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This title is printed to order. This book may have been self-published. If so, we cannot guarantee the quality of the content. In the main most books will have gone through the editing process however some may not. We therefore suggest that you be aware of this before ordering this book. If in doubt check either the author or publisher’s details as we are unable to accept any returns unless they are faulty. Please contact us if you have any questions.
This volume is the most complete updated catalogue on the transits of Mercury and Venus from -2000 BC to 4000 AD. All calculations are based on the latest theories on the motion of Mercury and Venus and a great space is given to the maps and to the details of the times. In fact, not only the times of the maximum transit were calculated, but also the beginning and end of each phase, the curves of the exterior and interior ingress and egress, the position angle, the least angular distance between the centres, the best topocentrical sites, minimum and maximum duration, with details about where all this happens, and other. A detailed discussion was made, six millennia of data, which may be useful for historical researches but also for stargazing astronomers and professionals.
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This title is printed to order. This book may have been self-published. If so, we cannot guarantee the quality of the content. In the main most books will have gone through the editing process however some may not. We therefore suggest that you be aware of this before ordering this book. If in doubt check either the author or publisher’s details as we are unable to accept any returns unless they are faulty. Please contact us if you have any questions.
This volume is the most complete updated catalogue on the transits of Mercury and Venus from -2000 BC to 4000 AD. All calculations are based on the latest theories on the motion of Mercury and Venus and a great space is given to the maps and to the details of the times. In fact, not only the times of the maximum transit were calculated, but also the beginning and end of each phase, the curves of the exterior and interior ingress and egress, the position angle, the least angular distance between the centres, the best topocentrical sites, minimum and maximum duration, with details about where all this happens, and other. A detailed discussion was made, six millennia of data, which may be useful for historical researches but also for stargazing astronomers and professionals.