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Today's weather from WTOC-TV by Pat Prokop The Home Port of Topi Tuomi Links to other Hale-Bopp pages This Page in Finnish! The Hale-Bopp Comet Page by Bill Drennon JPL - Ron Baalke JPL - Ron Baalke: HB Timeline - 1997 Other links - Ron Baalke JPL - Charles S. Morris Near-Live Comet Watching System (NASA) Gary W. Kronkg The Puckett Observatory Sky Online's Comet Page www. halebopp.com European Southern Observatory Instituto de Astrofisica de Canarias Jyväskylän Sirius Dale Ireland Charles Boley Starwatch by Erich Landstrom Statesboro Astronomy Club Crni Vrh Observatory, Slovenia Image Gallery Click on the images below to see a larger version
50k jpg Comet Hale-Bopp on Jan 31, 1997, by Tim Puckett, Ellijay, GA
39k jpg Comet Hale-Bopp on Mar 07, 1997, by Andy Blackburn, Savannah, GA. In the dark spot (Clyo, GA) the stars and the comet look like gems in the sky!
36k jpg Comet Hale-Bopp on Mar 07, 1997, by Andy Blackburn, Savannah, GA. In the dark spot (Clyo, GA).
42k jpg Comet Hale-Bopp on Mar 07, 1997, by Andy Blackburn, Savannah, GA. In the dark spot (Clyo, GA).
35k jpg Comet Hale-Bopp on Mar 07, 1997, by Andy Blackburn, Savannah, GA. In the dark spot (Clyo, GA).
14k jpg Comet Hale-Bopp on Mar 09, 1997, by Topi Tuomi, Savannah, GA. Canon EOS Rebel X 35mm 1:4, Kodak Royal Gold 1000ASA, 2 minutes. The breaking dawn already paints the sky blue in the east.
29k jpg Comet Hale-Bopp and Tybee Lighthouse on March 17, 1997, by Topi Tuomi, Savannah, GA. Canon EOS Rebel X 35mm 1:4, Kodak Royal Gold 400ASA, 30 seconds.
91k jpg Comet Hyakutake on Mar 25, 1996, by Andy Blackburn, Savannah, GA. Hale-Bopp seems to be outperforming Hyakutake! |
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in April, 1997. A view from Savannah, GA (32ºN, 81ºW) by Topi K. Tuomi Archive page; last update 04/30/1997 (One month past perihelion) Hale-Bopp was still well visible. Comet magnitude was about 0.3. February pictures and observations, March pictures and observations and May pictures and observations are on their own archive pages. Backyard Astronomy Page will continue from where Hale-Bopp fades away. Photographs of comet Hale-Bopp
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These months are very interesting in
astronomical sense. Comet C/1995 O1 (Hale-Bopp), discovered over a year and half ago
on the same night by two astronomers, Alan Hale and Thomas Bopp, made its closest
approach to Earth on March 22nd, and will be closest to the Sun (in perihelion) on
April first.
It used to be a very bright object on the morning sky, and now it's well visible on the
evening sky. Since the beginning of January the comet has been visible in the east
before the morning twilight, but has now moved out of sight from the morning sky.
In the evening sky it is visible in the nortwest
after the evening twilight, until about 11pm., best seen from 8:30 to 10:30pm.
The comet is a beautiful naked eye sight, as my photograph on the right shows.
This photo was taken in the evening twilight of April 7th. The lighthouse is
located on Tybee Island 20 miles east of Savannah. How to locate the comet in the evening skyBecause the comet is still near zero magnitude in brightness, you only need very general instructions to find it: After 8:45 (local daylight savings time) in the evening, go to a place providing an uninterrupted view of the western sky, where the comet is so prominent, that it's the first thing you'll notice there. You don't need any other instructions to find it, but to go out after dusk, look west and enjoy the view! The comet is moving south; you'll notice it has moved a little left every evening.
The comet sets about 10:30pm this weekend (April 26-27),
so if the sky happens to be clear between 8 and 10 in the evening, you should be able
to spot Hale-Bopp easily in the western sky.
Dale Ireland has a good
comet locator
map for April on his comet page, if you want to see where the comet is heading. Planet Jupiter (mag -2.0) is visible in the east before the sunrise, and is higher every morning. Mercury has been appearing as an evening star and had its best showing of the year in late March and early April. Mars is high in the east in the evening and in the west in the morning. Saturn and Venus are too close to the sun to be seen, but in a few weeks Saturn will start appearing as a morning star, and Venus as an evening star. April observations in Savannah, GAFebruary pictures and observations and March pictures and observations are on their own archive pages.Tuesday, April 01, 1997 Wednesday, April 02, 1997 Thursday, April 03, 1997 Friday, April 04, 1997 Saturday, April 05, 1997 Sunday, April 06, 1997 Monday, April 07, 1997 Tuesday, April 08, 1997 Wednesday, April 09, 1997 Thursday, April 10, 1997 Friday, April 11, 1997 Saturday, April 12, 1997 Sunday, April 13, 1997 Monday, April 14, 1997 Tuesday, April 15, 1997 Wednesday, April 16, 1997 Thursday, April 17, 1997 Friday, April 18, 1997 Saturday, April 19, 1997 Sunday, April 20, 1997 Monday, April 21, 1997 Tuesday, April 22, 1997 Wednesday, April 23, 1997 Thursday, April 24, 1997 Friday, April 25, 1997 Saturday, April 26, 1997 Sunday, April 27, 1997 Monday, April 28, 1997 Tuesday, April 29, 1997 Wednesday, April 30, 1997 May pictures and observations
are on their own archive page. What to expectThe following values are from the Orbit and Ephemeris Information by Don Yeomans. This table is greatly simplified; if you want to see more data, please refer to the original table. The distances of the comet from Earth and Sun are in Astronomical Units (AU=the mean distance Earth/Sun). Tmag1 is the prediction in the original tables (01/19/97 & 03/03/97), and Tmag2 is the actual observed values from Charles Morris (smallest/average/biggest m1 estimate).The comet reached its greatest brightness on the last days of March, and it was near magnitude -0.8. On April 30th the average of the observed values was 0.30, which was near the predicted value 0.4. Brightness development of comet Hale-Bopp
Table 1. Selected Ephemeris Values for Comet Hale-Bopp in 1997. Date R.A. Distance from #of (UT) J2000 Decl. Earth Sun TMag1 Tmag2 obs Feb 01 19 40 +15 28 2.004 1.368 2.5 2.1/2.30/2.9 11 Feb 02 19 42 +15 57 1.985 1.356 2.5 2.0/2.27/2.8 14 Feb 03 19 45 +16 27 1.965 1.344 2.4 1.8/2.10/2.4 10 Feb 04 19 48 +16 57 1.945 1.332 2.4 1.8/2.08/2.5 9 Feb 05 19 50 +17 29 1.925 1.320 2.3 1.7/1.90/2.1 9 Feb 06 19 53 +18 00 1.906 1.309 2.3 1.7/1.94/2.5 14 Feb 07 19 56 +18 33 1.886 1.297 2.2 1.4/1.79/2.4 13 Feb 08 19 58 +19 06 1.866 1.286 2.2 1.6/1.81/2.1 12 Feb 09 20 01 +19 40 1.846 1.274 2.1 1.3/1.68/2.4 24 Feb 10 20 04 +20 14 1.827 1.263 2.1 1.4/1.69/2.2 20 Feb 11 20 07 +20 50 1.807 1.251 2.0 1.3/1.70/2.2 20 Feb 12 20 10 +21 26 1.788 1.240 2.0 1.3/1.58/2.2 14 Feb 13 20 14 +22 02 1.769 1.229 1.9 1.3/1.52/1.9 17 Feb 14 20 17 +22 40 1.749 1.218 1.9 1.2/1.48/1.8 10 Feb 15 20 20 +23 18 1.730 1.207 1.8 1.1/1.34/1.8 18 Feb 16 20 24 +23 57 1.711 1.196 1.8 1.0/1.31/1.8 23 Feb 17 20 28 +24 36 1.693 1.186 1.7 1.1/1.36/2.0 12 Feb 18 20 31 +25 17 1.674 1.175 1.6 1.1/1.25/1.8 11 Feb 19 20 35 +25 58 1.656 1.164 1.6 1.0/1.18/1.4 22 Feb 20 20 39 +26 39 1.638 1.154 1.5 0.8/1.07/1.4 21 Feb 21 20 43 +27 21 1.620 1.144 1.5 0.9/1.12/1.5 13 Feb 22 20 47 +28 04 1.602 1.134 1.4 0.8/1.10/1.3 9 Feb 23 20 52 +28 48 1.585 1.124 1.4 0.7/1.01/1.2 22 Feb 24 20 56 +29 32 1.568 1.114 1.3 0.7/0.93/1.1 14 Feb 25 21 01 +30 16 1.552 1.104 1.3 0.6/0.94/1.3 21 Feb 26 21 06 +31 01 1.535 1.095 1.2 0.6/0.92/1.2 15 Feb 27 21 11 +31 46 1.519 1.086 1.2 0.7/0.82/1.0 10 Feb 28 21 16 +32 31 1.504 1.076 1.1 0.5/0.88/1.5 14 - Corrected ephemeris values by Don Yeomans - Mar 1 21 21 +33 17 1.489 1.067 0.7 0.4/0.69/1.2 12 Mar 2 21 27 +34 02 1.474 1.059 0.6 0.2/0.52/1.1 20 Mar 3 21 33 +34 48 1.460 1.050 0.6 0.2/0.54/1.0 19 Mar 4 21 39 +35 33 1.447 1.042 0.5 0.2/0.36/1.0 12 Mar 5 21 45 +36 19 1.434 1.033 0.5 0.1/0.28/0.5 13 Mar 6 21 52 +37 03 1.421 1.025 0.4 -.1/0.19/0.5 14 Mar 7 21 58 +37 47 1.409 1.018 0.4 -.1/0.04/0.2 19 Mar 8 22 05 +38 31 1.398 1.010 0.4 -.4/-.11/0.3 13 Mar 9 22 13 +39 13 1.387 1.003 0.3 -.4/-.05/0.3 28 Mar 10 22 20 +39 55 1.378 .996 0.3 -.4/-.15/0.1 15 Mar 11 22 28 +40 35 1.368 .989 0.2 -.4/-.19/0.3 18 Mar 12 22 36 +41 14 1.360 .982 0.2 -.6/-.24/0.0 16 Mar 13 22 44 +41 51 1.352 .976 0.2 -.6/-.29/0.3 14 Mar 14 22 53 +42 26 1.344 .970 0.1 -.7/-.45/-.1 11 - Corrected ephemeris values by Don Yeomans - Mar 15 23 02 +42 58 1.338 .964 -.5 -.5/-.28/0.1 5 Mar 16 23 11 +43 29 1.332 .959 -.6 -.9/-.47/0.0 13 Mar 17 23 20 +43 57 1.328 .953 -.6 -.9/-.47/0.0 13 Mar 18 23 29 +44 22 1.323 .949 -.6 -.7/-.57/-.3 9 Mar 19 23 39 +44 44 1.320 .944 -.6 -.8/-.60/-.3 12 Mar 20 23 49 +45 04 1.318 .940 -.7 -.8/-.58/-.3 9 Mar 21 23 58 +45 20 1.316 .936 -.7 -1.0/-.61/-.3 12 Mar 22 00 08 +45 32 1.315* .932 -.7 -1.0/-.59/-.3 8 Mar 23 00 19 +45 42 1.315 .929 -.7 -1.0/-.54/-.2 10 Mar 24 00 29 +45 48 1.316 .926 -.7 -1.0/-.61/0.1 10 Mar 25 00 39 +45 50* 1.318 .923 -.7 -1.2/-.74/-.3 9 Mar 26 00 49 +45 49 1.320 .921 -.8 -1.3/-.78/-.5 9 Mar 27 00 59 +45 44 1.323 .919 -.8* -1.1/-.79/-.4 14 Mar 28 01 09 +45 36 1.327 .917 -.8 -1.3/-.80/-.3 19 Mar 29 01 19 +45 25 1.332 .916 -.8 -1.1/-.75/-.5 6 Mar 30 01 28 +45 10 1.338 .915 -.8 -1.8/-.80/-.5 10 Mar 31 01 38 +44 53 1.344 .914 -.7 -1.1/-.82/-.4 10 Apr 1 01 47 +44 33 1.351 .914 -.7 -1.2/-.79/-.4 15 Apr 2 01 56 +44 10 1.359 .914 -.7 -1.0/-.66/-.3 13 Apr 3 02 05 +43 45 1.367 .915 -.7 -1.1/-.68/-.3 12 Apr 4 02 13 +43 17 1.376 .916 -.7 -.9/-.61/-.2 7 Apr 5 02 22 +42 47 1.385 .917 -.7 -1.3/-.65/-.3 11 Apr 6 02 30 +42 16 1.396 .918 -.6 -.7/-.50/-.2 12 Apr 7 02 38 +41 43 1.406 .920 -.6 -.7/-.53/-.3 6 Apr 8 02 45 +41 08 1.418 .922 -.6 -.9/-.54/-.1 11 Apr 9 02 52 +40 32 1.430 .925 -.6 -.7/-.55/-.2 6 Apr 10 02 59 +39 55 1.442 .928 -.5 -1.0/-.55/-.2 13 Apr 11 03 06 +39 17 1.455 .931 -.5 -.8/-.48/-.2 5 Apr 12 03 13 +38 38 1.468 .935 -.5 -.6/-.43/-.2 7 Apr 13 03 19 +37 58 1.482 .938 -.4 -.7/-.44/-.2 7 Apr 14 03 25 +37 18 1.496 .943 -.4 -.6/-.50/-.3 6 Apr 15 03 31 +36 38 1.510 .947 -.3 -.8/-.37/0.1 10 Apr 16 03 36 +35 57 1.525 .952 -.3 -.6/-.31/-.1 9 Apr 17 03 42 +35 16 1.540 .957 -.3 -.4/-.07/0.4 6 Apr 18 03 47 +34 35 1.555 .962 -.2 -.4/-.26/-.1 5 Apr 19 03 52 +33 54 1.571 .968 -.2 -.3/-.02/0.8 5 Apr 20 03 57 +33 13 1.586 .974 -.1 -.8/-.26/0.0 8 Apr 21 04 02 +32 32 1.602 .980 -.1 -.2/-.08/0.0 5 Apr 22 04 06 +31 51 1.619 .987 .0 -.2/-.08/0.3 4 Apr 23 04 10 +31 11 1.635 .994 .0 -.4/-.11/0.2 7 Apr 24 04 15 +30 31 1.651 1.001 .1 -.1/0.04/0.2 8 Apr 25 04 19 +29 51 1.668 1.008 .1 -.3/-.09/0.3 9 Apr 26 04 23 +29 12 1.685 1.015 .2 -.3/0.01/0.7 13 Apr 27 04 26 +28 32 1.702 1.023 .3 -.1/0.16/0.7 10 Apr 28 04 30 +27 54 1.719 1.031 .3 -.3/-.05/0.0 6 Apr 29 04 34 +27 15 1.736 1.039 .4 0.0/0.10/0.4 7 Apr 30 04 37 +26 37 1.753 1.047 .4 0.0/0.30/1.0 9 May 1 04 40 +26 00 1.770 1.056 .5 May 2 04 44 +25 23 1.787 1.065 .5 May 3 04 47 +24 46 1.804 1.074 .6 May 4 04 50 +24 10 1.822 1.083 .6 May 5 04 53 +23 35 1.839 1.092 .7 May 6 04 56 +23 00 1.856 1.102 .8 May 7 04 59 +22 25 1.873 1.111 .8 May 8 05 01 +21 51 1.890 1.121 .9 May 9 05 04 +21 17 1.907 1.131 .9 May 10 05 07 +20 44 1.924 1.141 1.0 May 11 05 09 +20 11 1.941 1.151 1.1 May 12 05 12 +19 38 1.958 1.161 1.1 May 13 05 14 +19 06 1.975 1.172 1.2 May 14 05 17 +18 34 1.992 1.182 1.2 May 15 05 19 +18 03 2.008 1.193 1.3 May 16 05 22 +17 32 2.025 1.204 1.3 May 17 05 24 +17 02 2.041 1.215 1.4 May 18 05 26 +16 32 2.057 1.226 1.5 May 19 05 28 +16 02 2.074 1.237 1.5 May 20 05 30 +15 33 2.090 1.248 1.6 May 21 05 33 +15 04 2.106 1.259 1.6 May 22 05 35 +14 35 2.121 1.271 1.7 May 23 05 37 +14 07 2.137 1.282 1.7 May 24 05 39 +13 39 2.153 1.294 1.8 May 25 05 41 +13 11 2.168 1.305 1.8 May 26 05 43 +12 43 2.183 1.317 1.9 May 27 05 45 +12 16 2.199 1.329 1.9 May 28 05 47 +11 49 2.214 1.340 2.0 May 29 05 48 +11 23 2.228 1.352 2.1 May 30 05 50 +10 56 2.243 1.364 2.1 May 31 05 52 +10 30 2.258 1.376 2.2 Jun 1 05 54 +10 04 2.272 1.388 2.2
Table 2. "Average" Atmospheric Extinction in Magnitudes for
Sea Level (z=degrees from zenith,
h=degrees from horizon)
z ext. h
0 0.3 90 (zenith)
10 0.3 80
20 0.3 70
30 0.3 60
40 0.4 50
45 0.4 45
50 0.4 40
55 0.5 35 For example, an object 35º above
60 0.6 30 the horizon looses 0.5 magnitudes
65 0.7 25 because of the atmospheric
70 0.8 20 extinction, but an object only 6º
75 1.1 15 above horizon looses 2.5 magnitudes.
80 1.6 10 Thus, if a comet at 6º looks as
82 1.9 8 bright as a star at 35º, it actually
84 2.5 6 is 2 magnitudes brighter.
85 2.9 5
86 3.5 4
87 4.2 3
88 5.4 2
89 7.4 1
90 11.2 0 (horizon)
Clear skies! If you have any comments, please
send email to Topi Tuomi. |