midterm review Flashcards

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…

A

density

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).

A

density

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
Q

why does the moon rise 50 minutes later each night

A

the earth has to move an extra 13° to catch up to the moon.

26
Q

This is why to go from fall moon to full moon it takes 29.5 days,
not 27.3 days.

A

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
Q

the moon revolves how much around the earth a day

A

13 degrees

28
Q

once every 27. 3 days or 13°/hr (synchronous rotation) is how

A

the moon revolves and rotates at the same rate

29
Q

What two factors affect orbital speed (gravitational attraction)

A

mass of the object and the distance between the objects

30
Q
  1. revolution
  2. tilt of axis
  3. axis always tilts the same direction
A

Causes of the seasons

31
Q

Earth orbits (revolves) around the sun on an

A

elliptical (oval, ellipse) path

32
Q

Because earth is tilted, it
receives

A

isolation (incoming solar radiation) at different angles (angle of isolation).

33
Q

Altitude of Polaris =

A

Latitude of Observer

34
Q

December 21 we have our… and least intense

A

shortest day (9hrs)… isolation.

35
Q

June 21st is the summer solstice and December 21 is the

A

Winter Solstice

36
Q

March 21st is the spring equinox and September 23rd is the

A

the fall equinox

37
Q

On June 21 we (New York) have our…. and most intense

A

longest day (16 hours)… isolation