NavList:
A Community Devoted to the Preservation and Practice of Celestial Navigation and Other Methods of Traditional Wayfinding
Time divisions
From: J Cora
Date: 2006 May 10, 16:57 -0500
From: J Cora
Date: 2006 May 10, 16:57 -0500
My last question was too vague, so ignore it.
I am interested in the historical aspects of time measurements as it relates to astronomy, mapping and navigation.
For the first pass, restrict the historical time to late 1500's early 1600's when Tycho Brahe and Johannes Kepler lived.
A while back I read a book by J.L. Heilbron, The sun in the Church: cathedrals as solar observatories. Although I need to reread the book to refresh my memory, I seem to recall that they could use a beam of light through a slit and some type of scale on the floor to measure time.
By using such an instrument, endevouring to measure the time interval of 24 hours or 1 day; If we use the suns meridian passage, it is discovered that the time interval varies with the seasons, ie. the equation of time.
Still we persevere and construct a variable rate timer which can count off 24 hours and divide each hour by 60 so we can now count up to 1440 minutes per day, with the hope that at the start of the next days count we are reasonably close to our previous days full count.
For the moment, I am ignoring the meaning of a second and focusing on the meaning of a minute during the late 1500's to the early 1600's.
Assuming we can build a timer with an accuracy of 1 minute from day to day or at least can be corrected in some manner, we have a time instrument that divides the day into 1440 parts and can be used for various scientific studies.
Now how do we decide to set the length of a day? If we use the interval of the sun's meridian passage on the equinoxes is that a reasonable comprimise? Otherwise how could we make a decision about the length of a minute or a second and adjust a timepiece to run so that it counts off 1440 minutes or 84600 seconds per day?
Although I don't use a kamal, crossstaff or astrolabe to measure angles, the way our predecessors accomplished similar tasks is of great interest to me. Keplers printing of the Rudolphine tables was based on T. Brahe's data which was accurate to 2 or 3 minutes of arc, all done without the aid of optics.
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To post to this group, send email to NavList@fer3.com
To , send email to NavList-@fer3.com
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I am interested in the historical aspects of time measurements as it relates to astronomy, mapping and navigation.
For the first pass, restrict the historical time to late 1500's early 1600's when Tycho Brahe and Johannes Kepler lived.
A while back I read a book by J.L. Heilbron, The sun in the Church: cathedrals as solar observatories. Although I need to reread the book to refresh my memory, I seem to recall that they could use a beam of light through a slit and some type of scale on the floor to measure time.
By using such an instrument, endevouring to measure the time interval of 24 hours or 1 day; If we use the suns meridian passage, it is discovered that the time interval varies with the seasons, ie. the equation of time.
Still we persevere and construct a variable rate timer which can count off 24 hours and divide each hour by 60 so we can now count up to 1440 minutes per day, with the hope that at the start of the next days count we are reasonably close to our previous days full count.
For the moment, I am ignoring the meaning of a second and focusing on the meaning of a minute during the late 1500's to the early 1600's.
Assuming we can build a timer with an accuracy of 1 minute from day to day or at least can be corrected in some manner, we have a time instrument that divides the day into 1440 parts and can be used for various scientific studies.
Now how do we decide to set the length of a day? If we use the interval of the sun's meridian passage on the equinoxes is that a reasonable comprimise? Otherwise how could we make a decision about the length of a minute or a second and adjust a timepiece to run so that it counts off 1440 minutes or 84600 seconds per day?
Although I don't use a kamal, crossstaff or astrolabe to measure angles, the way our predecessors accomplished similar tasks is of great interest to me. Keplers printing of the Rudolphine tables was based on T. Brahe's data which was accurate to 2 or 3 minutes of arc, all done without the aid of optics.
--~--~---------~--~----~------------~-------~--~----~
To post to this group, send email to NavList@fer3.com
To , send email to NavList-@fer3.com
-~----------~----~----~----~------~----~------~--~---
