Title: ASTR 111
1Lecture 2
- ASTR 111 Section 002
- Introductory Astronomy
- Solar System
Dr. Weigel
2Reading for this week
- The reading for this week is Chapter 1 (all) and
Chapter 2 (sections 2.1-2.2 only) - The quiz will cover this reading and the topics
covered in this weeks lectures - The quiz will be available on BlackBoard at 1015
am
3Outline
- Angular Measurements Review
- Accuracy, Precision, and Bias
- The Scientific Method
- Astronomical Distances
- Ancient Astronomy
4B
A
- What is the angular distance between points A and
B on this slide (In degrees and arcminutes).
Each student should take their own measurement.
Each student should also write down their height
alongside of their measurement. - Predict what will happen if you made your
measurement in two different parts of the room. - Next week you sit in the same chair but weigh 30
pounds less. Will your (angular) measurements
change? - Do you think there will be a relationship between
a persons height and the angle they measure?
5http//antwrp.gsfc.nasa.gov/apod/ap071025.html
6Outline
- Angular Measurements
- Accuracy, Precision, and Bias
- The Scientific Method
- Astronomical Distances
- Ancient Astronomy
7Precision, Accuracy, and Bias
- Whenever you take measurements, you should
account for them - Fundamental terms that you must understand when
interpreting measurements
8Accuracy vs. Precision
Target is red
Shots are black
9Accuracy vs. Precision
Target is red
Shots are black
High precision Low accuracy
High precision High accuracy
10Accuracy vs Precision
Mnemonic Youll get an A for Accuracy
11Bias
Target is red
Shots are black
- The left target shows bias the measurements
were made with high precision, but the were
consistently off in the same direction.
12Summary
- Accuracy all measurements or values are
clustered around the true value (youll get an A
for accuracy, because you are on the true value) - Precision all measurements are clustered but
are not centered on true value - Bias measurements are not centered on true value
Center of red dot is true value
No bias
13Group work ( 4 minutes)
- Draw a diagram like the ones on the previous
slide that show - Low precision and high bias
- High accuracy and very low precision
- On a piece of paper, write down
- Possible causes of low accuracy be specific!
(Dont say human error) - Possible causes of bias be specific!
- associated with your angular measurements
14Group work ( 3 minutes)
- Which diagram best represents the statement
Preliminary polling results indicated that Obama
won Virginia by a landslide because the
preliminary poll results were all from Northern
Virginia.
B
D
A
C
15Outline
- Angular Measurements
- Accuracy, Precision, and Bias
- The Scientific Method
- Astronomical Distances
- Ancient Astronomy
16The Scientific Method
17What is Science?
- A set of facts
- Something that professional scientists do
- The underlying Truth about the Universe
- The collection of data and formation of a
hypothesis - None of the above
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19The Scientific Methodthe process
- characterization of existing data
- formulation of a hypothesis
- formulation of a predictive test
- experimental testing, (important error
elimination and characterization) - report and peer review
- validate or revise hypothesis
20Outline
- Angular Measurements
- Accuracy, Precision, and Bias
- The Scientific Method
- Astronomical Distances
- Ancient Astronomy
21Parallax
22Parallax
10 20 30 40 50 60 70 80 90
23Parallax
- When the apparent position of an object (numbers
on speedometer) changes because of the change in
position of the observer (drivers seat to
passengers seat).
24The Parsec
25Astronomical distances are never measured in Car
hours, dotsecs, and Moon Units
- Car Hour (ch)
- the distance a car can travel in one hour at a
speed of about 60 miles/hour. How far is
Baltimore? About an hour. - Car Year (cy)
- the distance a car can travel in one year at a
speed of about 60 miles/hour - dotsec (ds)
- the distance at which the two dots on the screen
subtend an angle of 1 arcsec - Moon Unit (MU)
- One Moon Unit is the average distance between
Earth and the Moon
A time
A distance
26Astronomical distances are often measured in
astronomical units, parsecs, or light-years
- Light Year (ly)
- One ly is the distance light can travel in one
year at a speed of about 3 x 105 km/s or 186,000
miles/s - Parsec (pc)
- the distance at which 1 AU subtends an angle of 1
arcsec or the distance from which Earth would
appear to be one arcsecond from the Sun - Astronomical Unit (AU)
- One AU is the average distance between Earth and
the Sun - 1.496 X 108 km or 92.96 million miles
27Sun
Earth
Observers view of Sun and Earth from outer planet
28Gods-eye view - Looking down on Sun and Earth
Observers view
29Gods-eye view
Observers view
30Group Problem
- Form groups of exactly 4
- Optimal configuration is two students in one row
and two students in another row
No
Yes
31- Imagine that you are looking at the stars from
Earth in January. Use a straightedge to draw a
line from Earth in January, through the nearby
star (Star A), out to the Distant Stars. Which
of the distant stars would appear closest to Star
A in your night sky in January. Circle this
distant star and label it Jan. - Repeat Question 1 for July and label the distant
star July. - In the box below, the same distant stars are
shown as you would see them in the night sky.
Draw a small x to indicate the position of Star A
as seen in January and label it Star A Jan. - In the same box, draw another x to indicate the
position of Star A as seen in July and label it
Star A July. - Describe how Star A would appear to move among
the distant stars as Earth orbits the Sun
counterclockwise from January of one year,
through July, to January of the following year. - Consider two stars (C and D) that both exhibit
parallax. If Star C appears to move back and
forth by a greater amount than Star D, which star
do you think is actually closer to you? If
youre not sure, just make a guess. Well return
to this question later in this activity.
Distant Stars
Nearby Star (Star A)
1 AU
Earth (July)
Earth (January)
Based on Lecture Tutorials for Introductory
Astronomy, Prather et al., pg 35
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34Outline
- Angular Measurements
- Accuracy, Precision, and Bias
- The Scientific Method
- Astronomical Distances
- Ancient Astronomy
35http//www.google.com/sky/
36Naked-eye astronomy had an important place in
ancient civilizations
- Positional astronomy
- the study of the positions of objects in the sky
and how these positions change - Naked-eye astronomy
- the sort that requires no equipment but human
vision - Extends far back in time
- British Isles Stonehenge
- Native American Medicine Wheel
- Aztec, Mayan and Incan temples
- Egyptian pyramids
37Stonehenge
http//archaeoastronomy.wordpress.com/2005/06/15/s
tonehenge-astronomy-ii-solar-alignments/ See also
http//news.bbc.co.uk/2/hi/uk_news/england/wiltshi
re/7465235.stm
38Aztec, Mayan and Incan temples
39Eighty-eight constellations cover the entire sky
- Ancient peoples looked at the stars and imagined
groupings made pictures in the sky - We still refer to many of these groupings
- Astronomers call them constellations (from the
Latin for group of stars)
40Modern Constellations
- On modern star charts, the entire sky is divided
into 88 regions - Each is a constellation
- Most stars in a constellation are nowhere near
one another - They only appear to be close together because
they are in nearly the same direction as seen
from Earth