Astro 100


 

         

          Astro 100

             The Solar System

             IUPUI (Daytime)

                     

                    Brian Woodahl

                    bwoodahl@iupui.edu

                    (Don't Use Canvas to contact me, use email link)

                    Office: LD 156-S, 278-9244

                    Class: LE 101 on Tues and Thur 10:30 - 11:45

                    http://woodahl.physics.iupui.edu/Astro100

                    Is the University open/closed today?



Tuesday's On-Line Activity (November 20)


Quiz 11 (Tuesday, November 27)


Week 15 Images


Week 14 Image


Quiz 10 (Tuesday, November 13)


Week 13 Images


Quiz 9 (Tuesday, November 6)


Week 12 Images


Computing Your Current Grade


Exam 2 Scores


Week 11 Images


Exam 2 (Tuesday, October 30)


Exam 2 Study Guide


Quiz 8 (Tuesday, October 23)


Week 10 Images


Quiz 7 (Thursday, October 18)


Week 9 Images


Quiz 6 (Tuesday, October 9)


Week 8 Images


Quiz 5 (Tuesday, October 2)


BREAKING: Martian Cold Brines May Have Oxygen to Support Life


Week 7 Images


Week 6 Images


Exam 1 Scores


Exam 1 (Thursday, September 20)


Exam 1 Study Guide


Quiz 4 (Tuesday, September 18)


Week 5 Images


Quiz 3 (Tuesday, September 11)


Week 4 Images


Quiz 2 (Tuesday, September 4)


Week 3 Images


Quiz 1 (Tuesday, August 28)


Week 2 Images


Week 1 Images


Course Information


The TOTAL SOLAR ECLIPSE of 2017 (Monday, August 21st)


The Most Commonly Asked Question in Intro Astronomy

A solar eclipse only occurs if the New Moon is about within half a degree of the ecliptic plane (defined by the orbit path of Earth as it travels around the Sun). The Moon's orbital path, around the Earth, is (unfortunately) inclined by about 5 degrees to the ecliptic. Thus, there are only two opportunities each moonth (punning) when the Moon passes through the ecliptic. These points are called the nodes (ascending, descending). The Moon passing through a node is not sufficient, it must pass through the node during the New Moon lunar phase.

About twice a year, during an approximately 45 day window (based upon the orbital speeds of the Earth and Moon), the New Moon is close enough to a node that a solar eclipse can occur. Further complicating the motion, the Moon's orbital plane precesses relative to the ecliptic. Hence, the nodes precess around the ecliptic, completing one rotation about every 18.6 years. In addition, because the Moon's path around Earth is elliptical, during many solar eclipses the angular diameter of the Moon is not large enough to fully cover the Sun. Only when the New Moon is near a node and near perigee (i.e. closest to the Earth), does totality occur. On average, it takes about 400 years for totality to occur again at the same geographical location.


Amazon.com Links for Textbooks (New and Used)


Excellent Beginner's Telescope for General Astronomy



Imagining the Tenth Dimension


Gravity Simulator


FYI (and Just For Fun)


University Policy Regarding Sexual Harassment



Department of Physics, IUPUI - Updated on November 17, 2018 at 3:10 PM EST