Lecture 05: Mapping Earth & Sky

Lecture 05: Mapping Earth & Sky

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Lecture 06: Daily and Annual Motions

Why do celestial objects appear to rise and set every day? How does this depend on where you are on the Earth, or the time of year? In today's lecture we we set the heavens into motion and review the two most basic celestial motions. Apparent Daily Motion reflects the daily rotat ...  Afficher plus

Lecture 07: The Four Seasons

Why do we have different seasons? This lecture explores the consequences of the tilt of the Earth's rotation axis relative to its orbital plane combined with the apparent annual motions of the Sun around the Ecliptic. The most important factor for determining whether it is hot or ...  Afficher plus

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Welcome to Astronomy 161
Astronomy 161 - Introduction to Solar System Astronomy

Welcome to the Astronomy 161 Lecture Podcasts. This is a brief message from me explaining the podcasts, and welcoming new and old listeners. University. Lectures will begin on Wednesday, 2006 Sept 20, and run through Friday, 2006 December 1. New lectures will appear shortly befor ...  Afficher plus

Lecture 44: Life, the Universe, and Everything (Life Part II)
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How can we search for extraterrestrial intelligence, and what are we looking for? This second part of a 2-part lecture picks up where we left off yesterday by examining SETI, the Search for ExtraTerrestrial Intelligence, and reviews what we might look for and how. We will use thi ...  Afficher plus

Lecture 2: Astronomical Numbers
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Before we can begin our exploration of astronomy, we need to develop a common language for notating large numbers, and introduce the basic units of length, mass, and time that we will use throughout the quarter. We will first re-introduce the basic metric system, explaining how t ...  Afficher plus

Lecture 32: The Lives of Stars
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Why do stars shine? How long do they shine? This lecture describes the physics of stars on the main sequence, describes the mass-luminosity relation of main sequence stars, introduces nuclear fusion power and the nuclear fusion lifetimes of stars. From this we gain an important i ...  Afficher plus