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  • Thornthwaite, W. H. - Hints on reflecting and refracting telescopes and their accessories
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  • p.47 - vue 49/100
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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
47

Example : To' find a Virginis (Spica) at 11 o’clock mean time on June 30th, 1875, or at XVII. 35m. 25s. as shown by the sidereal clock.

A. —The declination of Spica on June 30th was io° 30' 43", and the

vernier was set to this position.

B. —The hour-circle which read from W. to E. was revolved till it

read to the upper vernier, the right ascension of Spica XIII. r 8m. 38s.

C. —The telescope was turned, so that the lower vernier read XVII.

35m. 25s. and the star was in the field of view.

If the circle had read from E. to W. the right ascension setting could have been effected thus :—

B. —The hour-circle is revolved till it reads XIII. 18m. 38s. to the

lower vernier.

C. —The telescope is turned till the movable vernier reads XVII.

35m. 25s., and the star is in the field.

Twenty-four hours of sidereal time may be roughly estimated as four minutes shorter than twenty-four hours of mean time, or a gain of ten seconds every hour; a watch thus regulated will keep fairly correct sidereal time. If time is not accurately known a slight movement in right ascension will often bring the object into the field. The correctness of the local time of any place may be easily ascertained by setting one vernier to the right ascension of a known star in the field, when the other vernier will show correct sidereal time. If this operation is quickly performed, a clock or watch may be accurately set at the commencement of the evening’s work. Time however can be most accurately ascertained by a meridian passage.

Example : Spica being brought in the centre of the field, and the right ascension circle set to XIII. i8m. 38s., the time shown by the other vernier was XVIII. 3m.

To convert Mean into Sidereal Time.

Mean time can be easily converted into sidereal; but data must be obtained from an almanac. Example :—To convert VII 50m. Greenwich mean time to sidereal time on July 10th, 1875 :—

Sidereal time at mean noon, July 1 oth ...VII. 12m. is.

Add sidereal interval for 7I1. 50m. ... VII. 51m. 17s.

Sidereal time

... XV. 3m. 18s.




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