Positional Astronomy Flashcards

1
Q

Altitude

A

the angular height measured from the observer’s horizon
(tilt of the observing instrument)

the altitude of the pole is equal to the observer’s latitude

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2
Q

Azimuth

A

The angle measured from the Observer’s meridian, in the easterly direction.
(twist angle)

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3
Q

Celestial equator

A

The projection of the Earth’s equator onto the celestial sphere.

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4
Q

Circumpolar

A

Stars that remain above the horizon at all times

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5
Q

Conjuction

A

A planet lying in the same direction as the sun when viewed from the Earth

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6
Q

spherical cosine formula

A

cosa=cosbcosc+sinbsinccosA

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7
Q

Declination

A

The equivalent of latitude on the celestial sphere

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8
Q

Direct motion

A

Appears to move in the same direction as its true orbital motion when viewed from Earth.
Eg: sun’s ecliptic longitude increases uniformly throughout the course of the year.

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9
Q

Diurnal motion

A

The rotation of the Earth about its N-S axis accounts for diurnal motion (day and night)

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10
Q

Ecliptic

A

apparent path taken by the sun

titled at ε with respect to celestial equator

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11
Q

Elongation

A

ε is defined at the Earth as the angle made by the planet’s geocentric radius vector with the sun’s geocentric radius vector.

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12
Q

Equation of time

A

EqT=RAMS-RAS

where RA is right ascension
MS is mean sun
S is true sun

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13
Q

Equinox

A

the two points on the ecliptic where it intersects the celestial equator
Sun’s declination is zero

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14
Q

Geocentric

A

coordinate system with Earth at centre
eg: hour angle and declination

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15
Q

Great Circles

A

a circle that has the same radius as the sphere on which it is drawn
eg: equator

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16
Q

Hour Angle

A

equivalent to longitude on the celestial sphere

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17
Q

Inferior planet

A

planets whose orbits lie inside the Earth’s orbit

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18
Q

Julian Calendar

A

defined every 4th year to be a leap year to account for the remainder in the tropical year duration.

led to slippage in the annual recurrence of the vernal equinox

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19
Q

Latitude

A

circles on the surface of the Earth that are parallel to the equator

ranges from +90 to -90 (N to S)
equator is the zero of the latitude scale

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20
Q

Local siderial time

A

the hour angle of ♈︎ for the observer

LST=HA♈︎

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21
Q

Longitude

A

All meridians of longitude curves are great circles (NOT PARALLEL)
Arbitrary zero is the Greenwich Meridian
longitude=(LMST-UT)x15°

22
Q

Maximum elongation

A

an inferior planet has maximum elongation when its geocentric radius vector is tangential to its orbit.

a superior planet has maximum elongation of 180°

23
Q

Mean solar time

A

watches and clocks read mean solar time

(discrepancies due to Earth’s elliptical orbit and the ecliptic is not parallel to the celestial equator)

24
Q

Mean sun

A

moves along celestial equator at same uniform average rate as the sun moves along the ecliptic.

M and S together at the equinoxes

25
Mean time
concept created using mean sun to have a uniform measure of time throughout the year
26
Nautical mile
the fraction of the Earth's circumference subtending 1 minute of arc at the centre, as measured at the equator. nautical mile is approximately 1.853km (using s=rθ)
27
North Celestial pole
The north pole of the Earth projected onto the celestial equator.
28
Obliquity of the ecliptic
the Earth's rotational axis is tilted at 23.5 degrees with respect to its orbital axis. This angle is the obliquity of the ecliptic
29
Observer's horizon
the projection of the observer's terrestrial horizon. the curve where the plane perpendicular to the line to the zenith
30
Observer's meridian
the great circle arc that passes through the NCP and the observer's zenith
31
Opposition
a superior planet that has an ecliptic longitude of 180 degrees from the sun Sun-Earth-planet system is a straight line inferior planets are never in opposition
32
Phase angle
Φ defined at the planet, by the Sun-Earth-Planet system
33
Quadrature
sets the value of planetary elongation to be 90 degrees
34
Retrograde Motion
At opposition, the planet appears to be moving in the direction opposite to its actual orbital motion when viewed from the Earth
35
Rise
non-circumpolar stars rise when it crosses from below the observer's horizon into the visible sky
36
Set
non-circumpolar stars set when it crosses below the observer's horizon
37
Siderial month
the moon completes its orbit around the Earth in 27.32 days relative to the distant stars
38
Siderial year
the time it takes Earth to complete one full orbit around the sun when viewed from distant stars
39
Spherical Sine formula
SinA/sina=SinB/sinb=SinC/sinc
40
Small circles
circles which do not have the same radius as the sphere
41
Solar time
The non-uniform time recorded by the sundial
42
Solstice
The points where the sun has maximum/minimum declination (21st June and 21st December)
43
Superior planet
planets whose orbit lies outside the Earth's orbit
44
Synodic period
Since the Earth is also in orbit around the sun, the period for the moon to complete its orbit is 2.2 days longer than the sidereal.
45
Topocentric
observer at the centre of the universe
46
Transit
when the star crosses the observer's meridian
47
Tropical year
the period from 1 vernal equinox to the next, comprising 365.2422 mean solar days
48
Tropics
the lines of latitude +/-ε define the tropics of cancer and capricorn
49
Zenith
the point directly over-head of the observer.
50
Zenith distance
the distance to the star as measured from the zenith down towards the horizon Zenith distance=90 degrees - a
51
Zodiac
13 constellations make up the zodiac sun appears to move steadily eastwards around the ecliptic, passing through each of the constellations.