Sky Motions Diurnal Motion Annual Motion DIURNAL MOTION

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Sky Motions þ Diurnal Motion ü Annual Motion

Sky Motions þ Diurnal Motion ü Annual Motion

DIURNAL MOTION o Daily East / West motion of the sky Due to the

DIURNAL MOTION o Daily East / West motion of the sky Due to the Earth’s rotation (15°/hour) [360°/24 hours = 15°/hour] [1° in 4 minutes] o Stars fall into two groups Circumpolar - never rise or set Equatorial

Circumpolar Stars

Circumpolar Stars

Equatorial Stars

Equatorial Stars

View from the North Pole

View from the North Pole

View from the Equator

View from the Equator

Coordinate System

Coordinate System

Celestial Meridian n Circle going through north and south points on the horizon and

Celestial Meridian n Circle going through north and south points on the horizon and the zenith Z

Celestial Meridian n Objects on the Meridian are at their highest point in the

Celestial Meridian n Objects on the Meridian are at their highest point in the sky (transit) n Astronomical noon is when Sun is on the Meridian. ¤Does not mean the Sun is directly overhead. ¤Midnight is when the Sun is on the Meridian below the horizon.

Zenith n n This is a measure of how high above the horizon the

Zenith n n This is a measure of how high above the horizon the star or planet is located. A star on the horizon has an altitude of 0 o while a star directly overhead (this point is called the z http: //astro. unl. edu/naap/motion 2/s tarpaths. html enith) has an altitude of 90 o.

What is the altitude of a star that is exactly halfway between the horizon

What is the altitude of a star that is exactly halfway between the horizon and the zenith?

Polaris and Altitude n Polaris “north star” ¤ 1 degee from NCP n Altitude

Polaris and Altitude n Polaris “north star” ¤ 1 degee from NCP n Altitude of polaris is always equal to the latitude of the observer. ¤Equator 0º altitude = 0º ¤North pole 90º altitude= 90º aka ¤Grosse pointe 42º altitude = 42º Zenith

South pole n Can you see polaris? ¤Nope!

South pole n Can you see polaris? ¤Nope!

Annual Motion

Annual Motion

ANNUAL MOTIONEarth’s revolution o Constellations move westward during the year. ¤Due to Earth’s orbital

ANNUAL MOTIONEarth’s revolution o Constellations move westward during the year. ¤Due to Earth’s orbital motion around the Sun ¤Sun appears to moves eastward 1°/day n o Path of the Sun called the ECLIPTIC Ecliptic inclined 23. 5° to Equator ¤Horizon calendar

Horizon Calendar

Horizon Calendar

Sunrises The Sky and. Dome Sunsets Polaris On the day of an summer solstice…

Sunrises The Sky and. Dome Sunsets Polaris On the day of an summer solstice… S W On the day of an winter solstice… On the day of an equinox… E N

Polaris W S Winter Solstice Vernal or Autumnal Equinox Summer Solstice N E Starting

Polaris W S Winter Solstice Vernal or Autumnal Equinox Summer Solstice N E Starting Points for the Sun

Sunrise in Athens

Sunrise in Athens

Stonehenge

Stonehenge

Earth’s Annual Motion Leo

Earth’s Annual Motion Leo

NCP Celestial Sphere Autumnal Equinox 23. 5° Ecliptic Vernal Equinox SCP Celestial Equator

NCP Celestial Sphere Autumnal Equinox 23. 5° Ecliptic Vernal Equinox SCP Celestial Equator

Sun’s Motion Tool

Sun’s Motion Tool

Inclined Pole causes Seasons Northern Hemisphere Summer N S Northern Hemisphere Winter 23. 5°

Inclined Pole causes Seasons Northern Hemisphere Summer N S Northern Hemisphere Winter 23. 5°

Sun’s motion along the Ecliptic Sun’s Motion

Sun’s motion along the Ecliptic Sun’s Motion

“Stars” o Fixed Stars ¤Modern concept of stars ¤Form the Constellations o Planets -

“Stars” o Fixed Stars ¤Modern concept of stars ¤Form the Constellations o Planets - traveling or wandering stars ¤ Sun, Moon, Mercury, Venus, Mars, Jupiter, and Saturn o o Meteors - “shooting stars” Comets - “long-haired stars”