An octant is an astronomical instrument used in measuring the angles of heavenly bodies such as the sun, moon and stars at sea in relation to the horizon. This measurement could then be used to calculate the altitude of the body measured, and then the latitude at sea could also be calculated. The angle of the arms of an octant is 45 degrees, or 1/8 of a circle, which gives the instrument its name. Two men independently developed the octant around 1730: John Hadley (1682–1744), an English mathematician, and Thomas Godfrey (1704–1749), a glazier in Philadelphia. While both have a legitimate and equal claim to the invention, Hadley generally gets the greater share of the credit. This reflects the central role that London and the Royal Society played in the history of scientific instruments in the eighteenth and nineteenth century's. There were also two others who are attributed to having created octanes during this period, Caleb Smith, an English insurance broker with a strong interest in astronomy (in 1734), and Jean-Paul Fouchy, a mathematics professor and astronomer in France (in 1732) In 1767 the first edition of the Nautical Almanac tabulated lunar distances, enabling navigators to find the current time from the angle between the sun and the moon. This angle is sometimes larger than 90°, and thus not possible to measure with an octant. For that reason, Admiral John Campbell, who conducted shipboard experiments with the lunar distance method, suggested a larger instrument and the sextant was developed. From that time onward, the sextant was the instrument that experienced significant development and improvements and was the instrument of choice for naval navigators. The octant continued to be produced well into the 19th century, though it was generally a less accurate and less expensive instrument. The lower price of the octant, including versions without a telescope, made it a practical instrument for ships in the merchant and fishing fleets. One common practice among navigators up to the late nineteenth century was to use both a sextant and an octant. The sextant was used with great care and only for lunar sightings while the octant was used for routine meridional altitude measurements of the sun every day. This protected the very accurate and pricier sextant while using the more affordable octant for general use where it performs well. The invention of the octant was a significant step in providing accuracy of a sailors latitude position at sea and his vessels distance from land when taking sightings of land-based landmarks.Octant with metal handle, three different colored shades are attached, in wooden wedge-shaped box lined with green felt. Key is attached. Two telescope eyepieces are in box. Some parts are missing. Oval ink stamp inside lid of box, scale is graduated to 45 degrees. Ink stamp inside lid of box "SHIPLOVERS SOCIETY OF VICTORIA. LIBRARY"instrument, flagstaff hill, warrnambool, shipwrecked coast, flagstaff hill maritime museum, maritime museum, shipwreck coast, flagstaff hill maritime village, great ocean road, octant, navigation, nautical instrument, navigation instrument, john hadley, sextant, astronomical instrument

An Octant is a doubly reflecting navigation instrument used primarily by sailors to measure the angular distance between two visible objects and was a forerunner of the sextant. The name comes from the Latin octo, or "one-eighth of a circle," for the Octan'ts arc which spans 45°, or one-eighth of a circle. The primary use of an Octant is to measure the angle between an astronomical object and the horizon for celestial navigation. The estimation of this angle, is known as sighting or shooting the object, or taking a sight. The angle, and the time when it was measured, can be used to calculate a position line on a nautical chart (latitude), for example, sighting the Sun at noon or Polaris at night (in the Northern Hemisphere) gives an angle by which the latitude can then be estimated. Sighting the height of a landmark on land can also give a measure of distance. This fine octant once belonged to Captain Farquhar Chisholm and was donated by his granddaughter, Margaret Ruth Greer (nee Chisholm, born 1914). The label inside the Octant's box reads “Thomas L. Ainsley, Instrument Maker … etc”. Farquhar Chisholm was born in 1832 in Inverness, Scotland. He regularly sailed on perilous voyages between Quebec, Canada and the Baltic ports of Europe. In 1854 he migrated to Australia during the Gold Rush, to a place called Fiery Creek (near Beaufort Victoria) where he was fairly successful in his quest for gold. In the years of the Great Gold Rush, it was said that there were over 40,000 diggers in the goldfields of the Beaufort area! In 1857 having made sufficient money, he hired another crew and returned to Clachnacuddin, Inverness shire, Scotland and in that same year, he studied and obtained his Master Mariner Certificate (which would have included the use of an octant for navigation). He was appointed to Mr George (or James) Walker, as commander of his sailing ship, the 3-masted ELIZABETH, built 1859 and known as “The Walker barque”. In 1870 he married, then in 1887 returned to Australia with his wife and children (Kenneth Chisholm (1871), Mary Bremner Chisholm (1873), Margaret Hood Chisholm (1874), Farquhar Chisholm (1878)). They arrived in Port Melbourne, Victoria and sadly, only six weeks after landing, his wife Caroline passed away (in Geelong,1888). In 1900 Capt. Chisholm lived in Camperdown (Victoria) and not long after this his daughter Margaret died of consumption. In his later years, he went to live in the manse of St. Paul’s Presbyterian Church, Wangaratta, with his son, Rev. Farquhar Chisholm. He died there on Sat, 23rd March 1912, 80 years old. He was known as “… quiet, unobtrusive and competent, respected by all with whom he came in contact”. Some other members of Captain Chisholm’s family are; his older son Kenneth Chisholm, who was a contractor in Camperdown; a nephew Donald Macintosh (of 23 Douglas Row, Inverness); a grandson Brian Jones (son of Caroline Belle-Jones nee Chisholm, who lived in Camperdown in the earlier part of her life).The octant, the forerunner of the sextant, was a significant step in providing accuracy of a sailors latitude position at sea & his vessels distance from land when taking sightings of land-based landmarks.Octant, once belonging to Captain Farquhar Chisholm. Wedge shape (the size of an eighth of a circle), made of wood, glass and metal. Used in the 1880s. Maker’s name across centre “L. SIMON - - - SHIELDS”. Three (3) light filtering, coloured glass shades. Two (2) eyepieces. Scale attached for measuring angles. Label inside the fitted, wedge-shaped case "Thomas L. Ainsley, Optician"Label inside case "Thomas L. Ainsley, Optician" Maker’s name across centre “L. SIMON - - - SHIELDS”.flagstaff hill, warrnambool, shipwrecked-coast, flagstaff-hill, flagstaff-hill-maritime-museum, maritime-museum, shipwreck-coast, flagstaff-hill-maritime-village, maritime navigation, navigation instrument, migration, captain chisholm, farquhar chisholm, sailing ship, the elizabeths, thomas l. ainsley, l. simons, shields england, octant, john hadley, chisholm

Two items relating to the Ormond Uniting Church (former Thomson Memorial Presbyterian Church): 1/ a book named "The Ormond Faith Story - The History Of The Ormond Uniting Church Centenary Edition 1903 – 2003". The front cover includes a colour photograph of the Church and the back cover includes a list of the Ministers during that time period. The Contents include several black and white photographs and an Appendices written by Rev Bill Morgan, Rev. Rod Horsfield, Rev. Robert Mcutchen and Rev. John Lamont, on what Ormond means to them. 2/ a black and white photograph of three ladies inscribed on the back as "Ormond Uniting Church Drop-in Centre, Cnr North & Booran Rds., Caulfield. Sept 84"A5-sized printed book of 64 pages plus colour back (photos of 9 men around Uniting Church insignia)and front (in red border is a colour photo of the Church) covers, with black and white images on the inside of these covers. It is mostly printed text with a number of black and white photos.ormond uniting church, anthony street, centenary edition, merton hall, anglican, maud street, presbyterian, wheatley road, methodist, ocean street, saint cuthberts, beattie james rev., jones hugh rev, chalinor john rev., hadley vincent rev., broughton david rev., morgan william rev., mcutchen robert rev., lamont john rev., horsfield rod rev., tregear george rev., kirkside independant living units, uniting church inaugurated, kids of the uniting church australia, kuca, after school program, saint kevins catholic church, father crimin, caulfield adult learning centre, daley daniel rev., green kevin rev, probin david rev, glen orme avenue, ormond, caulfield, plaza cinema, north road, manse, booran road, sunday school, glen orme, ladies church aid, ladies guild, dromana, playgroup, ucaf, booran road hall, fraser street hall, mordialloc, ormond park, new hall, reid christina rev., lamont john rev, cricket, tennis, glen orme avenue methodist church, ormond presbyterian church, st kevin’s catholic church, glen huntly presbyterian church, malane's corner, market gardens

A sextant is an astronomical instrument used to determine latitude and longitude at sea by measuring angular distances, especially the altitudes of the sun, moon, and stars. It is a doubly reflecting navigation instrument and used mainly by sailors to measure the angular distance between two visible objects. The name comes from the Latin sextans, or “sixth part of a unit,” because the sextant’s arc can be 60° or 120° of a circle depending on the model used. The primary use was to measure the angle between an astronomical object and the horizon for the purposes of celestial navigation. The estimation of this angle is known as sighting or shooting the object, or taking a sight. This angle and the time when it was measured is used in order to determine Greenwich Mean Time and hence longitude. Sighting the height of a landmark on land can also give a measure of distance from that object. History: The development of the sextant was as an improvement over the octant, an instrument designed to measure one's latitude. The octant was first implemented around 1731-present but can only measure angles up to 45°. As larger angles were needed to allow the measurement of lunar objects - moon, stars and the sun - at higher angles, the octant was superseded by the sextant. The sextant is a similar instrument but better made and allows larger angles from 60° to 120°. This improvement allows distances to be accurately calculated thereby giving longitude when used with a chronometer. The sextant was derived from the octant in 1757, eventually making all previous instruments used for navigational positioning obsolete. The sextant had been attributed to by John Hadley (1682–1744) and Thomas Godfrey (1704–1749), but reference to the sextant was also found later in the unpublished writings of Isaac Newton (1643–1727). Earlier links can be found to Bartholomew Gosnold (1571–1607) indicating that the use of a sextant for nautical navigation predates Hadley's implementation. In 1922, the sextant was modified for aeronautical navigation by Portuguese navigator and naval officer Gago Coutinho. It should be noted that the octant and quadrant are in the same family as they were, and all are, regarded as sextants. The sextant is representative of it's type and although not fully complete it demonstrates how 18th,19th and 20th century mariners determined their latitude and longitudinal to determine their position on a chart, allowing them to navigate there way across the world's oceans. It also demonstrates the skill and workmanship of the early instrument makers that operated scientific instrument businesses from London and other areas of England to provide most of the navigational instrumentation used by commercial and military navies of the time.Sextant with square, fitted box of polished wood, "Hezzanith" brand. Box contains many parts for the sextants use. On certificate "Heath & Co, London. Sextant Number Y 822". Catch on lid "DEFIANT LEVER" and "PATENT NUMBER 187.10". Maker's certificate is attached to the inside of the box.flagstaff hill, warrnambool, shipwrecked-coast, flagstaff-hill, flagstaff-hill-maritime-museum, maritime-museum, shipwreck-coast, flagstaff-hill-maritime-village, sextant box, sextant, hezzanith, heath & co, navigational instrument, george wilson heath, astronomical instrument, instrument manufacturers, scientific instrument, navigation, celestial navigation, octant, quadrant, lunar navigation

An Octant is a doubly reflecting navigation instrument used primarily by sailors to measure the angular distance between two visible objects and was a forerunner of the sextant. The name comes from the Latin octo, or “one-eighth of a circle,” for the Octant’s arc which spans 45°, or one-eighth of a circle. The primary use of an Octant is to measure the angle between an astronomical object and the horizon for the purposes of celestial navigation. The estimation of this angle is known as sighting or shooting the object, or taking a sight. The angle, and the time when it was measured, can be used to calculate a position line on a nautical chart (latitude), for example, sighting the Sun at noon or Polaris at night (in the Northern Hemisphere) gives an angle by which the latitude can then be estimated. Sighting the height of a landmark on land can also give a measure of distance. History: The principle of the Octant as an instrument to measure ones latitude was first implemented around 1742-present but was superseded by the improvement of the octant to a sextant, a very similar instrument, better made and able to measure bigger angles 120°, allowing the measurement of Luna distances to give longitude when used with an accurate chronometer. The sextant started to appear around 1730 and had been attributed to by John Hadley (1682–1744) and Thomas Godfrey (1704–1749), but reference to the sextant was also found later in the unpublished writings of Isaac Newton (1643–1727). Earlier links can be found to Bartholomew Gosnold (1571–1607) indicating that the use of a Sextant for nautical navigation predates Hadley's implementation. In 1922, the sextant was modified for aeronautical navigation by Portuguese navigator and naval officer Gago Coutinho. Henry Hemsley was a lesser-known instrument maker and optician working in London in the late 17th and early 18th century. However, it should be noted that there were two Henry Hemsley opticians and instrument makers around this period. (Henry Hemsley 1, 1786-89, who had premises at 85 Fleet St London and Henry Hemsley 2, 1828-56), whose workshop was at 135-138 Radcliff Highway London. Therefore, based on the inscribed workshop address Henry Hemsley 2 is responsible for making this example.The octant is representative of its type and although not fully complete it demonstrates how 18th and 19th-century mariners determined their latitude on a chart to navigate their way across the world's oceans in the 18th and 19th century. It also demonstrates the skill and workmanship of the early instrument makers that operated from London at this time and provided most of the navigational instrumentation use by commercial and military navies of the time.Octant, ebony wooden frame and handle. Scale is missing from recess in frame. "H. Hemsley 135-138 Ratliff Highway, London", no box"H. Hemsley 135-138 Ratcliff Highway, London"flagstaff hill, warrnambool, shipwrecked-coast, flagstaff-hill, flagstaff-hill-maritime-museum, maritime-museum, shipwreck-coast, flagstaff-hill-maritime-village, navigation, navigational instrument, instrument used for navigation, sextant, henry hemsley, instrument maker, london, octant

The Sir John Quick Committee was formed in 1991 to commemorate the achievements of Sir John Quick who played a prominent role in the federation of Australia. The Committee aimed to raise awareness of the contribution of Sir John Quick and to ensure that he was recognized for the part he played.Agenda for meeting of the Sir John Quick Committee held on 22.6.1999 with correspondence and reports. Five typed pages on white paper. Report from Secretary re latest updates for the Sir John Quick Museum Project. Letter to Secretary (Les Roberts) from Hadley Sides, re application for funding for the Centenary of Federation Project. dated 1.7.1998. Letter to John Balsillie re next steps for the Sir John Quick Federation project after funding approved.sir john quick committee, federation project, sir john quick federation project.

A5 Booklet - 12 Pagesnon-fictionA record of 100 years of congregational life and work at Scot's Presbyterian Church Dandenong - 1854-1954scots presbyterian church dandenong, rev j a finlay, stuart g brown, e w allison, g g byrne, l r hunt, d j mickle, a h murden, h g twiss, g crawford, angus facey, t fisher, h j godwin, a j gibson, bruce gibson, a hillard, h holcombe, j f hucker, g a ingram, s w laugher, j mckenzie, j w marsh, g e pigdon, j j simester, c taylor, v r tharle, margaret eddy, rev william macdermid, rev hugh buntine, rev james legge, rev john meers, rev vincent f hadley, rev jack a finlay, rev david mcfarlane

Dark brown honour board with gold text shaped like a rectangle with a protrusion at the top to accommodate for a large WHS logo and a PREFECTS heading.PREFECTS 1953 GLENEISE ROSS: B. SOUTHGATE,W. KNEEBONE, D. BARR, B. BRADSHAW, F. BRISBANE, R. BRYANT, E. CANING, M. LEAN, R. MACAULAY, C. PARK. DOUGLAS McLAUGHLIN: L. BARR, P. DINSDALE, J. HERRIN, T. PAPPAS 1954 CORAL PARK: J. BISHOP, D. CIRUTO, M. COCHNEAS, S. HERBLE, A. SAVAGE, D. STANDISH, D. WHITE. JOHN EMSLIE: C. BOURKE, D. ELLIS, P. STEVENS, W. STUDHAM 1955 SHIRLEY HEBERLE: D. CIRCITO, J. BISHOP, L. BRISBANE, E. CLARK, A. KENTMANN, J. PETTERSON, G. TUDDENHAM. JOHN BELL: E. JONES, J. SONNEMANN, W. STUDHAM 1956 JILL PETTERSON: G. TUDDENHAM, V. CROWTHER, M. DERRICK, L. HEBERLE, L. HOWELL, C. LEIGH, M. VINCENT. ERNEST JONES: J. SONNEMANN, B. HOPPER, K. SAVAGE 1957 MARION VINCENT: C. LEIGH, M. DERRICK, R. HOLMES, I. LEAN, E. MARENGO, B. NICOLL, N. THOMAS. KENNETH SAVAGE: K. HADLEY, J. HALL, K. JOHNSON, D. McDONAGH 1958 ROSEMARY HOLMES: P. McDONALD, J. MORELY, B. PRIESTLY, A. BOWFITCH, E. MAUGHER, C. EMSLIE, B. GLOVER, S. BRADSHAW. KENNETH HADLEY: D. McDONAGH, N. ROSENGREN, R. SQUIRE 1959 MARGOT FISHER: C. PROBYN, C. EMSLIE, N. JONES, J. PRATT, W. ROBERTS, M. SCAMBLER, L. SIMMONS, J. THOMPSON. ROSS SQUIRE: A. BARR, B. PENDLEBURY, K. SCAMMELL, T. TONURI 1960 BARBARA JOB: N. JONES, L. BENSON, S. EDGAR, R. FERRARI, H. GIBB, M. GROSSMAN, C. KNEEBONE, F. NEWLAND, D. POLMEAR. NEIL STEWART: B. SUTTON, L. FRY, M, KNEENAN, J. STONE, G. WATSON 1961 MARGARET DUNDAS: S, EDGAR, E. AMERY, R. ANGUS, D. BRADBURY, V. CROSS, S. EVERTON, W. GERRETT, D. GIBB, E. MORRISS, S. NICHOLL, J. POWELL, R. REID, J. SUTTON, M. WHITE, R. WOOD. FRANK COBHAM: M. KEENAN, G. DUSTIN, D. FLINN, R. GROWLING, L. LANG,B. RAE, R. STONE, L. SULLIVAN, J. WELCH 1962 SHIRLEY NICOLL: V. CROSS, J. ADAMTHWAITE, C. BADGER, H. CAMERON, B. CROCKETT, C. HENDERSON, J. LANG, N. KINIBURGH, H. MORRIS, M. OSMOND, J. POWER, B. REITH, R. TANSLEY, C. TIPPETT, J. WHITEHEAD. LAURIE LANG: D. FLINN, P. BENNETT, R. BOYD, G. DUNSTEN, G. GOWLING, R. McCONCHIE, C. SQUIRE, R. STONE, L. SULLIVAN 1963 CHERYL TIPPETT: HELEN MORRIS, R. BENTON, R. BERRY, H. CAMERON, H. CROCKETT, R. EDE, R. FERGUSON, N. KINIBURGH, J. LANG, M. McKENZIE, B. MUNCEY, M. OSMAND, V. ROSEGREN, E. STANTON, J. STEWART. LANCE SULLIVAN: GEOFFREY7 DUSTIN, B. HANSEN, M. IRVINE, R. McCONCHIE, N. MARTIN, W. SCHULTZ, C. SQUIRE, C. STONE, R. SWAN

This Day or Night telescope, made by John Dollond, was designed for use in a range of lighting conditions, as its name suggests. Telescopes are optical instruments that make distant objects appear larger and closer, thereby extending the range of what the human eye can observe. The development of the telescope was gradual, shaped by a series of important advances in optical science. In 1608, the Dutch spectacle-maker Hans Lippershey discovered that when two lenses were held apart in a particular way, distant objects appeared closer. He applied for a patent for this invention, creating the first documented telescope. In 1668, Isaac Newton produced the first successful reflecting telescope, using a two-inch concave spherical mirror. This marked a major step forward, demonstrating that mirrors could overcome some of the limitations of lenses and greatly improve magnification. Further progress followed in the eighteenth century. In 1729, Chester Moor Hall developed the achromatic lens by combining two types of glass with different refractive properties. This reduced colour distortion and produced a sharper image, although some edge distortion remained. That same year, the Scottish instrument maker James Short developed parabolic and elliptical mirrors that were better suited to reflecting telescopes because they reduced optical distortion. Building on these advances, John Dollond improved the achromatic objective lens by placing a concave flint-glass lens between two convex crown-glass lenses, considerably enhancing image quality. Maker’s information. John Dollond (1707–1761), of London, was a maker of optical, scientific and astronomical instruments best known for developing the achromatic refracting telescope. He also introduced a practical heliometer, a telescope fitted with a divided lens that could be used to measure the Sun’s diameter and the angular distance between celestial bodies. The son of Huguenot refugees, Dollond first learned the family trade of silk weaving before turning his attention to optics and astronomy, in which he became highly skilled. In 1753, Dollond patented his improved lenses, the same year he had introduced the heliometer. In 1761, John Dollond was appointed as optician to George III and the Duke of York. He was also elected a Fellow of the Royal Society in May 1761, but died suddenly later that year in November. His share of the patent then passed to his eldest son, Peter. In later disputes between Peter Dollond and rival London opticians who challenged the patent, Peter consistently argued that, whatever earlier precedents may have existed, his father had independently developed a practical method for producing achromatic lenses through his command of Newtonian optics. By successfully defending the patent, the Dollond firm became one of the leading manufacturers of optical instruments. During the eighteenth and nineteenth centuries, the name ‘Dollond’ was at times used almost generically to mean ‘telescope,’ reflecting the firm’s reputation. Genuine Dollond telescopes were regarded as among the finest available. Peter Dollond (1731–1820) was the driving force behind the family business. He had founded a small optical business in 1750 on Vine Street, Halton Garden, with his father's guidance. The success of the business led to his father joining him in partnership in 1752. In 1959, J Dollond and Son opened a shop on The Strand, London. Dollonds appear to have produced both reflecting and refracting telescopes, and they possessed the technical skill to manufacture significant numbers of lenses largely free from chromatic aberration. In 1766, Peter went into partnership with his younger brother, John, and they traded under the name P and J Dollond. They supplied optical instruments for Captain Cook and George Hadley, an English lawyer and Meteorologist. In 1769, Captain Cook travelled with a Dollond telescope on the voyage to observe the Transit of Venus. Other notable customers included Thomas Jefferson and Admiral Lord Nelson. In 1781, Peter Dollond made bifocal spectacles. In 1804, young John Dollond passed away. The following year, Peter Dollond went into partnership with his nephew, George Huggins, and Huggins legally changed his surname to Dollond, and the firm remained P and J Dollond. In the early 20th century, the company sold film cameras. The firm remained in the hands of Dollond family members until 1927, when Dollond & Co. merged with James Aitchison & Co. to form Dollond & Aitchison, the well-known high street chain of opticians, which continued making and selling prescription spectacles. Now fully part of Boots Opticians, the company no longer manufactures instruments and operates exclusively as a retail business. The telescope in the collection is an excellent example of one of Dollond’s early library telescopes. Its association with one of eighteenth-century England’s leading innovators in optical development gives it considerable historical significance and makes it an important object within the collection. John Dollond’s experiments in optics advanced the understanding of the divergent properties of lenses and made a lasting contribution to the development of practical optical science. His work helped lay the foundation for major improvements in the design and performance of optical instruments. In his own time, Dollond was celebrated as the “Father of practical optics” and received widespread recognition for his achievements in the field. Dollond telescopes were associated with the renowned mariners, Captain James Cook and Admiral Lord Nelson Telescope: Dollond's Telescope, Day or Night model navigational instrument. Telescope is mounted on wooden tripod stand that has folding legs. Brass telescope with leather sheath over barrel, adjustable angle fitting with brass wing nuts that join the legs to the top frame, which is then joined to the telescope pole by an adjustable screw fitting. Manufactured by Dollond, London. Inscription reads "Dollond London, Day or Night" and "DOLLOND LONDON"flagstaff hill maritime museum and village, maritime museum, maritime village, great ocean road, warrnambool, optical instrument, achromatic telescope, heliometer, light refraction, instrument maker, lens, transit of venus, astronomical telescope, concave lens, scientific instrument, navigation, navigational instrument, astronomy, dollond, dollond london, john dollond, peter dollond, dollond telescope, day or night telescope, floor-standing telescope, library telescope, hans lippershey, isaac newton, chester moor hall, james short, captain cook, thomas jefferson, admiral lord nelson, dollond & co, aitchison & co, dollond & aitchison, boots opticians, george iii, duke of york, george huggins, george dollond, p and j dollond, j dollond and son, spectacles, cameras

Photo from the estate of the late Charles Vincent (Vin) Sheahan, Born 12/01/1934 (Kilmore), Died 02/09/1990 (Cheltenham). Black and white picture Grade III & IV 1940 Charlton Primary School No 1480 Back Row ?? , Arthur Brambley, Ray Hommelhoff, Des Lyons, Jim Wall, Kevin Rosewall, Ted Allen, Howard Veins, Ian Watson, Robert Johnson 2nd Back Row Margaret Grose, ...... Sheffield, Joan Procter, Jean Brambley, Margaret Beanland, Pauline Dowling, ?????, Wilma Dowling 3rd Back Row ?????? , Joan Turner, Patsy Dew, Merle Ritchie, Faye Clarke, Rae Retallick Front Ian Kirkbride, John Pelchen, Keith Jackman, Norman Barton, Vince Sheahan, Hadley Perry, Kevin Smallcharlton primary school, arthur brambley, ray hommelhoff, des lyons, jim wall, kevin rosewall, ted allen, howard veins, ian watson, robert johnson, margaret grose, joan procter, jean brambley, margaret beanland, pauline dowling, wilma dowling, joan turner, patsy dew, merle ritchie, faye clarke, rae retallick, ian kirkbride, john pelchen, keith jackman, norman barton, vince sheahan, hadley perry, kevin small