Date | May 2016 | Marks available | 2 | Reference code | 16M.3.SL.TZ0.10 |
Level | Standard level | Paper | Paper 3 | Time zone | Time zone 0 |
Command term | Calculate | Question number | 10 | Adapted from | N/A |
Question
An astronomical telescope is used in normal adjustment. The separation of the lenses in the telescope is 0.84m. The objective lens has a focal length of 0.82m.
Calculate the magnification of this telescope.
Outline why sign convention is necessary in optics.
A student decides to reverse the positions of the same lenses without changing the separation to form an optical microscope in normal adjustment. The student’s near point is 0.25 m from her eye.
(i) Show, using a calculation, that the image formed by the objective lens is about 0.19 m from the eyepiece.
(ii) Calculate the distance between the objective lens of the microscope and the object.
(iii) Determine the overall magnification of the microscope.
Markscheme
Fo+fe=84 so fe=84-82=2cm
\( \ll M = \frac{{{f_{\rm{O}}}}}{{{f_{\rm{e}}}}} = \frac{{82}}{2} = \gg 41\)
a sign convention is a way to distinguish between real and virtual objects or images or converging and diverging lenses
(i) image will be virtual v=–25 cm
\(\frac{1}{u} = \frac{1}{{82}} + \frac{1}{{25}}\)
«=19cm or 0.19m»
Award [1 max] if v = +25 cm used to give u = –36 cm.
(ii) image will be real v=84-19=65cm
\( \ll \frac{1}{u} = \frac{1}{2} - \frac{1}{{65}} \gg \) so u=2.1cm
(iii) \({M_e} = \ll \frac{D}{{{f_{\rm{e}}}}} + 1 = \frac{{25}}{{82}} + 1 = \gg 1.3\) AND \({m_o} = \ll \frac{v}{{{f_{\rm{o}}}}} - 1 = \frac{{65}}{2} - 1 = \gg 31\) or 32
so \(M = \ll {M_{\rm{e}}}{m_{\rm{o}}} = 1.3 \times 31 = \gg 40\) or 41
Far point adjustment gives M = 9.3 (accept answers from interval 9.3 to 9.6), award [1 max] for full working.