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Transcript of RECAP - Saddleback College · completing a tutorial or you will get points deducted or get a zero!...
34 deg.
90 deg.
Latitude
Rotation
Daily Changes Revolution
Monthly Changes
Why do we see what we see??
Constellations – the 88 semi-rectangular regions that make up the sky
• Northern constellations have Latinized
Greek-mythology names:
– Orion, Cygnus, Leo, Ursa Major, Canis Major,
Canis Minor
• Southern constellations have Latin
names:
– Telescopium, Sextans, Pyxis
What do you think?
• What causes the stars to move?
• Do the stars actually move in the way they
appear from Earth?
• Do the stars stay in the same position in the
sky all day/night long?
Imagining a spinning
Celestial Sphere
surrounding Earth
aids in thinking
about the position
and motion of the
sky
Animation of Celestial Sphere
http://bcs.whfreeman.com/universe6e/pages/bcs-
main.asp?v=category&s=00110&n=01000&i=02110.02&o
=|02000|01000|&ns=0
Imagining a spinning Celestial
Sphere surrounding Earth aids in
thinking about the position and
motion of the sky
Celestial Sphere Rotation
Celestial Sphere
Rotation
North Star
Star A
Star B
1
1
3
3
2
2
4
4
Earth’s Equator
Figure 1
Celestial Sphere
Celestial Sphere Rotation
Celestial Sphere
Rotation
Celestial Sphere
Star A
Star B
1
1
3
2
2
4
4
3
Figure 2
Horizon
1) Explain how to find North on the horizon from the North star.
2) Where is the North star when you’re at the North pole?
Celestial Sphere
Celestial Sphere Rotation
Celestial Sphere
Rotation
Celestial Sphere
Star A
Star B
1
1
3
2
2
4
4
3
Figure 2
Horizon
1) Is the horizon shown a real
physical horizon, or an
imaginary plane that extends
from the observer and Earth
out to the stars?
2) Can the observer shown
see an object located below
the horizon?
3) Is there a star that is in an
unobservable position?
4)When a star travels from
being below the observer’s
horizon to being above the
observer’s horizon, is that star
rising or setting?
Tutorial: Position – p.1
PUT NAMES in Tutorials• Work with a partner
• Read the instructions and questions carefully
• Talk to each other and discuss your answers with each another
• Come to a consensus answer you both agree on
• If you get stuck or are not sure of your answer ask another group
• If you get really stuck or don’t understand what the Lecture Tutorial is asking ask your Professor for help
• I WILL BEGIN STAMPING TUTORIALS A LITTLE BEFORE YOU FINISH THE TUTORIAL SINCE THERE ARE 70+ OF YOU, BUT YOU MUST ALL FINISH THE TUTORIAL OR YOU WILL GET A ZERO! DO NOT WALK OUT OF THE ROOM OR GET OFF TASK WHEN WE ARE COMPLETING A TUTORIAL OR YOU WILL GET POINTS DEDUCTED OR GET A ZERO!
• IF THE TUTORIAL IS COMPLETED AT THE END OF LECTURE, NO ONE IS ALLOWED TO LEAVE EARLY UNLESS YOU CHECK WITH ME FIRST! IF YOU LEAVE EARLY YOU’LL GET A ZERO.
In what
direction is the
observer
facing?
A. toward the South
B. toward the North
C. toward the East
D. toward the West
Celestial Sphere
Celestial Sphere Rotation
Celestial Sphere
Rotation
Celestial Sphere
Star A
Star B
1
1
3
2
2
4
4
3
Figure 2
Horizon
Imagine that from your current location you
observe a star rising directly in the east.
When this star reaches its highest position
above the horizon, where will it be?
A. high in the northern sky
B. high in the southern sky
C. high in the western sky
D. directly overheadCelestial Sphere
Celestial Sphere Rotation
Celestial Sphere
Rotation
Celestial Sphere
Star A
Star B
1
1
3
2
2
4
4
3
Figure 2
Horizon
Where would
the observer
look to see the
star indicated by
the arrow?
A. High in the Northeast
B. High in the Southeast
C. High in the Northwest
D. High in the Southwest
Celestial Sphere
Celestial Sphere Rotation
Celestial Sphere
Rotation
Celestial Sphere
Star A
Star B
1
1
3
2
2
4
4
3
Figure 2
Horizon
Telescope Field of View
Field of View = Eyepiece apparent FOV ÷ Magnification
Large Magnification = Small field of view
Small Magnification = Large Field of view
Moon=0.5 deg.
Right Ascension (RA) and
Declination (Dec) are similar
to latitude and longitude on
the surface of the Earth.
Latitude and longitude are
fixed with respect to positions
on Earth. But RA and Dec
are fixed with respect to
positions of stars in the sky.
What is moving, the celestial
sphere or the Earth?
To an Earthling observer,
what appears to move?
Declination (like latitude) is measured in degrees north or south of the Celestial
equator.
Right ascension (like longitude) is measured in units of hours, minutes, and seconds
eastward from the position of the vernal equinox on the Celestial equator. The Vernal
Equinox is the position of the Sun on the first day of Spring.