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venus transits
venus stands between earth and sun
rare: a pair 8 years apart every 121.5 and 110.5 yrs apart
same situation reoccurs after 243 yrs
G = measuring the strength of gravity
G is small, gravity is weak
telescopes use…
lenses and mirrors to focus and collect light
rain/light collected is proportional to…
area of umbrella/mirror
refraction and reflection occur…
simultaneously
refraction
light bends when it passes from one material to another
light is slower in water/glass than in air
two types of telescopes
reflectors (mirrors)
refractors (lenses)
convex and concave lenses

magnification
determined by focal lengths of lenses
M = fobjective/feyepiece
does magnification = resolution?
no
chromatic abberation
different focus for different color light
image is distorted and has colored edges
effect is diminished for long focal lengths
1760s cure (Dollond): achromatic lens, combination of two lenses
reflectors
no chromatic aberration
invented by newton, 1670
metal mirror, only reflects 66%
newtonian reflectors
long tubes
open at front
eyepiece on side
star points from mirror struts
struts for the 2º mirror don’t block light, but they do distort it
1610
keplerian and galilean telescopes invented
17th century
aerial telescopes
long focal length to reduce lens errors
1672
newton invents reflector
1750
dollond patents the achromatic lens
late 1700s
herschel builds speculum reflectors
1858
foucault invents silverized mirrors
galilean telescopes
coverging and diverging lens
upright virtual image
keplerian telescopes
2 converging lenses
inverting
real image
cavendish
measures gravitational attraction between 2 lead balls
measuring astronmical unit (sun-earth distance)
project known distance on earth onto sun
deduce venus-earth distance
parallax
how to measure an astronomical unit
observe an event in the solar system from two different location to triangulate the distance
maselyne weighs the earth by…
force ratio + mountain mass