ASTR 200, reminder Center section = 'no laptop' zone
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1 ASTR 200, reminder Center section = 'no laptop' zone Laptops OK NO Laptops Blackboards 1 Laptops OK
2 ASTR 200 Frontiers of Astrophysics 2 Instructor: Professor Gladman Office: Hennings 300B Lectures here (Henn 202) 12:00 on M,W,F
3 Units for astronomy and astrophysics au 3
4 Units for astronomy and astrophysics au 4
5 Units for astronomy and astrophysics au +c 5
6 Their values depend on the system of units one is using! 6
7 A light year A Julian year is exactly days - (note: a tropical year is not) so: d * 24 h/d * 60 min/h * 60 s/min = 31,557,600 seconds = x 107 s unit c = x 108 m/s physical constant (what would it be in cm/s?) ly = x 108 m/s * x 107 s 15 = x 10 m This is a 'derived unit' based on a constant 7
8 Units for astronomy and astrophysics au 8
9 Angular Measurements Full circle = 360º 1º = 60 (arcminutes) 1 = 60 (arcseconds)
10 10
11 For those with integral calculus: Prove by integrating the surface element (sinθ dθ dφ) on a unit sphere that the area is 4π 11
12 12
13 angular diameter Diameter Angular diameter(o) Angular diameter = = Distance 360 o 2 radians
14 The Moon's angular diameter The angular diameter of the Moon when view from Earth is : 31 arcmin = (31/60) deg ~ 0.52 deg Question: Is that enough information to determine the physical diameter of the Moon? Diameter Angular diameter(o) Angular diameter = = Distance 360 o 2 radians
15 Starting our steps out into the universe The first human steps were to understand the scale of : Our planet The Moon The Sun 15
16 Observations of the Moon Aristotle realizes the Earth is a sphere Erathostenes uses simple geometry to determine the size of the Earth Aristarchus realizes this gives the diameter of the Moon via eclipse observations Once one knows the diameter of the Moon, you can calculate its distance!
17 Observations of the Moon Aristotle realizes the Earth is a sphere Erathostenes uses simple geometry to determine the size of the Earth Aristarchus realizes this gives the diameter of the Moon via eclipse observations Once one knows the diameter of the Moon, you can calculate its distance!
18 Lunar Eclipse Sequence
19 Lunar Phase Cycle
20 Lunar Eclipse Sequence
21 On the summer solstice, the sun shone straight down a well in Syene
22 On the summer solstice, the sun shone straight down a well in Syene On the same day, an obelisk in Alexandria cast a 7.2 degree shadow...
23 The Eratosthenes experiment Relies that Sun is far away. 7.2/360 must be distance from SyeneAlexandria divided by circumference ( D) of the Earth 5000 stades The distance from Syene to Alexandria was known, which gives Earth's diameter! D see also text Fig on p. 33
24 The Eratosthenes experiment Relies that Sun is far away. 7.2/360 must be distance from SyeneAlexandria divided by circumference ( D) of the Earth = πd 5000 stades The distance from Syene to Alexandria was known, which gives Earth's diameter! D 360*5000 see also text D = = 80,000 Fig on p. 33 st 7.2*π *0.185 km/st D=14,800 km
25 So, we knew the Earth's diameter How does that help get the MOON's diameter or distance?
26 So, we knew the Earth's diameter How does that help get the MOON's diameter or distance? Does the relation : Diameter Angular diameter(o) Angular diameter = = Distance 360 o 2 radians help???
27 Lunar Eclipse Sequence
28
29
30 Aristarchus Eclipse observations implied : Diameter of Moon about 1/3 diameter of Earth Thus, diameter of Moon about 5000 km This gives distance to Moon! Board : use angular diameter of Moon is 0.5 deg. Conclude: D ~ 573,000 km. km... Actually 385,000 Perspective: Are we thus 'wrong'? First step in the cosmic distance scale...
31 Distance to Sun Trickier... Aristarchus had an argument about the quarter moon, but was off by a lot (see text) Wasn't done correctly until transits of Venus were done using telecopes This didn't prevent (next week) accurately getting the RELATIVE scale of the planetary orbits
32 What about distances to Stars? The ancients had a REALLY tough time with this question IF stars are physical objects like planets, they SHOULD exhibit parallax... Geocentric parallax (diurnal) Heliocentric parallax (annual, stellar)
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