Tuesday, May 29, 2012

European Navigation

Route Finding

The art of Navigation is as much about knowing where you are and having moved knowing where you have arrived.
On the Land this knowledge was never difficult since there were usually named geographical and structural reference terminal and way points. Having noted these a return route is never a difficult task.
On the Oceans the beginning of a voyage has a reference harbour starting point. Once the craft has lost all land sight around the horizon reference points rely on an estimation of the heading direction and speed of travel.
The combined effects of wind, ocean currents and swells make the estimation of speed and direction a matter of experience and error correction. Frequently errors are cancelled but without accurate fixing of geographical position the errors accumulated can often end in disaster.
Although the Arabs and Europeans developed instruments to navigate in the Mediterranean Sea, Indian Ocean and lands south and north of the Straits of Gibralta the voyages were fairly modest in endeavour.
Many ships have foundered on rocky shores because of faulty navigation. This became a very important issue in the centuries of global exploration during the 15th to 18th Century when competing European nations sought to gain new lands and exploit the newly discovered riches. Up to the beginning of the 16th Century the Atlantic and Indian Oceans had been explored by European voyagers, mostly during the 15th Century.
The biggest prize was to establish a trade route to the S.E. Asia and it took a Portuguese sailor, Ferdinand Magellan, frustrated with a lack of support from his own ruling King, approached the King of Spain, Charles 1st, for support to find a route around Cape Horn to S.E. Asia. Magellan found a passage through the islands of the Horn and set sail North-East on a blissfully calm ocean which he named Pacific. He must have caught a rare calm week or two in a normally stormy location. He kept sailing missing all the islands of Polynesia until he sighted Guam, 14,400 km in a straight line from the Straits of Magellan. Unfortunately he got caught up in a local war in the Philippine Island of Mactan while assisting the Chief of the neighbouring Island of Cebu and was killed. His 2nd-in-Command Sebastian del Cano took over and completed the circumnavigation of the globe returning to Spain around the Cape of Good Hope. 
The commercial activities of Portugal in the early 15th century was a leap in progress in practical navigation. Trade expeditions were sent out by Henry the Navigator and led first to the discovery of the islands Porto Santo NE Madeira in 1418, the rediscovery of the Azores in 1427, the discovery of the  Cape Verde Islands in 1447 and Sierra Leone in 1462.  Henry worked to systemize the practice of navigation. In order to develop more accurate tables on the sun's declination he established an observatory at Sagres. Combined with the empirical observations gathered in oceanic seafaring, mapping winds and currents, Portuguese explorers took the lead in the long distance oceanic navigation. Henry's successor, John II continued this research, forming a committee on navigation. This group computed tables of the sun's declination and improved the mariner's astrolabe, believing it a good replacement for the cross-staff. These resources improved the ability of a navigator at sea to judge his latitude. However the lack of a means to gauge longitude on long voyages lead to huge errors in positin fixing. On the voyage of Magellan when the ships eventually arrived in the Philippines one navigator Alvo was nearly 53 degrees in error in his determination of logitude.  
http://en.wikipedia.org/wiki/History_of_navigation accessed 30 May 2012

Magellan navigational instruments consisted of 35 compasses, a wooden astrolabe, six metal astrolabes, 21 wooden quadrants, and 18 hour glasses.

The Astrolabe

An astrolabe
 An 18th Century Persian astrolabe – maker unknown. The points of the curved spikes on the front rete plate, mark the positions of the brightest stars. The name of each star being labeled at the base of each spike. The back plate, or mater is engraved with projected coordinate lines. From the Whipple Museum of the History of Science in Cambridge.


A wooden quadrant

For marine navigation, the earliest examples of the quadrant were found around 1460. They were not graduated in degrees but rather had the latitudes of the most common destinations directly scribed on the limb. When in use, the navigator would sail north or south until the quadrant indicated he was at the destination's latitude, turn in the direction of the destination and sail to the destination maintaining a course of constant latitude. After 1480, more of the instruments were made with limbs graduated in degrees.

http://en.wikipedia.org/wiki/Quadrant_(instrument) accessed 12/6/2012


The Cross-staff
A Jacobs cross staff
The cross-staff was difficult to use. In order to get consistent results, the observer had to position the end of the pole precisely against his cheek. He had to observe the horizon and a star in two different directions while not moving the instrument when he shifted his gaze from one to the other. In addition, observations of the sun required the navigator to look directly at the sun. This could be a painful exercise and made it difficult to obtain an accurate altitude for the sun. Mariners took to mounting smoked-glass to the ends of the transoms to reduce the glare of the sun.

The Backstaff
Backstaff is the name given to any instrument that measures the altitude of the sun by the projection of a shadow. It appears that the idea for measuring the sun's altitude using back observations originated with Thomas Harriot.[2] Many types of instruments evolved from the cross-staff that can be classified as backstaves. Only the Davis quadrant remains dominant in the history of navigation instruments. Indeed, the Davis quadrant is essentially synonymous with backstaff. However, Davis was neither the first nor the last to design such an instrument and others are considered here as well.

 
 
The Davis Quadrant as it evolved by the mid 17th century.
 
Captain John Davis invented a version of the backstaff in 1594. Davis was a navigator who was quite familiar with the instruments of the day such as the mariner's astrolabe, the quadrant and the cross-staff. He recognized the inherent drawbacks of each and endeavoured to create a new instrument that could reduce those problems and increase the ease and accuracy of obtaining solar elevations.
The instrument that is now identified with Davis is shown above.  This form evolved by the mid-17th century. The quadrant arc has been split into two parts. The smaller radius arc, with a span of 60°, was mounted above the staff. The longer radius arc, with a span of 30° was mounted below. Both arcs have a common centre. At the common centre, a slotted horizon vane was mounted (B). A moveable shadow vane was placed on the upper arc so that its shadow was cast on the horizon vane. A moveable sight vane was mounted on the lower arc (C).
Thus Davis was able to optimize the construction of the quadrant to have both a small and a large arc, allowing the effective accuracy of a single arc quadrant of large radius without making the entire instrument so large. This form of the instrument became synonymous with the backstaff. It was one of the most widely used forms of the backstaff. Continental European navigators called it the English Quadrant.

http://en.wikipedia.org/wiki/Backstaff accessed 21/6/2012




Mercury in Aviation

Mercury in 20th Century Aviation

The Short Mayo Composite was a piggy-back long-range seaplane/flying boat combination produced by Short Brothers to provide a reliable long-range air transport service to the United States and the far reaches of the British Empire and Commonwealth.

The Short-Mayo composite project comprised the Short S.21 Maia, which was a variant of the Short "C-Class" Empire flying-boat fitted with a trestle or pylon on the top of the fuselage to support the Short S.20 Mercury. Although generally similar to the Empire boat, Maia differed considerably in detail: the hull sides were flared and had "tumblehome" rather than being vertical as on the Empire to increase the planing surface (necessary for the higher takeoff weights); larger control surfaces; an increase in total wing area from 1,500 sq ft (140 m2) to 1,750 sq ft (163 m2); the engines were mounted further from the wing root to clear Mercury's floats and the rear fuselage was swept up to raise the tailplane relative to the wing. Like the Empire boats, Maia could be equipped to carry 18 passengers.  Maia first flew (without Mercury) on 27 July 1937.
The upper component, Mercury, was a twin-float, four-engine seaplane crewed by a single pilot and a navigator, who sat in tandem in a fully enclosed cockpit. There was capacity for 1,000 lb (456 kg) of mail. Mercury's flight controls, except for elevator and rudder trim tabs, were locked in neutral until separation. Mercury's first flight, also piloted by Parker, was on 5 September 1937.
The first successful in-flight separation was carried out from the Shorts works at Borstal, near Rochester, on 6 February 1938. Following further successful tests, the first transatlantic flight was made on 21 July 1938 from Foynes, on the west coast of Ireland, to Boucherville, Montreal, a flight of 2,930 miles (4,714.4 km). Maia, flown by Captain A.S. Wilcockson, took off from Southampton carrying Mercury piloted by Captain Don Bennett. As well as Mercury, the launch aircraft Maia was also carrying 10 passengers and luggage. Mercury separated from her carrier at 8 pm to continue what was to become the first commercial non-stop East-to-West transatlantic flight by a heavier-than-air machine. This initial journey took 20 hrs 21 min at an average ground speed of 144 mph (232 km/h).
A YouTube movie of the progress to launch and eventual arrival in Montreal can be seen at:
www.youtube.com/watch?v=bYtazEBQ1K8
http://en.wikipedia.org/wiki/Short_Mayo_Composite accessed 28th May 2012

Mercury in Mythology

Mercury was the Messenger who wore winged sandals, and a god of trade, thieves, and travel, the son of Maia and Jupiter in Roman mythology. His name is related to the Latin words merx, mercari (to trade), and merces (wages). Mercury's temple in the Circus Maximus in Rome was built in 495 BC as a chariot racing arena with viewing for 150,000 spectators. This was a fitting place to worship a swift god of trade and travel, since it was a major center of commerce as well as a racetrack. Since it stood between the plebian stronghold on the Aventine and the patrician center on the Palatine, it also emphasized the role of Mercury as a mediator.
  



In astronomy Maia is a star in the constellation Taurus and is the fourth brightest star in the Pleiades open star cluster, after Alcyone, Atlas and Electra, in that order. The name Maia originates with the Greek: Μαῖα and Latin: Maia. She is one of the daughters, and the most beautiful, of  Atlas and Pleione in Greek mythology - stars which are also included in the Pleaides star cluster (see below). Maia is a blue giant of spectral type B8 III, and a mercury-manganese star.
M45map.jpg

Maia was seduced by Jupiter (Zeus) and gave birth to Mercury. 
Maia and Hermes (Mercury)
 


According to Greek myth, the seven daughters Electra, Maia, Taygete, Alcyone, Celaeno, Asterope and Merope were wandering through the woods one day, they were spied by Orion, who gave chase. To save them from Orion’s dishonorable intentions, Zeus transformed them into stars and placed them in the sky. A number of ancient temples on the Acropolis in Athens face the direction where the Pleiades rise.

In Maori legend Pleiades, or Matariki literally means the ‘eyes of god’ (mata ariki) or ‘little eyes’ (mata riki). Some say that when Ranginui, the sky father, and Papatūānuku, the earth mother were separated by their offspring, the god of the winds, Tāwhirimātea, became angry, tearing out his eyes and hurling them into the heavens. Others say Matariki is the mother surrounded by her six daughters, Tupu-ā-nuku, Tupu-ā-rangi, Waitī, Waitā, Waipuna-ā-rangi and Ururangi. One account explains that Matariki and her daughters appear to assist the sun, Te Rā, whose winter journey from the north has left him weakened.

Matariki comes into view low on the north-eastern horizon, appearing in the tail of the Milky Way in the last days of May or in early June, just before dawn. This heralds the Māori New Year.
Various Māori tribes celebrated Matariki at different times. Some held festivities when Matariki was first seen in the dawn sky; others celebrated after the full moon rose or at the beginning of the next new moon. For all tribes, the importance of Matariki has been captured in proverbs and songs, which link it with the bright star Whānui (Vega):
Ka puta Matariki ka rere Whānui.
Ko te tohu tēnā o te tau e!
Matariki re-appears, Whānui starts its flight.
Being the sign of the [new] year!
Matariki is also associated with the winter solstice. It appears when the sun, drifting north on the shortest day in winter, reaches the north-eastern end of the horizon. The sun then turns around and begins its journey south.

http://en.wikipedia.org/wiki/Mercury_(mythology)/ accessed 28th May 2012
http://www.teara.govt.nz/en/matariki-maori-new-year/1 accessed 28th May 2012
http://en.wikipedia.org/wiki/Circus_Maximus/ accessed 28th May 2012
http://astrolosophy.net/universe/2011/05/maia_may_2011/ accessed 30th May 2012

Saturday, May 26, 2012

Mercury and Maia

Mercury Navigators

Whitianga has a long history of connections with marine navigators, from Kupe to Cook to Tupaia.
Capt. James Cook claimed New Zealand for the British Crown on 15th November 1769 in the Bay he named Mercury Bay (Te Whanganui-a-Hei) where he observed the Transit of Mercury on 9th November. 

Whitianga

The town and land surrounding the Bay has locations and street names reflecting the early explorers and places where they originated.
The full name of the town is Te Whitianga-o-Kupe (or the place where Kupe crossed over). Kupe arrived in Aotearoa in the 10th Century on the canoe Matahourua and named the headland at the northern end of Buffalo Beach and stream which flowed directly out into the Bay Taputapuatea, after the the old temple at Opoa on Ra'iatea, Society Islands. There is a place on Ra'iatea called Hitia'a, in Te Reo this is Whitianga.
In Whitianga there is Kupe Drive, Cook Drive, linked by Whitby Avenue; in Cooks Beach there is Captain Cook Road, Hicks Place, Charles Green Drive, Endeavour Place, Hardy Place, Banks Street and Resolution Rise.
Whitianga has recently been contemplating a Theme for the town and surrounding area and a Navigators Theme has been proposed to reflect the seafaring history of the location.  This and succeeding blogs will build the connections and background for the proposal and follow the development and uptake of the ideas.

The Objectives of the Theme are to:
to create a new focus of activity and enterprise complementing those already existing in the community

to create a major focus on the arts and science in all facets of navigation
to involve everyone who uses navigation every day
to involve all cultures in the area
to use existing geography in the town to create time-line pathways of navigation along the parallel Drives of Cook and Kupe and connected by Whitby Avenue,
to use existing geography in Ferry Landing, Shakespeare’s Cliff and Cook’s Beach
to establish a time-line of Cook’s Voyages along the streets of Cook's Beach
to establish a point of sale for navigation publications and hardware
to establish points of demonstration and use of maritime, aeronautical, terrestrial and celestial navigation
to establish a community activity in national navigation competitions
to establish links to other communities involved in navigation
to establish a navigation centre for tourism with displays of European and Polynesian navigation and viewing theatre
to support education programmes for personal navigation in life
to support links to the Health Navigator groups

http://www.ngatihei.iwi.nz/history.html accessed 27th May 2012
Edwards, Philip (2003) James Cook, The Journals. Prepared from the original manuscript by J.C.Beaglehole for the Hakluyt Society, 1955-67. London, Penguin Books