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ASTR-1010 Planetary Astronomy Day - 18
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Announcements Smartworks Chapters 4: Due Monday, March 1. Smartworks Chapter 5 is also posted Exam 2 will cover chapters 3, 4, & 5 -Target Wednesday, March 3
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ClassAction Stuff Splash page questions
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Telescopes & Instruments
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Telescopes Telescopes have three functions: 1.Gather light LGP ∝ Area = πR 2 2.Resolve objects Θ = 2.06 X 10 5 ( λ/D) 3.Magnify EXTENDED objects
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The light gathering power is proportional to the area
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Properties of light: Refraction The Speed of Light is less in glass than in vacuum
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Refraction through a plane of glass only shifts the light, a lens with curved surfaces focuses the light
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The refracting telescope uses two lenses
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Refractors suffer from Chromatic Aberration
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Chromatic Aberration distorts colors Rainbows appear around bright white objects
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ClassAction Stuff Simple Telescope Snell’s Law Splash page questions
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Correcting for Chromatic aberration can be expensive
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Large refractors can be very long and bulky. The largest has a 40” diameter
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The Yerkes 40” moves the floor to view at low angles
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Cheaper Way Mirrors
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Reflection is the bouncing of light off a surface
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A concave mirror focuses light
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There are several types of reflecting telescopes
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Spherical mirrors suffer from Spherical Aberration
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Spherical aberration can be eliminated by a parabolic shape or a corrector plate
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The Largest Optical Telescopes Keck I and II
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The 10 meter Keck Mirror
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The Hobby-Eberly Telescope
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Coming “soon” The 30m Telescope
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The resolution of a telescope depends on its size and the wavelength of the light
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The atmosphere limits the resolving power of a ground- based telescope
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Differences in the temperature and density of small portions of Earth’s atmosphere cause passing starlight to quickly change direction, making stars appear to twinkle.
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Earth’s atmosphere hinders astronomical research Image of stars taken with a telescope on the Earth’s surface Same picture taken with Hubble Space Telescope high above Earth’s blurring atmosphere
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