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Observer: ???
Location: Kumanmoto Civil Astronomical Observatory, Japan
Date: September 2, 1996
41cm F6L, 60 seconds.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 4, 1996
Image taken with a ST8 7" F/6.
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Copyright David Johnson
Observer(s): David Johnson
Location: Newport, United Kingdom
Date: September 5, 1996
2 minute exposure with Starlight Express colour CCD camera. Telescope 12 inch f5 Newtonian.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 6, 1996
Image taken with a ST8 7" F/6.
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Observer: Pedro Re
Location: Portugal
Date: August - September 1996
All images were obtained from central Portugal with a C14 and HISIS22 CCD Camera.
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Observer: Allen Ginzburg
Location: Aptos, California
Date: September 6, 1996 04:57 UT
CCD image of Hale Bopp. Telesope: 10" Meade LX-200 at f/6.3. Camera: Pixel211 CCD (field approx. 5.5' square). Exposure: 60 seconds. It seems to show the nucleus in 2 parts.
January 29, 1997 update: I discovered that the split nucleus is the result of Comet Hale-Bopp passing a 12th magnitude star.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 9, 1996
True color image taken with a ST8 7" F/6.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 11, 1996
Image taken with a ST8 7" F/6.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 13, 1996
Image taken with a ST8 7" F/6.
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Observer: Al Kelly
Location: Danciger, Texas
Date: September 14, 1996
I took several short exposures of H-B with my 32" f4 Newtonian and CB245 camera. After stacking seven 15-second exposures and running the composite image through a rank-order processing routine in Richard Berry's software, the tail structure(s) really started to show up.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 14, 1996
Image taken with a ST8 7" F/6.
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Observer: Mike DeMarquette
Location: Big Bear Lake, California
Date: September 15, 1996 04:45, 04:59 UT
Camera is a Minolta X-700 35mm camera with a 50mm lens at f/2.8 , film was ASA 400 some offmarket brand and the exposure times were 5min and 7min.
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Observers: Olivier Hainaut, Karen Meech, James Bauer
Location: Mauna Kea, Hawaii
Date: September 16, 1996
Image obtained at the Canada-France-Hawaii Telescope on Mauna Kea , with the 8192^2 pixel CCD camera built by the Institute for Astronomy (Hawaii). This image is a 2min exposure through a VR filter (very broad-band, enclosing most of the visible light from green to red), except the central region (saturated on the 2min exposure), which was extracted from a 15sec image taken just after. On this image, N is up, E is left. At the time of the observations, the Sun was on the right side of the image (almost 2deg up from W). At least 6 dust jets are visible close to the nucleus (they have been slightly enhanced by dividing the image by a smooth cometary profile); they curve away from the Sun, as the solar wind drags the dust particles, to fade into the huge tail.
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Observer: Otto Farago
Location: Swabian Obserwatory, Stuttgart, Germany
Date: September 16, 1996 19:13 UT
CCD-image of Hale-Bopp. ST-6 in focal length Celestron 14 (3190mm).
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Observer(s): Anthony Ferro, Susan Wyckoff, Rodney Heyd, Peter Wehinger
Location: Kitt Peak National Observatory, Arizona
Date: September 17, 1996
This image was taken with the 0.9-m (36-inch) telescope using a Harris-I band filter. The image shows the comet with several different dust jets clearly visible. The sunward direction is roughly toward the top of the image. At the time this 600s image was taken, the comet was just over 3 AU from the Sun and 2.9 AU from the Earth.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 18, 1996
Images taken with a ST8 7" F/6.
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Observers: H. Fukushima, N. Yamamoto
Location: National Astronomy Observatory, Japan
Date: July - December 1996
Images taken using the NAOJ 50cm reflector with a CCD camera.
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Observers: H. Fukushima, N. Yamamoto
Location: National Astronomy Observatory, Japan
Date: April - November 1996
Images taken using the NAOJ 50cm reflector with a CCD camera.
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Observers: Hal Weaver
Location: Hubble Space Telescope
Date: September 1995-1996
The above figure shows the temporal evolution of Comet Hale-Bopp over the course of about 1 year, as observed by the Hubble Space Telescope. In the far-left frame we caught the comet about 60 hours after a huge outburst of dust, and the image shows an impressive spiral structure reminescent of a water sprinkler observed from above. The middle frame shows the comet during a more quiescent phase in which hardly any structure is seen in the coma without employing a strong intensity contrast in the display. The image at the far-right shows that the comet has now taken on a "porcupine" appearance as at least five jets can be seen sprouting from the nucleus. The nucleus of the comet is located at the center of each frame, but most of the light observed is due to scattered sunlight from fine dust grains that are emitted from the nucleus and which produce the cometary "coma". Each frame above is 10 arcsec across. For the far-left frame this corresponds to 47,000 km at the comet, for the middle frame this corresponds to 49,000 km at the comet, and for the far-right frame this correponds to 21,000 km at the comet. (The comet was much closer to the Earth during the September 1996 observations.)
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Observer: Hal Weaver
Location: Hubble Space Telescope
Date: September 23-26, 1996
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 23, 1996
Images taken with a ST8 7" F/6. Second image is a false color image.
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Observers: David Renneke, Jeff Strasser
Location: Milan, Illinois
Date: September 28, 1996 15:36 UT
Image was taken at using a Meade 8" telescope and an SBIG ST-6 CCD camera. This was a 10 second exposure. The size of the photo is 28' x 18'. The comet was a distance of 2.97 AU from Earth. The moon was shining brightly being two days past full. The picture shows several jets.
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Observer: David Hanon
Location: Ringgold, Georgia
Date: September 30, 1996
Image taken with a ST8 7" F/6.