Astro 100 - Chapter 2 | Hunter College

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32 Terms

1

Why do seasons exist?

Earth’s axis tilt

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2

How are seasons determined?

Position and axis tilt of Earth when orbiting the Sun

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3

Four Special Points of Season Progression

Winter Solstice (December)

Spring Equinox (March)

Summer Solstice (June)

Fall Equinox (September)

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4

Sun’s path during the Summer Solstice

Highest path; rise and sets at most extreme north due east

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5

Sun’s path during the Winter Solstice

Lowest path; rise and sets at most extreme south due east

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6

Sun’s path during equinoxes

Sun precisely rises due east and sets due west

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7

How much sunlight does the Northern Hemisphere get during each solstice and equinox?

Summer Solstice: Most sunlight

Spring & Fall Equinox: Equal sunlight on both hemispheres

Winter Solstice: Least sunlight

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8

Why do lunar phases occur?

Moon’s orbit around Earth

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9

What is the moon illuminated by?

Half from the Sun and half is dark

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10

How long is the moon phase cycle?

29.5 days

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11

Phases of the Moon (Waxing)

New → Crescent → First Quarter → Gibbous → Full

Visible during afternoon/evening

Reveals itself more and rises later each day

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12

Phases of the Moon (Waning)

Full → Gibbous → Third Quarter → Crescent

Visible during late night/morning

Starts disappearing and sets later each day

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13

Lunar Eclipse

Earth’s shadow falls on the moon, giving it a reddish color

Can only occur during full moon

Can be Penumbral, Partial, or Total

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14

Solar Eclipse

Moon’s shadow falls on the Earth

Can only occur during new moon

Can be Total, Partial, or Annular

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15

Constellation

A region of the sky

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16

How many constellations are there?

88 constellations

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17

Celestial Sphere

A sphere where all the constellations lie at but at different distances

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18

Ecliptic

Sun’s apparent path throughout the celestial sphere

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19

Location of north and south celestial pole

North celestial pole: Above Earth’s North Pole

South celestial pole: Above Earth’s South Pole

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20

The Milky Way

A wave of light circling the celestial sphere

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21

How to know the location of an object in your local sky?

Its altitude and direction

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22

Zenith

Directly above you(90 degrees)

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23

Horizon

All points that are 90 degrees away from the zenith

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24

Meridian

A line that passes through the Zenith and connects the North and South poles

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25

Angular Measurements

Full Circle = 360 degrees

1 degree = 60’ arcminutes

1’ arcminute = 60” arcseconds

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26

Visibility of Stars

Stars in the north celestial pole are circumpolar and never set

Cannot see stars in the south celestial pole

All other stars rise east and set west

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27

Why do we see different constellations?

Position of Earth and the time of year

Ex: Sagittarius - Summer / Orion - Winter

(RAHHHHHH Beyblade taught me all these constellations)

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28

What planets were known during ancient times?

Mercury - Most difficult to see, always near the sun in the SKY

Venus - Very bright when visible; morning/evening “star”

Mars - Noticeably red

Jupiter - Very bright

Saturn - Moderately Bright

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29

Planetary Motion

When planets usually move a little eastward every night

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30

Apparent Retrograde Motion

When the stars move westwards for a few weeks

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31

Stellar Parallax

Using the Earth’s orbit(every 6 months) and distant “fixed” stars to determine the position of a nearby star

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32

Ancient Greek’s conclusion on observable parallax

Earth does not orbit the sun; it is the center of the universe

Explanation: They didn’t think the stars could be THAT far away, meaning they tried using stellar parallax with the naked eye but couldn’t find any difference in star positions, hence the making of Earth-centered systems.

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