1 Flashcards
Standard Time Meridians to Zone Descriptions : Heading East 15*, 30*, 45*, .... 180* Heading West 15*, 30*, 45*, .... 180*
East :
-1, -2, -3, …. -12
West:
+1, +2, +3, …. +12
How should clocks be changed to maintain timezones?
Exactly between meridians DEPENDING ON THE DIRECTION YOU ARE HEADING
730’ E , 2230’ E,…, 17230’ E, 17230’ W,…, 2230’ W, 730’ W,
It continues in either direction
The date is the same all over the world at
1200 GMT
Reference point to determine GMT is mean sun over
180* longitude
Universal time (UT1) is
Greenwich mean time
Measurement of local time is based on Sun over
Lower branch of observers meridian
3 REASONS Mean sun is used as reference for solar time
Motion of apparent sun is along ecliptic
Speed of earths revolution is not constant
Variations in the earths rotational speed
NOT a reason why sun is used for solar time
Measurement of time is along equator
Daylight savings time adopts
One zone to the east
Apparent time
Visible sun moving along the ecliptic
Difference between mean and apparent time
Apprx 16 minutes
Primary use of apparent time
Determine time of meridian transit
The difference between local apparent time (LAT) and local mean time (LMT) is indicated by the
Equation of time
The equation of time measures
Time between passage of the mean sun and the apparent sun over a meridian
When equation of time is taken from Nautical Almanac for use in celestial nav, it determines
Time of local apparent noon
Local sidereal time =
LHA of Aries
Sidereal time is NOT used
In sight reduction of planet observations
Sidereal day begins
First point of Aries is over upper branch of reference meridian
Sidereal day apprx how much shorter than solar day?
4 minutes
Diff of sidereal day(shorter) to solar day is due to
Use of different reference points
Apprx positions of the stars are based on sidereal time, which is based upon rotation of earth relative to
Vernal equinox
Length of year w respect to vernal equinox
Tropical year
Tropical year differs from which year by 20 minutes?
Sidereal year.
Lunar day is known as
Tidal day
Lunar day
Longer than solar day
Lunar day
24h 50m 00s
Time diagram observed from above
South celestial pole
Time diagram on plane of
Celestial equator
At meridian transit, diagram to illustrate angles involved based on
Plane of observers meridian
D005NG
Date is one day later than GMT
In East longitude
Sun has already passed the lower branch of observers meridian
D008NG
Represents morning Sun sight
Meridian angle of Sun is east