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75 lines
3.7 KiB
75 lines
3.7 KiB
15 years ago
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From rabaca@nova.ov.ufrj.br Fri Oct 20 23:12:11 2000
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Return-Path: <rabaca@nova.ov.ufrj.br>
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Delivered-To: coolo@master.kde.org
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Received: (qmail 22568 invoked by uid 1055); 20 Oct 2000 21:12:11 -0000
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Delivered-To: kde.org-coolo@kde.org
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Received: from nova.ov.ufrj.br (root@146.164.112.17)
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by max.tat.physik.uni-tuebingen.de with SMTP; 20 Oct 2000 21:12:07 -0000
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by nova.ov.ufrj.br (8.9.3/8.9.3) id TAA09140
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for coolo@kde.org; Fri, 20 Oct 2000 19:14:00 -0200
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From: Carlos Roberto Raba<E7>a <rabaca@nova.ov.ufrj.br>
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Reply-To: rabaca@nova.ov.ufrj.br
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Organization: Observatorio do Valongo - UFRJ
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To: Stephan Kulow <coolo@kde.org>
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Subject: Re: Moon tool
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Date: Fri, 20 Oct 2000 17:10:39 -0200
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X-Mailer: KMail [version 1.0.29]
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Content-Type: text/plain
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References: <00102016004500.08951@nova.ov.ufrj.br> <39F09247.5715C35D@kde.org>
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In-Reply-To: <39F09247.5715C35D@kde.org>
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MIME-Version: 1.0
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Message-Id: <00102019130700.09050@nova.ov.ufrj.br>
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Content-Transfer-Encoding: 8bit
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Status: O
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X-Status:
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Stephan,
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> In KDE2 I implemented free choice view angle, so I could also slide
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> it some degrees off to see it like I see it here :)
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It is nice to hear that! Unfortunately, I still use KDE 1.1.2.... By the way,
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when is the final release o 2.0?
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> But if you're an expert, I would like your advise on the correct
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> terms. Where on the earth you see the moon in the the default view
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> you can see on web pages etc.?
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As you know, the moon keeps always the same face turned to earth (the so called
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near side). This is a composition of its period of orbital motion and rotation:
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they are approximately the same. The moon's orbit is inclined with respect to
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the equator by (only) 5 degrees, and for our purposes, keeps the polar
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orientation in the sky unchanged. This means that the angle that you
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see the moon in the sky changes by a composition of two factors only: 1)
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latitude of the observer, and 2) time of the day that you look at the moon. If
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you look at the moon over many hours, the change of orientation in the sky is
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moon's orbital plane is close to the equator (as I said before) the discussion
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of orientation looses any meaning. At these positions, the passage by the
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meridian happens very close to the top of your head. So, I can be facing east
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and move my head up to see the moon, or I can be facing west and move my head
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up. Which rotation should I addopt? That is why I told you to use 0 or 180
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degrees. Otherwise, you would need to incorporate in your code many otherif he
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relations, including the latitude of the observer.he will see the first quarter
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moon as a C and the last quater moon as a D (see
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> The current kmoon uses the pictures of this site:l) when the moon is over
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> http://timbeauchamp.tripod.com/moon/, but a (german) colleague ofes over his
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> yours pointed out that the images are mirrored horizontally, son is reversed.
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> we corrected that (the larger craters appear on the left ontor. Since the
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> the moon I see in the sky, while they are right on the web).
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My colleague is correct. The east-west sides in the pictures are wrong, so you
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should flip them sideways. For an observer in the northern hemisthere this is
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all you need to do. For an observer in the southern hemisphere, you need to
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rotate this new set of images by 180 degrees. Keep in mind that in the sky if
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north is up east is to the left, if south is up east is to the right. You can
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easily see this if you lay down ;-/ on the floor with you head/legs pointing to
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the north/south line. Now, try to point your left arm to the geographic
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east while facing up.
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I hope this helps you. If you like more info, it will be a pleasure to
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help. Best wishes,
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Carlos
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