Unit 1 Flashcards

1
Q

If the net force acting on the object increases while the mass of the object remains constant, what happens to acceleration?

A

It increases

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2
Q

If Earth moved to half its current distance from the sun, how would the force of the sun’s gravity on earth change

A

It’d become 4 times stronger

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3
Q

What did Newton’s Law of universal gravitation tell us about how gravity works?

A

The force of gravity from the sun will be stronger on an object with more mass

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4
Q

Earth radius is about 6400 km. If in orbit in the space station 150 km up, the force of gravity felt from earth would be

A

Weaker than when standing on earth

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5
Q

Mars has 1/0 the mass of the Earth and 1/2 the radius of Earth. What’s Mars’s surface gravity relative to that of earth

A

4/10th

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6
Q

What would happen to earth if the Sun’s gravity turned off instantaneously?

A

It would continue to move in the same direction it was going in when the gravity turned off

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7
Q

What causes seasons?

A

The tilt of a body with respect to the plane in which they orbit the sun

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8
Q

Earth’s tilt

A

23.3 degrees, meaning the Northern and Southern Hemispheres are alternating lay tipped towards or away from the sun

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9
Q

Influence of axial tilt on seasons

A

Planets with more dramatic tilt have more extreme differences in seasonal temperature differences. Planets with no tilt have no seasons

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10
Q

Why doesn’t distance from the sun matter in seasons?

A

Bc planets have nearly circular orbits with very little variation

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11
Q

Newton’s Laws

A

Objects at motion or at rest stay that way unless acted upon by a force

The magnitude of force necessary to produce a certain acceleration on a body will be directly proportional to its mass. More mass = more force

For every action there is an equal and opposite reaction

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12
Q

Force formula

A

Force = mass * acceleration

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13
Q

When is the moon transiting

A

When it’s at the highest point in its orbit

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14
Q

When does the waxing crescent rise

A

9 AM

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15
Q

When does the waning gibbous set

A

9 am

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16
Q

Lunar Eclipse

A

Moon is fully visible, but earth’s shadow moves across the moon, covering it partially or completely.

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17
Q

Solar Eclipse

A

When the moon blocks the sun’s light, or a location on earth is passing under the moon’s shadow

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18
Q

Why don’t solar eclipses happen once a month

A

The moon’s orbit around earth is tilted 5 degrees relative to earth’s orbit of the sun. The geometry only lines up about twice a year

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19
Q

Penumbra

A

Moon’s outer shadow, where partial eclipses are seen

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20
Q

Umbra

A

Moon’s inner shadow, where total eclipses are seen

21
Q

Inclination

A

The tilt of a moon’s orbit compared to that of the planet around the sun. Earth’s moon’s is about 5 degrees, explaining the rarity of eclipses

22
Q

seven principles of design

A

Balance
Rhythm
Pattern
Emphasis
Contrast
Unity
Movement

23
Q

Scattering

A

Reflection or re-direction of light by small particles

24
Q

Ecliptic Plane

A

Plane in which the earth orbits the sun. Other planets orbit close to the ecliptic plane

25
Precessions
The earth wobbling as it rotates
26
Constellation
Region in the sky
27
Asterism
A shape traced out in the sky by imagining connecting lines between stars
28
Zodiac
Subset of constellations crossed by the ecliptic line of the sun
29
Magnification
Takes view of a small area of sky and blows it up
30
What happens when you magnify an object with a telescope
Your field of view gets smaller, but its clarity doesn’t change
31
If you double the width of a telescope’s circular mirrors
Its light gathering power gets multiplied by a factor of four
32
Refracting telescope
Uses lenses to focus light
33
Reflecting telescope
Uses mirrors to focus light
34
Chromatic aberration
Scattering of light’s components
35
Strength of Gravity Formula
G= M/R^2 Where M is planet mass and R is its radius
36
More mass means
More gravity
37
Order of Moon Phases
New – Waxing Crescent – First Quarter – Waxing Gibbous – Full – – Waning Gibbous – Third Quarter – Waning Crescent
38
Movement of moon phase
Rises ~6 hours before its overhead and sets 6 hours later
39
How do you tell what season a constellation is
They are the ones opposite the Sun in a given season
40
Forms of light (high to low energy)
Gamma Ray, x-ray, UV, visible, infrared, microwave, radio
41
Relationship between light and color
Energy corresponds to frequency and wavelength Ex: high energy =high frequency = short wavelength= blue Low=low=long=red
42
Blackout spectrum
Higher temperature = more light in total, with a peak at a shorter wavelength
43
Continuum spectrum
Light at all wavelengths
44
absorption spectrum
Shows absorption lines (produced when electrons absorb photons) superimposed on a continuum spectrum
45
Emission spectrum
Shows emission lines (produced when electrons jump from higher to lower energy levels, emitting photons of those specific energies
46
Important telescope qualities
light gathering power, angular resolution, and power. Magnification doesn’t really matter
47
How do telescopes gather light
In proportion to the area of their mirrors (proportional to diameter^2)
48
Angular resolution
Ability to distinguish or separate two nearby light sources (with good angular resolution). Limited by Earth’s atmosphere