chapter 2b: the sky. the celestial sphere (ii) from geographic latitude l (northern hemisphere), you...

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Chapter 2b: The Sky

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Page 1: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Chapter 2b:

The Sky

Page 2: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

The Celestial Sphere (II)• From geographic

latitude l (northern hemisphere), you see the celestial north pole l degrees above the horizon;

• From geographic latitude –l (southern hemisphere), you see the celestial south pole l degrees above the horizon.

• Celestial equator culminates 90o – l above the horizon.

l

90o - l

Page 3: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Example:New York City: l ≈ 40.70

HorizonNorth

Celestial North Pole

40.70

South

49.30

Celestial Equator

The Celestial South Pole is not visible from the northern hemisphere.

Horizon

Page 4: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

The Celestial Sphere (III)

Page 5: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Apparent Motion of the Celestial Sphere

Looking north, you see stars circling counterclockwise around the celestial north pole.

Page 6: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Apparent Motion of the Celestial Sphere II

Over the course of the night, stars rise on the east, travel from east to west (left to right if viewed from the northern hemisphere) through the southern sky, and set in the west.

Page 7: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Precession (I)

Gravity is pulling on a slanted top. => Wobbling around the vertical.

The Sun’s gravity is doing the same to the Earth.

The resulting “wobbling” of the Earth’s axis of rotation around the vertical w.r.t. the Ecliptic takes about 26,000 years and is called

precession.

Page 8: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Precession (II)

As a result of precession, the celestial north pole follows a circular pattern on the sky, once every 26,000 years.

It will be closest to Polaris ~ A.D. 2100.

~ 12,000 years from now, it will be close to Vega in the

constellation Lyra.

There is nothing peculiar about Polaris at all (neither particularly bright nor nearby etc.)

Page 9: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Knowledge CheckWhy does the sky look strange to someone from the northern hemisphere?

Page 10: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

Coming Attraction:Milankovitch Hypothesis

• Hypothesis proposed in 1920, that small changes in Earth’s orbit, precession, inclination and other effects may affect the Earth’s climate and trigger ice ages. Controversial at first but becoming more mainstream. There will be a paper in the resources section of the course web site to read regarding this idea which goes beyond the material in the book. You should read this before next Wednesday.

Page 11: Chapter 2b: The Sky. The Celestial Sphere (II) From geographic latitude l (northern hemisphere), you see the celestial north pole l degrees above the

The Annual Motion of the Sun

Due to Earth’s revolution around the sun, the sun appears to move through the zodiacal constellations.

The Sun’s apparent path on the sky is called the Ecliptic.

Equivalent: The Ecliptic is the projection of Earth’s orbit onto the celestial sphere.