopp

     DATE...... R.A.       DEC      R (AU) D   EL SKY  MAG
    10-15-95   18hl7m    -28.6d    6.43  6.66  72  E  10.2
    11-04-95   18h23m    -27.7d    6.25  6.79  54  E  10.1
    11-24-95   18h31m    -26.8d    6.07  6.85  36  E  10.0
    12-14-95   18h42m    -26.Od    5.89  6.82  18  E   9.9
    01-03-96   18h55m    -25.Od    5.70  6.69   2  E   9.7
    01-23-96   l9hO8m    -24.Od    5.52  6.45  17  E   9.5
    02-12-96   l9h20m    -22.8d    5.33  6.11  34  M   9 2
    03-03-96   l9h32m    -21.6d    5.14  5.69  52  M   8.9
    03-23-96   l9h40m    -20.3d    4.94  5.20  70  M   8.5
    04-12-96   l9h45m    -18.8d    4.74  4.67  88  M   8.1
    05-02-96    l9h44m   -17.3d    4.54  4.14 107  M   7.7
    05-22-96    l9h36m   -15.6d    4.34  3.64 128  M   7.2
    06-11-96    l9hl9m   -13.8d    4.13  3.22 150  M   6.7
    07-01-96    18h55m   -11.8d    3.91  2.91 168  M   6.3
    07-21-96    18h26m   -09.8d    3.70  2.76 154  E   5.9
    08-10-96    18hOOm   -08.ld    3.48  2.74 130  E   5.6
    08-30-96    17h41m   -06.6d    3.25  2.81 107  E   5.4
    09-19-96    17h31m   -05.5d    3.02  2.92  86  E   5.1
    10-09-96    17h31m   -04.5d    2.79  3.01  68  E   4.8
    10-29-96    17h39m   -03.4d    2.55  3.05  51  E   4.5
    11-18-96    17h53m   -01.9d    2.30  3.00  38  E   4.0
    12-08-96    18hl3m   +00.4d    2.05  2.86  29  E  +3.4
    12-28-96    18h38m   +04.Od    1.80  2.61  27  M  +2.6
    01-17-97    l9hllm   +09.6d    1.54  2.28  32  M  +1.7
    02-06-97    l9h56m   +18.3d    1.30  1.90  40  M  +0.6
    02-26-97    21hlOm   +31.4d    1.09  1.53  45  M  -0.6
    03-18-97    23h35m   +44.4d    0.95  1.33  46  M  -1.5
    04-07-97    02h41m   +41.4d    0.93  1.42  41  E  -1.5
    04-27-57    G4h,8m   +28.4d    1.03  1.71  33  E  -0.6
    05-17-97    05h25m   +17.Od    1.23  2.05  26  E  +0.4
    06-06-97    06hO4m   +08.0d    1.46  2.35  22  E  +1.5
    06-26-97    06h36m   +00.3d    1.71  2.59  23  E   2.4
    07-16-97    07hO2m   -07.Od    1.96  2.78  30  M   3.1
    08-05-97    07h26m   -14.3d    2.21  2.91  39  M   3.8
    08-25-97    07h46m   -22.Od    2.46  3.00  49  M   4.3
    09-14-97    08hOlm   -30.ld    2.70  3.07  60  M   4.7
    10-04-97    08hllm   -38.5d    2.94  3.13  70  M   5.2
    10-24-97    08hllm   -46.8d    3.17  3.21  79  M   5.5
    11-13-97    07h59m   -54.4d    3.40  3.32  86  M   5.9
    12-03-97    07h29m   -60.3d    3.62  3.48  91  M   6.3
    12-23-97    06h42m   -63.6d    3.84  3.67  93  M   6.7
    01-12-98    05h54m   -63.8d    4.05  3.89  92  M   7.0
    02-01-98    05hl9m   -61.8d    4.26  4.15  90  M   7.4
    02-21-98    05hO2m   -58.4d    4.47  4.42  87  M   7.7
    03-13-98    05hOOm   -55.6d    4.67  4.69  83  M   8.1
CC206.TXT Don Machholz (916) 346-8963

Elongation: the angle made by the comet, the Earth, and the Sun. In other words, the number of degrees of angle that separate the Sun and the comet.

Magnitude: The brightness of an object. The magnitude number increases as the brightness decreases. The dimmest magnitude star that can be seen by someone with good vision is about magnitude 6. Bright stars are magnitude 1 and the brightest stars are magnitude 0 or -1. A bright planet, like Venus can be as bright as -4 magnitude.

(Last Update: 9/26/96 )
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