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  • Thornthwaite, W. H. - Hints on reflecting and refracting telescopes and their accessories
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  • p.45 - vue 47/100
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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
45

another star twelve hours distant, and observe the declination error Half this will be the vernier error. The vernier can be altered this amount, and the star refound by again shifting the foot. All that now will be requisite will be to re-adjust the polar axis on a meridian star. Example 3.

Example i.

Meridian East West ... ... a Tauri ... 160 15' read as 160 15' 1 ... a Ursa Majoris 62° 25' ,, 540 20' ... a Andromeda 28° 24' ,, 26° 9' 1 1 Error 0 8° S' 2° 15'

2 | — IO° 20'

Vernier error — 5° io'

Example 2.

Meridian East West ... ... i Cancri ... 290 14' read as 290 14' ... k Bootis ... 52° 24' ,, 5o°4o' ... y Andromeda 410 42' ,, 420 56' Error + 0 1° 44' i° 14'

2 — 3°'

Vernier error — 15'

Example 3.

Meridian East ... West ... ... a Leonis ... 120 36'read as 12° 36' ... i\ Draconis ... 6i° 48' ,, 6i° 48' ... £ Pegasi ... 390 38' ,, 410 24' Error + 0 0 i° 46'

Vernier error 53' 2 + i° 46'

Set vernier to 40° 31' + 53'

The foot was shifted until t Pegasi was in the centre of the field, the vernier altered so that it read 390 38', and finally the latitude screw re-corrected.

To set the Right Ascension Vernier.

The right ascension and hour-circle of an equatorial should always be movable, for, if not, a distinct calculation must be made before each observation. A movable hour-circle is fitted with two verniers, one reading time, and the other right ascension, and one of these can be shifted for preliminary adjustment. Two data are requisite before this can be done. Greenwich time can generally be obtained at the nearest Postal Telegraph Office, but as this will be only correct for places of the same longitude, the longitude of the place of observation can be easily determined from an ordnance map, and the distance converted to time (15' longitude == im time). If the place is east of Greenwich, this amount must be added; if west, the contrary. Accurate mean local time having been thus ascertained, look in an almanac opposite the date of observation for the mean time of transit of a convenient star or planet, which is given for every day of the year.




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