midterm review Flashcards

(37 cards)

1
Q

energy needed to change temperature (ESRT)

A

Specific Heat

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2
Q

energy needed to change phases (ESRT)

A

Latent heat

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3
Q

what can happen to incoming solar radiation

A

Scattered, Transmitted, Absorbed, Reflected, Refracted

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4
Q

heat transfer through contact

A

conduction

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5
Q

heat transfer through density difference

A

convection

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6
Q

heat transfer through electromagnetic waves (this is how we get energy from the sun)

A

radiation

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7
Q

the range of energy we receive from the sun

A

Electromagnetic Spectrum

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8
Q

because the earth changes its position while orbiting the sun

A

some constellation can be seen only during the winter, some only during the winter

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9
Q

when two air masses meet…

A

meet, there will usually
be some form of precipitation

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10
Q

an interface between two air masses is a

A

a front

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11
Q

The temperature is in Fahrenheit, The pressure is in millibars… these are codes for

A

station models

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12
Q

the amount of water vapor in the air compared to how much
could be

A

Relative humidity

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13
Q

the temperature at which the air becomes saturated

A

dew point

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14
Q

what is the only way to change dew point

A

add or take away moisture

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15
Q

the inner planets, and the rock.

A

Terrestrial Planets

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16
Q

gas giants are the outer planets.

A

Jovial planets

17
Q

mass over d/v is used to figure out…

18
Q

the relation between an objects mass (how much “stuff” makes up the object)
and it Volume (the amount of space something takes up).

19
Q

when the mass of an object changes, its volume
would change proportionally, and therefore the

A

density would not change

20
Q

how many eclipse are there and what are their names

A

two, lunar eclipse (moon) and solar eclipse (sun)

21
Q

when the sun is blocked out by the moon during the new moon phase

A

solar eclipse

22
Q

when the moon passes through earth’s shadow, during the full moon phase

A

lunar eclipse

23
Q

The gravitation between the Earth, Moon, and Sun results of a

A

cyclic rise and fall of ocean waters, also known as tides.

24
Q

an observer on earth will see varying amounts of the
lighted portion as it moves through its orbit because

A

the moon revolves around us in 27.3 days

25
why does the moon rise 50 minutes later each night
the earth has to move an extra 13° to catch up to the moon.
26
This is why to go from fall moon to full moon it takes 29.5 days, not 27.3 days.
each month the moon has to catch up to Earth and takes an extra 2.2 days to get back to the same starting position
27
the moon revolves how much around the earth a day
13 degrees
28
once every 27. 3 days or 13°/hr (synchronous rotation) is how
the moon revolves and rotates at the same rate
29
What two factors affect orbital speed (gravitational attraction)
mass of the object and the distance between the objects
30
1. revolution 2. tilt of axis 3. axis always tilts the same direction
Causes of the seasons
31
Earth orbits (revolves) around the sun on an
elliptical (oval, ellipse) path
32
Because earth is tilted, it receives
isolation (incoming solar radiation) at different angles (angle of isolation).
33
Altitude of Polaris =
Latitude of Observer
34
December 21 we have our... and least intense
shortest day (9hrs)... isolation.
35
June 21st is the summer solstice and December 21 is the
Winter Solstice
36
March 21st is the spring equinox and September 23rd is the
the fall equinox
37
On June 21 we (New York) have our.... and most intense
longest day (16 hours)... isolation