Getting Oriented: Astronomical Coordinate Systems Why are we doing this? Lecture material for next week’s lab Basis for many important technological accomplishments.

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Presentation transcript:

Getting Oriented: Astronomical Coordinate Systems Why are we doing this? Lecture material for next week’s lab Basis for many important technological accomplishments (Pyramid of Cheops)

The basic idea Express the position in the sky of an astronomical object in terms of numbers One part of the Greek concept that there is a mathematical basis to nature

First reference system: the Horizon System Two coordinates: altitude and azimuth

Coordinates in the horizon system Altitude angle goes from 0d to 90d Azimuth angle goes from 0d to 360d

In Horizon System, we see motions in the sky The Sun rises in the east, reaches highest altitude angle due south, sets in the west When the Sun sets, it gets dark and we see the stars and planets The Moon “ “ “ “ “ The Moon rises at a different time each night and is seen against a different constellation The constellations in the evening sky are different in different seasons

Fundamental astronomical observation: The rising and setting of the Sun. Most people don’t realize other astronomical objects do this as well

Question for the audience: What is going on to cause this east-to- west motion of all objects, rising in east and setting in west? Demo

There are other aspects of the night sky (and daytime sky) that are not obvious to modern people

Seasonal Variations in the Position of the Sun (back in horizon system) This year, September 22, 10:09 PM

The changes in the rising (and setting) locations of the Sun are big

Seasonal differences in the night sky: go out tonight at 9 PM Constellations Bootes in west Bright star Vega straight overhead Constellation of Scorpius (with bright star Antares) low in southwest. Constellations of Pegasus and Andromeda just rising Check it out with the help of star charts!

There is a phenomenon that could be called the “Parade of the Constellations”? By the end of the semester, the situation will be entirely Different.

Measuring the position of the Sun against the background stars

The path of the Sun through the stars

The “parade of the constellations” Demo

Obliquity of the Ecliptic and the Altitude Angle of the Sun

Explanation of Seasonal Variations: tilt of the Earth’s axis: obliquity of the ecliptic

Two Lines on the Sky The ecliptic The celestial equator See Figure 2.11

For new purposes, we need a different coordinate system Analogy: I am riding my bike on a dirt road near Lone Tree, and want to describe to someone in London the location of a radio tower I see in the distance. Question: what system of coordinates do I use?

A New Coordinate System: Celestial Coordinates The stars “stick together” and define their own reference system. The planets move with respect to them Celestial coordinates are Right Ascension and Declination Right Ascension ….. Longitude Declination ….latitude