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phy sci
models of the universe and the early astronomy
modern astronomy
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major distinct characteristics of modern astronomy:
the observations became more quantitative in
nature.
the theories formulated are based on
logical
and
mathematical
concepts.
Nicolaus
Copernicus
corrected the
geocentric
theory and proposed the heliocentric theory with the following postulates:
Earth is considered only one of the planets
Earth rotates on its axis daily and revolves around the sun once a year
Earth experiences an annual tilting of its axis
earth's motion explains the retrograde motion of the planets
the distance from Earth to sun is small compared to Earth's distance from the stars
Nicolaus proposed the heliocentric theory by:
Earth is considered to be only one of the planets Earth
rotates
on its axis daily and revolves around the sun once a
year.
earth experiences
nicolaus
copernicus
tilting of the earth and the four seasons
Tycho Brahe
he modified the
geocentric
model of the universe
built massive
instruments
used to make precise measurements of the positions of the planets
discovered a
supernova
in the constellation
Cassiopeia
in 1572
made observations of planetary motions that are important to the development of
Kepler's
laws and other models of the solar system
Tychonic
system
Galileo Galilei
he discovered
sunspots
and rough surface of the
moon
discovered the four famous moons of
Jupiter
venus
has phases like moon.
known as the
galilean moons
lo,
europa
,
ganymede
, callisto
johannes kepler
first law states that the planets' orbits are
eclipses
with the
sun
at one focus
second law- an
imaginary line
drawn from the
sun
to a planet sweeps out equal areas in equal intervals
third law- the
cube
of the radius of the orbit of a planet around the sun is proportional to the square of its period of
revolution.
periphelion
nearest to the
sun
aphelion
farthest
from the sun