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Titlebook: Visually Observing Comets; David A. J. Seargent Book 2017 Springer International Publishing Switzerland 2017 Amateur comet-hunting.How to

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發(fā)表于 2025-3-23 10:04:45 | 只看該作者
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發(fā)表于 2025-3-23 16:57:35 | 只看該作者
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發(fā)表于 2025-3-23 18:02:00 | 只看該作者
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發(fā)表于 2025-3-24 01:50:50 | 只看該作者
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發(fā)表于 2025-3-24 04:28:40 | 只看該作者
David A. J. Seargent7) were measured by increment threshold techniques in patients suffering from acquired colour vision deficiencies, caused either by drugs or by hereditary retinal degenerations. Compared with normal observers (n =11) Diphenylbutylpiperidine (IMAP?, 1.5mg/week over 18 months) reversibly decreases the
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發(fā)表于 2025-3-24 10:06:35 | 只看該作者
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發(fā)表于 2025-3-24 14:14:04 | 只看該作者
Comets in Motion was able to show that the bright comet that had graced the morning skies during November and early December of 1680 was actually the same as the even more magnificent apparition that emerged from the evening twilight just prior to Christmas. He also correctly demonstrated that this comet had passed unusually close to the Sun around mid-month.
18#
發(fā)表于 2025-3-24 15:01:50 | 只看該作者
The Formation of Tails to a distance equal to that of Earth and the Sun, while ions from the tail of Comet Hyakutake in 1996 were detected by spacecraft at over 3 times that distance from the comet’s head. Then, in 2007, the great Comet McNaught extended a magnificent tail as long as that of Ikeya-Seki but around 65 million km wide!
19#
發(fā)表于 2025-3-24 22:13:00 | 只看該作者
The Value of Visual Observing in a Photo-Happy World comet seen today with one seen in decades, centuries or even millennia past. Only by comparing visual observations of a periodic comet during a contemporary return can we ascertain whether any changes in that object’s activity have taken place since astronomers of a century ago described that same body during its earlier apparitions.
20#
發(fā)表于 2025-3-25 02:49:48 | 只看該作者
The Kreutz Sungrazing Comet Group: A Special Opportunity for Visual Comet Hunters?orbit had been calculated, it was found to have passed an incredibly close 0.005 AU from the center of the Sun. At its closest approach, it was actually closer to the solar photosphere than the tops of some of the prominences!
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