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How do we study the Universe?

How do we study the Universe?. SPECTROSCOPY Uses visible wavelength split into colors

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Page 1: How do we study the Universe?. SPECTROSCOPY Uses visible wavelength split into colors

How do we study the Universe?

Page 2: How do we study the Universe?. SPECTROSCOPY Uses visible wavelength split into colors

SPECTROSCOPY

• Uses visible wavelength split into colors

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Doppler shift

• Wavelengths change when object is moving

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Red/ Blue Shift

• RECEDING (moving away) objects show a INCREASE in WAVELENGTH- red shift

• APPROACHING objects show a DECREASE in WAVELENGTH- blue shift

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• Star Approaching

• Star Receding

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RED-SHIFTING STAR (Moving Away From Us)

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BLUE-SHIFTING STAR (Moving Towards Us)

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sun

Red or blue shift?

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Star MOVING AWAY from us.(RED-SHIFTING)

REFERENCE SPECTRUM

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Mauna Kea Observatory

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Mauna KeaAug. 2011

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Optical telescopes

• Need clear weather• Away from city lights (light pollution)• Above clouds (mountain tops)

– Less distortion

• Many in AZ and HI

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Kitt Peak, Arizona

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REFRACTING TELESCOPES

Use multiple lenses to focus light and magnify images.

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The USNO 26-inch Refracting Telescope

                                                     

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REFRACTORS• Lenses are expensive• Chromatic aberration (halo affect;bad)• good for observing solar system objects

• See details (good contrast)

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Lowell Observatory, Flagstaff AZdiscovered Pluto

24” refractor

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REFLECTING TELESCOPES

Uses a series of mirrors to gather and focus light.

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Reflectors

• Mirrors are cheaper • See farther than refractors

– Lose detail

• Can build larger (10 meters vs. 1 meter)• “Coma” problem

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“coma problem

• Stars need edge of field have “tails”

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8” REFLECTOR

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Keck Observatory10 m reflector

largest in world

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LBTLarge Binocular Telescope

• Two 8.4 m mirrors

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CATADIOPTRIC TELESCOPEScombines the best features of refractors and reflectors

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Dobsonian telescope

• Cheap • Reflector• need dark skies• Only azimuth mount• Good beginner telescope

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Radio telescopes

• Gather incoming radio waves• Convert waves to colors• Produce false color images

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Radio telescopes

• Best for out of solar system objects– Galaxies– Supernovas– quasars

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Very Large ArraySocorro, NM

• Arrays use many telescopes that act as one telescope

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Very Large Baseline Array Sites

Kitt Peak, AZ

New Mex. Texas New Mex. Virgin Islands

Hawaii California Washington Iowa New Hampshire

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40 meter radio telescope

Green Bank, WV

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305 meterArecibo Radio Telescope

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Signal is received by telescope

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Signal is amplified

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Jan

skie

s

Minutes

Signal is converted to false colors

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SUPERNOVA REMNANT

All declinations combined make a picture

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THE MOON

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A GALAXY

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Jupiter

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Planet forming

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Advantages of Radio Telescopes

• Use anytime (day, clouds, etc)• No dome needed• Detect object much further away

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Infrared

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Advantages of Space Telescopes

• No atm. Interference– See clearer

• NOT CLOSER• Can detect wavelength

that atm. blocks

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Hubble

• reflector• Last service mission (2010) will keep

operating to at least 2014

• In 2018 Hubble will be replaced by James Webb telescope (IR)

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James Webb telescope

• Mission length: 5 years • Remain stationary above Earth

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Hubble vs. Webb

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Other space telescopes

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Spitzer infrared telescopelaunched 2003

                

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GLAST- gamma ray telescope

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Chandra X-ray telescopelaunched 1999

                              

                   

                                                           

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HUT (HOPKINS UV TELESCOPE)

Clumpy universe

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COBEmicrowave

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