1. Announcements: Announcements: Simple numerical error analysis procedure on the website Simple numerical error analysis procedure on the website Office hours changing Office hours changing Monday: 1:30-2:30 Monday: 1:30-2:30 Wednesday: 1:30-2:30 Wednesday: 1:30-2:30 Lab 2

2. Lab 1 Grade Distribution Average (without zeros):71 Average (without zeros):71 Average (with zeros):59 Average (with zeros):59

3. Telescopes We use telescopes to magnify distant objects We use telescopes to magnify distant objects There are two major types of telescopes There are two major types of telescopes Refractors – use lenses Refractors – use lenses Reflectors – use mirrors Reflectors – use mirrors Many modern telescopes are a hybrid of the two Many modern telescopes are a hybrid of the two Our telescopes are primarily reflectors, but have a corrector plate (big lens) on the front Our telescopes are primarily reflectors, but have a corrector plate (big lens) on the front

4. Magnification The magnification is determined by the focal lengths of the telescope and eyepiece. (M=f telescope /f eyepiece )‏ The magnification is determined by the focal lengths of the telescope and eyepiece. (M=f telescope /f eyepiece )‏ Focal length is the distance between the lens/mirror and where an object coming from infinity is focused Focal length is the distance between the lens/mirror and where an object coming from infinity is focused This is why many telescopes are long This is why many telescopes are long Reflectors advantageous here – can fit a longer focal length inside a smaller region Reflectors advantageous here – can fit a longer focal length inside a smaller region Can you have too much magnification? Can you have too much magnification?

5. Too Much Magnification Its tempting to zoom in as much as possible, but everything has limits Its tempting to zoom in as much as possible, but everything has limits More magnification makes image dimmer More magnification makes image dimmer Light spread over a larger area Light spread over a larger area You not only magnify your target, but everything in between as well (atmosphere)‏ You not only magnify your target, but everything in between as well (atmosphere)‏

6. Brighter Images Most of what we look at through telescopes are far away and dim Most of what we look at through telescopes are far away and dim We want to make our images bright! We want to make our images bright! How do we get brighter images  collect more light  make telescope wider How do we get brighter images  collect more light  make telescope wider Refractors at a disadvantage – can only be so wide Refractors at a disadvantage – can only be so wide Some times this is not enough Some times this is not enough Many images are long exposures Many images are long exposures Hubble Ultra Deep Field (11 days- worth of light collecting!!!)‏ Hubble Ultra Deep Field (11 days- worth of light collecting!!!)‏

8. Celestial Coordinate Systems Right Ascension and Declination (RA/DEC)‏ Right Ascension and Declination (RA/DEC)‏ Units? Units? Why is it advantageous over other systems like latitude and longitude? Why is it advantageous over other systems like latitude and longitude?

9. And now tonight’s lab We’ll be measuring field of view of our telescope ( angular size seen through the telescope)‏ We’ll be measuring field of view of our telescope ( angular size seen through the telescope)‏ Primary Method – timing of stars crossing the field of view Primary Method – timing of stars crossing the field of view Can do this because the Earth rotates at a constant speed (15 degrees per hour)‏ Can do this because the Earth rotates at a constant speed (15 degrees per hour)‏ Time with a velocity gives a distance Time with a velocity gives a distance In case of clouds In case of clouds Can put the telescope into a rough alignment-->turns on the tracking motor Can put the telescope into a rough alignment-->turns on the tracking motor Look at a stationary object, moves like a star in the sky-->mimics the original process Look at a stationary object, moves like a star in the sky-->mimics the original process

10. Procedural Notes Measure FOV crossing time at least 3 times and take an average. Measure FOV crossing time at least 3 times and take an average. Don't forget to find theoretical field of view and compare it to your measured field of view. Don't forget to find theoretical field of view and compare it to your measured field of view. You'll need a couple of specs for the telescope and eyepiece – see the handout You'll need a couple of specs for the telescope and eyepiece – see the handout Mind your units! Mind your units!  (degrees)=15(degrees/hour) x t(hours)‏  (degrees)=15(degrees/hour) x t(hours)‏  (arcminutes)=15(arcminutes/minute) x t(minutes)‏  (arcminutes)=15(arcminutes/minute) x t(minutes)‏  (arcseconds)=15(arcseconds/second) x t(seconds)‏  (arcseconds)=15(arcseconds/second) x t(seconds)‏