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Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

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Page 1: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

Physics 202: Introduction to Astronomy – Lecture 2

Carsten Denker

Physics DepartmentCenter for Solar–Terrestrial

Research

Page 2: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Prologue Constellations Celestial sphere North and south

celestial poles Celestial equator Celestial coordinates Declination and

right ascension Solar and sidereal

day

Ecliptic Zodiac Seasons Summer and winter

solstice Vernal and

autumnal equinox Tropical and

sidereal year Precession

Page 3: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Constellations in the Sky

Page 4: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Celestial Coordinates

Page 5: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Solar and Sidereal Day

Page 6: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Long-Term Changes ‒ Precession

Page 7: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Group ProblemHow and why does a day measured

by the Sun differ from a day measured by the stars?

Assume that the Earth would orbit the Sun in the opposite direction. How would that affect the solar and sidereal day?

Page 8: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

The Orbit of the MoonPhasesNew, quarter, and full MoonSidereal month (27.3 days) and

synodic month (29.5 days)Solar and lunar eclipsesTotal, annular and partial solar

eclipseUmbra and penumbra

Page 9: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Lunar Phases

Page 10: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Lunar Eclipse

Page 11: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Solar Eclipse

Page 12: Physics 202: Introduction to Astronomy – Lecture 2 Carsten Denker Physics Department Center for Solar–Terrestrial Research

January 20, 2006 Center for Solar-Terrestrial Research

Group ProblemWhy aren’t there lunar and solar

eclipses every month