The problem again:
The star Canopus (RA = 6h 20m) is observed to have a local hour angle = 45 deg on Feb. 10th for a given location.
What is the local sidereal time?
Find the local time of transit (L.T.T.)
Solution:
L..S.T.= HA + RA of object
Hour angle (HA) = 45 deg so convert to hours:
HA = 45 deg/ 15 deg/ h = 3 h
RA of object = 6 h 20 m
Then:
L.S.T. = 3 h + 6h 20 m = 9 h 20 m
Local time of transit (L.T.T.) = Star's RA - Sun's RA
To get Sun's RA we note Feb. 10th is 39 days before March 21st (vernal equinox so 0 h) and assume non leap year.
Then Sun's RA = 0 h - 39 d x (4 m/ day) =
0 h - 156 m = 0h - 2h 36 m
So Sun's RA = 24 h - 2 h 36 m = 21 h 24 m
Then L.T.T. = 6 h 20 m - 21 h 24 m = - 17 h 36 m
Or: 24 h 00m - 17 h 36 m = 6h 24 m
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