10 - the earth-moon-sun system ___1 Flashcards
3 - the earth-moon-sun system (39 cards)
what did eratosthenes and aristarchus use to successfully determine the diameters of the earth, moon and sun and the distances to the moon and the sun
observations of the moon and sun
what did eratosthenes and aristarchus successfully determine using observations of the moon and sun
diameters of the earth, moon and sun
the distances to the moon and the sun (from earth)
story of eratosthenes
came to his attention that at noon on the summer solstice (june 21)
the sun lay directly over a deep well in the city of syene
+ there were no shadows cast by pillars at that time
these observations implied that the sun was directly overhead syene
what was the state of alexandria at that same time
the sun was not directly overhead
vertical poles and column did cast a shadow
what did eratosthenes sought to do
use such a pole (the ones in alexandria that cast shadows) to determine the angle between the sun and the vertical
how was eratosthenes able to calculate ‘angle A’ whose value was just over 7°
by measuring the height of his pole
and the length of its shadow at noon
what did he assume
the sun was so distant that its rays of light were parallel
assuming the rays of light were parallel, what did eratosthenes conclude
angles A and B were alternate angles and therefore equal to eachother
what equation did he use
earth circumference / distance from syene to alexandria
360 / 7
what did eratosthenes discover
circumference of the earth
what did aristarchus discover
relative diameter of the moon compared with that of the earth
how did aristarchus discover the diameter of the moon
observed a total lunar eclipse
when observing the total lunar eclipse
what did aristarchus assume
a lunar eclipse was produced when the moon passed into the earth umbra
the sun was so far away that its rays were parallel when reaching earth
the moon’s path took it through the centre of the earth’s umbra which had the same diameter as that of earth
what did aristarchus show
equation
diameter of earth
=
time interval from U1 to U2
—————
time interval from U2 to U4
what are U1, 2, 3 and 4
stages of contact
thus, U1-2 = diameter of the moon and U2-4 = diameter of the earth
lowk but not exactly
what causes tides on earth
mainly by the gravitational pull of the moon
and also (lesser) the sun
what are spring tides and when do they occur
extra high and extra low tides
occur when the sun, moon and earth are aligned
(during new and full moon)
what are neap tides and when do they occur
weaker tides (lower high and higher low)
occur when the sun and moon are perpendicular to each other
(during first and last quarters)
why are spring tides stronger than neap tides
because the gravitational forces of the moon and sun combine during alignment
producing a greater tidal range
why are neap tides weaker
because the sun’s gravity partially cancels out that of the moon’s
reducing the difference between high and low tides
precession
slow wobble of earth’s axis
taking about 26,000 years to complete one full cycle
how does precession affect what we see in the sky
changes the position of stars, constellations and where the sun and moon rise and set over long periods of time
how does precession affect the north star
its position shifts
so different stars become the north star over thousands of years
what is archeoastronomy
study of how ancient cultures observed and used the sky
often in religion, agriculture and architecture