Chapter 3 Flashcards

1
Q

moonrise/set times

A

New moon – sunrise to sunset
1st quarter – noon to midnight
Full moon – sunset to sunrise
3rd quarter – midnight to noon

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2
Q

synchronous rotation

A

when an object rotates once during an orbit; this causes one side of the moon to always face away from Earth

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3
Q

siderial month

A

amount of time required for the moon to complete one full orbit of Earth with respect to the stars

27.32 days

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4
Q

synodic month

A

also known as lunar month; equal to a lunar day

time required for the moon to complete a full cycle of phases (based on sun)

29.53 days

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5
Q

inclination of moon’s orbit

A

about 5 degrees from Earth’s orbit (the ecliptic)

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6
Q

line of nodes

A

intersection of the moon and Earth’s orbital planes

eclipses can only occur when the sun and moon lie on the line of nodes

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7
Q

phases of eclipses

A

solar eclipses only occur at new moon and lunar eclipses only occur at full moon

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8
Q

umbra

A

the fully shaded inner region of a shadow cast by an opaque object, especially the area on the earth or moon experiencing the total phase of an eclipse

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9
Q

penumbra

A

the partially shaded outer region of the shadow cast by an opaque object.

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10
Q

classifications of lunar eclipse

A

penumbral, partial, total lunar eclipse

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11
Q

maximum length of total lunar eclipse

A

1 h 42 min

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12
Q

color of light which passes through Earth’s atmosphere

A

mostly red

causes the moon to appear red during an eclipse

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13
Q

apogee

A

the point in the orbit of the moon or a satellite at which it is furthest from the earth

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14
Q

annular solar eclipse

A

a solar eclipse where the moon does not completely cover the sun because it is near apogee

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15
Q

perigee

A

the point in the orbit of the moon or a satellite at which it is closest to the earth

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16
Q

eclipse year

A

the amount of time between identical allignments of the line of nodes

346.6 d

17
Q

saros

A

time between identical orientations of the earth, moon, and sun

they saros cycle is used to predict eclipses. it takes 3 saros cycles for an eclipse to fall on the same place again.

223 synodic months or 18 y 11d 8h

18
Q

ancient measurments of the size of the Earth

A

In 200 BCE Eratosthenes approximated the size of the Earth by comparing the angles of the sun at local noon in Alexandria and Syene.