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  • Thornthwaite, W. H. - Hints on reflecting and refracting telescopes and their accessories
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  • p.15 - vue 17/100
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  • TABLE DES MATIÈRES
  • TABLE DES ILLUSTRATIONS
  • RECHERCHE DANS LE DOCUMENT
  • TEXTE OCÉRISÉ
  • Première image
  • PAGE DE TITRE
    • Preface to the third edition (p.R2)
    • Contents (p.R3)
    • Introduction (p.5)
    • The various forms of telescopes. Their construction and advantages (p.7)
    • Refracting telescopes (p.11)
      • The perspective and opera-glasses (p.11)
      • The ordinary refracting telescope (p.12)
      • Stands for refracting telescopes (p.16)
      • Reflecting telescopes (p.19)
        • Direct vision reflectors. The gregorian telescope (p.19)
        • The cassegrainian telescope (p.20)
      • Stands for direct vision reflectors (p.21)
        • Indirect-vision reflectors. Nasmyth's modification of the cassegrainian telescope (p.21)
        • The herschelian telescope (p.22)
        • The newtonian telescope (p.23)
        • Adjustments of a newtonian telescope (p.24)
    • Stands for indirect-vision reflectors (p.31)
      • The alt-azimuth stand (p.31)
      • Equatorial stands (p.36)
      • Horne and thornthwaite's portable equatorial (p.36)
      • Berthon's patent equatorials (p.37)
    • Equatorial adjustments (p.41)
      • To place the Polar Axis in the Méridian (p.41)
      • To correct the Declination Vernier (p.41)
      • To adjust the Polar Axis to the Latitude of Observation (p.43)
      • To test the accuracy in position of the Telescope (p.43)
        • To set the Right Ascension Vernier (p.45)
        • To find a Celestial Object by means of the Declination and Hour Circles (p.46)
        • To convert Mean into Sideral Time (p.47)
        • Table of Refractions (Bessel) (p.48)
        • To adjust the “Finder” (p.48)
    • To silver and polish glass specula (p.49)
      • Apparatus (p.49)
      • To support the Mirror in the Silvering Vessel (p.50)
      • To clean the mirror (p.51)
      • To immerse the mirror (p.51)
      • To prepare the Silvered surface for polishing (p.52)
      • To polish the Silvered surface (p.53)
      • To separete the Mirror from the Wooden Support (p.54)
      • Martin's process of silvering (p.54)
      • Dr. Henry Draper's formula for silvering (p.56)
      • The sugar of milk process for silvering (p.56)
      • General, hints on silvering (p.57)
    • Accessories to the telescope (p.58)
      • Eye-pieces (p.59)
      • Solar eye pieces (p.59)
      • Barlow's lens (p.59)
      • The micrometer (p.60)
      • The double image micrometer (p.61)
      • Berthon's dynamometer (p.61)
      • The astronomical spectroscope (p.62)
      • Horne & thornthwaite's miniature universal spectroscope (p.65)
    • Observatories (p.66)
      • To construct an observatory on the Romsey model (p.67)
      • References to illustrations (p.71)
      • Horne & thornthwaite's astronomical clock (p.72)
      • Hints on observation (p.74)
    • Defining and separating tests (p.78)
    • Light tests (p.79)
    • Catalogue of reflecting and retracting telescops and their accessories (p.81)
      • Achromatic perspective glasses (p.81)
      • Achromatic opera glasses (p.81)
      • Achromatic field glasses (p.81)
      • Achromatic telescopes (p.83)
      • Horne and thornthwaite's binocular telescopes (p.83)
      • Refracting telescopes for astronomical purposes (p.84)
      • Astronomical object glasses (p.87)
      • Astronomical reflecting telescopes (p.89)
      • Silvered-glass specula (p.93)
      • Silvered-glass diagonal mirrors (p.93)
      • The “romsey” observatory (p.93)
      • Silvering and polishing specula (p.94)
      • Apparatus for silvering (p.94)
        • Silvering vessels (p.94)
        • Glass measures (p.94)
        • Chemicals (p.94)
      • Set of silvering apparatus (p.94)
      • Astronomical eye pieces (p.95)
        • Huyghenian construction (p.95)
        • Ramsden's construction (p.95)
        • Aplanatic construction (p.95)
        • Kellner's construction (p.95)
      • Solar eye pieces (p.95)
      • Micrometers (p.95)
      • Astronomical spectroscopes (p.96)
      • Trabsit instruments (p.96)
      • Works on astronomy (p.96)
  • Dernière image
  • Première image
  • PAGE DE TITRE
    • The german equatorial stand (p.17)
    • The victoria equatorial (p.18)
    • The alt-azimuth stand (p.32)
    • Horne and Thornthwaite's equatorial reflector (p.34)
    • Horne and Thornthwaite's portable equatorial reflector (p.35)
    • The berthon equatorial (p.38)
    • The berton equatorial (p.39)
    • The victoria equatorial telescope (p.85)
    • Berthon patent equatorial stand (p.90)
    • The alt-azimuth stand (p.92)
    • Binoclar microscope (p.97)
  • Dernière image
*5

be found in the work of a careful optician, but will result from an accidental circumstance.

The lenses of a telescope should never be cleaned, unless it is absolutely necessary. If dust has settled, first brush it off with a clean dry camel’s hair pencil, and then very gently wipe clean with a piece of very fine wash-leather, or a soft silk or cambric handkerchief. Any material thus employed should be specially kept for this purpose alone, and when not in use carefully protected from dust. Should the lenses require to be removed from their mounts for cleaning, or otherwise, take care that they are correctly replaced. The edges of an object-glass generally have marks which should be placed together. It will hardly require notice that the convex glass always is next the object viewed. Before screwing in any cell or mount, give half a turn in a contrary direction, when the first thread will generally drop home, thus ensuring truth, and avoiding the risk of the threads of the screw being spoiled.

As it is impossible, with our present knowledge, to perfectly correct the secondary spectrum of an object-glass, a slightly coloured image of a bright object is unavoidable. A good glass should give a very slight tinge of bluish purple at focus, and rather more purple within and green without the focal point. Should, however, the object have a red or an orange colour at the focus, and within the focus the expanded disc show a purple centre and red margin, and without a red centre and purple margin, the marginal colours being the most apparent, the object glass is under-corrected for colour. A slight separation of the lenses may tend to diminish this. In an overcorrected lens the colours will be exactly in the reverse order, but nothing can be done by the amateur to correct them.

I have now mentioned all the principal defects of a telescope that an amateur may attempt to remedy, but it will be far better policy for him to ask a practical optician to attempt the correction than to try it himself, as he may do irreparable damage. None of the remedies here mentioned can do the slightest damage if carefully applied.

An optician can generally remove any error except irregular density, by repolishing one or more of the glasses, but as they have been edged from worked discs considerably larger than the object-glass itself, there is a risk of injuring the centering and figure of the lenses if they are worked after being edged. It will therefore be better for the possessor of an inferior object-glass to procure a new one of similar size and focus, or if the imperfect glass is of large size, and it is necessary to have it re-worked, let it also be re-edged to a smaller cell. ~ '




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