|Back to astronomy || Go to lesson 1 || Go to lesson 2 || Go to lesson 3 || Go to lesson 4 || Go to lesson 5 || Go to page 6 || Go to lesson 7 || The End ||

Astronomy for Physical Science 112

Lesson 3: Motion of the Sky

Key terms with links- Astronomy facts

Tahsiri: Lecture notes :

Kenealy: Read chapters (1-6).

Please click on the Virtual library www reference guides after the red arrow for further Discussions and Illustrations on the important terms relevant to my lectures.


Virtual library www Reference Guides

1) The Daily Motion of thr Sky

* The daily or diurnal, westward paths of stars are circles that are centered on the north celestial pole. The diurnal circles grow smaller for stars that are nearer the north celestial pole.

* The celestial equator: is a line on the celestial sphere that divides it into northern and southern hemispheres.

* The Equtoral System: is used to locate stars on the celestial sphere. This system resembles the terrestrial system of longitude and latitude. In the equatorial system,

* Declination describes the angular distance of a star north or south of the celestial equator.

* Right ascension describes the east-west location of a star on the celestial sphere.

a) Illustrations(1) Diurnal Motion (2) The Daily Motion of the Celestial Sphere (3) Daily Motion (4) Solar Motion (5) Prictice Questions (6) Motion of Sun and Stars (7) Diurnal Motion Focus Questions (8) Right ascention and Declination (9) Right Ascension & Declination (10) Right Ascension Converting between RA angles in degrees and in hours:minutes


2) The Apparent Motion of the Sun

* Ecliptic: The plane of the Earth's orbit about the Sun. As a result of the Earth's motion, the Sun appears to move eastward among the stars, following a path that is also called the ecliptic.
and its motion is repeated annually.

* The ecliptic is inclined with respect to the celestial equator, so the declination of the Sun varies during the year.

* The Season:  Changes in the declination of the Sun produce an annual pattern of change in its rising and setting points as well as change in its altitude at noon. These changes are responsible for the Seasons.

* Apparent Solar Time: Time kept according to the actual position of the Sun in the sky. Apparent solar noon occurs when the Sun crosses an observer's meridian. The variable rate of the Sun's motion on the ecliptic causes changes in the length of the solar day throughout the year.

b) Illustrations(1) The Ecliptic (2) Ecliptic Plane (3) The Ecliptic (4) Ecliptic and the motion of the Sun (5) The Earth, Sun, and Moon (6) Motion of the Sun



  3) The phases of the Moon

* The phase of the Moon happen because the part of the Moon's illuminated hemisphere that we see varies throughout a Synodic month .

* The length of a synotic month is 29.53 days between successive occurrences of the same phase of the Moon

c) Illustrations(1) Moon Phases (2) Virtual Reality Moon Phase Pictures (3) Phase of the Moon (4) Phases of the Moon and Percent of the Moon Illuminated (5) Moon Phases for 20001 (6) Synaotic and Sidereal Mounth (7) Sydereal and Synotic Mounth (8) Synotic&Sidereal (9) The Sidereal Month


4) The Motion of the Moon

*  The Moon appears to move eastward among the stars, returning to the same place after a Sidereal month

d) Illustrations(1) Motion of the Moon (2) Homework with Solutions (3) Daily Motion of the Moon


5) The Motions of the Planets

*  The planets usually appear to move eastward among the stars. However, at regular intervals they appear to move westward during periods of Retrograde motion. The motions of the planets among the stars are quite complex.

f) Illustrations(1) The retrograde motion of planets (2) Retrograde Motion (3) Retrograde Motion Simulation (4) Retrograde Motion with Animation


Astonomy Facts

 

1. Which of the following coordinates describes the angular distance of an object north or south of the celestial equator? Declination


2. Suppose there is a star which rises at 10 p.m. tonight. At what time did it rise one month ago? Midnight


3. An observer in Quito, Ecuador (latitude 0 deg) sees the Sun at the zenith at noon on which day(s)? Spring and Fall equinox


4. The sun moves eastward among the stars at the rate of about one degree per day


5. The time that your wristwatch keeps is mean solar time


6. The occurrence of seasons on the Earth is due to the Earth's axis being inclined to the ecliptic


7. At approximately what time does the new moon rise? Sunrise


8. Relative to the stars, the moon moves eastward


9. In which of the following circumstances is it possible to observe the full moon? Rising at sunset


10. Which of the following is true of the motion of the planet Mars among the stars? retrograde loops always are separated by the same interval of time

 

|Back to astronomy || Go to lesson 1 || Go to lesson 2 || Go to lesson 3 || Go to lesson 4 || Go to lesson 5 || Go to page 6 || Go to lesson 7 || The End ||