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TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

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TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)
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Page 1: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

TELESCOPESAstr 221 Lec 3 Spring 2015(Ch. 5 in Nightwatch)

Page 2: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

TELESCOPES

Outline:1. Types of Telescopes2. Most Important Properties3. Sky Limitations and Overcoming Them4. What Kind of Telescope Is Best for YOU?

Page 3: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

What are the two basic designs of telescopes?

• Refracting telescope: Focuses light with lenses

• Reflecting telescope: Focuses light with mirrors

Page 4: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

The Galilean Telescope (1609)

Page 5: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Kepler’s Modified Refractor

Page 6: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Refracting Telescope

• Refracting telescopes need to be very long, with large, heavy lenses

Page 7: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Reflecting Telescope

• Reflecting telescopes can have much greater diameters

• Most modern telescopes are reflectors

Page 8: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)
Page 9: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

AstronomialTelescopes invertAnd sometimes flip(reverse) images

Page 10: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Binoculars - “inverting the inverted” image

Page 11: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

What are the two most important properties of a telescope?

1. Light-collecting area: Telescopes with a larger collecting area can gather a greater amount of light in a shorter time.

2. Angular resolution: Telescopes that are larger are capable of taking images with greater detail.

Page 12: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Bigger is better

Page 13: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Mirrors in Reflecting Telescopes

Twin Keck telescopes on Mauna Kea in Hawaii

Segmented 10-meter mirror of a Keck telescope

Page 14: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Light Collecting Area

• A telescope’s diameter tells us its light-collecting area: Area = π(diameter/2)2

• The largest telescopes currently in use have a diameter of about 10 meters

• Mag Limit = 9.5 + 5logD(inches) (7.5) (cm)

Page 15: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Angular Resolution• The minimum

angular separation that the telescope can distinguish.

Page 16: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Angular Resolution• Ultimate limit to

resolution comes from interference of light waves within a telescope.

• Larger telescopes are capable of greater resolution because there’s less interference

Page 17: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Angular Resolution• The rings in this

image of a star come from interference of light wave.

• This limit on angular resolution is known as the diffraction limit

Close-up of a star from the HubbleSpace Telescope

Page 18: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Angular Resolution

Dawes Limit = 4.56arcsec/D(in) (theoretical) = 11.6arcsec/D(cm)

Rayleigh Limit = 5.5arcsec/D(in)(observational) = 14arcsec/D(cm)

e.g., RUCO 16”: Dawes = 0.28 arcsecRayleigh = 0.34 arcsec

Page 19: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Interferometry

• Interferometery is a technique for linking two or more telescopes so that they have the angular resolution of a single large one

Page 20: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Twinkling and Turbulence

Turbulent air flow in Earth’s atmosphere distorts our view, causing stars to appear to twinkle

Star viewed with ground-based telescope

Same star viewed with Hubble Space Telescope

Page 21: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Adaptive Optics

Rapidly changing the shape of a telescope’s mirror compensates for some of the effects of turbulence

Without adaptive optics

With adaptive optics

Page 22: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Two More Important Things About Telescopes

3. Magnification:

m = f.l. objective / f.l. eyepiece (variable ==> good eyepieces!)

4. Mount:

(a) sturdy but portable(?)

(b) Fine motions (knobs or motors)

(c) “Clock” drive

Page 23: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)
Page 24: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Mounts are veryImportant!

Page 25: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)
Page 26: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Light Pollution!

Page 27: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Calm, High, Dark, Dry

• The best observing sites are atop remote mountains

Summit of Mauna Kea, Hawaii

Page 28: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Why do we put telescopes into space?

Page 29: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Transmission in Atmosphere

• Only radio and visible light pass easily through Earth’s atmosphere

• We need telescopes in space to observe other forms

Page 30: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Future of Astronomy in Space?

• The Moon would be an ideal observing site

Page 31: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

OK, What telescope should I get?

Page 32: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

f ratio = focal length / diameterof objective

f/10 == “slow” (fl=2000mm, d=200mm)(big but faint images)

f/5 == “fast” (fl=1000mm, d=200mm)

Usually “slow” telescopes are long and used to only view bright objects like moon and planets.

For deep sky objects, “fast”telescopes are better (~f/5)

Page 33: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Answer: Depends on what you want to observe…and your pocketbook!

Refractor or Reflector?

Page 34: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

DOBSONIAN

“LIGHT

BUCKETS”

If you want to see faint deep-sky objects (starclusters, nebulae, andgalaxies) and want a simple to set up and use telescope -- “Dobs”are for you! ($500 willget you an 8inch)

Page 35: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Computerized “go-to” telescopes: $400up (~$1500 really)

Page 36: TELESCOPES Astr 221 Lec 3 Spring 2015 (Ch. 5 in Nightwatch)

Reggie’s Steps to Buying a Telescope

• Read his handouts from Astronomics!• Get a copy of Sky&Tel or Astronomy magazine• Visit Land, Sea, & Sky on Richmond Ave. (tell

Darren or Art that Reggie sent you!)• Check out Astronomics.com or Telescopes.com• Look through lots of telescopes before buying• Visit George Observatory (Astronomy Day is

Saturday, October 8th)• Buy the best you can afford…


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