telescopes and spacecraft astronomy 311 professor lee carkner lecture 7
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![Page 1: Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7](https://reader035.vdocuments.net/reader035/viewer/2022062714/56649d2a5503460f949fe290/html5/thumbnails/1.jpg)
Telescopes and Spacecraft
Astronomy 311Professor Lee
CarknerLecture 7
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If it is low tide where you are standing right now, how many total places on Earth are at low tide right now? How many total places on Earth are at high tide right now?a) 1 and 0b) 1 and 1c) 1 and 2d) 2 and 2e) 4 and 4
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Which of the following would the Earth’s magnetic field have no effect on?
a) An ionb) An electronc) A neutral oxygen atomd) A negative hydrogen atome) A positive helium atom
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How Do Telescopes Work?
Telescopes: Focus light to produce an image
Light gathering ability (not magnification) is the most important attribute of a telescope telescopes make faint things brighter
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Lenses
Need a lens Lenses bend light (refraction) and
focus all of the light incident on the front to a point (focus) a certain distance behind the lens (focal length)
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Lenses and Refraction
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Refracting Telescope
This produces a refracting telescope
mag.= f.l. objective / f.l. eyepiece in practice the magnification you can achieve is
limited by the blurring effects of the Earth’s atmosphere
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Refracting Telescope
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Refractors and Reflectors
Makes them
A curved mirror can be used to gather and focus the light instead (reflecting telescope) large mirrors are easier to make and support
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Reflecting Telescopes
Problem: The focal point is between the mirror and the sky
Cassegrain Telescope -- secondary reflects light through a hole in the primary, most common type of large telescope
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Cassegrain Reflecting Telescope
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Telescope Misconceptions Magnification is the most important property of a
telescope image quality and light gathering ability (size) are what
is important Astronomers peer through an eyepiece
Telescopes stick out of the dome
Telescopes fold up like a giant pirate’s spyglass
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Spacecraft
Types of spaces probes: Fly-by -- collects data as it passes by
Example:
Orbiter -- circle planet and study for a long time Example:
Lander -- land on the planet and take samples Example:
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Least Energy Orbit
Once in space they coast to the planets, following Kepler’s Laws
An orbit that intersects the Earth’s orbit at one point and the other planet’s orbit at another point (on the opposite side of the Sun)
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Least Energy Orbit to Mars
Sun
Earth
Mars
Spacecraft Orbit
Time to get to Mars P2=a3
aEarth = 1 AU
aMars =1.5 AU Time = =
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The Electromagnetic Spectrum
Every photon (light particle) has a wavelength which places it in the electromagnetic spectrum
long wavelength -- low energy short wavelength -- high energy
We see different wavelengths of visible light as colors red -- blue --
We want to view all types of electromagnetic radiation
So we can explore all physical processes
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The Electromagnetic Spectrum
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Telescope Taxonomy Radio and Millimeter
penetrates atmosphere and everything else
Infrared (IR) some penetrates atmosphere, but to observe all IR wavelengths
need to go into space Optical
it helps to get above atmosphere (no blurring = sharper
images)
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More Telescope Taxonomy Ultraviolet (UV)
some penetrates atmosphere, but to observe all UV
wavelengths need to go into space X-ray
all X-rays blocked by atmosphere
Gamma Ray all Gamma rays blocked by atmosphere
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Next Time
Read 15.1-15.4 , 6.7 Quiz #1 on Monday
Study hard!
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Summary
Refracting Telescopes use a lens to bend light to a focus
Reflecting Telescopes use a mirror to reflect light to a focus Most large research telescopes are
reflectors Astronomers today record and
analyze data digitally
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Summary To observe the entire
electromagnetic spectrum you need many different types of telescopes, some of them in space
Spacecraft have allowed close up study of the planets Spacecraft reach their destinations by
using the gravity of the Sun (or sometimes planets)