1. Angle of deflection, 0 = 3.5° Distance of the screen from the mirror, D = 1.5 m The reflected rays get deflected by an amount twice the angle of deflection i.e., 20 = 7.0° The displacement (d) of the reflected spot of light on the screen is given as: tan 20 = d/1.5 => d = 1.5 x tan 7° = 0.184 m =Read more

    Angle of deflection, 0 = 3.5°

    Distance of the screen from the mirror, D = 1.5 m

    The reflected rays get deflected by an amount twice the angle of deflection i.e., 20 = 7.0°

    The displacement (d) of the reflected spot of light on the screen is given as:

    tan 20 = d/1.5 => d = 1.5 x tan 7° = 0.184 m = 18.4 cm

    Hence, the displacement of the reflected spot of light is 18.4 cm.

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  2. The following figure shows a Cassegrain telescope consisting of a concave mirror and a convex mirror. Distance between the objective mirror and the secondary mirror, d = 20 mm Radius of curvature of the objective mirror, R1= 220 mm Hence, focal length of the objective mirror, f1= R1/R2 = 110 mm RadiRead more

    The following figure shows a Cassegrain telescope consisting of a concave mirror and a convex mirror.

    Distance between the objective mirror and the secondary mirror, d = 20 mm

    Radius of curvature of the objective mirror, R1= 220 mm

    Hence, focal length of the objective mirror, f1= R1/R2 = 110 mm

    Radius of curvature of the secondary mirror, R2 = 140 mm

    Hence, focal length of the secondary mirror, f2 =R2 /2= 70 mm

    The image of an object placed at infinity, formed by the objective mirror, will act as a virtual object for the secondary mirror.

    Hence, the virtual object distance for the secondary mirror, u = f1-d = 110 -20 =90mm

    Applying the mirror formula for the secondary mirror, we can calculate image distance (v) as:

    1/v + 1/u = 1/f2

    1/v = 1/f2– 1/u

    = 1/70 -1/90 = (9-7)/630 = 2/630

    Therefore ,V = 630/2 = 315 mm

    Hence, the final image will be formed 315 mm away from the secondary mirror.

     

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  3. Focal length of the objective lens, f0 = 140 cm Focal length of the eyepiece, fe = 5 cm Ans (a). In normal adjustment, the separation between the objective lens and the eyepiece = f0 + fe = 140 + 5 = 145 cm Ans (b). Height of the tower, h₁= 100 m Distance of the tower (object) from the telescope, uRead more

    Focal length of the objective lens, f0 = 140 cm

    Focal length of the eyepiece, fe = 5 cm

    Ans (a).

    In normal adjustment, the separation between the objective lens and the eyepiece = f0 + fe = 140 + 5 = 145 cm

    Ans (b).

    Height of the tower, h₁= 100 m

    Distance of the tower (object) from the telescope, u = 3 km = 3000 m The angle subtended by the tower at the telescope is given as:

    0 = h1/u = 100/3000 = 1/30 rad

    The angle subtended by the image produced by the objective lens is given as:

    0 = h2/f0= h2/140 rad

    Where, h2 = Height of the image of the tower formed by the objective lens

    1/30 = h2/140

    Therefore , h2 = 140/30 = 4.7 cm

    Therefore, the objective lens forms a 4.7 cm tall image of the tower.

    Ans (c).

    Image is formed at a distance, d = 25 cm

    The magnification of the eyepiece is given by the relation:

    m = 1 + d/fe

    = 1+ 25/5 = 1 + 5 =6

    Height of the final image = mh2 = 6 x 4.7 = 28.2 cm

    Hence, the height of the final image of the tower is 28.2 cm

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  4. Focal length of the objective lens, f0 = 140 cm Focal length of the eyepiece, fe = 5 cm Least distance of distinct vision, d = 25 cm Ans (a). When the telescope is in normal adjustment, its magnifying power is given as: m = f0/fe =140/5 = 28 Ans (b). When the final image is formed at d, the magnifyiRead more

    Focal length of the objective lens, f0 = 140 cm

    Focal length of the eyepiece, fe = 5 cm

    Least distance of distinct vision, d = 25 cm

    Ans (a).

    When the telescope is in normal adjustment, its magnifying power is given as:

    m = f0/fe =140/5 = 28

    Ans (b).

    When the final image is formed at d, the magnifying power of the telescope is given as:

    m = f0/f[1 + fe/d]

    = 140/5 [1 + 5/25] = 28 [1+ 0.2] =28 x 1.2 = 33.6

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  5. Focal length of the objective lens, f0 = 1.25 cm Focal length of the eyepiece, fe = 5 cm Least distance of distinct vision, d = 25 cm Angular magnification of the compound microscope = 30X Total magnifying power of the compound microscope, m = 30 The angular magnification of the eyepiece is given byRead more

    Focal length of the objective lens, f0 = 1.25 cm

    Focal length of the eyepiece, fe = 5 cm

    Least distance of distinct vision, d = 25 cm

    Angular magnification of the compound microscope = 30X

    Total magnifying power of the compound microscope, m = 30

    The angular magnification of the eyepiece is given by the relation:

    m= ( 1 + d/fe) = (1 + 25/5 ) = 6
    The angular magnification of the objective lens (m0) is related to me as: m0me = m

    m0= m/me  = 30/6 = 5

    We also have the relation:

    m0 = Image distance for the objective lens (v0)/Object distance for the objective lens (-u0)

    5 = v0/(-u0)

    Therefore , v0= -5u0————–Eq-1
    Applying the lens formula for the objective lens:

    1/f0 =1/v0 -1/u 0

    1/1.25 = 1/(-5u0)  –  1/u0) = -6/5u0

    Therefore u0 = -6/5 x 1.25 = -1.5 cm

    and v0 = -5u

    = -5 x (-1.5) = 7.5cm

    The object should be placed 1.5 cm away from the objective lens to obtain the desired magnification.

    Applying the lens formula for the eyepiece:

    1/ve -1/ue = 1/fe

    Where, ve = Image distance for the eyepiece = – d = – 25 cm

    ue = Object distance for the eyepiece

    1/ue = 1/v-1/fe

    = -1/25 -1/5 = -6/25

    Therefore , ue =-4.17 cm

    Separation between the objective lens and the eyepiece = |ue| + |v0| = 4.17 + 7.5 = 11.67 cm Therefore, the separation between the objective lens and the eyepiece should be 11.67 cm.

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