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Astronomy 1010-H Planetary Astronomy Fall_2015 Day-21.

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Presentation on theme: "Astronomy 1010-H Planetary Astronomy Fall_2015 Day-21."— Presentation transcript:

1 Astronomy 1010-H Planetary Astronomy Fall_2015 Day-21

2

3 Course Announcements How is the sunset/sunrise observing going? Dark Sky nights – Wed. 10/7 starting at 7:30pm – at the Observatory. Exam-2 will be Friday, Oct. 9; Ch. 3, 4, & 5 SW-chapter 5 posted: due Fri. Oct. 9 No lab next week – Fall Break

4 The refracting telescope uses two lenses Since the eye already has a lens, the eyepiece is needed to bring the light rays back to parallel for the eye to see

5 Large refractors can be very long and bulky

6 The Largest Lens is 40” Built in the late 1890’s, it is the last great refracting telescope.

7 Lenses and refractors suffer from Chromatic Aberration This applies to camera lenses, your eye, telescopes and anything else that uses a lens to focus light

8 Correcting for Chromatic aberration can be expensive The compound lens takes two lenses of different materials and combines them to correct for color distortion

9 Color separation is useful in a prism so that we can obtain a spectrum of light Since it is meant to be separated we don’t call it an aberration. Instead, it is called dispersion

10 A diffraction grating works on interference of light waves Diffraction is much more efficient at separating light into its colors than dispersion

11 Unfortunately, diffraction also leads to problems Look closely enough at stars and they aren’t just points of light but rings, too

12 Refractors have many problems They are large and bulky and difficult to maneuver They suffer from chromatic aberration Even the best glass cuts off the IR and UV wavelengths

13  Reflecting telescopes use mirrors.  There are primary and secondary mirrors.  Focal length is determined by the path the light takes reflecting off the mirrors.

14 Reflection is the bouncing of light off a surface Mirrors do not suffer from chromatic aberration and they do not cut off long or short wavelengths

15 A concave mirror focuses light to a focal point Telescope mirrors are made so that the focus is a plane instead of a point

16 Reflecting Telescopes Suffer From Spherical Aberration

17 There are several types of reflecting telescopes

18 Definitions & Terms -1 Photon: A particle of light. Spectrum: The flux of an object as a function of wavelength.


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