chapter 2 (pt. 2) Flashcards

Earth-viewed celestial cycle and time (55 cards)

1
Q

Sun Cycle

A

rotation, ecliptic

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2
Q

season

A

revolution, vernal/autumnal equinox, summer/winter solstice, perihelion, aphelion

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3
Q

Moon Cycle

A

phase (waxing or waning of full, gibbous, quarter, crescent, new)

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4
Q

eclipses

A

solar eclipse, penumbra, umbra, annular eclipse, lunar eclipse, Saros cycle
rare, the occurrence can be mathematically calculated, lunar is more common than solar

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5
Q

time keeping

A

solar day, sidereal day/month/year, synodic month, tropical year (solar year), apparent solar time

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6
Q

constellation

A

sky region and/or a star pattern

88 chosen by International Astronomical Union (IAU)

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7
Q

asterism

A

star group (Big Dipper) not primary constellation, may cross regions (Great Square of Pegasus)

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8
Q

apparent visual magnitude

A

measure of brightness (seen with human eye) (Sun ~.27, Sirius -1.47)
Hubble sees magnitude ~30 (faint)

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9
Q

flux

A

measure of light energy reaching a m^2 in one second

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10
Q

celestial sphere

A

ancient belief the sky is a ceiling (sphere) surrounding Earth with attached objects, now a scientific model to describe the observed sky

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11
Q

scientific model

A

way to think about nature, not necessarily true

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12
Q

star trail

A

bright line or curve left by star on untracked time-lapse image of the night sky

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13
Q

circumpolar constellation

A

never rise or set, circling a polar star for latitudes away from the equator cardinal directions (north point, south point, east point, west point)

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14
Q

zenith

A

centre of sky above (opposite is nadir on hidden half)

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15
Q

precession

A

slow circular sweep in orientation of Earth axis of rotation (like a toy top spins)

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16
Q

Messier object

A

Catalogued by Charles Messier, 1760s

103 non-comet objects (all binocular viewable)

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17
Q

declination (dec)

A

latitude in degrees, arc min., arc sec. of north (+), or south (-), of celestial equator - equator (dec=0º), north celestial pole (dec = +90º)

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18
Q

right ascension (RA)

A

extension of longitude, in hours (h), min. (m), sec. (s) within 24 h - longitudunal line of the spring equinox (RA = 0º)

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19
Q

north celestial pole

A

apparent pivot point, opposite south celestial pole, divided by celestial equator

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20
Q

angular distances

A

measured in units of degree, arc minute (1/60th degree), arc second (1/60th minute - from horizon to pole is the latitude of observer (the base principle of celestial navigation)

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21
Q

Ursa Major

A

the Great Bear - part of the big Dipper (not a constellation) a pointer for Polaris

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22
Q

Canis Major

A

the Great Dog

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23
Q

Sirius

A

Dog Star, 8.6 ly

brightest star in the sky

24
Q

Ursa Minor

A

the Little Bear

25
Polaris
the North Star (Alpha Ursa Minoris)
26
axis
imaginary line through centre of rotation of planet (Earth tipped 23.5º, fixed as it revolves)
27
rotation
motion around an axis (Earth produces day and night) [24 h, 1700km/h]
28
ecliptic
Earth's orbit projected on the celestial sphere
29
evening star
planet in the sunset sky, close to Sun over horizon
30
morning star
in dawn sky
31
seasons
change in the amount of solar energy in Northern and Southern hemispheres
32
revolution (orbital motion)
about a point outside a body (earth almost a perfect circle, 30 km/s)
33
aphelion
Jul. 5 ~1.7% further from Sun
34
perihelion
Jan. 3 ~1.7% closer, and seasonal cycle
35
vernal equinox
March 20* spring begins (date varies)
36
summer solstice
June 22* summer begins (date varies)
37
autumnal equinox
September 22* fall begins (date varies)
38
winter solstice
December 22* winter begins (date varies)
39
synodic
meeting of the Sun and the Moon at new Moon
40
month
with a phase cycle of the Moon cycle
41
new Moon
dark, see no moon at all
42
full Moon
fully lit
43
solar eclipse
Moon passes between the Earth and Sun, always at new Moon | blocking part of the Sun and causes penumbra and umbra
44
penumbra
partial shadow
45
umbra
in total shadow
46
annular eclipse
totality when the annulus ("ring") of the Sun's atmosphere is visible around Moon
47
lunar eclipse
Moon moves through the shadow of the Earth, always at a new Moon, up to 1h 45min
48
Saros cycle
18y 11 1/3 day pattern of solar and lunar eclipses, due to Moon tip of 5º to the ecliptic
49
solar day
average length of time between successive passes of Sun across local meridian, 23 hr. 52 min.
50
sidereal day
time of successive passes for a star across the local meridian, 23 hr. 56 min.
51
sidereal month
time for Moon to orbit Earth once relative to a star, 27.32 days
52
sidereal year
time for a complete orbit of Earth around the Sun relative to the stars, 365.26 days
53
synodic month
time for complete cycle of lunar phases, 29.52 days
54
tropical year (solar year)
time between successive spring (or autumn) equinoxes, 365.25 days
55
apparent solar time
``` used most Sun on the local meridian noon ante (before, a.m.) post (after, p.m.) ```