Telescopes
Galileo 1609
The Moon as a World
Jupiter has Moons
Refracting telescopes
Isaac Newton’s reflecting telescope
Reflecting telescope Objective mirrors instead of lenses
Three Powers Magnifying Resolving Light Gathering
Magnifying Power Ability to make objects appear larger in angular size One can change the magnifying power of a telescope by changing the eyepiece used with it Mag Power = focal length of objective divided by the focal length of the eyepiece
Resolving Power Ability to see fine detail Depends on the diameter of the objective lens or mirror
Light Gathering Power The ability to make faint objects look brighter Depends on the area of the objective lens or mirror Thus a telescope with an objective lens 2 inches in diameter has 4 times the light gathering power of a telescope with a lens 1 inch in diameter
Herschel & Lord Rosse
19 th century: epoch of the large refractors
Refracting telescopes Vienna Lick
Yerkes Observatory
20 th century Large Reflectors Come of Age Mount Wilson
Palomar (5-m)
4 meter Reflecting telescope
Objective Mirror
Dome of 4 meter Kitt Peak
Keck Telescopes
Rooftop telescopes
MSU Campus Observatory
SOAR Telescope
SOAR Telescope -- Cerro Pachon
Astronomical “seeing” Blurring effect of looking through air Causes stars to twinkle
Bad seeing on this side Good seeing on this side
Electromagnetic Spectrum
Radio Telescopes Arecibo
Very Large Array
Observing from space No clouds Perfect seeing Can see wavelengths of light blocked by the earth’s atmosphere
Hubble Space Telescope