[time-nuts] reply re Harrison's timing method - #13 in Vol 176, Issue 44 digest
jimlux
jimlux at earthlink.net
Wed Mar 27 01:18:30 UTC 2019
On 3/26/19 3:48 PM, Bob Holmstrom wrote:
> Ben Bradley stated > "Perhaps closer to your question: I recall in my
> readings about clockmaker John Harrison (likely either in "The Quest
> for Longitude” or Dava Sobel's "Longitude") that he would look from
> the edge of his window at a particular star each night and note (while
> counting the ticks he heard from his clock) the exact moment it would
> disappear behind a nearby chimney, and knowing the Earth's rotation
> takes four minutes and some (I forget) seconds off from a day, he used
> this to calibrate and test the precision and accuracy of his long
> clocks. It was suggested he could get within less than second with
> this method."
>
> From Sobel - Chapter 7 > "The Harrison brothers tested the accuracy of
> their gridiron-grasshopper clocks against the regular motions of the
> stars. The crosshairs of their homemade astronomical tracking
> instrument, with which they pinpointed the stars' positions, consisted
> of the border of a windowpane and the silhouette of the neighbor's
> chimney stack. Night after night, they marked the clock hour when
> given stars exited their field of view behind the chimney. From one
> night to the next, because of the Earth's rotation, a star should
> transit exactly 3 minutes, 56 seconds (of solar time) earlier than the
> previous night. Any clock that can track this sidereal schedule proves
> itself as perfect as God's magnificent clockwork.”
>
> This would be an excellent project for time-nuts to verify. First, a
> better explanation of John Harrison’s method is in order. A vertical
> window edge is not sufficient - a second vertical reference at a
> distance is required - Harrison used a chimney on a neighbor's house.
>
To get 1 second accuracy, you need 360/86400 = 0.004 degree
measurements. That's 0.073 milliradian - 1 cm at 140 meter distance.
I'm not sure an "edge" is sharp enough (diffraction, etc.), although
your eye is pretty good at "deconvolving" the linear equivalent of an
Airy disk/rings.
A small telescope and a camera might work, lining up with the two edges
as a "fixed offset knife edges". It could also work in day time (you
can see Polaris in the day time with a 28x telescope with a 1" objective
- a surveyor's theodolite)
There's a collection of navigation papers from ION available on CD-ROM
and there's a fair amount of info in there about celestial trackers and
detectors.
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