the Night Sky Historically patterns in the sky

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the Night Sky

the Night Sky

Historically, patterns in the sky helped people navigate and keep time. Egyptian skychart

Historically, patterns in the sky helped people navigate and keep time. Egyptian skychart

The Sky Orion Stars appear in fixed patterns called constellations. (Planets, “wanderers, ” appear

The Sky Orion Stars appear in fixed patterns called constellations. (Planets, “wanderers, ” appear to move. )

Note that the stars that make up constellations are at different distances. • What

Note that the stars that make up constellations are at different distances. • What we see is their projection onto a virtual “Celestial Sphere. ”

The Earth’s rotation makes the sky appear to revolve around us.

The Earth’s rotation makes the sky appear to revolve around us.

Polaris: does not appear to move because it's aligned with the Earth's axis.

Polaris: does not appear to move because it's aligned with the Earth's axis.

Seasonal Constellations: stars closer to the equator will rise and set and we will

Seasonal Constellations: stars closer to the equator will rise and set and we will see different constellations through the year.

 Axial Tilt: the Earth’s axis is tilted 23. 5 o from the plane

Axial Tilt: the Earth’s axis is tilted 23. 5 o from the plane of the Earth’s orbit. So the Sun and planets appear to move along a tilted line in the sky

The Seasons And when our hemisphere is tilted toward the Sun, we have summer;

The Seasons And when our hemisphere is tilted toward the Sun, we have summer; away, we have winter. Summer Solstice: Longest day (Sun at highest point) Winter Solstice: Shortest day Equinoxes: Equal Night/Day

Precession: Long Term Changes Over 26, 000 years the Earth’s axis moves in a

Precession: Long Term Changes Over 26, 000 years the Earth’s axis moves in a complete circle. (Polaris was not always the pole star. )

The Motion of the Planets The planets wander on the sky along the ecliptic:

The Motion of the Planets The planets wander on the sky along the ecliptic: mostly West to East but occasionally backwards – retrograde motion

Ptolemy’s model (~140 CE) used 80 circles. -this didn't explain retrograde motion.

Ptolemy’s model (~140 CE) used 80 circles. -this didn't explain retrograde motion.

 Heliocentric Model: Copernicus felt a Suncentred system could explain the motion more simply.

Heliocentric Model: Copernicus felt a Suncentred system could explain the motion more simply.

 Heliocentrism and Retrograde motion

Heliocentrism and Retrograde motion

Galileo Galilei Galileo: did not invent the telescope but was the first to study

Galileo Galilei Galileo: did not invent the telescope but was the first to study astronomy with it (1609).