Exam 1 Study Guide Flashcards

(50 cards)

1
Q

A scientific hypothesis must be…

A

testable and falsifiable (never provable)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Stars circle the same location every…

A

23 hours, 56 minutes, 04 seconds

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

The Sun returns to the same approximate location every…

A

24 hours

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Motion of the Sun and Moon is ______ with respect to the stars

A

East

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Mars, Jupiter and Saturn also move __________ with respect to the stars, but _____________ when opposite the sun.

A

Eastward (most of the time), Westward

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Mercury and Venus move _________, but _________ after maximum Eastward elongation (ie. as far East as they are going to go)

A

Eastward (most of the time), Westward

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

The whole sky is marked out in a grid like longitude and latitude, but called…

A

Right Ascension and Declination

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

The angle between a line drawn from an observer to an object and a second line drawn from the observer to a different object is the _________ of those objects

A

angular separation

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

The angle between a line drawn from an observer to one end of an object and a second line drawn from the observer to the other end of the object is the _________ of the object

A

angular size

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Trivium

A

The beginning studies of medieval universities: grammar, local, and rhetoric

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Quadrivium

A

Medieval preparatory work for philosophy and theology: arithmetic, astronomy, geometry, and music

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

The stars appear to circle the star _______ in one _____________

A

Polaris, sidereal day

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

An incorrect model used to understand motions is the _________, which is a transparent sphere with Earth spinning inside

A

Celestial Sphere

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

The Ecliptic

A

The pathway that the sun takes (1 year); tilt of 23/5%

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

The moon follows a different path near the ecliptic which takes about __________ to make an entire trip, with respect to the stars

A

27 days

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Solar Eclipses occur when….

A

The Sun and Moon align and the Moon is on the ecliptic

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

Lunar Eclipses occur when…

A

The Sun and Moon are opposite and the Moon is near the Ecliptic

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

Retrograde Motion

A

An APPARENT change in the movement of the planet through the sky. It is not REAL in that the planet does not physically start moving backwards in its orbit. It just appears to do so because of the relative positions of the planet and Earth and how they are moving around the Sun.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

The sun ___________ its own light, but the moon only ________, allowing us to understand lunar phases from the relative positions of the sun and moon

A

emits its own light, reflects

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

Order of Moon Phases

A
New Moon
First Quarter
Full Moon
Third Quarter
New Moon
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

Because the ecliptic and celestial equator are not the same, the sun is sometimes _______ in the sky at noon, sometimes _______

A

higher, lower

22
Q

zenith

A

point directly above in the sky

23
Q

Solstices

A

The points farthest North and South in the Sun’s travels along the ecliptic

24
Q

Equinoxes

A

The Sun’s crossings of the celestial equator

25
Seasons occur because...
of the changing angle with which the sunlight hits the Earth
26
Stars appear to circle a fixed point each sidebar day from ____ to ____
East, West
27
The ____ and ____circle more or less with the _____, but take longer to complete the circle
Sun, Moon, stars
28
The _____ and _____ appear further ____ each day with respect the stars
Sun, Moon, east
29
The Sun and Moon also move ____ and ____ as they migrate Eastward
North, South
30
The planets usually appear further ___ each day, but occasionally appear further _____
East, West
31
Occasional retrograde motion always occur at opposition for ___, _____, and _____
Mars, Jupiter, and Saturn
32
Occasional retrograde motion always occur after maximum eastward elongation for _____ and _______
Mercury and Venus
33
The planets do not move the same _________ each day
Angular distance
34
The phases of the moon are due to...
Differing illumination
35
The seasons are due to the changing _______ position of the sun
North-South
36
Evidence for "Fixed Earth"
1. We throw something up, it comes back down in the same place 2. The stars do not show visible parallax (changing apparent position due to our changing point of view)
37
The Influence of Aristotle
1. All motion in the heavens is uniform circular motion. (otherwise a void is opened, which is impossible). 2. The objects in the heavens are made from perfect spheres and cannot change their intrinsic properties (e.g., their brightness). 
 3. The Earth is at the center of the Universe.
38
Predictions of the Geocentric Model
- Mars, Jupiter and Saturn should be brighter during retrograde, since they are closer at that time - Mercury and Venus, if illuminated by the sun, should always appear in crescent/new phase. - Stars should show no parallax
39
Difference between Geocentric Model and Heliocentric Model:
``` Geo = Earth is center of universe Helio = Sun is center of universe ```
40
Difficulties with Copernican Model
The moon still went around the earth, requiring 2 centers of motion, Did NOT work as well as the geocentric model, because it used perfect circles, Whether it was "pleasing to the mind" was a matter of opinion. It still had multiple circles to get positions right
41
Kepler's Laws
Law 1: (1609) The orbit of each planet is an ellipse, with the sun at one focus. Law 2: (1609) A line drawn from a planet to the sun sweeps out equal areas in equal times. Law 3: (1618) The square of the orbital period of a planet is directly proportional to the cube of its average distance from the sun.
42
Kepler's Law Equation
p squared/a cubed = k
43
Kepler's Law Explained
``` P = period of time A = distance Au = astronomical unit ```
44
Stellar Motion Photos
90 degrees = horizontal 0 degrees = vertical 45 degrees = slanted
45
Velocity
the change in position of an object with respect to time
46
Acceleration
the change in velocity of an object with respect to time
47
Law 1: Inertial Law
A body at rest or moving with constant velocity reminds in that state until upon by a force
48
Law 2: Force Law
A body acted upon by a force will change its velocity. The acceleration will be in the direction of the force applied and directly proportional to the force applied, but inversely proportional to the body's mass
49
Law 3: Reaction Law
For every applied force, a force of equal size but opposite direction arises
50
Parallax
the effect whereby the position or direction of an object appears to differ when viewed from different positions, e.g. through the viewfinder and the lens of a camera