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Telescopes Telescopes

Telescopes - PowerPoint Presentation

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Telescopes - PPT Presentation

Jon Holtzman NMSU Astronomy Telescopes are light buckets bigger buckets collect more light and faint far away objects dont produce much light Why build bigger telescopes In principle bigger telescopes make sharper images ID: 400291

light telescopes chile bigger telescopes light bigger chile hawaii cerro images sharper observatory mauna kea telescope atmosphere diameter blur

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Slide1

Telescopes

Jon Holtzman

NMSU AstronomySlide2

Telescopes are light buckets: bigger buckets collect more light, and faint (far away) objects don’t produce much light!

Why build bigger telescopes?Slide3

In principle, bigger telescopes make sharper images:

Why build bigger telescopes?

But, in practice, this doesn’t usually work, because as light comes in through the Earth’s atmosphere, motions and

inhomgeneties

in our atmosphere blur out images: once you get bigger than several inches in diameter, images don

t get sharper!Slide4

So how big do telescopes get? Consider NMSU telescopes:

The telescopes in the domes are 12 inches (0.3m) in diameter

The telescope outside is

16

inches (0.4m

) in diameter: it collects about twice as much lightSlide5

Tortugas Mt. Telescope

Also 24” inches (0.6m) in diameter

Used a lot in 70’s & 80’s to monitor planets, but hasn’t been used much in last 20 years

We’re working to renovate and start getting it used again!Slide6

Apache Point Observatory

Observatory operated by NMSU for the Astrophysical Research Corporation

Four telescopes on site:

0.5m ARCSAT

1.0m NMSU

2.5m SDSS3.5m ARC

Small visitor center at nearby National Solar Observatory

ARC

3.5m collects more than 100x the light of the campus observatory telescopes!Slide7

Other “medium-sized” telescopes

5.0m Hale Palomar Mountain, California

4.2 William Herschel Canary Islands, Spain

SOAR Cerro Pachon, Chile LAMOST

Xinglong Station, China 4.0 Victor Blanco Cerro Tololo, Chile

Vista Cerro Paranal, Chile 3.9 AAT NSW, Australia 3.8

Mayall Kitt Peak, Arizona UKIRT Mauna Kea, Hawaii

3.7 AEOS Maui, Hawaii 3.6 "360" Cerro La Silla, Chile. Canada-France-Hawaii Mauna Kea, Hawaii

Telescopio Nazionale Galileo, Canary Islands 3.5 MPI-CAHA

Calar Alto, Spain New Technology Cerro La Silla, Chile

ARC A pache Point, New Mexico WIYN , Kitt

Peak NMSlide8
Slide9
Slide10

Bigger telescopes: single BIG mirrors

8.3

Subaru

Mauna Kea, Hawaii 4100 m

NAOJ 8.2 FOUR VLT telescopes Cerro Paranal

, Chile 8.1 Gillett Mauna Kea, Hawaii aka Gemini North8.1 Gemini South

Cerro Pachon, Chile 6.5 MMT Mt. Hopkins, Arizona

6.5  Walter Baade La Serena, Chile aka Magellan I6.5 Landon Clay aka Magellan II

6.0 Bolshoi Teleskop Azimutalnyi Nizhny Arkhyz, RussiaSlide11
Slide12

Bigger telescopes: no longer single pieces of glass!

10.4

Gran Telescopio Canarias

La Palma, Canary Islands, 10.0

Keck Mauna Kea, Hawaii

~10 SALT South African Astronomical Observatory

9.2 Hobby-Eberly Mt. Fowlkes, Texas 8.4 -> 12

Large Binocular Telescope Mt. GrahamSlide13
Slide14

What about getting sharper images?

Remember, bigger telescope collect more light, but they don’t generally give sharper images because images are blurred as light from objects passes through the Earth’s atmosphere

So what can we do?Slide15

Telescopes in Space!

Hubble Space Telescope: 2.4m diameter (so not so big), but above the atmosphere

 sharp images!

-> also can observe in ultraviolet lightSlide16

Another cool idea: “deblur” the atmosphere

New technology uses small “bendable” mirrors to take the atmospheric blur out of the picture.

Blur changes fast, so mirrors need to move fast!

But need to measure what the blur is first – need a nearby bright star

There aren’t enough bright stars in the sky! So what can you do

 make your own star!Slide17

Telescopes of the future: bigger and sharper!!