"Stargazers and Skywatchers," section #1 : on disk Ssky.htm, on the web
          http://www.phy6.org/stargaze/Ssky.htm , now supplemented by Lesson plan #1
and
"The Celestial Sphere," section #1a : on disk Scelsph.htm, on the web
          http://www.phy6.org/stargaze/Scelsph.htm now supplemented by Lesson plan #1a

"From Stargazers to Starships" home page and index: on disk Sintro.htm, on the web
          http://www.phy6.org/stargaze/Sintro.htm

• Understand the apparent rotation of the night sky, the special role of the Pole Star and the reason which sets that star apart.
• The student will also realize that other celestial objects--Sun, Moon and planets--share the rotation (and hence rise and set), even though their positions among the stars slowly change.
• [Optional: Understand the mounting of astronomical telescopes.]

Terms: Celestial sphere, constellation, celestial pole, the Pole Star ("Polaris"), celestial equator, rotation of the Earth, planets [theodolite, equatorial axis].

Stories and extras: Psalm 19 (A poetic impression of the sky)

    Start the class with a discussion of the night sky: how many have seen the sky on a really dark night, away from streetlights and w/ith no Moon? What was it like?
    What is a constellation? Do you recognize constellations? Did you see the Pleiades? Did you see the Milky Way?    (Do you know what it is? Billions of distant stars in our galaxy. The galaxy is a flat wheel, and we are looking through it side-on.). Has anyone visited a planetarium show? What was it like?
    The quoted part of psalm 19 may be read by someone at a proper moment

    After this, present the material. The questions below may be used in the presentation, the review afterwards or both

When we view the stars at night, it seems as if we are at the center of a huge sphere and the stars are points of light distributed across it. That is "the celestial sphere." In ancient times people believed such a sphere actually existed and was rotating around us.
We know better now, stars are actually very far away, and the Earth is the object that rotates. Still, the celestial sphere remains a convenient tool for describing the positions of the stars in the sky.)

Yes, which is why we have patterns, constellations, of fixed shapes. Over time the stars themselves move, but the distances to them are so great, the movement appears to be small. A few "planets" (wanderers) move quickly among them, including Venus and Jupiter, brighter than any fixed star.

They rise and set, like the Sun and Moon, because of the rotation of the Earth.

The Earth rotates around an imaginary line connecting its north pole and south pole.[This may be illustrated using a globe or an apple or any round object]

About 24 hours--more accurately, 4 minutes less than 24 hours, as will be explained in a later class.

Counterclockwise. When it is 12 o'clock in New York and that part of the Earth directly faces the Sun, it is only 9 o'clock in California. In 3 hours California will have rotated to the position where New York was.

One may explain that "clockwise" and "counterclockwise" is relative, it depends on the place from which one views the motion--it is not something absolute. Hold a plate vertically in your left hand, on your left side, with the top of the plate facing the class, Slowly circle a finger around it in a clockwise direction. Then gradually swing the arm to your right, with the finger continuing in the same circle. The class now watches the bottom of the plate, and the same motion seems to be counterclockwise.]

The Pole Star is the star around which all other stars in the Northern Hemisphere appear to rotate.

No. On clear nights, in the continental US or Europe, the Pole Star and the ones near it may be seen at any time.

No, stars near the southern pole of the sky never rise. Similarly, the Pole Star is never visible from Australia.

Stars will appear to rush through your field of view. When you see the Sun rise or set, it seems to move very slowly, as do stars that rise or set, but a telescope greatly magnifies this motion and makes it appear fast.

[Note: The book "First Light" by Richard Preston describes how astronomers at the 200-inch telescope on Mt. Palomar--for many years the largest in the world--deliberately clamped down the telescope, to make it sweep across long strips of the sky, searching for distant galaxies. A recommended, well-written book by a writer who spent some months living with the astronomers at the observatory.]

The mounting of a telescope, allowing it to rotate around an axis parallel to that of the Earth. One keeps the star in view by rotating the telescope