astronomy exam 1 review Flashcards

1
Q

distance

A

speed x time

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2
Q

stars

A

balls of gas that radiate heat and light, they are sources of light

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3
Q

constellations

A

stellar patterns identified by names, pieces of the ski

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4
Q

asterism

A

a pattern of stars that is not a constellation
example, the big dipper

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5
Q

depth perception or parallax

A

the apparent shift in the position of an object when viewed from two different points

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6
Q

alpha

A

brightest star in constellation

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7
Q

beta

A

second brightest star

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8
Q

greek

A

used for naming stars

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9
Q

magnitude

A

brightness

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10
Q

hipparchus

A

tried to organize stars with brightest classification
1st class is the brightest star
6th class is barely visible with the naked eye

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11
Q

apparent visual magnitude

A

brightness of star as seen by human eyes on earth

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12
Q

zenith

A

whats directly above your head

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13
Q

nadar

A

what’s directly under you

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14
Q

longitude

A

east and west

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15
Q

latitude

A

north and south

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16
Q

radian

A

angle where arc length equals radius of a circle

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17
Q

equinox

A

12 hours of light and dark

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18
Q

ecliptic

A

path of the sun through the stars over a year (zodiac signs)

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19
Q

are moon plains parallel

A

no

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20
Q

waxing

A

more full

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21
Q

waning

A

less full

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22
Q

lunar synodic period

A

29.5 days

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23
Q

lunar sidereal period

24
Q

when moon is in penumbra

A

partial lunar eclipse

25
when moon is in umbra
full lunar eclipse the moon needs to be full for this to happen
26
magnitude scale
astronomical brightness scale, the larger the number, the fainter the star
27
flux
amount of light energy that hits one square meter in one second
28
angular distance
angle between 2 lines extending from your eye to two objects
29
arc minutes
1/60 degree
30
angular diameter
angular distance from one edge to another
31
circumpolar constellations
never rise or set because their located near a pole
32
scientific model
intellectual construct that helps us understand real world but isnt completely true or accurate
33
precession
slow change in direction of earth's axis of rotation
34
celestial sphere
scientific model of the sky
35
average diameter
linear diameter/distance
36
1 AU
1.5 x 10^8 km
37
smallest to largest (earth, moon, sun, nearest star, milky way and nearest galaxy)
1. Earth to moon 2. Earth to sun 3. sun to nearest star 4. milky way to next nearest galaxy
38
AU
average distance between the earth and the sun
39
the lower the magnitude of a star
the brighter it is
40
compare visual magnitude of stars equation
2.5 log (1/4)
41
if two stars differ in magnitude equation
(Fa/Fb) = (2.512)^(mbxma)
42
degrees of north and south celestial
north (90) and south (180)
43
motion of a star
along the celestial equator is due to the earth's rotation on its axis
44
density
mass/volume
45
annular eclipse
a rare event that occurs when the moon passes between the Earth and the sun, but doesn't completely cover the sun
46
lunar eclipse
Earth comes between the sun and the moon, blocking the sunlight falling on the moon.
47
umbra
the dark center of the moon's shadow on the earth during a solar eclipse, where the sun is completely blocked
48
penumbra
the outer part of the moon's shadow that partially blocks the sun during a solar eclipse
49
why do we have seasons?
Earth has seasons because of its tilted axis and elliptical orbit around the sun. The Earth's axis is tilted relative to its orbital plane, which changes the angle at which sunlight hits the Earth's surface. When the Earth's axis points towards the sun, it is summer for that hemisphere. For example, when the North Pole tilts toward the Sun, it's summer in the Northern Hemisphere
50
brightest star in constellation perseus
Alpha Persei
51
phase of the moon during a solar eclipse
new moon
52
the larger the apparent visual magnitude of a star
the harder to see with the naked eye
53
difference between the sidereal period of the moon and the synodic period of the moon
The sidereal period of the moon is the time it takes for the moon to complete one orbit around the Earth, while the synodic period is the time it takes for the moon to return to the same position in the sky relative to the sun.
54
relative position of the Earth, sun and moon when the moon is at first quarter phase
half moon (the moon is directly to the side of the earth and the sun is in front of it)
55
will polaris always be the north star?
No, Polaris is not always the North Star because Earth's rotation axis wobbles over time, causing the celestial pole to move in a circle past different stars. This phenomenon is called axial precession. In about 12,000 years, the star Vega will become the North Star, as it will sweep past Polaris and point to it again