lec 2: 29 august 2011 chapter 1: powers of 10, angles, the...
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Lec 2: 29 August 2011 Chapter 1: Powers of 10, Angles, The Sky TODAY - The Layout of the Sky
• The Appearance of the Sky (from Earth) • Angular Size and Angular Distance • Describing “Location” on the Sky
NEXT - The Daily Motion of the Sky • Chapter 2 Pre-Quiz • Celestial Coordinate Systems • Spherical, Rotating Earth • Begin: Daily Motion of the Sky
ANNOUNCEMENTS: First Labs: This Tuesday and Thursday
Chapter 2 PreQuiz on Wednesday
The 2 Greatest Challenges for You 1. SCALE: How Big? How Far?
– astronomy deals with the LARGEST and SMALLEST scales • e.g. spatial, mass, time, temperature • single set of physical laws describes it all !
– how do you deal with a huge range of scales? • visualize & compare • conceptualize • use Scientific Notation (review Appendix)
– Video: “Powers of 10”
The 2 Greatest Challenges (continued) 2. PERSPECTIVE: (egocentric->heliocentric)
– 3-dimensional universe projected onto a 2-dimensional sky
– spherical geometry (Earth and Sky) – everything is moving, including us! – you must learn to shift your point of view
• imagine how things will appear when you look up at the sky from the Earth
• get used to looking at the sky; take every opportunity early in the semester to become familiar with the sky and how it “moves”
• mostly it is due to the motion of the Earth (and us)
The Sky (viewed from Earth) • The Sky APPEARS to us as if all the “celestial” bodies
(Sun, Moon, planets, stars, etc.) are on the inside of a sphere (2-Dimensional surface)
• Really, they are distributed in a 3-Dimensional space – demo: class photos – demo: Orion in 3-D
• We see one half of this sphere at any given time • The Earth blocks out the other half • The Sky is dark about half the time, when the Sun is
“below” the HORIZON • The Sky is bright when Sun is above horizon (Why?) • What celestial objects are visible in the daytime?
Are You Really 2-Dimensional? It Looks That Way.
Our 2-D view of the constellation Orion
The 3-D layout of the stars that appear to us as Orion
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The Sky (viewed from Earth) • We see one half of this sphere at any given time
– the Earth blocks out the other half • The Sky is dark about half the time
– when the Sun is “below” the horizon • The Sky is bright when Sun is above horizon
– Why? – What celestial objects are visible in the daytime?
• Everything in the sky moves in a regular, predictable way, but you’ve got to watch it night after night, year after year to fully grasp the patterns (or just take this class :-)
Our Goals for Today...
• How can we describe LOCATION on the sky?
• How can we describe DISTANCE between objects on the sky?
• How can we describe SIZE of objects on the sky?
• In-class Exercise: Describing location on the sky
Location in the Sky. I. “Local” • “Altitude-Azimuth” Coordinate System
– depends on your location on Earth (different positions on Earth see same thing but at different altitudes or azimuths and at different times)
• ALTITUDE (aka “Elevation”) – angle measured up from horizon (0 to 90 degrees)
• AZIMUTH (aka “heading” or “bearing”) – angle measured along the horizon circle – same as compass heading – measured from North toward the East – examples: North=0o, East=90o, South=180o
• HORIZON - circle where Earth and Sky appear to intersect • ZENITH - point straight overhead • MERIDIAN - circle (or semi-circle) on sky dividing through N, zenith, and S
These depend on your location on Earth, time of day, & time of year
Angular Units • Subdivide complete CIRCLE into 360 degrees
• Subdivide one degree into 60 arcminutes – minutes of arc – abbreviated as 60 arcmin or 60´
• Subdivide one arcminute into 60 arcseconds – seconds of arc – abbreviated as 60 arcsec or 60”
1° = 60 arcmin = 60´ 1´ = 60 arcsec = 60” “Angular Size” of Moon : ~1/2 degree
in this example, Moon is about 50 degrees “above the horizon”
Angular Size and Angular Distance
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Pointer stars in Big Dipper about 5o apart
[ so you could fit 10 Full Moons between them! ]
Location in the Sky. II. “Geographic” • CONSTELLATIONS - names given to patterns
of stars in the sky; have boundaries analogous to state boundaries
• analog: describe locations on Earth in terms of accepted boundaries; e.g. Charleston, South Carolina, United States, N. America
• how did they get their names? • why constellations aren’t a good way to describe
location (at least not accurately) • how are constellations used now?
Eighty-eight constellations cover the sky
• Ancient peoples looked at the stars and imagined groupings made pictures in the sky
• Different patterns named by different cultures; modern names come from a variety of sources
ORION (the hunter)
Modern Constellations • Entire sky divided into 88
“constellations”
– internationally agreed upon names and boundaries
– boundary lines drawn on the sky so that all stars are in only one constellation
– different shapes and sizes; fit together like a jigsaw puzzle
– many star names come from the constellation they are in (e.g. Alpha Centauri)
the stars in a constellation only appear to be close together (on the sky), because they are in nearly the same direction as seen from Earth
Looking North