HISTORY 135C

Department of History
University of California, Irvine
 Instructor:    Dr. Barbara J. Becker

Lecture 10.  Time and Place.

The Problem of Longitude

The Earth spins on a north-south axis that hardly changes its orientation from century to century.  This accounts for the relative stability in the north-south orientation of the map of the fixed stars.  Using familiar celestial markers as guides (the star Polaris, for example), a navigator out in the open sea can readily determine her geographic latitude (position north or south of the equator).  Figuring out her longitude (position in the east-west direction) is a different story.  There is nothing comparable to the equator or the poles for the navigator to use as reference points.

It is inconvenient for everyone around the globe to awaken, work and sleep according to a schedule defined by a single global clock.  Most people in Hong Kong, Los Angeles and Nairobi prefer to rise with the Sun, mark the noon hour when the Sun crosses the local meridian and sleep after the Sun has set. 

The Earth makes one complete turn on its axis nearly every twenty-four hours.  As shown in the illustration above, every 15° of longitude (360° ÷ 24) marks a difference of one hour in local time.  Longitude measures are intimately connected to time -- in particular, to comparisons of local time in different parts of the globe. 

To see how a navigator in the open sea can use time to determine her longitude, imagine that each day, when her trusty chronometer tells her it is precisely noon in London, she determines her own local time by observing the Sun's position on the sky.  On the first day, when her chronometer strikes twelve noon, she notes her local time is 11 a.m., a reading that lets her know she is currently located 15° west of London.  On the second day, she sees that her local time is only 10 a.m., an indication that she is now 30° west of London.  Unfortunately, her chronometer falls and breaks on the third day!  With no way of knowing when it is precisely noon in London, she has no signal to tell her when to measure her local time.  Unable to compare her local time with time in London, she is left with no easy way to determine her longitude.

Reliable and accurate chronometers are a modern invention.  Mariners have ventured across the open sea for centuries.  How did the early seafaring adventurers determine their longitude?

Significant Events in the Search for a Solution to the Longitude Problem

1514

Johannes Werner (1468-1522) of Nuremberg proposed a method of "lunar distances".  The Moon moves fairly rapidly from West to East against the background array of the fixed stars. 

Astronomers in or near a port city created tables based on years of careful mapping of the Moon's motion. The tables list -- for each hour of the day -- the expected separation of the Moon from a set of easily recognized bright stars. 

After measuring the Moon's distance from a particular star, a mariner can use the prepared tables to find out what time it is in his port city.  Once that time is known, he can compare it to his local time and calculate his longitude.

1530

Gemma Frisius (1508-1555) of Antwerp proposed using a portable mechanical clock that could be set to a port city's local time before setting out to sea.  So long as the clock could be relied upon to keep accurate time, a mariner would only have to measure his local time in order to determine his longitude.

1550

"Why do we put up with these pilots, with their bad language and barbarous manners; they know neither sun, moon nor stars, nor their courses, movements or declinations; or how they rise, how they set and to what part of the horizon they are inclined; neither latitude nor longitude of the places on the globe, nor astrolabes, quadrants, cross staffs or watches, nor years common or bissextile, equinoxes or solstices?"
-- Pero Nuñes, Portuguese mathematician

1585
Jost Bürgi (1552-1632), Swiss clockmaker, developed a more accurate mechanical clock.
1598
Philip III of Spain offered a large monetary prize to the individual who solved the longitude problem -- a perpetual pension of 6,000 ducats, a life annuity of 2,000 ducats, and a cash prize of 1,000 ducats.
1610
Galileo (1564-1642) discovered 4 moons of Jupiter.
1636
Galileo proposed using a mechanical clock and the moons of Jupiter to determine longitude.
1657
Christiaan Huygens (1629-1695), Dutch astronomer, physicist, mathematician created the first working pendulum clock.
1660
Huygens began working on improved pendulum clock for use at sea.
1667

Paris Observatory founded.

1668
A chart showing pictures of the predicted positions of Jupiter's satellites at 7 p.m. on each day in January 1668.  Mariners could estimate their local time at sea by observing Jupiter with a telescope and then comparing the arrangement of Jupiter's moons they saw with those depicted on the chart.
1675
John Flamsteed (1646-1719) was appointed the first Astronomer Royal by King Charles II.  He was the first (and for a long time, the only) scientist paid an annual salary for service to the English crown.

Astronomers Royal (1675-turn of the 20th c)
Name
Dates
Dates served
John Flamsteed
1646-1719
1675-1719
Edmond Halley
1656-1742
1720-1742
James Bradley
1693-1762
1742-1762
Nathaniel Bliss
1700-1764
1762-1764
Nevil Maskelyne
1732-1811
1765-1811
John Pond
1767-1836
1811-1835
George Biddle Airy
1801-1892
1835-1881
William H. M. Christie
1845-1922
1881-1910

1676

Flamsteed took up residence at Greenwich Observatory, located near London atop a high hill bordering the Thames River.  The building was designed by Christopher Wren for the Astronomer Royal's use.  Although Flamsteed was given a building from which to observe, no provision was made for the purchase observing instruments!  Flamsteed purchased or commissioned the construction of many instruments at his own expense.

1707
Loss of Admiral Clowdisley Shovell's fleet off the coast of the Scilly Isles -- 1,647 perished.
1714
Queen Anne (1665-1714) of Great Britain and Ireland established a longitude prize -- £20,000!!
John Harrison and the Longitude Prize

John Harrison (1693-1776)
Notable Events in Harrison's Life
1693
born in Yorkshire
1725
investigated effects of temperature change on expansion and contraction of metals

used results of experiments to design gridiron pendulum

1726
completed two "regulators" made of wood, accurate to within one second per month
1730
John Hadley (1682-1744) invented a new, more accurate altitude-measuring instrument -- the "octant" or "Hadley's quadrant"

accurate to within 3 minutes of a degree (~ 3 mi)


Hadley's quadrant
1730
Harrison obtained support from Astronomer Royal Edmond Halley and clockmaker George Graham for his plan to build H1
1735
H1 completed

H1
weight = 75 lbs
  size = 4' X 4' X 4'
1736
H1 sent on trial run to Lisbon
1737
Commissioners of the Board of Longitude met for the first time
  • examined H1
  • advanced Harrison £250 toward production costs of H2
  • promised additional £250 when H2 is completed

H2
weight = 86 lbs
size ~ H 4.5' X W 2'
(never tested at sea)

H3
weight = 60 lbs
size = H 2' X  W 1'
(never tested at sea)

1739
H2 completed
1740
Harrison started work on H3
1742
death of Halley; James Bradley (1693-1762) appointed third Astronomer Royal
1749
Harrison awarded the Royal Society's prestigious Copley medal
1757
most of the work on H3 completed
1769
H4 completed

H4
weight = 3 lbs
size = 5 in. diameter
1761-2
first voyage to test H4 made to Jamaica on the Deptford

by determining their position at sea using H4, the crew of the Deptford was able to correct the ship's course and avoid delays that would have resulted had they relied solely on estimates based on traditional methods

1763
Nevil Maskelyne (1732-1811) published the first Mariner's Guide
1764
second voyage to test H4 made to Barbados on the Tartar (return to England on the New Elizabeth).
1765
Maskelyne appointed fifth Astronomer Royal

H4 examined by committee appointed by Board of Longitude

Harrison awarded half of longitude prize money!!

Board ordered Harrison to turn over--

  • H4
  • drawings
  • written explanations of mechanisms 
1766
Harrison ordered to turn over H1, H2, and H3

H1 is dropped and damaged in transit

1767
Larcum Kendall requested to make copy of H4

Harrison began work on H5

1770
Kendall completed H4 copy called K1
  • K1 used by Capt. James Cook on his second voyage (1772-1775)
Harrison completes work on H5, improved version of H4 
1772
Harrison wrote to King George III
1773
Harrison given £8,750 by special act of parliament
1774
new act of parliament set out terms for winning the prize; all entries must:
  • be submitted in duplicate
  • undergo trials of one year testing at Greenwich
  • be further tested on at least two sea voyages of Board's choosing
1776
death of Harrison

Rupert T. Gould (1890-1948) and H2
Gould discovered H1 in 1920 and spent 13 years restoring all the Harrison clocks to their original condition.

 
Go to:
  • The World, or Treatise on Light (1629-1633), by René Descartes (1596-1650)
  • The Description of a New World, Called The Blazing World (1666), by Margaret Cavendish, Duchess of Newcastle (1623-1673)
  • Conversations on the Plurality of Worlds (1686), by Bernard le Bovier de Fontenelle (1657-1757)
  • Micromegas:  A Tale of Interplanetary Travel (1752), by Voltaire (François Marie Arouet; 1694-1778)
  • An Original Theory or New Hypothesis of the Universe (1750), by Thomas Wright (1711-1786)
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