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Transcript
Science 9
Unit 5: Space Exploration
Name: Danielle Murray
Topic 1 - For Our Eyes Only
Frames of Reference
A frame of reference is a set of axes of any kind that is used to describe positions or
motions of things. The stars, the Sun and the planets do not rotate around the Earth,
but seem to because the Earth is rotating on its axis. The Earth is our fixed frame of
reference. To locate positions on Earth, the equator and the prime meridian (latitude
and longitude) are the axes used.
What Our Ancestors Saw
Objects in the sky have fascinated humans throughout time. The explanations of how
these celestial objects came to be are even more fascinating. Ancients developed their
ideas of what was happening in the sky and explained it with their frame of reference.
The constellations were patterns that seemed to tell stories about people. Stars are not
always in the sky at the same time, but change positions over time – giving rise to the
creation of calendars. The Sun and the Moon have their own pattern or rising and
setting – the Moon also has phases. Mercury, Venus, Mars, Jupiter, and Saturn were
special ‘stars’ called planets – meaning ‘wanderer’.
Ancient Myths
Myths, folklore and legends were used to explain what ancient people observed in the
night sky.
 First Nations people of the Pacific Northwest – believed the night sky was a
pattern on a great blanket overhead, which was held up by a spinning ‘world
pole’ resting on the chest of a woman named Stone Ribs.
 Aboriginal tribes – Algonquin, Iroquois and Narragansett believed the
constellation Ursa Major was a bear running from hunters.
 Inuit in the high Arctic – used a mitt to determine when seal pups would be
born, by holding the mitt at arm’s length at the horizon.
 Ancient Egyptians - The Sun God – Ra – was carried in a sacred boat across the
sky every day.
Solstice represents the shortest and longest periods of daylight
Winter solstice - shortest period of daylight (Northern hemisphere - Dec. 21)
Summer solstice – longest period of daylight (Northern hemisphere - June 21)
 The Ancient Celts set up megaliths, in concentric circles, at Stonehenge to
mark the winter and summer solstices.
 Ancient African cultures set large rock pillars into patterns to predict the
timing of the solstices as well.
Equinox represents periods of equal day and night
Autumnal equinox – occurs in the fall (Northern hemisphere - Sept. 22)
Vernal equinox – occurs in the spring (Northern hemisphere - Mar. 21)
 The Mayans of Central America built an enormous cylinder shaped tower, at
Chichen Itza, to celebrate the two equinoxes.
 The Ancient Egyptians built many pyramids and other monuments to align
with the seasonal position of certain stars.
 Aboriginal Peoples of Southwestern Alberta used key rocks, which aligned with
certain stars, in their medicine circles.
Constellations are the groupings of stars we see as patterns in the night sky. There
are 88 constellations and many are explained in Greek Mythology. (ex. Ursa Major)
Asterisms are also groupings of stars, but are not officially recognized as
constellations.
(Example: Ursa Major- Constellation or the Big dipper – asterism)
Sky Co-ordinates
Altitude and Azimuth are calculated from the observer's (the person in blue)
position:
Altitude tells you "how far above the horizon the object is"; the point straight
overhead has an altitude of +90 degrees; straight underneath, an altitude of -90
degrees. Points on the horizon have 0 degree altitudes. An object halfway up in the
sky has an altitude of 45 degrees.
Azimuth determines "which compass direction it can be found in the sky." An
azimuth of zero degrees puts the object in the North. An azimuth of 90 degrees puts
the object in the East. An azimuth of 180 degrees puts the object in the South, and
one of 270 degrees puts the object in the west. Thus, if you are told that an object is
at altitude 30 degrees, azimuth 80 degrees - look a little North of due East, about a
third of the way from the horizon to the zenith.
Zenith is the position in the sky directly overhead. The path in the sky along which
the Sun takes is called the ecliptic. The Celestial Sphere is the name given to the very
large imaginary ‘sphere of sky’ surrounding the Earth.
The Stars as a Frame of Reference
Ancient cultures tried to explain the motions of the stars and planets, with their frame
of reference being the Earth. To track the actual motion of each celestial body in
space, you need to use the stars as your frame of reference, instead of the Earth. To do
this you would make an observation of which celestial body you are studying and
include other stars in relation to it. Make subsequent observations and include those
same stars. Over a period of time you would be able to determine in which direction
the celestial body you are studying is moving.
The Earth-Centred Model
Geocentric Model-The Earth was fixed and the center of the solar
system with all celestial bodies in space rotating around it.
Aristotle’s Model - Assisted by Pythagoras and Euclid
The stars were ‘the firmament of fixed stars’ One of the problems
this model faced was trying to explain the
retrograde motion (reversal of direction) of Mars, Jupiter and
Saturn. To account for this Ptolemy developed a model
that gave Aristotle’s planets another level of circular
motion called epicycles.
The Sun-Centred Model
Heliocentric Model- Nicholas Copernicus developed this model, in
which the Sun was fixed and a rotating Earth revolved around it.
Copernicus’ Model - Confirmed by Galileo and Kepler
Kepler also said that the planets had an elliptical orbit rather than
circular.
Topic 1 Assignment
Vocabulary: (Define each of the following)
Frame of reference- A set of axes of any kind that is used to describe the positions or
motions of things.
Celestial bodies- All objects seen in the sky (the sun, Moon, stars and planets)
Constellations- Groupings of stars that form patterns, which appear like objects and
are given names (such as Orion, the hunter)there are 88 constellations and many are
explained in Greek Mythology. (ex. Ursa Major)
Asterism- are also groupings of stars, but are not officially recognized constellations.
(example: Ursa Major- Constellation or the Big Dipper- asterism)
Planets- Celestial bodies in our solar system, including Earth, that orbit the Sun.
Altitude- Is the angle measured above the horizon in degrees when measuring
altitude-azimuth co-ordinates.
Azimuth- Is the angle measured clockwise from north when measuring altitudeazimuth co-ordinates.
Astrolabe- Is a device used to measure the altitude of an object.
Compass- a device used to measure an object’s azimuth.
Geocentric model- a model of universe that places Earth at the Centre with the Sun,
moons, and planets revolving around it.
Heliocentric model- A model of the universe that places the Sun at the centre with
Earth, the planets, and moons revolving around it.
Elliptical orbit- A figure that looks like a squashed circle; planets in the solar system
move in elliptical orbits around the Sun.
1. Why did ancient peoples think that Earth was at the centre of the universe?
Ancient peoples thought that Earth was at the centre of the universe because of
Earth’s rotation, stars and planets appear to circle above us and use stars to track
motion in the sky instead of the Earth. Ancient peoples still believed that the stars
circle around earth. Then they made such thing as an Earth-Centred or geocentric
model of the universe.
2. What are two differences between the geocentric model and the heliocentric
models.
The two differences between the geocentric model and the heliocentric models is that
the geocentric model is a model of universe that places Earth at the centre with the
sun, moons, and planets revolving around it. The heliocentric model is a model of
universe that places the Sun at the centre with Earth, the planets, and moons revolving
around it.
Altitude and Azimuth
What to Do
Answer the questions in the space provided.
1. Use the following diagram to identify the star with each of these coordinates:
Star
D
B
A
C
Altitude
80º
45º
70º
25º
Azimuth
330º
135º
245º
50º
D
A
B
C
N
W
E
S
2. Place stars at the following (approximate) co-ordinates on the following picture:
Star
P
Q
R
S
Altitude
50º
10º
70º
45º
Azimuth
180º
260º
30º
110º
3. Suppose that you recorded the alt-azimuth coordinates of the top of a tall building and of the
moon. Two hours later, would these coordinates have changed? Explain your reasoning.
No I don’t think that the coordinates would change that much over two hours
because the building doesn’t move and the moon moves slowly.
N
W
E
S