Presentation Transcript
A105 Stars and Galaxies :A105 Stars and Galaxies News quiz today
Moon worksheet due Thursday
Finish units 5, 6, 10 in text
Office hour/Solar Lab at Kirkwood Obs. TODAY, 11:00 – noon Today’s APOD
The Sun Today :The Sun Today Solar
Orbiting
Heliospheric
Observatory
(SOHO) Orbits between the Sun and Earth, about a million miles away – a constant view of the Sun
First News Quiz :First News Quiz Put your USERNAME on the scantron form
You may consult with your neighbors
No books, notes, papers
2 minutes per question
Modern science relies on observations and experiments! :Modern science relies on observations and experiments!
Understanding Science :Understanding Science Purpose – to understand the universe well enough to figure out the basic relationships that govern it
A process for understanding and predicting
will it rain tomorrow?
what will be on the quiz?
what will happen if…? What about facts?
new discoveries
better data
new theories
facts change!
An Ongoing Process :An Ongoing Process The process of science has been so successful because
results are widely shared and evaluated
experiments are reproduced and checked
value of ideas based on observation and usefulness, not authority
Debating Scientific Issues :Debating Scientific Issues How do we tell who is correct?
Majority vs. minority opinions
Majority isn’t always right
Debate is a poor technique for deciding
EVIDENCE and DATA
How was the experiment done?
Was it repeated by others
Is a new theory TESTABLE?
Warning Signs of Bad Science :Warning Signs of Bad Science How is it announced? Is the source reliable?
How good is the evidence?
is it anecdotal? does it appeal to authority?
does it fit what you already know?
does it violate widely-accepted laws or theories?
is contrary evidence ignored?
What kind of reasoning is used?
Can the claim be tested? The Baloney Detection Collection Phil Plait's Bad Astronomy: Home Page
Slide 9:Sound travels at a speed of 300 meters per second. In analogy to the light-year, what does 1 sound-minute equal?
a) The time sound takes to travel 300 meters.
b) The time delay of a sound heard 300 meters away.
c) The distance traveled by sound in 1 minute.
d) The speed of sound 1 minute later. A Little Review….
The Sky! :The Sky! From wunderground.com The brightness of a star is shown by the size of its dot
Getting Started :Getting Started Which way is north?
To find Polaris:
find the Big Dipper
follow to Polaris
Orion rising :Orion rising The night sky is familiar, but few people look
closely at (or think about) the complex phenomena
we observe in sky.
Patterns in the Sky :Patterns in the Sky What does the universe look like from Earth?
Why do stars rise and set?
Why do the constellations we see depend on latitude and time of year?
What causes the seasons?
What does the universe look like from Earth? :What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars, as well as the Milky Way The Milky Way is band of light making a circle around the celestial sphere.
What is it? Our view into the plane of our galaxy.
The Celestial Sphere :The Celestial Sphere The stars all appear to lie on a large sphere surrounding the Earth (the celestial sphere)
Really, the stars are all at different distances
The Celestial Sphere :The Celestial Sphere The 88 official (defined by the International Astronomical Union) constellations cover the celestial sphere.
Constellations :Constellations A constellation is a region of the sky. The regions of the constellations are irregular in shape
Investigating a Constellation :Investigating a Constellation The stars in a constellation are not all at the same distance from the Sun.
They do not form a real group in space.
The Big Dipper is part of the constellation Ursa Major :The Big Dipper is part of the constellation Ursa Major The stars of the Big Dipper are not all at the same distance from the Sun
Review: Coordinates on the Earth :Review: Coordinates on the Earth Latitude: position north or south of equator
Longitude: position east or west of prime meridian (runs through Greenwich, England)
Angular Measurements :Angular Measurements Full circle = 360º
1º = 60 (arcminutes)
1 = 60 (arcseconds)
Slide 22:We measure the sky using angles
Angular Size :Angular Size An object’s angular size appears smaller if it is farther away
The Local Sky :The Local Sky An object’s altitude (above horizon) and direction (along horizon) gives its location in your local sky
Explore_Celestial_Sphere.swf
Definitions:The Local Sky :Definitions:The Local Sky Zenith: The point directly overhead
Horizon: All points 90° away from zenith
Meridian: Line passing through zenith and connecting N and S points on horizon
Why do stars rise and set? :Why do stars rise and set? Earth rotates east to west, so stars appear to circle from west to east.
Our view from Earth: :Our view from Earth: Stars near the north celestial pole are circumpolar and never set.
All other stars (and Sun, Moon, planets) rise in east and set in west. Celestial Equator Your Horizon A circumpolar star never sets This star never rises in Indiana
The Earth spins under Polaris :The Earth spins under Polaris (Polaris is NOT
the brightest
star in the sky!)
Altitude of the celestial pole = your latitude :Altitude of the celestial pole = your latitude
The North Star (Polaris) is 50° above your horizon, due north. Where are you? :The North Star (Polaris) is 50° above your horizon, due north. Where are you? You are on the equator.
You are at the North Pole.
You are at latitude 50°N.
You are at longitude 50°E.
You are at latitude 50°N and longitude 50°E.
The sky changes as Earth orbits the Sun :The sky changes as Earth orbits the Sun As the Earth orbits the Sun, the Sun appears to move eastward along the ecliptic
At midnight, the stars on our meridian are opposite the Sun in the sky
Slide 32:Where on the Earth is it possible to see the most stars through the year?
a) From the north pole
b) From latitude 23.5 degrees
c) From the equator
d) anywhere, since latitude makes no difference.
Why do the constellations we see depend on latitude and time of year? :Why do the constellations we see depend on latitude and time of year? They depend on latitude because your position on Earth determines which constellations remain below the horizon.
They depend on time of year because Earth’s orbit changes the apparent location of the Sun among the stars.
Precession! :Precession! Over time, the direction of the Earth’s rotation axis drifts around a circle.
At different times, different stars (other than Polaris) are close to the pole
Vocabulary Review :Vocabulary Review Constellation
Ecliptic
Equator
Celestial sphere
Latitude
Longitude Meridian
Zenith
Horizon
Altitude
North and south celestial poles
Slide 36:Moon worksheet due Thursday
Finish units 5, 6, 10
News Quiz on Tues., Sept. 12 For Thursday...