Midterm 1 Flashcards

(48 cards)

1
Q

How is Earth moving in our solar system? (2 ways)

A

It rotates on its axis once a day and orbits the Sun at a distance of 1 AU = 150 million kilometers.

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2
Q

How is our solar system moving in the Milky Way Galaxy?

2 ways

A

Stars in the Local Neighborhood move randomly relative to one another and orbit the center of the Milky Way in about 230 million years.

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3
Q

How do galaxies move within the universe and what does their distance from us imply?

A

All galaxies beyond the Local Group are moving away from us with expansion of the universe: the more distant they are, the faster they’re moving.

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4
Q

How has the study of astronomy affected human history? (4 things)

A
  • Earth is not the center of the universe (Copernicus)
  • Study of planetary motion led to Newton’s laws of motion and gravity
  • Newton’s laws laid the foundation of the industrial revolution.
  • Modern discoveries expand our “cosmic perspective.”
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5
Q

In what ways do all humans use scientific thinking? (1 way)

A

Scientific thinking involves the same type of trial and error thinking that we use in our everyday live

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6
Q

How did astronomical observations benefit ancient societies? (3 ways)

A

Keeping track of:

  • time
  • seasons
  • navigation.
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7
Q

What did ancient civilizations achieve in astronomy? (4 things)

A
  • To tell the time of day and year
  • to track cycles of the Moon
  • to observe planets and stars
  • Ancient structures aided in astronomical observations.
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8
Q

Why does modern science trace its roots to the Greeks?

A

They developed models of nature and emphasized that the predictions of models should agree with observations. (developed scientific method in that way)

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9
Q

How did Ptolemy explain planetary motion?

A

The Ptolemaic model had each planet move on a small circle whose center moves around Earth on a larger circle.

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10
Q

Who challenged the earth centered model?

3 people

A

Copernicus, Brahe, Kepler

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11
Q

What are Kepler’s three laws of planetary motion?

A
  1. The orbit of each planet is an ellipse with the Sun at one focus.
  2. As a planet moves around its orbit it sweeps out equal areas in equal times.
  3. More distant planets orbit the Sun at slower average speeds: p2 = a3.
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12
Q

What is the distance between earth and sun in km?

A

150 mil km

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13
Q

What is perihelion?

A

The part of the earths orbit where it moves faster and is closer to the sun

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14
Q

What is aphelion?

A

The part of the earths orbit where it moves slower and is farther away from the sun

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15
Q

Galileo overcame 3 Aristotelian objections of the heliocentric model which are:

A
  • Earth cannot be moving because objects in air would be left behind.
  • Non-circular orbits are not “perfect” as the heavens should be.
  • We would detect stellar parallax if earth were orbiting the sun
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16
Q

Galileo discovered what law of motion?

A

All objects in motion stay in motion (Newton’s first law)

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17
Q

How did Copernicus, Tycho and Kepler challenge the Earth-centered idea?

A
  • Copernicus created a sun-centered model
  • Tycho provided the data needed to improve this model
  • Kepler found a model that fit Tycho’s data.
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18
Q

What was Galileo’s role in solidifying the Copernican revolution?

A

His experiments and observations overcame the remaining objections to the Sun-centered solar system model.

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19
Q

Universal law of gravitation (3 points)

A
  • Every mass attracts every other mass.
  • Attraction is directly proportional to the product of their masses.
  • Attraction is inversely proportional to the square of the distance between their centers.
    F=(m1*m2)/d^2
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20
Q

A scientific theory must: (3 points)

A
  • Explain a wide variety of observations with a few simple principles
  • Be supported by a large, compelling body of evidence, - Have not failed any crucial test of its validity.
21
Q

How do we experience light? (2)

A
  • Light is a form of energy.

- Light comes in many colors that combine to form white light.

22
Q

How do light and matter interact? (4+1)

A

Matter can:

  • emit light
  • absorb light
  • transmit light
  • reflect (or scatter) light.
  • Interactions between light and matter determine the appearance of everything we see.
23
Q

What is light? (3)

A
Light as a wave:
- Is a vibration of electric and magnetic fields.
- Has a wavelength and a frequency.
Light as a particles:
- Are photons
24
Q

What is the electromagnetic spectrum? (2)

A
  • The entire range of wavelengths of light is known as the electromagnetic spectrum
  • humans cannot see most of it
25
What is the structure of matter? (2)
Atoms: - nucleus: protons and neutrons - surrounded by a cloud of electrons.
26
What are the phases of matter? (3)
- Solid, liquid, gas, plasma - heat breaks chemical bonds, allows dissociation into atoms - ionization strips atoms of electrons in plasma phase
27
How is energy stored in atoms?
- Atoms have electrons which correspond to particular energy levels.
28
Continuous spectrum: What is it? When does it occur?
- spans all visible wavelengths, without interruption | - Emitted by dense materials (e.g. dense gas or solid).
29
Emission line spectrum: What is it? When does it occur?
- has emission lines for particular wavelengths or frequencies - Emitted by thin gas.
30
Absorption line spectrum: What is it? When does it occur?
- has dark absorption lines for particular wavelengths or frequencies - Occurs if light is sent through a thin gas.
31
Which colour of star is the hottest?
Blue
32
What are the three basic type of spectra?
- Continuous spectrum - emission line spectrum - absorption line spectrum
33
How does light tell us what things are made of?
- by looking for their fingerprints in the spectrum, we can tell which atoms something is made of
34
How does light tell us the temperatures of planets and stars?
- Large or dense objects emit a continuous spectrum that depends on temperature. - The spectrum of that thermal radiation tells us the object’s temperature
35
How does light tell us the speed of a distant object?
The Doppler effect tells us how fast an object is
36
How does light tell us the rotation rate of an object?
The width of an object’s spectral lines can tell us how fast it is rotating.
37
How does your eye form an image? And when is an image in focus?
- It uses refraction to bend parallel light rays so that they form an image. - The image is in focus if the focal plane is at the retina
38
How do we record images?
- Cameras focus light like your eye and record the image with a detector.
39
What are the two most important properties of a telescope?
- Collecting area: determines how much light a telescope can gather. - Angular resolution: the minimum angular separation a telescope can distinguish.
40
What are the two basic designs of telescopes?
- Refracting telescopes focus light with lenses. - Reflecting telescopes focus light with mirrors. (majority of professional telescopes are reflectors)
41
What do astronomers do with telescopes? (3)
- Imaging - Spectroscopy - Timing
42
How does Earth’s atmosphere affect ground-based observations? (3)
- light pollution - atmospheric turbulence - bad weather
43
Why do we put telescopes into space? (2)
- To detect forms of light other than visible and radio waves (which do not get past the atmosphere) - no turbulence.
44
How can we observe invisible light? (2)
- modified versions of reflecting telescopes. | - Many of those are in space.
45
Visible light and radio waves can be observed with ground based telescopes (How large do we make them?)
- largest optical telescopes D = 10 m | - largest radio telescope D = 500 m
46
CCD
detector
47
What is our physical place in the universe?
Earth< ss
48
How did we come to be?
- Hydrogen, heluim, lithium, beryllium produced after big bang - sun from h, he